Solar Neutrinos

Only neutrinos, with their extremely small interaction cross sections,
can enable us to see into the interior of a star,
and thus verify directly the hypothesis of nuclear energy generation in stars.

John N. Bahcall (1964)

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References

1 - Books

[1-1]
Neutrinos in high energy and astroparticle physics, Jorge Romao, Jose W. F. Valle, Wiley, 2015. ISBN 978-3-527-41197-9. http://eu.wiley.com/WileyCDA/WileyTitle/productCd-3527411976.html.
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[1-2]
Neutrinos in particle physics, astronomy and cosmology, Zhi-zhong Xing, Shun Zhou, Zhejiang University Press, Hangzhou, 2011. ISBN: 978-7308080248. http://www.zjupress.com/en/redir.php?catalog_id=64&book_id=1446.
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[1-3]
Introduction to the physics of massive and mixed neutrinos, Samoil Bilenky, Springer-Verlag Berlin Heidelberg, 2010. Lecture Notes in Physics, Volume 817; ISBN 978-3-642-14042-6. http://www.springer.com/physics/book/978-3-642-14042-6.
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[1-4]
Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. ISBN 978-0-19-850871-7. http://www.oup.com/uk/catalogue/?ci=9780198508717.
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Stars as laboratories for fundamental physics: The astrophysics of neutrinos, axions, and other weakly interacting particles, G.G. Raffelt, University of Chicago Press, 1996. ISBN 0-226-70272-3. http://wwwth.mpp.mpg.de/members/raffelt/pages/mybook.html.
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[1-6]
Neutrino Astrophysics, J. N. Bahcall, Cambridge University Press, 1989.
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[1-7]
Cauldrons in the Cosmos, Claus E. Rolfs, William S. Rodney, The University of Chicago Press, 1988.
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2 - Reviews - Experiment

[2-1]
The Sudbury Neutrino Observatory, A. Bellerive, J.R. Klein, A.B. McDonald, A.J. Noble, A.W.P. Poon (SNO), Nucl. Phys. B908 (2016) 30-51, arXiv:1602.02469.
[Bellerive:2016byv]
[2-2]
Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos, Arthur B. McDonald, Rev. Mod. Phys. 88 (2016) 030502.
[McDonald:2016ixn]
[2-3]
Solar Neutrino Measurements, A.B. McDonald, New J. Phys. 6 (2004) 121, arXiv:astro-ph/0406253. http://www.iop.org/EJ/S/3/648/5thmNQS.a4iurwqXcRsyZw/abstract/1367-2630/6/1/121.
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[2-4]
Neutrino Masses and Oscillations: Triumphs and Challenges, R.D. McKeown, P. Vogel, Phys. Rep. 394 (2004) 315, arXiv:hep-ph/0402025.
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[2-5]
Astrophysical Neutrino Telescopes, A. B. McDonald et al., Rev. Sci. Instrum. 75 (2004) 293, arXiv:astro-ph/0311343.
[McDonald:2003xn]

3 - Reviews - Experiment - Conference Proceedings

[3-1]
Low-energy neutrinos, Livia Ludhova, J. Phys. Conf. Ser. 718 (2016) 022012, arXiv:1601.08234. TAUP 2015, 7-11 September 2015, Torino (Italy).
[Ludhova:2016wbn]
[3-2]
An Experimental Review of Solar Neutrinos, Jeanne R. Wilson, arXiv:1504.04281, 2015. NuPhys2014.
[Wilson:2015qga]
[3-3]
Everything Under the Sun: A Review of Solar Neutrino, G. D. Orebi Gann, arXiv:1504.02154, 2015.
[Gann:2015yta]
[3-4]
Low Energy Neutrino Measurements, Davide D'Angelo, Pramana 79 (2012) 757-780, arXiv:1211.5359. XXV Lepton Photon, 22 to 27 August 2011.
[DAngelo:2012jch]
[3-5]
Solar Neutrinos in 2011, Alvaro Chavarria, arXiv:1201.6311, 2012. XXXI Physics in Collision 2011.
[Chavarria:2012sd]
[3-6]
Spectroscopy of Solar Neutrinos, Michael Wurm et al., Astron.Nachr. 331 (2010) 512, arXiv:1004.0831. Annual Fall Meeting of the German Astronomische Gesellschaft in Potsdam (Sep 2009).
[Wurm:2010am]
[3-7]
Solar Neutrinos, Marco Pallavicini, arXiv:0910.3304, 2009. XXIX Physics in Collisions conference - Kobe, Japan - 2009.
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[3-8]
Solar neutrino detection, Lino Miramonti, AIP Conf. Proc. 1123 (2009) 166-173, arXiv:0901.3443. III School on Cosmic Rays and Astrophysics August 25 to September 5, 2008 Arequipa (Peru).
[Miramonti:2009hm]
[3-9]
Radiochemical solar neutrino experiments, V. N. Gavrin, B. T. Cleveland, Nucl. Phys. Proc. Suppl. 221 (2011) 90-97, arXiv:nucl-ex/0703012. XXII Int. Conf. on Neutrino Physics and Astrophysics, Santa Fe, 13-19 June 2006.
[Gavrin:2007wc]
[3-10]
Solar Neutrinos, R.G.H. Robertson, Prog. Part. Nucl. Phys. 57 (2006) 90, arXiv:nucl-ex/0602005. International School on Nuclear Physics; 27th Course: 'Neutrinos in Cosmology, in Astro, Particle and Nuclear Physics' in Erice, Sicily, Italy; September 16 - 24, 2005.
[Robertson:2006pk]
[3-11]
Review of Solar and Reactor Neutrinos, A.W.P. Poon, Int. J. Mod. Phys. A21 (2006) 1855-1868, arXiv:hep-ex/0509024. XXII International Symposium on Lepton and Photon Interactions at High Energy (Lepton-Photon 2005, June 30 to July 5, 2005, Uppsala, Sweden).
[Poon:2005qu]
[3-12]
Evidence for Neutrino Mass: A Decade of Discovery, K.M. Heeger, arXiv:hep-ex/0412032, 2004. SEESAW25: International Conference on the Seesaw Mechanism and Neutrino Mass, Paris, France, 10-11 June 2004.
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[3-13]
Recent Results of non-accelarator-based neutrino experiments, Yifang Wang, Int. J. Mod. Phys. A20 (2005) 5244, arXiv:hep-ex/0411028. '32nd International Conference on High Energy Physics', Aug. 16-22, 2004, Beijing, P.R. China.
[Wang:2004wu]
[3-14]
Review of Solar Neutrino Experiments, Alain Bellerive, Int. J. Mod. Phys. A19 (2004) 1167, arXiv:hep-ex/0312045. XXI International Symposium on Lepton and Photon Interactions at High Energies, Fermilab, USA, 11-16 August 2003.
[Bellerive:2003rj]
[3-15]
Neutrino Physics: Experimental Status, T. Kajita, 2003. 19th International Workshop on Weak Interactions and Neutrinos, WIN2003, October 6-11, Lake Geneva, Wisconsin, USA. http://conferences.fnal.gov/win03/Talks/Takaaki%20Kajita.pdf.
Comment: The slide n. 19 shows the $ 90 \% $ C.L. allowed contours for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by different atmospheric neutrino experiments. The figure in slide n.24 shows the $ 90 \% $ C.L. allowed contour for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by Super-Kamiokande. [M.L.].
[Kajita:WIN2003]
[3-16]
Solar Neutrinos, K. Nishikawa, 2002. Topical Seminar on Frontier of Particle Physics 2002: Neutrinos and Cosmology, 20-25 August 2002, Beijing, China. http://bes.ihep.ac.cn/particle/2002/presentation/K.Nishikawa/TALK_1.ZIP.
[Nishikawa-talk:2002a]

4 - Reviews - Experiment - Slides

[4-1]
Radiochemical solar neutrino experiments, successful and otherwise, Richard L. Hahn, 2008. Neutrino 2008, 26-31 May 2008, Christchurch, New Zealand. http://www2.phys.canterbury.ac.nz/~jaa53/presentations/Hahn.pdf.
[Hahn-Nu2008]

5 - Reviews - History

[5-1]
How the sun shines, John N. Bahcall, SLAC Beam Line 31N1 (2001) 2-12, arXiv:astro-ph/0009259.
[Bahcall:2000xc]

6 - Reviews - Astrophysics

[6-1]
Global Seismology of the Sun, Sarbani Basu, arXiv:1606.07071, 2016.
[1606.07071]
[6-2]
Frontiers in Nuclear Astrophysics, Carlos A. Bertulani, Toshitaka Kajino, Prog.Part.Nucl. Phys. 89 (2016) 56-100, arXiv:1604.03197.
[Bertulani:2016eru]
[6-3]
The Global Solar Dynamo, R. H. Cameron, M. Dikpati, A. Brandenburg, arXiv:1602.01754, 2016.
[1602.01754]
[6-4]
Solar and Stellar Photospheric Abundances, Carlos Allende Prieto, arXiv:1602.01121, 2016.
[1602.01121]
[6-5]
Interaction Between Convection and Pulsation, Gunter Houdek, Marc-Antoine Dupret, arXiv:1601.03913, 2016.
[1601.03913]
[6-6]
Solar neutrinos, helioseismology and the solar internal dynamics, S. Turck-Chieze, S. Couvidat, Rept. Prog. Phys. 74 (2011) 086901, arXiv:1009.0852.
[TurckChieze:2010gc]
[6-7]
Solar fusion cross sections II: the pp chain and CNO cycles, E. G. Adelberger et al., Rev. Mod. Phys. 83 (2011) 195, arXiv:1004.2318.
[Adelberger:2010qa]
[6-8]
Astrophysics in 2005, V. Trimble, M.J. Aschwanden, C.J. Hansen, Publ.Astron.Soc.Pac. 118 (2006) 947, arXiv:astro-ph/0606663.
[Trimble:2006gt]
[6-9]
Solar hydrogen burning and neutrinos, W. C. Haxton, P. D. Parker, C. E. Rolfs, Nucl. Phys. A777 (2006) 226-253, arXiv:nucl-th/0501020.
[Haxton:2005rw]
[6-10]
Helioseismology, H. M. Antia, J. Astrophys. Astr. 26 (2005) 161-169.
[Antia-JAA-26-161-2005]
[6-11]
The Solar Hep Process, Kuniharu Kubodera, Tae-Sun Park, Ann. Rev. Nucl. Part. Sci. 54 (2004) 19, arXiv:nucl-th/0402008.
[Kubodera:2004zm]
[6-12]
Fusion cycles in stars and stellar neutrinos, G. Wolschin, arXiv:astro-ph/0210032, 2002.
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[6-13]
Solar fusion cross-sections, Eric G. Adelberger et al., Rev. Mod. Phys. 70 (1998) 1265-1292, arXiv:astro-ph/9805121.
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[6-14]
Standard Solar Composition, N. Grevesse, A. J. Sauval, Space Sci. Rev. 85 (1998) 161-174.
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[6-15]
The Internal Constitution of the Stars, A. S. Eddington, Observatory 43 (1920) 353.
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7 - Reviews - Astrophysics - Conference Proceedings

[7-1]
Solar neutrinos and the sun, Aldo Serenelli, arXiv:1109.2602, 2011. XIV International Workshop on 'Neutrino Telescopes', March 15-18, 2011, Venice, Italy.
[Serenelli:2011ea]
[7-2]
Nuclear Astrophysics: CIPANP 2006, W. C. Haxton, AIP Conf. Proc. 870 (2006) 33-43, arXiv:nucl-th/0609006. CIPANP 2006.
[Haxton:2006ae]
[7-3]
Helioseismology, Neutrinos and Radiative Zones, S. Turck-Chieze, S. Couvidat, L. Piau, EAS Publ.Ser. 17 (2005) 149, arXiv:astro-ph/0511008. Mons 2005: Element Stratifications in Stars: 40 Years of Atomic Diffusion: Meeting in Honor of Georges Michaud, Mons, France, 6-10 June 2005.
[TurckChieze:2005th]
[7-4]
The solar chemical composition, Martin Asplund, Nicolas Grevesse, Jacques Sauval, Nucl. Phys. A777 (2006) 1-4, arXiv:astro-ph/0410214. International Symposium on Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in Honor of Professor David Lambert, Austin, Texas, 17-19 June 2004.
[Asplund:2004eu]
[7-5]
Solar Fusion and The Coulomb Dissociation of 8B; What Have We Learned and Where Do We Go From Here?, Moshe Gai, Heavy Ion Phys. 21 (2004) 335, arXiv:nucl-ex/0303009. 19th Winter Workshop on Nuclear Dynamics, Breckenridge, Colorado, 9-15 Feb 2003.
[Gai:2003yr]
[7-6]
Review of solar models and helioseismology, S. Turck-Chieze, Nucl. Phys. Proc. Suppl. 91 (2001) 73-79.
[Turck-Chieze:2001te]

8 - Reviews - Phenomenology

[8-1]
Solar neutrinos: Oscillations or No-oscillations?, A. Yu. Smirnov, arXiv:1609.02386, 2016.
[Smirnov:2016xzf]
[8-2]
Alive and well: a short review about standard solar models, Aldo Serenelli, Eur.Phys.J. A52 (2016) 78, arXiv:1601.07179.
[Serenelli:2016dgz]
[8-3]
Solar neutrinos and neutrino physics, Michele Maltoni, Alexei Yu. Smirnov, Eur.Phys.J. A52 (2016) 87, arXiv:1507.05287.
[Maltoni:2015kca]
[8-4]
Neutrino oscillations, G. Bellini, L. Ludhova, G. Ranucci, F.L. Villante, Adv.High Energy Phys. 2014 (2014) 191960, arXiv:1310.7858.
[Bellini:2013wra]
[8-5]
Advancements in solar neutrino physics, Vito Antonelli, Lino Miramonti, Int.J.Mod.Phys. E22 (2013) 1330009, arXiv:1304.6304.
[Antonelli:2013nua]
[8-6]
Phenomenology of light sterile neutrinos: a brief review, Antonio Palazzo, Mod.Phys.Lett. A28 (2013) 1330004, arXiv:1302.1102.
[Palazzo:2013me]
[8-7]
Solar Neutrinos: Status and Prospects, W.C. Haxton, R.G. Hamish Robertson, Aldo M. Serenelli, Ann.Rev.Astron.Astrophys. 51 (2013) 21-61, arXiv:1208.5723.
[Robertson:2012ib]
[8-8]
Solar Neutrinos, V. Antonelli, L. Miramonti, C. Pena-Garay, A. Serenelli, Adv.High Energy Phys. 2013 (2013) 351926, arXiv:1208.1356.
[Antonelli:2012qu]
[8-9]
Neutrino Physics and The Solar Neutrino Problem, Andrew John Lowe, arXiv:0907.3658, 2009.
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[8-10]
The Scientific Life Of John Bahcall, W. C. Haxton, Ann. Rev. Nucl. Part. Sci. 59 (2009) 1-20, arXiv:0904.2865.
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[8-11]
Phenomenology with Massive Neutrinos, M. C. Gonzalez-Garcia, Michele Maltoni, Phys. Rept. 460 (2008) 1-129, arXiv:0704.1800.
[GonzalezGarcia:2007ib]
[8-12]
Global analysis of three-flavor neutrino masses and mixings, G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, Prog. Part. Nucl. Phys. 57 (2006) 742-795, arXiv:hep-ph/0506083.
[Fogli:2005cq]
[8-13]
Report of the Solar and Atmospheric Neutrino Experiments Working Group of the APS Multidivisional Neutrino Study, H. Back et al., arXiv:hep-ex/0412016, 2004.
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[8-14]
Solar models and solar neutrino oscillations, John N. Bahcall, Carlos Pena-Garay, New J. Phys. 6 (2004) 63, arXiv:hep-ph/0404061.
[Bahcall:2004mz]
[8-15]
Low Energy Neutrino Physics after SNO and KamLAND, Lothar Oberauer, Mod. Phys. Lett. A19 (2004) 337, arXiv:hep-ph/0402162.
[Oberauer:2004ji]
[8-16]
Evidence for the MSW effect, Gianluigi Fogli, Eligio Lisi, New J. Phys. 6 (2004) 139.
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[8-17]
Theoretical neutrino physics, H. Murayama, Eur. Phys. J. C33 (2004) s51-s66. http://www.edpsciences.org/articles/epjc/pdf/2004/19/10052S51.pdf?access=ok.
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[8-18]
Neutrino Mixing, Carlo Giunti, Marco Laveder, arXiv:hep-ph/0310238, 2003. In 'Developments in Quantum Physics - 2004', p. 197-254, edited by F. Columbus and V. Krasnoholovets, Nova Science, Hauppauge, NY. http://novapublishers.com/catalog/product_info.php?products_id=1633.
[Giunti:2003qt]
[8-19]
Solar neutrino physics: Historical evolution, present status and perspectives, L. Miramonti, F. Reseghetti, La Rivista del Nuovo Cimento 25 (2002) 1, arXiv:hep-ex/0302035.
[Miramonti:2002wz]
[8-20]
Direct observation of neutrino oscillations at the Sudbury Neutrino Observatory, B. Ananthanarayan, Ritesh K. Singh, Curr. Sci. 83 (2002) 553, arXiv:physics/0208096.
[Ananthanarayan:2002hx]
[8-21]
Neutrino Masses and Mixing: Evidence and Implications, M.C. Gonzalez-Garcia, Y. Nir, Rev. Mod. Phys. 75 (2003) 345-402, arXiv:hep-ph/0202058.
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[8-22]
The solar neutrino problem and its oscillation solution, M. B. Smy, Mod. Phys. Lett. A17 (2002) 2163-2178.
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[8-23]
Solar neutrinos, M. F. Altmann, R. L. Mossbauer, L. J. N. Oberauer, Rept. Prog. Phys. 64 (2001) 97-146.
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[8-24]
Solar neutrinos, Yoichiro Suzuki, Int. J. Mod. Phys. A15S1 (2000) 201-228.
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Phenomenology of neutrino oscillations, S. M. Bilenky, C. Giunti, W. Grimus, Prog. Part. Nucl. Phys. 43 (1999) 1, arXiv:hep-ph/9812360.
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Solar neutrinos: Beyond standard solar models, V. Castellani, S. Degl'Innocenti, G. Fiorentini, M. Lissia, B. Ricci, Phys. Rep. 281 (1997) 309-398, arXiv:astro-ph/9606180.
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The Solar interior, S. Turck-Chieze et al., Phys. Rep. 230 (1993) 57-235.
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On using a neutrino magnetic moment to attack the solar neutrino problem, X. Shi, D.N. Schramm, R. Rosner, D.S. Dearborn, Comments Nucl.Part.Phys. 21 (1993) 151-182.
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Particle physics confronts the solar neutrino problem, Palash B. Pal, Int.J.Mod.Phys. A7 (1992) 5387-5460.
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The Solar neutrino problem and the neutrino magnetic moment, Joao Pulido, Phys.Rept. 211 (1992) 167-199.
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Neutrino oscillations in matter, T. K. Kuo, James Pantaleone, Rev. Mod. Phys. 61 (1989) 937.
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Resonance oscillations of neutrinos in matter, S. P. Mikheev, A. Yu. Smirnov, Sov. Phys. Usp. 30 (1987) 759-790.
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9 - Reviews - Phenomenology - Conference Proceedings

[9-1]
Neutrino Astrophysics, Cristina Volpe, Acta Phys.Polon.Supp. 9 (2016) 769, arXiv:1609.06747. 52th Winter School of Theoretical Physics, Ladek Zdroj, 14-21 February 2016.
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[9-2]
Oscillations at low energies, D.A. Dwyer, L. Ludhova, Nucl. Part. Phys. Proc. 265-266 (2015) 339-345, arXiv:1506.01998. Neutrino Oscillation Workshop, 2014.
[Dwyer:2015exa]
[9-3]
Neutrino astrophysics : recent advances and open issues, Cristina Volpe, J. Phys. Conf. Ser. 631 (2015) 012048, arXiv:1503.01355. DISCRETE 2014.
[Volpe:2015yya]
[9-4]
Recent advances in neutrino astrophysics, Cristina Volpe, PoS FFP14 (2016) 127, arXiv:1411.6533. Frontiers of Fundamental Physics 2014, July 15-18, Marseille.
[Volpe:2014rca]
[9-5]
Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data, Vito Antonelli, Lino Miramonti, arXiv:1311.2575, 2013. 14th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications (Villa Olmo, Como - September 2013).
[Antonelli:2013eva]
[9-6]
Neutrino 2012: Outlook - theory, A. Yu. Smirnov, Nucl. Phys. Proc. Suppl. 235-236 (2013) 431-440, arXiv:1210.4061. XXV International Conference on Neutrino Physics and Astrophysics, June 3 - 9, 2012, Kyoto, Japan.
[Smirnov:2012ei]
[9-7]
Neutrinos and the stars, Georg Raffelt, Proc.Int.Sch.Phys.Fermi 182 (2012) 61-143, arXiv:1201.1637. ISAPP School 'Neutrino Physics and Astrophysics', 26 July-5 August 2011, Villa Monastero, Varenna, Italy.
[Raffelt:2012kt]
[9-8]
New Results on Solar Neutrinos, Alain Bellerive, PoS ICHEP2010 (2010) 529, arXiv:1012.2493. 35th International Conference of High Energy Physics, Paris, France, July 22-28, 2010.
[Bellerive:2010xw]
[9-9]
Lectures on neutrino phenomenology, Walter Winter, Nucl. Phys. B, Proc. Suppl. 203-204 2010 (2010) 45-81, arXiv:1004.4160. Schladming Winter School 2010 'Masses and Constants'.
[Winter:2010hb]
[9-10]
Significance of neutrino cross-sections for astrophysics, A.B. Balantekin, AIP Conf. Proc. 1189 (2009) 11-15, arXiv:0909.0226. NUINT2009 (6th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region), May 18-22, 2009, Sitges, Barcelona, Spain.
[Balantekin:2009qq]
[9-11]
Muons and Neutrinos 2007, Thomas K. Gaisser, arXiv:0801.4542, 2008. 30th International Cosmic Ray Conference, Merida, Yucatan, July, 2007.
[Gaisser:2008cp]
[9-12]
Solar Neutrinos: Models, Observations, and New Opportunities, W. C. Haxton, Publ. Astron. Soc. Austral. 25 (2008) 44-51, arXiv:0710.2295. Nuclear Astrophysics 1957:2007: Beyond the First 50 Years, Caltech, July, 2007.
[Haxton:2007kg]
[9-13]
Global fits to neutrino oscillation data, Thomas Schwetz, Phys. Scripta T127 (2006) 1-5, arXiv:hep-ph/0606060. SNOW2006 workshop, Stockholm, 2-6 May 2006.
[Schwetz:2006dh]
[9-14]
Neutrino oscillations: Current status and prospects, Thomas Schwetz, Acta Phys. Polon. B36 (2005) 3203, arXiv:hep-ph/0510331. XXIX International Conference of Theoretical Physics, 'Matter To The Deepest: Recent Developments In Physics of Fundamental Interactions', 8-14 September 2005, Ustron, Poland.
[Schwetz:2005jr]
[9-15]
Status of the Standard Solar Model Prediction of Solar Neutrino Fluxes, Moshe Gai, Phys. Atom. Nucl. 69 (2006) 1805-1811, arXiv:nucl-ex/0510081. Fifth International Conferenceon Non-Accelerator New Physics, Dubna, June 20-25, 2005.
[Gai:2005md]
[9-16]
Neutrino mass and mixing parameters: A short review, G.L. Fogli et al., arXiv:hep-ph/0506307, 2005. 40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005.
[Fogli:2005gs]
[9-17]
Solar Models and Solar Neutrinos: Current Status, John N. Bahcall, Phys. Scripta T121 (2005) 46, arXiv:hep-ph/0412068. Nobel Symposium 2004, Enkoping, Sweden, August 19-24, 2004.
[Bahcall:2004qv]
[9-18]
Three-flavour effects and CP- and T-violation in neutrino oscillations, Evgeny Akhmedov, Phys. Scripta T121 (2005) 65, arXiv:hep-ph/0412029. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
[Akhmedov:2004ve]
[9-19]
Physics of Massive Neutrinos, J. W. F. Valle, Nucl. Phys. Proc. Suppl. 149 (2005) 3, arXiv:hep-ph/0410103. Sixth International Conf. on Neutrino Factories and SuperBeams (NuFact04) Osaka, Japan, July 26-August 1, 2004.
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[9-20]
Neutrino 2004: Concluding Talk, Guido Altarelli, Nucl. Phys. Proc. Suppl. 143 (2005) 470, arXiv:hep-ph/0410101. Neutrino 2004, Paris, 14-19 June 2004.
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[9-21]
Global Analysis of Neutrino Data, M. C. Gonzalez-Garcia, Phys. Scripta T121 (2005) 72, arXiv:hep-ph/0410030. Nobel Symposium on Neutrino Physics, Haga Slott, Enkoping, Sweden.
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[9-22]
Solar Neutrino Oscillation - An Overview, D. P. Roy, arXiv:hep-ph/0409336, 2004. Xth International Symposium on Particles, Strings and Cosmology (PASCOS), Boston, 16-22 August 2004.
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[9-23]
Solar Neutrino Oscillation Parameters in Experiments with Reactor Anti-Neutrinos, Sandhya Choubey, arXiv:hep-ph/0402288, 2004. 2nd International Workshop on Neutrino oscillations in Venice (NOVE), December 3-5, 2003, Venice, Italy.
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[9-24]
Neutrinos: '...annus mirabilis', A. Yu. Smirnov, arXiv:hep-ph/0402264, 2004. 2nd Int. Workshop on Neutrino oscillations in Venice (NOVE) December 3-5, 2003, Venice, Italy.
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[9-25]
Neutrino physics, recent results, E. Lisi, 2004. IFAE-2004, 14-16 April 2004, Torino, Italy. http://agenda.cern.ch/askArchive.php?base=agenda&categ=a041654&id=a041654s3t6/transparencies. http://www.ph.unito.it/ifae/Proceedings/Sessioni/Neutrinos.pdf.
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[9-26]
Global analysis of neutrino oscillation, S. Goswami, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/goswami.pdf.
[Goswami-Nu2004]
[9-27]
Solar neutrino oscillation phenomenology, S. Goswami, Pramana 62 (2004) 241, arXiv:hep-ph/0307224. 9th International Symposium on Particles, Strings and Cosmology (PASCOS 03), Mumbai, India, 3-8 Jan 2003.
[Goswami:2003ek]
[9-28]
Neutrino masses twenty-five years later, J. W. F. Valle, Aip Conf. Proc. 687 (2003) 16, arXiv:hep-ph/0307192. MRST'03 (Joe-Fest), Syracuse, NY, May 2003.
[Valle:2003rh]
[9-29]
Neutrino oscillations in the framework of the tree-neutrino mixing, S. M. Bilenky, arXiv:hep-ph/0307186, 2003. Ist Yamada Symposium Om neutrinos and Dark Matter in Nuclear Physics, June 9-14, 2003, Nara, Japan.
[Bilenky:2003rb]
[9-30]
Neutrino Physics after KamLAND, A. Yu. Smirnov, arXiv:hep-ph/0306075, 2003. 4th Workshop on 'Neutrino Oscillations and their Origin' (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Smirnov.pdf.
[Smirnov:2003uu]
[9-31]
Status of Neutrino Fits, C. Giunti, arXiv:hep-ph/0305139, 2003. XXXVIIIth Rencontres de Moriond, ElectroWeak Interactions and Unified Theories, 15-22 March 2003, Les Arcs, France. http://moriond.in2p3.fr/EW/2003/Transparencies/1_Sunday/1_2_afternoon/1_2_6_Giunti/C.Giunti.pdf.
[Giunti:2003vf]
[9-32]
The MSW effect and Solar Neutrinos, A. Yu. Smirnov, arXiv:hep-ph/0305106, 2003. 11th workshop on Neutrino Telescopes, Venice, March 11- 14, 2003.
[Smirnov:2003da]
[9-33]
Neutrino Masses and Mixing: Where We Stand and Where We are Going, M. C. Gonzalez-Garcia, arXiv:hep-ph/0211054, 2002. 10th International Conference on Supersymmetry and Unification of Fundamental Interactions, SUSY02 (June 17-23, 2002, DESY, Hamburg).
[GonzalezGarcia:2002sm]
[9-34]
Theory of Neutrino Masses and Mixing, M. C. Gonzalez-Garcia, Nucl. Phys. Proc. Suppl. 117 (2003) 186, arXiv:hep-ph/0210359. 31st international conference on high energy physics (ICHEP 2002), Amsterdam, 24-31 July 2002.
[GonzalezGarcia:2002sz]
[9-35]
Current Status of Neutrino Masses and Mixings, C. Giunti, Nucl. Phys. Proc. Suppl. 117 (2003) 24-28, arXiv:hep-ph/0209103. 31st International Conference on High Energy Physics 'ICHEP02', 24-31 July 2002, Amsterdam. http://www.ichep02.nl/Transparencies/NEU/NEU-2/NEU-2-1.giunti.ps.
[Giunti:2002sr]
[9-36]
Global analysis of solar neutrinos, S. Choubey, 2002. Fourth NuFact '02 Workshop on Neutrino Factories based on Muon Storage Rings, Imperial College, London, 1-6 July 2002. http://www.hep.ph.ic.ac.uk/NuFact02/Scientific-programme/files/Wednesday/wg2/A01_choubey.ps.
[Choubey-talk:2002a]
[9-37]
Actuality and potentiality of neutrino mixing, C. Giunti, 2002. IIIrd International Workshop on Low Energy Solar Neutrinos - LowNu 2002, 22-24 May 2002, Heidelberg, Germany. http://www.mpi-hd.mpg.de/nubis/www_lownu2002/transparency/giunti_lownu_2002.pdf.
[Giunti-LowNu2002]

10 - Experiment

[10-1]
Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino, M. Agostini et al. (Borexino), arXiv:1701.07970, 2017.
[Agostini:2017iiq]
[10-2]
Solar Neutrino Measurements in Super-Kamiokande-IV, K. Abe et al. (Super-Kamiokande), Phys. Rev. D94 (2016) 052010, arXiv:1606.07538.
[Abe:2016nxk]
[10-3]
Measurement of neutrino flux from the primary proton-proton fusion process in the Sun with Borexino detector, O. Y. Smirnov et al. (Borexino), Phys.Part.Nucl. 47 (2016) 995-1002, arXiv:1507.02432.
[Smirnov:2015lxy]
[10-4]
7Be Solar Neutrino Measurement with KamLAND, A. Gando et al. (KamLAND), Phys.Rev. C92 (2015) 055808, arXiv:1405.6190.
[Gando:2014wjd]
[10-5]
Neutrinos from the primary proton-proton fusion process in the Sun, G. Bellini et al. (Borexino), Nature 512 (2014) 383-386.
[Bellini:2014uqa]
[10-6]
First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation, A. Renshaw et al. (Super-Kamiokande), Phys. Rev. Lett. 112 (2014) 091805, arXiv:1312.5176.
[Renshaw:2013dzu]
[10-7]
New limits on heavy sterile neutrino mixing in ${^{8}\rm{B}}$-decay obtained with the Borexino detector, G. Bellini et al. (Borexino), Phys. Rev. D 88, 072010 (2013) 072010, arXiv:1311.5347.
[Bellini:2013uui]
[10-8]
Final results of Borexino Phase-I on low energy solar neutrino spectroscopy, G. Bellini et al. (Borexino), Phys. Rev. D89 (2014) 112007, arXiv:1308.0443.
[Bellini:2013lnn]
[10-9]
First evidence of pep solar neutrinos by direct detection in Borexino, G. Bellini et al. (Borexino), Phys. Rev. Lett. 108 (2012) 051302, arXiv:1110.3230.
[Collaboration:2011nga]
[10-10]
Combined Analysis of all Three Phases of Solar Neutrino Data from the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Phys. Rev. C88 (2013) 025501, arXiv:1109.0763.
[Aharmim:2011vm]
[10-11]
Measurement of the $\nu_e$ and Total $^{8}$B Solar Neutrino Fluxes with the Sudbury Neutrino Observatory Phase-III Data Set, B. Aharmim et al. (SNO), Phys. Rev. C87 (2013) 015502, arXiv:1107.2901.
[Aharmim:2011yq]
[10-12]
Measurement of the 8B Solar Neutrino Flux with KamLAND, S. Abe et al. (KamLAND), Phys. Rev. C84 (2011) 035804, arXiv:1106.0861.
[Abe:2011em]
[10-13]
Absence of day-night asymmetry of 862 keV $^7\text{Be}$ solar neutrino rate in Borexino and MSW oscillation parameters, G. Bellini et al. (Borexino), Phys. Lett. B707 (2012) 22-26, arXiv:1104.2150.
[Bellini:2011yj]
[10-14]
Precision measurement of the $^7\text{Be}$ solar neutrino interaction rate in Borexino, G. Bellini et al. (Borexino), Phys. Rev. Lett. 107 (2011) 141302, arXiv:1104.1816.
[Bellini:2011rx]
[10-15]
Solar neutrino results in Super-Kamiokande-III, K. Abe et al. (Super-Kamiokande), Phys. Rev. D83 (2011) 052010, arXiv:1010.0118.
[Abe:2010hy]
[10-16]
Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS, G. Bellini (Borexino), Phys. Lett. B696 (2011) 191-196, arXiv:1010.0029.
[Bellini:2010gn]
[10-17]
Reanalysis of the GALLEX solar neutrino flux and source experiments, F. Kaether, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, Phys. Lett. B685 (2010) 47-54, arXiv:1001.2731.
[Kaether:2010ag]
[10-18]
Low Energy Threshold Analysis of the Phase I and Phase II Data Sets of the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Phys. Rev. C81 (2010) 055504, arXiv:0910.2984.
[Aharmim:2009gd]
[10-19]
Searches for High Frequency Variations in the $^8\text{B}$ Solar Neutrino Flux at the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 710 (2010) 540-548, arXiv:0910.2433.
[Collaboration:2009qz]
[10-20]
Measurement of the solar neutrino capture rate with Gallium metal, Part III, J. N. Abdurashitov et al. (SAGE), Phys. Rev. C80 (2009) 015807, arXiv:0901.2200.
[Abdurashitov:2009tn]
[10-21]
Measurement of the solar $^{8}\text{B}$ neutrino flux with 246 live days of Borexino and observation of the MSW vacuum-matter transition, G. Bellini et al. (Borexino), Phys. Rev. D82 (2010) 033006, arXiv:0808.2868.
[Bellini:2008mr]
[10-22]
The Borexino detector at the Laboratori Nazionali del Gran Sasso, G. Alimonti et al. (Borexino), Nucl. Instrum. Meth. A600 (2009) 568-593, arXiv:0806.2400.
[Alimonti:2008gc]
[10-23]
An Independent Measurement of the Total Active 8B Solar Neutrino Flux Using an Array of 3He Proportional Counters at the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Phys. Rev. Lett. 101 (2008) 111301, arXiv:0806.0989.
[Aharmim:2008kc]
[10-24]
New results on solar neutrino fluxes from 192 days of Borexino data, C. Arpesella et al. (Borexino), Phys. Rev. Lett. 101 (2008) 091302, arXiv:0805.3843.
[Arpesella:2008mt]
[10-25]
Solar neutrino measurements in Super-Kamiokande-II, J.P. Cravens et al. (Super-Kamiokande), Phys. Rev. D78 (2008) 032002, arXiv:0803.4312.
From the abstract: The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time-variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity.
[Cravens:2008aa]
[10-26]
First real time detection of ${}^{7}\text{B}$ solar neutrinos by Borexino, C. Arpesella et al. (Borexino), Phys. Lett. B658 (2008) 101-108, arXiv:0708.2251.
[Arpesella:2007xf]
[10-27]
Measurement of the $\nu_e$ and Total ${}^{8}\text{B}$ Solar Neutrino Fluxes with the Sudbury Neutrino Observatory Phase I Data Set, B. Aharmim et al. (SNO), Phys. Rev. C75 (2007) 045502, arXiv:nucl-ex/0610020.
[Aharmim:2007nv]
[10-28]
A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 653 (2006) 1545-1551, arXiv:hep-ex/0607010.
[Aharmim:2006wq]
[10-29]
Search for electron antineutrino interactions with the Borexino Counting Test Facility at Gran Sasso, M. Balata et al. (Borexino), Eur. Phys. J. C47 (2006) 21-30, arXiv:hep-ex/0602027.
[Balata:2006db]
[10-30]
The SAGE@LNGS experiment: Measurement of solar neutrinos at LNGS using gallium from SAGE, J. N. Abdurashitov et al., Astropart. Phys. 25 (2006) 349-354, arXiv:nucl-ex/0509031.
[Abdurashitov:2005ax]
[10-31]
Solar neutrino measurements in Super-Kamiokande-I, J. Hosaka et al. (Super-Kamkiokande), Phys. Rev. D73 (2006) 112001, arXiv:hep-ex/0508053.
[Hosaka:2005um]
[10-32]
A Search for Periodicities in the $^8\text{B}$ Solar Neutrino Flux Measured by the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Phys. Rev. D72 (2005) 052010, arXiv:hep-ex/0507079.
From the abstract: The variation at a period of one year is consistent with modulation of the $^8\text{B}$ neutrino flux by the Earth's orbital eccentricity. No significant sinusoidal periodicities are found with periods between 1 day and 10 years.
[Aharmim:2005iu]
[10-33]
Complete results for five years of GNO solar neutrino observations, M. Altmann et al. (GNO), Phys. Lett. B616 (2005) 174, arXiv:hep-ex/0504037.
[Altmann:2005ix]
[10-34]
Electron Energy Spectra, Fluxes, and Day-Night Asymmetries of $^8\text{B}$ Solar Neutrinos from the 391-Day Salt Phase SNO Data Set, B. Aharmim et al. (SNO), Phys. Rev. C72 (2005) 055502, arXiv:nucl-ex/0502021.
[Aharmim:2005gt]
[10-35]
Electron Antineutrino Search at the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Phys. Rev. D70 (2004) 093014, arXiv:hep-ex/0407029.
[Aharmim:2004uf]
[10-36]
Limit On the Neutrino Magnetic Moment Using 1496 Days of Super-Kamiokande-I Solar Neutrino Data, D. W. Liu et al. (Super-Kamiokande), Phys. Rev. Lett. 93 (2004) 021802, arXiv:hep-ex/0402015.
[Liu:2004ny]
[10-37]
Precise Measurement of the Solar Neutrino Day/Night and Seasonal Variation in Super-Kamiokande-I, M. B. Smy et al. (Super-Kamiokande), Phys. Rev. D69 (2004) 011104, arXiv:hep-ex/0309011.
[Smy:2003jf]
[10-38]
Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity, S. N. Ahmed et al. (SNO), Phys. Rev. Lett. 92 (2004) 181301, arXiv:nucl-ex/0309004.
[Ahmed:2003kj]
[10-39]
A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I, J. Yoo et al. (Super-Kamiokande), Phys. Rev. D68 (2003) 092002, arXiv:hep-ex/0307070.
[Yoo:2003rc]
[10-40]
Search for $\bar\nu_e$ from the sun at Super-Kamiokande-I, Y. Gando et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 171302, arXiv:hep-ex/0212067.
From the article: For the ${}^8\mathrm{B}$ spectrum the upper limit to the solar $\bar{\nu}_e$ flux is $8 \times 10^{-3}$ of the SSM $\nu_e$ flux prediction for total energy = 8 Mev - 20 MeV.
[Gando:2002ub]
[10-41]
Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data, S. Fukuda et al. (Super-Kamiokande), Phys. Lett. B539 (2002) 179-187, arXiv:hep-ex/0205075.
[Fukuda:2002pe]
[10-42]
Measurement of the Solar Neutrino Capture Rate by the Russian-American Gallium Solar Neutrino Experiment During One Half of the 22-Year Cycle of Solar Activity, J. N. Abdurashitov et al. (SAGE), J. Exp. Theor. Phys. 95 (2002) 181-193, arXiv:astro-ph/0204245.
From the abstract: Combined analysis of the data of 92 runs during the 12-year period January 1990 through December 2001 gives a capture rate of solar neutrinos with energy more than 233 keV of 70.8 +5.3/-5.2 (stat.) +3.7/-3.2 (syst.) SNU. This represents only slightly more than half of the predicted standard solar model rate of 130 SNU.... Using a simple analysis of the SAGE results combined with those from all other solar neutrino experiments, we estimate the electron neutrino pp flux that reaches the Earth to be (4.6 ± 1.1) × 1010 cm-2 s-1. Assuming that neutrinos oscillate to active flavors the pp neutrino flux emitted in the solar fusion reaction is approximately (7.7 ± 1.8) × 1010 cm-2 s-1, in agreement with the standard solar model calculation of (5.95 ± 0.06) × 1010 cm-2 s-1.
[Abdurashitov:2002nt]
[10-43]
Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters, Q. R. Ahmad et al. (SNO), Phys. Rev. Lett. 89 (2002) 011302, arXiv:nucl-ex/0204009. http://www.sno.phy.queensu.ca/sno/results_04_02/DayNight.
[Ahmad:2002ka]
[10-44]
Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory, Q. R. Ahmad et al. (SNO), Phys. Rev. Lett. 89 (2002) 011301, arXiv:nucl-ex/0204008. http://www.sno.phy.queensu.ca/sno/results_04_02/NC.
[Ahmad:2002jz]
[10-45]
Search for radiative decays of solar neutrinos during a solar eclipse, G. Giacomelli, V. Popa, arXiv:hep-ex/0110013, 2001.
[Giacomelli:2001zb]
[10-46]
Measurement of the Rate of $\nu_e + d \to p + p + e^-$ Interactions Produced by $^8$B Solar Neutrinos at the Sudbury Neutrino Observatory, Q. R. Ahmad et al. (SNO), Phys. Rev. Lett. 87 (2001) 071301, arXiv:nucl-ex/0106015.
[Ahmad:2001an]
[10-47]
Solar $^8\mathrm{B}$ and $hep$ neutrino measurements from 1258 days of Super-Kamiokande data, S. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 86 (2001) 5651-5655, arXiv:hep-ex/0103032.
[Fukuda:2001nj]
[10-48]
Measurement of the solar neutrino capture rate by SAGE and implications for neutrino oscillations in vacuum, J. N. Abdurashitov et al. (SAGE), Phys. Rev. Lett. 83 (1999) 4686-4689, arXiv:astro-ph/9907131.
[Abdurashitov:1999bv]
[10-49]
Measurement of the solar neutrino capture rate with gallium metal, J. N. Abdurashitov et al. (SAGE), Phys. Rev. C60 (1999) 055801, arXiv:astro-ph/9907113.
[Abdurashitov:1999zd]
[10-50]
GALLEX solar neutrino observations: Results for GALLEX IV, W. Hampel et al. (GALLEX), Phys. Lett. B447 (1999) 127.
[GALLEX-99]
[10-51]
Measurement of the solar neutrino energy spectrum using neutrino electron scattering, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2430-2434, arXiv:hep-ex/9812011.
[Fukuda:1998ua]
[10-52]
Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super- Kamiokande, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 1810-1814, arXiv:hep-ex/9812009.
[Fukuda:1998rq]
[10-53]
Measurements of the solar neutrino flux from Super- Kamiokande's first 300 days, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1158-1162, arXiv:hep-ex/9805021.
[Fukuda:1998fd]
[10-54]
Measurement of the solar electron neutrino flux with the Homestake chlorine detector, B. T. Cleveland et al. (Homestake), Astrophys. J. 496 (1998) 505.
[Cleveland:1998nv]

11 - Experiment - Conference Proceedings

[11-1]
The Main Results of the Borexino Experiment, A. Derbin et al., arXiv:1605.06795, 2016. Third Annual Large Hadron Collider Physics Conference, St. Petersburg, Russia, 2015.
[Derbin:2016cfw]
[11-2]
Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun, P. Mosteiro et al., Nucl. Part. Phys. Proc. 265-266 (2015) 87-92, arXiv:1508.05379. NOW (Neutrino Oscillation Workshop) 2014.
[Mosteiro:2015boa]
[11-3]
Solar neutrino with Borexino: results and perspectives, O. Smirnov et al. (Borexino), Phys.Part.Nucl. 46 (2015) 166-173, arXiv:1410.0779. International Workshop on Prospects of Particle Physics, 'Neutrino Physics and Astrophysics', Valday, Russia, January 26 - February 02, 2014.
[Smirnov:2014hbh]
[11-4]
Recent Borexino results and prospects for the near future, D. D'Angelo et al. (Borexino), EPJ Web Conf. 126 (2016) 02008, arXiv:1405.7919. Rencontres de Moriond EW 2014.
[DAngelo:2014lmb]
[11-5]
Solar Neutrino Results from Super-Kamiokande, Andrew Renshaw (Super-Kamiokande), Phys.Procedia 61 (2015) 345-354, arXiv:1403.4575.
[Renshaw:2014awa]
[11-6]
Solar neutrino analysis of Super-Kamiokande, Hiroyuki Sekiya (Super-Kamiokande), arXiv:1307.3686, 2013. 33rd International Cosmic Ray Conference, Rio De Janeiro 2013 (ICRC2013).
[Sekiya:2013hda]
[11-7]
Solar neutrino physics with Borexino I, L. Ludhova et al. (BOREXINO), arXiv:1205.2989, 2012. Moriond 2012 EW session.
[Ludhova:2012tb]
[11-8]
Low Energy Neutrino Astronomy in Super-Kamiokande, Michael Smy, arXiv:1110.0012, 2011. DPF 2011.
[Smy:2011tm]
[11-9]
The Recent Results of the Solar Neutrino Measurement in Borexino, Yusuke Koshio (Borexino), arXiv:1106.3055, 2011. Recontres de Moriond EW session 2011.
[Koshio:2011vq]
[11-10]
Results from the solar neutrino experiment BOREXINO, Lothar Oberauer (Borexino), J. Phys. Conf. Ser. 203 (2010) 012081.
[Oberauer:2010zz]
[11-11]
Solar neutrino results from Borexino and main future perspectives, M. Pallavicini (Borexino), Nucl. Instrum. Meth. A630 (2011) 210-213, arXiv:0910.3367. RICAP 2009.
[Pallavicini:2009ph]
[11-12]
Solar Neutrino Measurement at SK-III, B.S. Yang (Super-Kamiokande), arXiv:0909.5469, 2009. DPF-2009, Detroit, MI, July 2009.
[Yang:2009hp]
[11-13]
Searching for hep Neutrinos using the Sudbury Neutrino Observatory, Chris Howard (SNO), arXiv:0906.0040, 2009.
[Howard:2009uz]
[11-14]
Results from the Neutral Current Detector phase of the Sudbury Neutrino Observatory, Ryan Martin (SNO), arXiv:0905.4907, 2009. Lake Louise Winter Institute 2009.
[Martin:2009pb]
[11-15]
Results from the Borexino Experiment, Timo Lewke (Borexino), arXiv:0905.2526, 2009. Moriond 2009 EW session.
[Lewke:2009ry]
[11-16]
The first year of Borexino, Borexino (Borexino), arXiv:0905.1044, 2009. Heavy Quarks and Leptons, Melbourne, 2008.
[Franco:2009wg]
[11-17]
Measurement of the Solar Neutrino Flux with an Array of Neutron Detectors in the Sudbury Neutrino Observatory, Blair Jamieson, for the SNO Collaboration (SNO), arXiv:0810.3760, 2008. ICHEP08.
[Jamieson:2008wd]
[11-18]
Recent Results from Super-Kamiokande, H. Sekiya et al. (Super-Kamiokande), arXiv:0810.0595, 2008. ICHEP08, Philadelphia, USA, July 2008.
[Sekiya:2008nb]
[11-19]
Results and perspectives of the solar neutrino experiment Borexino, G. Ranucci (Borexino), arXiv:0810.0176, 2008. ICHEP08, Philadelphia, USA, July 2008.
[Ranucci:2008ng]
[11-20]
Search for possible solar neutrino radiative decays during total solar eclipses, S. Cecchini et al., arXiv:hep-ex/0606037, 2006. SPSE2006, Waw an Namos, Libya, 27-29 March 2006.
[Cecchini:2006fz]
[11-21]
Integral Fluxes, Day-Night, and Spectrum Results from SNO's 391-Day Salt Phase, Juergen Wendland et al. (SNO), arXiv:hep-ex/0507058, 2005. Lake Louise Winter Institute: Fundamental Interactions, Lake Louise, Alberta, Canada, Feb 20-26 2005.
[Wendland:2005kj]
[11-22]
Results from the Salt Phase of SNO, K. Miknaitis (SNO), arXiv:hep-ex/0505071, 2005. XXXXth Rencontres de Moriond: Electroweak Interactions and Unified Theories, La Thuile, Italy, March 5-12, 2005.
[Miknaitis:2005rw]
[11-23]
Measurement of the SAGE Response to Neutrinos from Ar37 Source, V.N. Gavrin (SAGE), 2005. XI International Workshop on Neutrino Telescopes, February 22-25, 2005, Venice, Italy. http://www.pd.infn.it/~laveder/unbound/talks/exp/sage/VE05-Gavrin.pdf.
Comment: The ratio of the production rate (measured/predicted) is $0.79 +0.09 -0.10$.
[Gavrin:Venice2005]
[11-24]
Sudbury Neutrino Observatory Results, A.B. McDonald et al. (SNO), Phys. Scripta T121 (2005) 29, arXiv:hep-ex/0412060. Nobel Symposium 129, August 19-24, 2004, Enkoping, Sweden.
[McDonald:2004rx]
[11-25]
Super Kamiokande results: atmospheric and solar neutrinos, M.Ishitsuka (Super-Kamiokande), arXiv:hep-ex/0406076, 2004. XXXIX Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, March 21-28-2004. http://moriond.in2p3.fr/EW/2004/transparencies/3_Wednesday/3_2_afternoon/3_2_3_Ishitsuka/Ishitsuka.pdf.
[Ishitsuka:2004un]
[11-26]
High Sensitivity Anti-Neutrino Detection by KamLAND, S. Hatakeyama et al. (KamLAND), arXiv:hep-ex/0405001, 2004. Moriond EW04.
[Hatakeyama:2004gm]
[11-27]
Search for neutrino radiative decays during a total solar eclipse, V. Popa, PoS AHEP2003 (2003) AHEP2003/068, arXiv:hep-ex/0402014. AHEP2003, Valencia.
[Popa:2004nx]
[11-28]
SuperKamiokande's solar neutrino results, M. Nakahata (Super-Kamiokande), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/nakahata.pdf.
[Nakahata-Nu2004]
[11-29]
Results from radiochemical solar neutrino experiments, C. Cattadori, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/cattadori.ppt.
[Cattadori-Nu2004]
[11-30]
The Sudbury Neutrino Observatory, J. Wilkerson (SNO), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/wilkerson.pdf.
[Wilkerson-Nu2004]
[11-31]
KamLAND: updated results, K. Inoue, 2004. Neutrino Oscillation Workshop NOW 2004, September 11-17, 2004, Conca Specchiulla (Otranto, Italy). http://www.ba.infn.it/~now2004/talks/12_09_04/plen/KamLAND.pdf.
[Inoue:2004]
[11-32]
Recent Results from the Sudbury Neutrino Observatory, A. W. P. Poon (SNO), Eur. Phys. J. C33 (2004) S823, arXiv:hep-ex/0312002. International Europhysics Conference on High Energy Physics (EPS2003).
[Poon:2003xx]
[11-33]
Recent Results from KamLAND, J. Detwiler (KamLAND), eConf C0307282 (2003) TW04, arXiv:hep-ex/0311007. SLAC Summer Institute, July 2003.
[Detwiler:2003fb]
[11-34]
The Solar Neutrino Day/Night Effect in Super-Kamiokande, M. B. Smy (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 138 (2005) 91, arXiv:hep-ex/0310064. TAUP 2003.
[Smy:2003sb]
[11-35]
Latest News from SNO, K. Graham (SNO), eConf C030626 (2003) THAT02, arXiv:hep-ex/0310039. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Graham:2003pu]
[11-36]
A study of short-time periodic variation of the B8 solar neutrino flux at Super-Kamiokande, J. Yoo (Super-Kamiokande), eConf C030626 (2003) FRAP01, arXiv:hep-ex/0309048. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Yoo:2003ky]
[11-37]
KamLAND results, K. Inoue (Kamland), arXiv:hep-ex/0307030, 2003. XXXVIIIth Recontres de Moriond Electroweak Interactions and Unified Theories.
[Inoue:2003qs]
[11-38]
The recent results of solar neutrino measurements in Super-Kamiokande, Y. Koshio (Super-Kamiokande), arXiv:hep-ex/0306002, 2003. XXXVIIIth Recontres de Moriond Electroweak Interactions and Unified Theories.
[Koshio:2003py]
[11-39]
The Gallium Neutrino Observatory (GNO), E. Bellotti (GNO), 2003. TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington. http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Parallel/People/Bellotti_E/GNO-Bellotti.pdf.
[Bellotti:TAUP03]
[11-40]
Results from SNO and Other Solar Neutrino Experiments, R. Robertson, 2003. TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington. http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Plenary/People/Robertson_H/SNO_and_Others-Robertson.pdf.
[Robertson:TAUP03]
[11-41]
KamLAND Results, K. Inoue (Kamland), 2003. The 4th Workshop on Neutrino Oscillations and their Origin (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Inoue-KamLAND.pdf.
[Inoue:NOON2003]
[11-42]
Solar Neutrino Observations at the Sudbury Neutrino Observatory, A. W. P. Poon (SNO), eConf C020805 (2002) TTH01, arXiv:hep-ex/0211013. SLAC Summer Institute Topical Conference (SSI02-TTh01), 2002.
[Poon:2002ae]
[11-43]
Solar Neutrinos, A. B. McDonald, eConf C020620 (2002) SAAT02, arXiv:hep-ex/0209056. Physics in Collision Conference, Stanford, California, June, 2002.
[McDonald:2002fx]
[11-44]
Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data, M. B. Smy (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 118 (2003) 25, arXiv:hep-ex/0208004. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/smy.
[Smy:2002rz]
[11-45]
Five Years of Neutrino Physics with Super-Kamiokande, M. B. Smy (Super-Kamiokande), arXiv:hep-ex/0206016, 2002. XXXVII Rencontres de Moriond: Electroweak Interactions and Unified Theories.
[Smy:2002hr]
[11-46]
An update on progress at KamLAND, S. A. Dazeley (KamLAND), arXiv:hep-ex/0205041, 2002.
[Dazeley:2002yf]
[11-47]
First Results from KamLAND: Evidence for $\bar{\nu}_e$ disappearance, G. Gratta (Kamland), 2002. SLAC Colloquium, December 2002. http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.
[Gratta:SLAC2002]
[11-48]
The Sudbury Neutrino Observatory, A. Hallin (SNO), 2002. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/hailin.
[Hallin-talk:2002a]
[11-49]
KamLAND: Examination of the LMA solution with reactor neutrinos, A. Suzuki (Kamland), 2002. XVI International Conference on Particles and Nuclei, Osaka, Japan, September 30 - October 4, 2002. http://www.rcnp.osaka-u.ac.jp/Divisions/np2/PaNic02/Suzuki.pdf.
[Suzuki-Panic02]

12 - Experiment - Slides

[12-1]
SNO : Low Energy Treshold Analysis (LETA), A. Orebi Gann, 2009. 5th International Workshop on Low energy neutrino physics, 19-21 October 2009, Reims, France. http://neutrino-champagne.in2p3.fr/Talks/LowNu_OrebiGann_noanim.pdf.
[Gann:LowNu09]

13 - Experiment - Neutrino Oscillations

[13-1]
Reactor On-Off Antineutrino Measurement with KamLAND, A. Gando et al. (KamLAND), Phys. Rev. D88 (2013) 033001, arXiv:1303.4667.
[Gando:2013nba]
[13-2]
Enhanced Constraints on $\theta_{13}$ from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND, A. Gando et al. (KamLAND), Phys. Rev. D83 (2011) 052002, arXiv:1009.4771.
[Gando:2010aa]
[13-3]
Precision Measurement of Neutrino Oscillation Parameters with KamLAND, S. Abe et al. (KamLAND), Phys. Rev. Lett. 100 (2008) 221803, arXiv:0801.4589.
From the abstract: Combining with solar neutrino data, we obtain $ \Delta m^{2}_{21} = 7.59^{+0.21}_{-0.21} \times 10^{-5} \, \text{eV}^{2} $ and $ \tan^2 \vartheta_{12} = 0.47^{+0.06}_{-0.05} $.
From the article: The spectrum indicates almost two cycles of the periodic feature expected from neutrino oscillation.
[Abe:2008aa]
[13-4]
Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion, T. Araki et al. (KamLAND), Phys. Rev. Lett. 94 (2005) 081801, arXiv:hep-ex/0406035.
[Araki:2004mb]
[13-5]
A High Sensitivity Search for $\bar{\nu}_{e}$'s from the Sun and Other Sources at KamLAND, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 92 (2004) 071301, arXiv:hep-ex/0310047.
From the abstract: Data corresponding to a KamLAND detector exposure of 0.28 kton-year has been used to search for $\bar{\nu}_e$'s in the energy range $ 8.3 \, \text{MeV} < E_{\bar{\nu}_e} < 14.8 \, \text{MeV}$. No candidates were found for an expected background of $1.1{\pm}0.4$ events. This result can be used to obtain a limit on $\bar{\nu}_{e}$ fluxes of any origin. Assuming that all $\bar{\nu}_e$ flux has its origin in the Sun and has the characteristic $^8\text{B}$ solar $\nu_e$ energy spectrum, we obtain an upper limit of $ 3.7 \times 10^2 \, \text{cm}^{-2} \, \text{s}^{-1} $ (90\% C.L.) on the $\bar{\nu}_e$ flux. We interpret this limit, corresponding to $2.8{\times}10^{-4}$ of the Standard Solar Model $^8\text{B}$ $\nu_e$ flux, in the framework of spin-flavor precession and neutrino decay models.
[Eguchi:2003gg]

14 - Experiment - Neutrino Oscillations - Conference Proceedings

[14-1]
Results from the KamLAND experiment, G. Gratta (KamLAND), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/gratta.pdf.
[Gratta-Nu2004]

15 - Experiment - Neutrino Oscillations - Slides

[15-1]
KamLAND (Anti-Neutrino Status), I. Shimizu (KamLAND), 2007. TAUP 2007, 11-15 September 2007, Sendai, Japan. http://www.awa.tohoku.ac.jp/taup2007/slides/workshop14/roomA/02-KamLAND-AntiNeutrino-Status-Shimizu.pdf.
[Shimizu-TAUP07]
[15-2]
Results from the KamLAND experiment, G. Gratta (KamLAND), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/gratta.pdf.
[Gratta-Nu2004]
[15-3]
KamLAND: updated results, K. Inoue (KamLAND), 2004. Neutrino Oscillation Workshop NOW 2004, September 11-17, 2004, Conca Specchiulla (Otranto, Italy). http://www.ba.infn.it/~now2004/talks/12_09_04/plen/KamLAND.pdf.
[Inoue:2004]
[15-4]
KamLAND Results, K. Inoue (KamLAND), 2003. The 4th Workshop on Neutrino Oscillations and their Origin (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Inoue-KamLAND.pdf.
[Inoue:NOON2003]
[15-5]
KamLAND: Examination of the LMA solution with reactor neutrinos, A. Suzuki (Kamland), 2002. XVI International Conference on Particles and Nuclei, Osaka, Japan, September 30 - October 4, 2002. http://www.rcnp.osaka-u.ac.jp/Divisions/np2/PaNic02/Suzuki.pdf.
[Suzuki-Panic02]
[15-6]
First Results from KamLAND: Evidence for $\bar{\nu}_e$ disappearance, G. Gratta (Kamland), 2002. SLAC Colloquium, December 2002. http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.
[Gratta:SLAC2002]

16 - Experiment - Astrophysical Cross Sections

[16-1]
LUNA: Nuclear Astrophysics Deep Underground, Carlo Broggini, Daniel Bemmerer, Alessandra Guglielmetti, Roberto Menegazzo, Ann. Rev. Nucl. Part. Sci. 60 (2010) 53-73, arXiv:1010.4165.
[Broggini:2010mu]
[16-2]
The 3He(alpha,gamma)7Be S-factor at solar energies: the prompt gamma experiment at LUNA, H. Costantini et al., Nucl. Phys. A814 (2008) 144-158, arXiv:0809.5269.
[Costantini:2008ub]
[16-3]
The 3He + 4He - > 7Be Astrophysical S-factor, T. A. D. Brown et al., Phys. Rev. C76 (2007) 055801, arXiv:0710.1279.
[Brown:2007sj]
[16-4]
3He(alpha,gamma)7Be cross section at low energies, Gy. Gyurky et al., Phys. Rev. C75 (2007) 035805, arXiv:nucl-ex/0702003.
[Gyurky:2007qq]
[16-5]
S-factor of 14N(p,gamma)15O at astrophysical energies, G. Imbriani et al. (LUNA), Eur. Phys. J. A25 (2005) 455, arXiv:nucl-ex/0509005.
[Imbriani:2005jz]
[16-6]
Astrophysical S-factor of 14N(p,g)15O, A. Formicola et al. (LUNA), Phys. Lett. B591 (2004) 61, arXiv:nucl-ex/0312015.
[Formicola:2003hp]
[16-7]
Precise measurement of the $^7\mathrm{Be}(p,gamma)^8\mathrm{B}$ S-factor, A. R. Junghans et al., Phys. Rev. C68 (2003) 065803, arXiv:nucl-ex/0308003.
[Junghans:2003bd]
[16-8]
Precise measurement of cross section of 3He(3He,2p)4He by using He-3 doubly charged beam, Nobuyuki Kudomi et al., Phys. Rev. C69 (2004) 015802, arXiv:astro-ph/0306454.
[Kudomi:2003xq]
[16-9]
The solar neutrino problem: Low energy measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ cross section, F. Hammache et al., Nucl. Phys. A688 (2001) 273-276.
[Hammache:2001ib]
[16-10]
Indirect measurements of the solar neutrino production reaction ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$, T. Motobayashi, Nucl. Phys. A693 (2001) 258-268.
[Motobayashi:2001qy]
[16-11]
Precision measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ reaction with radioactive beams and the $^8\mathrm{B}$ solar neutrino flux, Moshe Gai, Prog. Part. Nucl. Phys. 46 (2001) 89-96, arXiv:nucl-ex/0010014.
[Gai:2000yw]
[16-12]
First Measurement of the He3+He3- > He4+2p Cross Section down to the Lower Edge of the Solar Gamow Peak, R. Bonetti et al. (LUNA), Phys. Rev. Lett. 82 (1999) 5205-5208, arXiv:nucl-ex/9902004.
[Bonetti:1999yt]

17 - Experiment - Background

[17-1]
Study of the Production of Radioactive Isotopes through Cosmic Muon Spallation in KamLAND, S. Abe et al. (KamLAND), Phys. Rev. C81 (2010) 025807, arXiv:0907.0066.
[Abe:2009aa]

18 - Experiment - Astrophysics

[18-1]
Solar Neutron Events of October-November 2003, K. Watanabe et al., Astrophys. J. 636 (2006) 1135, arXiv:astro-ph/0509527.
[Watanabe:2005pd]

19 - Neutrino Flux

[19-1]
A new Generation of Standard Solar Models, Nuria Vinyoles et al., arXiv:1611.09867, 2016.
[1611.09867]
[19-2]
Solar models with new low-metal abundances, Wuming Yang, arXiv:1603.01666, 2016.
[1603.01666]
[19-3]
Generalised form factor dark matter in the Sun, Aaron C. Vincent, Aldo Serenelli, Pat Scott, JCAP 1508 (2015) 040, arXiv:1504.04378.
[Vincent:2015gqa]
[19-4]
Astrophysical implications of the proton-proton cross section updates, E. Tognelli, S. Degl'Innocenti, L. E. Marcucci, P.G. Prada Moroni, Phys.Lett. B742 (2015) 189-194, arXiv:1411.5480.
[Tognelli:2014axa]
[19-5]
The estimation of neutrino flux produced by $\mathbf{pep}$ reactions in the Sun, B.F. Irgaziev, V.B. Belyaev, Jameel-Un Nabi, Phys.Scripta 89 (2014) 084010, arXiv:1408.4532.
[Irgaziev:2014hfa]
[19-6]
The mixing in the solar core and the neutrino fluxes, Anatoly Kopylov, Valery Petukhov, arXiv:1209.3719, 2012.
[Kopylov:2012bc]
[19-7]
Solar models with accretion. I. Application to the solar abundance problem, Aldo M. Serenelli, Wick C. Haxton, Carlos Pena-Garay, Astrophys. J. 743 (2011) 24, arXiv:1104.1639.
Comment: SHP11.
[Serenelli:2011py]
[19-8]
Seismic and dynamical solar models i-the impact of the solar rotation history on neutrinos and seismic indicators, Sylvaine Turck-Chieze, Ana Palacios, Joao Marques, P. Nghiem, Astrophys. J. 715 (2010) 1539-1555, arXiv:1004.1657.
[TurckChieze:2010vk]
[19-9]
New Solar Composition: The Problem With Solar Models Revisited, Aldo Serenelli, Sarbani Basu, Jason W. Ferguson, Martin Asplund, Astrophys. J. 705 (2009) L123-L127, arXiv:0909.2668.
[Serenelli:2009yc]
[19-10]
Solar neutrinos and the solar composition problem, Carlos Pena-Garay, Aldo Serenelli, arXiv:0811.2424, 2008.
[PenaGaray:2008qe]
[19-11]
10,000 Standard Solar Models: a Monte Carlo Simulation, John N. Bahcall, Aldo M. Serenelli, Sarbani Basu, Astrophys. J. Supp. Ser. 165 (2006) 400-431, arXiv:astro-ph/0511337.
[Bahcall:2005va]
[19-12]
What Is The Neon Abundance Of The Sun?, John N. Bahcall, Sarbani Basu, Aldo M. Serenelli, Astrophys. J. 631 (2005) 1281, arXiv:astro-ph/0502563.
From the abstract: We have evolved a series of thirteen complete solar models that utilize different assumed heavy element compositions.... The predicted solar neutrino fluxes are affected by the uncertainties in the composition by less than their $1\sigma$ theoretical uncertainties.
[Bahcall:2005dd]
[19-13]
New solar opacities, abundances, helioseismology, and neutrino fluxes, John N. Bahcall, Aldo M. Serenelli, Sarbani Basu, Astrophys. J. 621 (2005) L85-L88, arXiv:astro-ph/0412440.
From the abstract: We construct solar models with the newly calculated radiative opacities from the Opacity Project (OP) and recently determined (lower) heavy element abundances.... For all the variations we consider, solar models that are constructed with the newer and lower heavy element abundances advocated by Asplund and others (2005) disagree by much more than the estimated measuring errors with helioseismological determinations of the depth of the solar convective zone, the surface helium composition, the internal sound speeds, and the density profile. Using the new OP radiative opacities, the ratio of the $^8$B neutrino flux calculated with the older and larger heavy element abundances (or with the newer and lower heavy element abundances) to the total neutrino flux measured by the Sudbury Neutrino Observatory is 1.09 (0.87) with a 9\% experimental uncertainty and a 16\% theoretical uncertainty, $1\sigma$ errors.
Comment: BS05.
[Bahcall:2004pz]
[19-14]
How do Uncertainties in the Surface Chemical Abundances of the Sun Affect the Predicted Solar Neutrino Fluxes?, John N. Bahcall, Aldo M. Serenelli, Astrophys. J. 626 (2005) 530, arXiv:astro-ph/0412096.
[Bahcall:2004mq]
[19-15]
Surprising Sun, S. Turck-Chieze et al., Phys. Rev. Lett. 93 (2004) 211102, arXiv:astro-ph/0407176.
[TurckChieze:2004mg]
[19-16]
What do we (not) know theoretically about solar neutrino fluxes?, John N. Bahcall, M. H. Pinsonneault, Phys. Rev. Lett. 92 (2004) 121301, arXiv:astro-ph/0402114.
From the abstract: Solar model predictions of ${}^8\mathrm{B}$ and $pp$ neutrinos agree with the experimentally-determined fluxes (including oscillations): $\phi(pp)_{\text{measured}} = \left(1.02 \pm 0.02 \pm 0.01\right) \phi(pp)_{\text{theory}}$, and $\phi({}^8\mathrm{B})_{\text{measured}} = \left(0.88 \pm 0.04 \pm 0.23\right) \phi({}^8\mathrm{B})_{\text{theory}}$, $ 1 \sigma $ experimental and theoretical uncertainties, respectively.
From the article: The 15\% increase in the calculated ${}^8\mathrm{B}$ neutrino flux is the only significant change in the best-estimate fluxes.
Comment: BP04.
[Bahcall:2004fg]
[19-17]
Solar seismic models and the neutrino predictions, S. Couvidat, Sylvaine Turck-Chieze, A.G. Kosovichev, Astrophys.J. 599 (2003) 1434-1448.
[Couvidat:2003ba]
[19-18]
Our Sun. IV. The Standard Model and Helioseismology: Consequences of Uncertainties in Input Physics and in Observed Solar Parameters, Arnold I. Boothroyd, I.-Juliana Sackmann, Astrophys. J. 583 (2003) 1004, arXiv:astro-ph/0210127.
[Boothroyd:2002qw]
[19-19]
Solar models: Current epoch and time dependences, neutrinos, and helioseismological properties, J. N. Bahcall, M. H. Pinsonneault, S. Basu, Astrophys. J. 555 (2001) 990-1012, arXiv:astro-ph/0010346.
Comment: BP00.
[Bahcall:2000nu]
[19-20]
How uncertain are solar neutrino predictions?, J. N. Bahcall, S. Basu, M. H. Pinsonneault, Phys. Lett. B433 (1998) 1-8, arXiv:astro-ph/9805135.
Comment: BP98.
[Bahcall:1998wm]
[19-21]
Gallium solar neutrino experiments: Absorption cross sections, neutrino spectra, and predicted event rates, John N. Bahcall, Phys. Rev. C56 (1997) 3391, arXiv:hep-ph/9710491.
[Bahcall:1997eg]
[19-22]
Are standard solar models reliable?, J. N. Bahcall, M. H. Pinsonneault, S. Basu, J. Christensen-Dalsgaard, Phys. Rev. Lett. 78 (1997) 171-174, arXiv:astro-ph/9610250.
[Bahcall:1996qw]
[19-23]
Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes, N. Itoh, H. Hayashi, A. Nishikawa, Y. Kohyama, Astrophysical Journal Supplement 102 (1996) 411-424.
[1996ApJS..102..411I]
[19-24]
Solar models with helium and heavy element diffusion, J. N. Bahcall, M. H. Pinsonneault, Rev. Mod. Phys. 67 (1995) 781-808, arXiv:hep-ph/9505425.
Comment: BP95.
[Bahcall:1995bt]
[19-25]
The Be-7 solar neutrino line: A Reflection of the central temperature distribution of the sun, J. N. Bahcall, Phys. Rev. D49 (1994) 3923-3945.
[Bahcall:1994cf]
[19-26]
Toward a unified classical model of the sun: On the sensitivity of neutrinos and helioseismology to the microscopic physics, S. Turck-Chieze, I. Lopes, Astrophys. J. 408 (1993) 347-367.
[Turck-Chieze:1993dw]
[19-27]
Standard solar models, with and without helium diffusion and the solar neutrino problem, J. N. Bahcall, M. H. Pinsonneault, Rev. Mod. Phys. 64 (1992) 885-926.
Comment: BP92.
[Bahcall:1992hn]
[19-28]
Solar models, neutrino experiments and helioseismology, J. N. Bahcall, Roger K. Ulrich, Rev. Mod. Phys. 60 (1988) 297-372.
Comment: BU88.
[Bahcall:1988jc]
[19-29]
Standard solar models and the uncertainties in predicted capture rates of solar neutrinos, J. N. Bahcall, Walter F. Huebner, Stephen H. Lubow, Peter D. Parker, Roger K. Ulrich, Rev. Mod. Phys. 54 (1982) 767.
[Bahcall:1982zh]
[19-30]
Present status of the theoretical predictions for the Cl-36 solar neutrino experiment, John N. Bahcall, Neta A. Bahcall, G. Shaviv, Phys. Rev. Lett. 20 (1968) 1209-1212.
[Bahcall:1968hc]
[19-31]
Solar neutrinos. I: Theoretical, J. N. Bahcall, Phys. Rev. Lett. 12 (1964) 300-302.
[Bahcall:1964gx]
[19-32]
J. N. Bahcall, W. A. Fowler, I. Iben, R. L. Sears, Astrophys. J. 137 (1963) 344.
[Bahcall-63]
[19-33]
Nuclear Reactions in Stars and Nucleogenesis, A. G. W. Cameron, Pub. Astron. Soc. Pac. 69 (1957) 201.
[Cameron-PASP-69-201-1957]
[19-34]
E. M. Burbidge, G. R Burbidge, W. A. Fowler, F. Hoyle, Rev. Mod. Phys. 29 (1957) 547.
[Burbidge-Burbidge-Fowler-Hoyle-RMP-29-547-1957]
[19-35]
Energy Production in Stars, H. A. Bethe, Phys. Rev. 55 (1939) 434-456.
[Bethe-PR-55-434-1939]

20 - Neutrino Flux - Conference Proceedings

[20-1]
New Results on Standard Solar Models, Aldo M. Serenelli, Astrophys. Space Sci. 328 (2010) 13-21, arXiv:0910.3690. Synergies between solar and stellar modelling, Rome, June 2009.
[Serenelli:2009ww]
[20-2]
Progress report on solar age calibration, G. Houdek, D.O. Gough, Phys. Rev. A78 (2008) 062104, arXiv:0807.3443. The Art of Modelling Stars in the 21st Century, Proc. IAU Symp. No. 252.
[Houdek:2008rw]
[20-3]
Solar Models and Solar Neutrinos, John N. Bahcall, eConf C030626 (2003) THAT04, arXiv:astro-ph/0310030. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Bahcall:2003jg]

21 - Astrophysics

[21-1]
The effect of ionic correlations on radiative properties in the solar interior and terrestrial experiments, Menahem Krief, Yair Kurzweil, Alexander Feigel, Doron Gazit, arXiv:1611.09339, 2016.
[Krief:2016vyp]
[21-2]
Magnetic helicity estimations in models and observations of the solar magnetic field. Part I: Finite volume methods, Gherardo Valori et al., arXiv:1610.02193, 2016.
[1610.02193]
[21-3]
Bayesian Estimation of Thermonuclear Reaction Rates, Christian Iliadis, Kevin Anderson, Alain Coc, Frank Timmes, Sumner Starrfield, Astrophys.J. 831 (2016) 107, arXiv:1608.05853.
[Iliadis:2016vkw]
[21-4]
Reconstruction of Solar Subsurfaces by Local Helioseismology, Alexander G. Kosovichev, Junwei Zhao, arXiv:1607.05681, 2016.
[1607.05681]
[21-5]
Model description of non-Maxwellian nuclear processes in the solar interior, Victor T. Voronchev, Yasuyuki Nakao, Yukinobu Watanabe, arXiv:1606.00612, 2016.
[1606.00612]
[21-6]
Implications of solar wind measurements for solar models and composition, Aldo Serenelli et al., Mon.Not.Roy.Astron.Soc. 463 (2016) 2-9, arXiv:1604.05318.
[Serenelli:2016nms]
[21-7]
A successful solar model using new solar composition data, Sunny Vagnozzi, Katherine Freese, Thomas H. Zurbuchen, arXiv:1603.05960, 2016.
[Vagnozzi:2016cmr]
[21-8]
Line broadening and the solar opacity problem, M. Krief, A. Feigel, D. Gazit, arXiv:1603.01153, 2016.
[1603.01153]
[21-9]
Sunspot Numbers from ISOON: A Ten-Year Data Analysis, K. S. Balasubramaniam, T. W. Henry, arXiv:1602.07741, 2016.
[1602.07741]
[21-10]
Chameleon fields and solar physics, Andrea Zanzi, Barbara Ricci, Mod.Phys.Lett. A30 (2015) 1550053, arXiv:1405.1581.
[Zanzi:2014aia]
[21-11]
The chemical composition of the Sun from helioseismic and solar neutrino data, F.L. Villante, A.M. Serenelli, F. Delahaye, M.H. Pinsonneault, Astrophys.J. 787 (2014) 13, arXiv:1312.3885.
[Villante:2013mba]
[21-12]
Planetary influence on the young Sun's evolution: the solar neutrino probe, Ilidio Lopes, Joseph Silk, Mon.Not.Roy.Astron.Soc. 435 (2013) 2109-2115, arXiv:1309.7571.
[Lopes:2013iia]
[21-13]
What have we learned from helioseismology, what have we really learned, and what do we aspire to learn?, Douglas Gough, Solar Phys. 287 (2013) 9, arXiv:1210.0820.
[Gough:2012tb]
[21-14]
Analytical results connecting stellar structure parameters and extended reaction rates, H.J. Haubold, D. Kumar, J.Astrophys. 2014 (2014) 656784, arXiv:1109.5613.
[Haubold:2011kk]
[21-15]
The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos, Sylvaine Turck-Chieze, Laurent Piau, Sebastien Couvidat, Astrophys.J. 731 (2011) L29, arXiv:1103.2620.
[TurckChieze:2011tm]
[21-16]
Radioactivities in Low- and Intermediate-Mass Stars, Maria Lugaro, Alessandro Chieffi, Lect.Notes Phys. 218 (2011) 83-152, arXiv:1010.1304.
[Lugaro:2010ia]
[21-17]
The Extreme Energies Lines in the Solar Neutrino Spectrum, B.I. Goryachev, arXiv:1005.3458, 2010.
[Goryachev:2010am]
[21-18]
Fresh insights on the structure of the solar core, Sarbani Basu, William J. Chaplim, Yvonne Elsworth, Roger New, Aldo M. Serenelli, Astrophys. J. 699 (2009) 1403-1417, arXiv:0905.0651.
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[21-19]
Variations of the solar granulation motions with height using the GOLF/SoHO experiment, S. Lefebvre, R.A. Garcia, S.J. Jimenez-Reyes, S. Turck-Chieze, S. Mathur, Astron.Astrophys. 490 (2008) 1143, arXiv:0808.0422.
[Lefebvre:2008am]
[21-20]
Bayesian Analysis of Solar Oscillations, M. S. Marsh, J. Ireland, T. Kucera, Astrophys. J. 681 (2008) 672-679, arXiv:0804.1447.
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[21-21]
New Evidence for the Solar Oxygen Crisis from Spectro-Polarimetric Observations, H. Socas-Navarro, R. Centeno, Astrophys.J. 682 (2008) L61, arXiv:0803.0990.
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[21-22]
Update on g-mode research, R.A. Garcia et al., Astron. Nachr. 329 (2008) 476-484, arXiv:0802.4296.
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[21-23]
Are solar cycles predictable?, Manfred Schuessler, Astron.Nachr. 328 (2007) 1087-1091, arXiv:0712.1917.
[Schuessler:2007rq]
[21-24]
The energy of high frequency waves in the low solar Chromosphere, Aleksandra Andic, Solar Phys. 242 (2007) 1-2, arXiv:astro-ph/0703721.
[Andic:2007wy]
[21-25]
Modeling the (upper) solar atmosphere including the magnetic field, H. Peter, Adv. Space Res. 39 (2007) 1814-1825, arXiv:astro-ph/0703575.
[Peter:2007yx]
[21-26]
The solar oxygen crisis: Probably not the last word, H. Socas-Navarro, A. A. Norton, Astrophys.J.Lett. (2007), arXiv:astro-ph/0702162.
[SocasNorton:2007th]
[21-27]
Probing the internal solar magnetic field through g-modes, Timur I. Rashba, V. B. Semikoz, S. Turck-Chieze, J. W. F. Valle, Mon. Not. Roy. Astron. Soc. 377 (2007) 453, arXiv:astro-ph/0611728.
[Rashba:2006jp]
[21-28]
Low abundances of heavy elements in the solar outer layers: comparisons of solar models with helioseismic inversions, M. Castro, S. Vauclair, O. Richard, Astron.Astrophys. 463 (2007) 755-758, arXiv:astro-ph/0611619.
[Castro:2006qu]
[21-29]
Solar Atmospheric Oscillations and the Chromospheric Magnetic Topology, A. Vecchio et al., Astron. Astrophys. 461 (2007) L1-L4, arXiv:astro-ph/0611206.
[Vecchio:2006yi]
[21-30]
Origin of solar torsional oscillations, Matthias Rempel, Astrophys. J. 655 (2007) 651-659, arXiv:astro-ph/0610221.
[Rempel:2006zu]
[21-31]
Solar abundances and helioseismology: fine structure spacings and separation ratios of low-degree p modes, Sarbani Basu et al., Astrophys. J. 655 (2007) 660-671, arXiv:astro-ph/0610052. To appear in ApJ.
[Basu:2006vh]
[21-32]
Local helioseismology and correlation tracking analysis of surface structures in realistic simulations of solar convection, Dali Georgobiani et al., Astrophys. J. 657 (2007) 1157-1161, arXiv:astro-ph/0608204.
[Georgobiani:2006ty]
[21-33]
Damping and excitation variations of the solar acoustic modes using LOWL observations, D. Salabert, S.J. Jiménez-Reyes, Astrophys. J. 650 (2006) 451-460, arXiv:astro-ph/0607346.
[Salabert:2006td]
[21-34]
A Comparative Study on Lithium Abundances in Solar-Type Stars With and Without Planets, Y. Q. Chen, G. Zhao, Astron. J. 131 (2006) 1816, arXiv:astro-ph/0607295.
[Chen:2006fr]
[21-35]
Neon Abundances in B-Stars of the Orion Association: Solving the Solar Model Problem?, Katia Cunha, Ivan Hubeny, Thierry Lanz, Astrophys. J. 647 (2006) L143-L146, arXiv:astro-ph/0606738.
[Cunha:2006jf]
[21-36]
Long-term Variability in the Length of the Solar Cycle, Michael L. Rogers, Mercedes T. Richards, Donald St.P. Richards, arXiv:astro-ph/0606426, 2006.
[Rogers:2006bg]
[21-37]
Can Galactic Cosmic Rays Account for Solar 6Li Without Overproducing Gamma Rays?, T. Prodanovic, B. D. Fields, Astrophys. J. 645 (2006) L125-L128, arXiv:astro-ph/0605675.
[Prodanovic:2006fm]
[21-38]
The Sun's Interior Metallicity Constrained by Neutrinos, Guillermo Gonzalez, Mon. Not. Roy. Astron. Soc. Lett. 370 (2006) L90, arXiv:astro-ph/0605647.
[Gonzalez:2006zd]
[21-39]
Determining solar abundances using helioseismology, H.M. Antia, Sarbani Basu, Astrophys. J. 644 (2006) 1292-1298, arXiv:astro-ph/0603001.
[Antia:2006zy]
[21-40]
Total Solar Irradiance Variability and the Solar Activity Cycle, Probhas Raychaudhuri, arXiv:astro-ph/0601335, 2006.
[Raychaudhuri:2006zc]
[21-41]
The Solar Heavy Element Abundances: I. Constraints from Stellar Interiors, Franck Delahaye, Marc Pinsonneault, Astrophys. J. 649 (2006) 529-540, arXiv:astro-ph/0511779.
[Delahaye:2005ed]
[21-42]
Angular Momentum Transport by Gravity Waves in the Solar Interior, Tamara M. Rogers, Gary A. Glatzmaier, Astrophys. J. 653 (2006) 756-764, arXiv:astro-ph/0511739.
[Rogers:2005yz]
[21-43]
Radiative zone solar magnetic fields and g-modes, Timur I. Rashba, V. B. Semikoz, J. W. F. Valle, Mon. Not. Roy. Astron. Soc. 370 (2006) 845, arXiv:astro-ph/0511708.
[Rashba:2005uj]
[21-44]
7Be(p,gamma)8B S-factor from ab initio wave functions, P. Navratil, C.A. Bertulani, E. Caurier, Phys. Lett. B634 (2006) 191, arXiv:nucl-th/0511029.
[Navratil:2005xm]
[21-45]
The solar model problem resurrected, M. Asplund, N. Grevesse, M. Guedel, A.J. Sauval, Nature 436 (2005) 525, arXiv:astro-ph/0510377.
[Asplund:2005js]
[21-46]
The Ne/O abundance ratio in the quiet Sun, P.R. Young, Astron.Astrophys. (2005), arXiv:astro-ph/0510264.
[Young:2005ke]
[21-47]
Neon Lights Up a Controversy: the Solar Ne/O Abundance, J.T. Schmelz et al., Astrophys. J. 634 (2005) L197, arXiv:astro-ph/0510230.
[Schmelz:2005cm]
[21-48]
Seismic analysis of the second ionization region of helium in the Sun: I. Sensitivity study and methodology, M.J.P.F.G. Monteiro, M.J. Thompson, Mon. Not. Roy. Astron. Soc. 361 (2005) 1187, arXiv:astro-ph/0506286.
[Monteiro:2005cb]
[21-49]
The Solar Model Problem Solved by the Abundance of Neon in Stars of the Local Cosmos, Jeremy J. Drake Paola Testa, Paola Testa, Nature 436 (2005) 525, arXiv:astro-ph/0506182.
[Drake:2005hn]
[21-50]
Can Enhanced Diffusion Improve Helioseismic Agreement for Solar Models with Revised Abundances?, J. Guzik, L. S. Watson, A. Cox, Astrophys. J. 627 (2005) 1049, arXiv:astro-ph/0502364.
[Guzik:2005db]
[21-51]
The discrepancy between solar abundances and helioseismology, H. M. Antia, Sarbani Basu, Astrophys. J. 620 (2005) L129, arXiv:astro-ph/0501129.
[Antia:2005mg]
[21-52]
Does solar structure vary with solar magnetic activity?, Sarbani Basu, Anna Mandel, Astrophys. J. 617 (2004) L155, arXiv:astro-ph/0411427.
[Basu:2004kq]
[21-53]
Helioseismological Implications of Recent Solar Abundance Determinations, John N. Bahcall, Sarbani Basu, Marc Pinsonneault, Aldo M. Serenelli, Astrophys. J. 618 (2005) 1049, arXiv:astro-ph/0407060.
[Bahcall:2004yr]
[21-54]
Determination of S17(0) from published data, R. H. Cyburt, B. Davids, B. K. Jennings, Phys. Rev. C70 (2004) 045801, arXiv:nucl-th/0406011.
[Cyburt:2004jp]
[21-55]
How Accurately Can We Calculate the Depth of the Solar Convective Zone?, John N. Bahcall, Aldo M. Serenelli, Marc Pinsonneault, Astrophys. J. 614 (2004) 464, arXiv:astro-ph/0403604.
[Bahcall:2004aq]
[21-56]
The $^{14}\mathrm{N}(p, \gamma)^{15}\mathrm{O}$ reaction, solar neutrinos and the age of the globular clusters, S. Degl'Innocenti, G. Fiorentini, B. Ricci, F.L. Villante, Phys. Lett. B590 (2004) 13, arXiv:astro-ph/0312559.
[DeglInnocenti:2003yia]
[21-57]
How Accurately Do We Know the Formation of Solar 8B?, Moshe Gai, arXiv:nucl-ex/0312003, 2003.
[Gai:2003ef]
[21-58]
On Solar Radius Variation with Magnetic Field, A. R. Choudhuri, P. Chatterjee, arXiv:astro-ph/0311028, 2003.
[Choudhuri:2003we]
[21-59]
A Millennium Scale Sunspot Number Reconstruction: Evidence For an Unusually Active Sun Since the 1940's, I. G. Usoskin et al., Phys. Rev. Lett. 91 (2003) 211101, arXiv:astro-ph/0310823.
[Usoskin:2003au]
[21-60]
Helioseismic Probing of Solar Variability: The Formalism and Simple Assessments, W.A. Dziembowski, P.R. Goode, Astrophys. J. 600 (2004) 464, arXiv:astro-ph/0310095.
[Dziembowski:2003vb]
[21-61]
Towards a Solution to the Early Faint Sun Paradox: A Lower Cosmic Ray Flux from a Stronger Solar Wind, N. J. Shaviv, J.Geophys.Res. A108 (2003) 1437, arXiv:astro-ph/0306477.
[Shaviv:2003hq]
[21-62]
Precise measurement of cross section of 3He(3He,2p)4He by using He-3 doubly charged beam, Nobuyuki Kudomi et al., Phys. Rev. C69 (2004) 015802, arXiv:astro-ph/0306454.
[Kudomi:2003xq]
[21-63]
Resonant origin for density fluctuations deep within the Sun: helioseismology and magneto-gravity waves, C. P. Burgess et al., Mon. Not. Roy. Astron. Soc. 348 (2004) 609, arXiv:astro-ph/0304462.
[Burgess:2003fj]
[21-64]
Bounds on the Magnetic Fields in the Radiative Zone of the Sun, Alexander Friedland, Andrei Gruzinov, Astrophys. J. 601 (2004) 570, arXiv:astro-ph/0211377.
[Friedland:2002is]
[21-65]
Possible in situ Tests of the Evolution of Elemental and Isotopic Abundances in the Solar Convection Zone, S. Turcotte, R. F. Wimmer-Schweingruber, J.Geophys.Res. A107 (2002) 1442, arXiv:astro-ph/0210219.
[Turcotte:2002wz]
[21-66]
Our Sun. V. A Bright Young Sun Consistent with Helioseismology and Warm Temperatures on Ancient Earth and Mars, I.-J. Sackmann, A. I. Boothroyd, Astrophys. J. 583 (2003) 1024, arXiv:astro-ph/0210128.
[Sackmann:2002qx]
[21-67]
Screened thermonuclear reactions in astrophysical plasmas: Improving Salpeter's and Mitler's models, Theodore E. Liolios, Eur. Phys. J. A18 (2003) S1-S25, arXiv:nucl-th/0210031.
[Liolios:2002zv]
[21-68]
The State Be7 in the Core of the Sun and the Solar Neutrino Flux, G. Shaviv N. J. Shaviv, Mon. Not. Roy. Astron. Soc. 341 (2003) 119, arXiv:astro-ph/0209253.
[Shaviv:2002kn]
[21-69]
Constraints on proton-proton fusion from helioseismology, D.B. Guenther K.I.T. Brown, M.N. Butler, arXiv:nucl-th/0207008, 2002.
[Brown:2002ih]
[21-70]
Seismic test of solar models, solar neutrinos and implications for metal-rich accretion, R. A. Winnick, Pierre Demarque, Sarbani Basu, D. B. Guenther, Astrophys. J. 576 (2002) 1075, arXiv:astro-ph/0111096.
[Winnick:2001uc]
[21-71]
A possible solution to the solar neutrino problem: Relativistic corrections to the Maxwellian velocity distribution, Jian-Miin Liu, arXiv:physics/0110002, 2001.
[Liu:2001qh]
[21-72]
Velocity distribution of high-energy particles and the solar neutrino problem, Jian-Miin Liu, arXiv:astro-ph/0108304, 2001.
[Liu:2001rm]
[21-73]
The luminosity constraint on solar neutrino fluxes, J. N. Bahcall, Phys. Rev. C65 (2002) 025801, arXiv:hep-ph/0108148.
[Bahcall:2001pf]
[21-74]
Solar models with helioseismic constraints and the solar neutrino problem, Satoru Watanabe, Hiromoto Shibahashi, Publ. Astron. Soc. Jap. 53 (2001) 565-575, arXiv:astro-ph/0105445.
[Watanabe:2000tx]
[21-75]
The solar neutrino problem: Low energy measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ cross section, F. Hammache et al., Nucl. Phys. A688 (2001) 273-276.
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[21-76]
Indirect measurements of the solar neutrino production reaction ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$, T. Motobayashi, Nucl. Phys. A693 (2001) 258-268.
[Motobayashi:2001qy]
[21-77]
Precision measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ reaction with radioactive beams and the $^8\mathrm{B}$ solar neutrino flux, Moshe Gai, Prog. Part. Nucl. Phys. 46 (2001) 89-96, arXiv:nucl-ex/0010014.
[Gai:2000yw]
[21-78]
The $hep$ reaction and the solar neutrino problem, L. E. Marcucci, Nucl. Phys. A689 (2001) 280-289, arXiv:nucl-th/0009066.
[Marcucci:2000bg]
[21-79]
Is it possible to determine the S-factor of the HEP process from a laboratory experiment?, W. M. Alberico, J. Bernabeu, Samoil M. Bilenky, W. Grimus, Phys. Lett. B478 (2000) 208-214, arXiv:hep-ph/0002029.
[Alberico:2000qe]
[21-80]
On a possibility to determine the S-factor of the hep process in experiments with thermal (cold) neutrons, W. M. Alberico, Samoil M. Bilenky, W. Grimus, Astropart. Phys. 15 (2001) 211-215, arXiv:hep-ph/0001245.
[Alberico:2000sx]
[21-81]
Neutrinos and solar models, W. A. Dziembowski, Acta Phys. Polon. B31 (2000) 1389-1401.
[Dziembowski:2000sa]
[21-82]
First Measurement of the He3+He3- > He4+2p Cross Section down to the Lower Edge of the Solar Gamow Peak, R. Bonetti et al. (LUNA), Phys. Rev. Lett. 82 (1999) 5205-5208, arXiv:nucl-ex/9902004.
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[21-83]
Effects of solar magnetosonic waves in new solar neutrino observations, J. H. Colonia, M. M. Guzzo, N. Reggiani, Astropart. Phys. 8 (1997) 51-57.
[Colonia:1997ft]

22 - Astrophysics - Conference Proceedings

[22-1]
Relativistic implications of solar astrometry, Costantino Sigismondi, Int. J. Mod. Phys. Conf. Ser. 03 (2011) 464-474, arXiv:1106.2202. Friedmann Seminar, CBPF Rio de Janeiro, Brasil, 30 May - 3 June 2011.
[Sigismondi:2011fr]
[22-2]
CN-Cycle Neutrinos and Solar Metalicity, W. C. Haxton, A. M. Serenelli, arXiv:0902.0036, 2009. PANIC08, Eilat, Israel.
[Haxton:2009jh]
[22-3]
Measuring Solar Abundances with Seismology, Katie Mussack, Douglas Gough, ASP Conf.Ser. 416 (2009) 203, arXiv:0810.2722. GONG 2008/SOHO XXI.
[Mussack:2008pp]
[22-4]
Low-Energy Nuclear Astrophysics - the Fascinating Region of A=7, Michael Hass, Prog.Part.Nucl. Phys. 59 (2007) 131, arXiv:nucl-ex/0611039. Erice School on Nuclear Physics, 2006.
[Hass:2006zv]
[22-5]
Prospects for helio- and asteroseismology, J. Christensen-Dalsgaard, ESA Spec.Publ. 624 (2006) 41, arXiv:astro-ph/0610614. SOHO 18 / GONG 2006 / HELAS I Conference: Beyond the spherical Sun.
[ChristensenDalsgaard:2006sp]
[22-6]
Solar Mean Magnetic Field Near the Surface and its Variation During a Cycle, P.A.P. Nghiem, R.A. Garcia, S.J. Jimenez-Reyes, ESA Spec.Publ. 624 (2006) 70, arXiv:astro-ph/0608109. SOHO 18 / GONG 2006 / HELAS I.
[Nghiem:2006wp]
[22-7]
Solar Gravity Modes: Present and Future, Sylvaine Turck-Chieze, Adv.Space Res. 37 (2006) 1569, arXiv:astro-ph/0511126. COSPAR 2004.
[TurckChieze:2005im]
[22-8]
Do We Accurately Know the Formation of Solar 8B?, Moshe Gai, Nucl. Phys. Proc. Suppl. 143 (2005) 495, arXiv:nucl-ex/0410031. Neutrino 04, Paris, June 14-19, 2004.
[Gai:2004gt]
[22-9]
(Two) Open Questions in Stellar Nuclear Physics, Moshe Gai, AIP Conf.Proc. 726 (2004) 109, arXiv:astro-ph/0405100. StuFiesta, Cocoyoc, Mexico, April 19-22, 2004.
[Gai:2004xi]
[22-10]
How helioseismology constrains solar neutrinos, S. Turck-Chieze, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/turck-chieze.pdf.
[Turck-Chieze-Nu2004]
[22-11]
Nuclear reactions in the Sun after SNO and KamLAND, G. Fiorentini, B. Ricci, arXiv:astro-ph/0310753, 2003. Beyond the Desert '03, Fourth International Conference on Physics Beyond the Standard Model, Schloss Ringberg, Germany, June 9-14, 2003.
[Fiorentini:2003vj]
[22-12]
New precision 7Be(p,g)8B cross section measurements and the astrophysical factor S_17, A.R. Junghans, 2003. TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington. http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Parallel/People/Junghans_A/S17-Junghans.pdf.
[Junghans:TAUP03]

23 - Astrophysical Cross Sections

[23-1]
Halo effective field theory constrains the solar Beryllium-7 + proton - > Boron-8 + photon rate, Xilin Zhang, Kenneth M. Nollett, D. R. Phillips, Phys. Lett. B751 (2015) 535-540, arXiv:1507.07239.
[Zhang:2015ajn]
[23-2]
Ab initio many-body calculation of the 7Be(p,gamma)8B radiative capture, Petr Navratil, Robert Roth, Sofia Quaglioni, Phys. Lett. B704 (2011) 379-383, arXiv:1105.5977.
[Navratil:2011sa]
[23-3]
The 14C(n,g) cross section between 10 keV and 1 MeV, R. Reifarth et al., Phys. Rev. C77 (2008) 015804, arXiv:0910.0106.
[Reifarth:2008zz]
[23-4]
Determination of the $ {}^3\text{He} + \alpha \to {}^7\text{Be} $ asymp. normalization coefficients (nucl. vertex constants) and their application for extrapolation of the $ {}^3\text{He} (\alpha,\gamma) {}^7\text{Be} $ astroph. S-factors to the solar energy region, S. B. Igamov, K. I. Tursunmakhatov, R. Yarmukhamedov, Phys. Rev. C85 (2012) 045807, arXiv:0905.2026.
[Igamov:2009eh]
[23-5]
Isospin Effects on Astrophysical S-Factors, Sachie Kimura, Aldo Bonasera, Phys. Rev. C76 (2007) 031602, arXiv:0706.3864.
[Kimura:2007rv]
[23-6]
Astrophysical S-factor of the 3He(alpha,gamma)7Be reaction measured at low energy via prompt and delayed gamma detection, F. Confortola et al. (LUNA), Phys. Rev. C75 (2007) 065803, arXiv:0705.2151.
[Confortola:2007nq]
[23-7]
Study of the 12C+12C fusion reactions near the Gamow energy, T.Spillane et al., Phys. Rev. Lett. 98 (2007) 122501, arXiv:nucl-ex/0702023.
[Spillane:2007xc]
[23-8]
Activation measurement of the 3He(alpha,gamma)7Be cross section at low energy, D. Bemmerer et al., Phys. Rev. Lett. 97 (2006) 122502, arXiv:nucl-ex/0609013.
[Bemmerer:2006xa]
[23-9]
Influence of protons on the capture of electrons by the nuclei of 7Be in the Sun, V. B. Belyaev, M. Tater, E. Truhlik, Phys. Rev. C75 (2007) 034608, arXiv:astro-ph/0606679.
[Belyaev:2006qt]
[23-10]
${}^{7}\text{Be}(p,gamma){}^{8}\text{B}$ S-factor from ab initio no-core shell model wave functions, P. Navratil, C.A. Bertulani, E. Caurier, Phys. Rev. C73 (2006) 065801, arXiv:nucl-th/0601019.
[Navratil:2006tt]
[23-11]
Scattering of $^{7}\text{Be}$ and $^{8}\text{B}$ and the astrophysical $S_{17}$ factor, G. Tabacaru et al., Phys. Rev. C73 (2006) 025808, arXiv:nucl-ex/0508029.
[Tabacaru:2005hv]
[23-12]
Is There a Significant Difference Between the Results of the Coulomb Dissociation of 8B and the Direct Capture 7Be(p,g)8B Reaction?, Moshe Gai, Phys. Rev. C74 (2005) 025810, arXiv:nucl-ex/0502020.
[Gai:2005bn]
[23-13]
Astrophysical $S_{17}(0)$ factor from a measurement of $d({}^{7}\text{Be},{}^{8}\text{B})n$ reaction at $E_{c.m.} = 4.5 MeV$, J.J. Das et al., arXiv:nucl-ex/0409017, 2004.
[Das:2004dx]
[23-14]
The ${}^{8}\text{B}$ neutrino spectrum, W. T. Winter, S. J. Freedman, K. E. Rehm, J. P. Schiffer, Phys. Rev. C73 (2006) 025503, arXiv:nucl-ex/0406019.
[Winter:2004kf]
[23-15]
Determination of $S_{17}(0)$ from published data, R. H. Cyburt, B. Davids, B. K. Jennings, Phys. Rev. C70 (2004) 045801, arXiv:nucl-th/0406011.
[Cyburt:2004jp]
[23-16]
Electromagnetic dissociation of ${}^{8}\text{B}$ and the astrophysical $S$ factor for ${}^{7}\text{Be}(p,gamma){}^{8}\text{B}$, B. Davids, S. Typel, Phys. Rev. C68 (2003) 045802, arXiv:nucl-th/0304054.
From the abstract: ... we take a weighted average of the results of four direct and three indirect measurements to obtain a recommended value for $S_{17}(0)$ of $19.0 \pm 1.0 \, \text{eV} \, \text{b}$ (95% confidence level).
From the article: If this value were adopted in solar models, the ${}^{7}\text{Be}(p,\gamma){}^{8}\text{B}$ reaction rate would no longer represent the dominant uncertainty in the theoretical prediction of the high-energy solar neutrino flux.
Comment: In the BP2000 SSM [19-19] $S_{17}(0) = 19 {}^{+2.7}_{-1.3} \, \text{eV} \, \text{b}$ (see [40-1]), taken from [6-13].
[Davids:2003aw]

24 - Astrophysical Cross Sections - Conference Proceedings

[24-1]
Structure of ^8B and astrophysical S_{17} factor, Shashi K. Dhiman, R. Shyam, J. Phys. G31 (2005) S1531, arXiv:nucl-th/0504062. NUSTAR05.
[Dhiman:2005sv]

25 - Detection Cross Sections

[25-1]
Precision evaluation of the Ga71(\u03bde,e\u2212) solar neutrino capture rate from the (He3,t) charge-exchange reaction, D. Frekers, T. Adachi, H. Akimune, M. Alanssari, B.A. Brown et al., Phys. Rev. C91 (2015) 034608.
[Frekers:2015wga]
[25-2]
Penning-trap Q-value determination of the reaction using threshold charge breeding of on-line produced isotopes, D. Frekers et al., Phys. Lett. B722 (2013) 233-237.
[Frekers-etal-PLB-722-233-2013]
[25-3]
The Ga-71(He-3, t) reaction and the low-energy neutrino response, D. Frekers, H. Ejiri, H. Akimune, T. Adachi, B. Bilgier et al., Phys. Lett. B706 (2011) 134-138.
[Frekers:2011zz]
[25-4]
Model dependence of the neutrino-deuteron disintegration cross sections at low energies, B. Mosconi, P. Ricci, E. Truhlik, P. Vogel, Phys. Rev. C75 (2007) 044610, arXiv:nucl-th/0702073.
[Mosconi:2007tz]
[25-5]
Constraining the leading weak axial two-body current by SNO and super-K, Jiunn-Wei Chen, Karsten M. Heeger, R. G. Hamish Robertson, Phys. Rev. C67 (2003) 025801, arXiv:nucl-th/0210073.
[Chen:2002pv]
[25-6]
Parameter-free effective field theory calculation for the solar proton fusion and hep processes, T. S. Park et al., Phys. Rev. C67 (2003) 055206, arXiv:nucl-th/0208055.
[Park:2002yp]
[25-7]
Solar-neutrino reactions on deuteron in effective field theory, S. Ando, Y. H. Song, T. S. Park, H. W. Fearing, K. Kubodera, Phys. Lett. B555 (2003) 49, arXiv:nucl-th/0206001.
[Ando:2002pv]
[25-8]
Nonlocality of the Nucleon Axial Charge and Solar Neutrino Problem, N. I. Kochelev, arXiv:hep-ph/0204235, 2002.
[Kochelev:2002fj]
[25-9]
Neutrino-deuteron reactions at solar neutrino energies, S. Nakamura et al., Nucl. Phys. A707 (2002) 561-576, arXiv:nucl-th/0201062.
[Nakamura:2002jg]
[25-10]
On the normalization of the neutrino deuteron cross section, J. F. Beacom, Stephen J. Parke, Phys. Rev. D64 (2001) 091302, arXiv:hep-ph/0106128.
[Beacom:2001hr]
[25-11]
QED corrections to neutrino electron scattering, M. Passera, Phys. Rev. D64 (2001) 113002, arXiv:hep-ph/0011190.
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[25-12]
Neutrino reactions on deuteron, S. Nakamura, T. Sato, V. Gudkov, K. Kubodera, Phys. Rev. C63 (2001) 034617, arXiv:nucl-th/0009012.
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[25-13]
Neutrino deuteron scattering in effective field theory at next-to-next-to-leading order, Malcolm Butler, Jiunn-Wei Chen, Xinwei Kong, Phys. Rev. C63 (2001) 035501, arXiv:nucl-th/0008032.
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[25-14]
The angular distribution of the reaction anti-nu/e + p - > e+ + n, P. Vogel, J. F. Beacom, Phys. Rev. D60 (1999) 053003, arXiv:hep-ph/9903554.
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[25-15]
Cross section uncertainties in the gallium neutrino source experiments, W. C. Haxton, Phys. Lett. B431 (1998) 110-118, arXiv:nucl-th/9804011.
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[25-16]
Gallium solar neutrino experiments: Absorption cross sections, neutrino spectra, and predicted event rates, J. N. Bahcall, Phys. Rev. C56 (1997) 3391, arXiv:hep-ph/9710491.
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Standard Neutrino Spectrum from $^8$B Decay, J. N. Bahcall et al., Phys. Rev. C54 (1996) 411-422, arXiv:nucl-th/9601044.
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[25-19]
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Solar neutrino experiments, John N. Bahcall, Rev. Mod. Phys. 50 (1978) 881-903, American Physical Society. http://link.aps.org/doi/10.1103/RevModPhys.50.881.
[Bahcall-RevModPhys.50.881]

26 - Detection Cross Sections - Conference Proceedings

[26-1]
Radiative Corrections to Low-Energy Neutrino-Deuteron Reactions Revisited, Takahiro Kubota, AIP Conf. Proc. 842 (2006) 886-888, arXiv:hep-ph/0601081. 'Particles and Nuclei International Conference' (PANIC'05, at Santa Fe in U.S.A., October 2005).
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Interactions of the solar neutrinos with the deuterons, B. Mosconi, P. Ricci, E. Truhlik, Eur. Phys. J. A27 (2006) 67-72, arXiv:nucl-th/0507029.
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Neutrino-deuteron reactions at solar neutrino energies, S. Nakamura et al., Nucl. Phys. A721 (2003) 549, arXiv:nucl-th/0212059. PaNic02, Osaka, Japan, September 30 - October 4, 2002.
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QED corrections to the scattering of solar neutrinos and electrons, M. Passera, J. Phys. G29 (2003) 141-152, arXiv:hep-ph/0102212. 50 Years of Electroweak Physics: A Symposium in Honor of Professor Alberto Sirlin's 70th Birthday, New York, New York, 27-28 Oct 2000.
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27 - Detector

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Calibration of liquid argon and neon detectors with $^{83}Kr^m$, W.H. Lippincott et al., Phys. Rev. C81 (2010) 045803, arXiv:0911.5453.
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[27-2]
Self-Calibration of Neutrino Detectors using characteristic Backgrounds, Joachim Kopp, Manfred Lindner, Alexander Merle, Nucl. Instrum. Meth. A582 (2007) 456-461, arXiv:hep-ph/0703055.
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[27-3]
Reconstruction of Composite Events in Neutrino Telescopes, Mathieu Ribordy, Nucl. Instrum. Meth. A574 (2007) 137-143, arXiv:astro-ph/0611604.
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27-5.
L. W. Alvarez, 1949. University of California Radiation Laboratory Report UCRL 328.
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27-6.
B. Pontecorvo, 1946. Chalk River Report PD 205.
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28 - Phenomenology

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The Dark Side of MSW: Solar Neutrinos as a Probe of Dark Matter-Neutrino Interactions, Francesco Capozzi, Ian M. Shoemaker, Luca Vecchi, arXiv:1702.08464, 2017.
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Scanning the Earth with solar neutrinos and DUNE, Ara Ioannisian, Alexei Smirnov, Daniel Wyler, arXiv:1702.06097, 2017.
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[28-3]
New neutrino physics and the altered shapes of solar neutrino spectra, Ilidio Lopes, Phys. Rev. D95 (2017) 015023, arXiv:1702.00447.
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Low-energy electronic recoil in xenon detectors by solar neutrinos, Jiunn-Wei Chen, Hsin-Chang Chi, C.-P. Liu, Chih-Pan Wu, arXiv:1610.04177, 2016.
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Influence of solar flares on behavior of solar neutrino flux, O. M. Boyarkin, G. G. Boyarkina, Astropart.Phys. 85 (2016) 39-42, arXiv:1609.05860.
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Detection of sub-GeV Dark Matter and Solar Neutrinos via Chemical-Bond Breaking, Rouven Essig, Jeremy Mardon, Oren Slone, Tomer Volansky, Phys.Rev. D95 (2017) 056011, arXiv:1608.02940.
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Projections for measuring the size of the solar core with neutrino-electron scattering, Jonathan H. Davis, Phys. Rev. Lett. 117 (2016) 211101, arXiv:1606.02558.
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[28-8]
Solar neutrinos as background in dark matter searches involving electron detection, A. Thomas, J.D. Vergados, J. Phys. G43 (2016) 07LT01, arXiv:1605.08008.
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[28-9]
Comparative analyses of 90Sr/90Y90 decay measurements at the Physikalisch-Technische Bundesanstalt and 222Rn decay measurements at the Geological Survey of Israel. Evidence of a solar influence, Peter Sturrock, Gideon Steinitz, Ephraim Fischbach, Alexander Parkhomov, Jeffrey Scargle, Astropart.Phys. 84 (2016) 8-14, arXiv:1605.03088.
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[28-10]
The Solar Solution: Tracking the Sun with Low Energy Neutrinos, Nicole Hartman, Stephen Sekula, arXiv:1605.01787, 2016.
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[28-11]
Generalized Lomb-Scargle periodogram analysis of Super-Kamiokande and Sudbury Neutrino Observatory solar neutrino datasets, Shantanu Desai, Dawei W. Liu, Astropart.Phys. 82 (2016) 86, arXiv:1604.06758.
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[28-12]
Physics from solar neutrinos in dark matter direct detection experiments, David G. Cerdeno et al., JHEP 1605 (2016) 118, arXiv:1604.01025.
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[28-13]
Limits on CPT violation from solar neutrinos, Jorge S. Diaz, Thomas Schwetz, Phys. Rev. D93 (2016) 093004, arXiv:1603.04468.
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[28-14]
Solar neutrino interactions with liquid scintillators used for double beta decay experiments, Hiroyasu Ejiri, Kai Zuber, J. Phys. G43 (2016) 045201, arXiv:1602.00364.
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[28-15]
Combined effect of NSI and SFP on solar electron neutrino oscillation, Deniz Yilmaz, Adv.High Energy Phys. 2016 (2016) 1435191, arXiv:1601.03161.
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[28-16]
Updated determination of the solar neutrino fluxes from solar neutrino data, Johannes Bergstrom et al., JHEP 1603 (2016) 132, arXiv:1601.00972.
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[28-17]
Comparative Analysis of Brookhaven National Laboratory Nuclear Decay Data and Super-Kamiokande Neutrino Data: Indication of a Solar Connection, P.A. Sturrock, E. Fischbach, arXiv:1511.08770, 2015.
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[28-18]
Minicharged Particles from the Sun: A Cutting-Edge Bound, Nuria Vinyoles, Hendrik Vogel, JCAP 1603 (2016) 002, arXiv:1511.01122.
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[28-19]
Peculiar seasonal effects in the neutrino day-night asymmetry, Oleg G. Kharlanov, arXiv:1509.08073, 2015.
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[28-20]
Neutrino Decay and Solar Neutrino Seasonal Effect, R. Picoreti, M. M. Guzzo, P. C. de Holanda, O. L. G. Peres, Phys.Lett. B761 (2016) 70-73, arXiv:1506.08158.
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[28-21]
Constraining Big Bang lithium production with recent solar neutrino data, Marcell P. Takacs, Daniel Bemmerer, Tamas Szucs, Kai Zuber, Phys. Rev. D91 (2015) 123526, arXiv:1505.07620.
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[28-22]
On the detection of neutrinos from solar flares using pion-decay photons to provide a time window template, G. de Wasseige, K. Hanson, N. van Eijndhoven, P. Evenson, K.-L. Klein, arXiv:1505.05837, 2015.
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[28-23]
Spallation Backgrounds in Super-Kamiokande Are Made in Muon-Induced Showers, Shirley Weishi Li, John F. Beacom, Phys. Rev. D91 (2015) 105005, arXiv:1503.04823.
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[28-24]
Oscillations of the $^7$Be solar neutrinos inside the Earth, A. N. Ioannisian, A. Yu. Smirnov, D. Wyler, Phys. Rev. D92 (2015) 013014, arXiv:1503.02183.
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[28-25]
Hypothesis about semiweak interaction and experiments with solar neutrinos, L.M. Slad, arXiv:1502.03262, 2015.
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[28-26]
New axion and hidden photon constraints from a solar data global fit, Nuria Vinyoles et al., JCAP 1510 (2015) 015, arXiv:1501.01639.
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[28-27]
Solar Neutrinos and the Decaying Neutrino Hypothesis, Jeffrey M. Berryman, Andre de Gouvea, Daniel Hernandez, Phys. Rev. D92 (2015) 073003, arXiv:1411.0308.
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[28-28]
ecCNO Solar Neutrinos: A Challenge for Gigantic Ultra-Pure Liquid Scintillator Detectors, F.L. Villante, Phys.Lett. B742 (2015) 279-284, arXiv:1410.2796.
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[28-29]
Updated fit to three neutrino mixing: status of leptonic CP violation, M.C. Gonzalez-Garcia, Michele Maltoni, Thomas Schwetz, JHEP 1411 (2014) 052, arXiv:1409.5439.
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[28-30]
No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results, R. Bernabei et al., Eur.Phys.J. C74 (2014) 3196, arXiv:1409.3516.
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Comment on 'Fitting the annual modulation in DAMA with neutrons from muons and neutrinos', P.S. Barbeau, J.I. Collar, Yu. Efremenko, K. Scholberg, Phys. Rev. Lett. 113 (2014) 229001, arXiv:1409.3185.
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[28-32]
Detecting gravity modes in the solar $^8B$ neutrino flux, Ilidio Lopes, Sylvaine Turck-Chieze, Astrophys.J. 792 (2014) L35, arXiv:1408.6671.
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[28-33]
Detecting the Upturn of the Solar $^8$B Neutrino Spectrum with LENA, Randolph Mollenberg et al., Phys.Lett. B737 (2014) 251-255, arXiv:1408.0623.
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[28-34]
Fitting the annual modulation in DAMA with neutrons from muons and neutrinos, Jonathan H. Davis, Phys. Rev. Lett. 113 (2014) 081302, arXiv:1407.1052.
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[28-35]
Neutrino oscillations refitted, D. V. Forero, M. Tortola, J. W. F. Valle, Phys. Rev. D90 (2014) 093006, arXiv:1405.7540.
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Status of three-neutrino oscillation parameters, circa 2013, F. Capozzi, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, A. Palazzo, Phys. Rev. D89 (2014) 093018, arXiv:1312.2878.
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[28-37]
Electron events from the scattering with solar neutrinos in the search of keV scale sterile neutrino dark matter, Wei Liao, Xiao-Hong Wu, Hang Zhou, Phys. Rev. D89 (2014) 093017, arXiv:1311.6075.
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[28-38]
Active and sterile neutrino oscillations inside the Sun in a phenomenological (3+1+2)-model, V. V. Khruschov, S. V. Fomichev, arXiv:1310.5817, 2013.
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[28-39]
Search for global f-modes and p-modes in the 8B neutrino flux, Ilidio Lopes, Astrophys.J. 777 (2013) L7, arXiv:1310.3467.
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[28-40]
The charged current neutrino cross section for solar neutrinos, and background to $\beta\beta(0\nu)$ experiments, H. Ejiri, S.R. Elliott, Phys. Rev. C89 (2014) 055501, arXiv:1309.7957.
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[28-41]
Constraining Alternative Gravity Theories Using Solar Neutrino Problem, Sumanta Chakraborty, Class.Quant.Grav. 31 (2014) 055005, arXiv:1309.0693.
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[28-42]
Probing the Sun's inner core using solar neutrinos: a new diagnostic method, Ilidio Lopes, Phys. Rev. D88 (2013) 045006, arXiv:1308.3346.
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[28-43]
Reexamination of constrains on the Maxwell-Boltzmann distribution by Helioseismology, Jian-jun He, Li-yong Zhang, Su-qing Hou, Shi-wei Xu, Chin.Phys. C37 (2013) 104001, arXiv:1307.0573.
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[28-44]
Day-Night Asymmetries in Active-Sterile Solar Neutrino Oscillations, H.W. Long, Y.F. Li, C. Giunti, JHEP 1308 (2013) 056, arXiv:1306.4051.
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Non-Standard Models, Solar Neutrinos, and Large $\theta_{13}$, R. Bonventre et al., Phys. Rev. D88 (2013) 053010, arXiv:1305.5835.
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CP-violating Phases in Active-Sterile Solar Neutrino Oscillations, H.W. Long, Y.F. Li, C. Giunti, Phys. Rev. D 87, 113004 (2013) 113004, arXiv:1304.2207.
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Analytical treatment of long-term observations of the day-night asymmetry for solar neutrinos, S. S. Aleshin, O. G. Kharlanov, A. E. Lobanov, Phys. Rev. D87 (2013) 045025, arXiv:1302.7201.
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Quasi-Dirac neutrinos and solar neutrino data, F. Rossi-Torres, A.C.B. Machado, V. Pleitez, Eur.Phys.J. C73 (2013) 2596, arXiv:1302.5590.
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Solar neutrino physics oscillations: Sensitivity to the electronic density in the Sun's core, Ilidio Lopes, Sylvaine Turck-Chieze, Astrophys.J. 765 (2013) 14, arXiv:1302.2791.
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[28-50]
MCMC Sampling in the global analysis of solar and reactor neutrino data, W. Liu, Y.F. Li, Q.Y. Liu, Int.J.Mod.Phys. A28 (2013) 1350005.
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[28-51]
Spectral Content of 22Na/44Ti Decay Data: Implications for a Solar Influence, Daniel O'Keefe et al., Astrophys.Space Sci. 344 (2013) 297-303, arXiv:1212.2198.
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[28-52]
New limits on neutrino magnetic moment through non-vanishing 13-mixing, Marcelo Moraes Guzzo, Pedro Cunha de Holanda, Orlando Luis Goulart Peres, arXiv:1212.1396, 2012.
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[28-53]
Using the Standard Solar Model to Constrain Composition and S-Factors, Aldo Serenelli, Carlos Pena-Garay, W. C. Haxton, Phys. Rev. D87 (2013) 043001, arXiv:1211.6740.
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An Analysis of Apparent r-Mode Oscillations in Solar Activity, the Solar Diameter, the Solar Neutrino Flux, and Nuclear Decay Rates, with Implications Concerning the Solar Internal Structure and Rotation, and Neutrino Processes, P.A. Sturrock et al., Astropart. Phys. 42 (2013) 62-69, arXiv:1211.6352.
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Update of Short-Baseline Electron Neutrino and Antineutrino Disappearance, C. Giunti, M. Laveder, Y.F. Li, Q.Y. Liu, H.W. Long, Phys. Rev. D86 (2012) 113014, arXiv:1210.5715.
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Solar constraints on asymmetric dark matter, Ilidio Lopes, Joseph Silk, Astrophys. J. 757 (2012) 130, arXiv:1209.3631.
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Global fit to three neutrino mixing: critical look at present precision, M.C. Gonzalez-Garcia, Michele Maltoni, Jordi Salvado, Thomas Schwetz, JHEP 12 (2012) 123, arXiv:1209.3023.
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Analysis of Solar Neutrino Data from SuperKamiokande I and II: Back to the Solar Neutrino Problem, H. J. Haubold, A. M. Mathai, R. K. Saxena, Entropy 16 (2014) 1414, arXiv:1209.1520.
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Constraining Non-Standard Interactions of the Neutrino with Borexino, Sanjib Kumar Agarwalla, Francesco Lombardi, Tatsu Takeuchi, JHEP 12 (2012) 079, arXiv:1207.3492.
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Global analysis of neutrino masses, mixings and phases: entering the era of leptonic CP violation searches, G.L. Fogli et al., Phys. Rev. D86 (2012) 013012, arXiv:1205.5254.
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Global status of neutrino oscillation parameters after Neutrino-2012, D.V. Forero, M. Tortola, J.W.F. Valle, Phys. Rev. D86 (2012) 073012, arXiv:1205.4018.
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Elastic scattering signals of solar neutrinos with enhanced baryonic currents, Maxim Pospelov, Josef Pradler, Phys. Rev. D85 (2012) 113016, arXiv:1203.0545.
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Exploring nu signals in dark matter detectors, Roni Harnik, Joachim Kopp, Pedro A. N. Machado, J. Phys. Conf. Ser. JCAP07 (2014) 026, arXiv:1202.6073.
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Solar neutrino records: Gauss or non-Gauss is the question, A. Haubold, H. J. Haubold, D. Kumar, arXiv:1202.1549, 2012.
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An estimate of $\vartheta_{14}$ independent of reactor antineutrino fluxes, Antonio Palazzo, Phys. Rev. D85 (2012) 077301, arXiv:1201.4280.
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The Variation of the Solar Neutrino Fluxes over Time in the Homestake, GALLEX(GNO) and Super-Kamiokande Experiments, K. Sakurai, H. J. Haubold, T. Shirai, Space RADIATION5 (2011) 207-216, arXiv:1111.5530.
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Global Neutrino Data Analysis and the Quest to Pin Down $\sin\vartheta_{13}$ in Different Mixing Matrix Parametrizations, Melin Huang, S. D. Reitzner, Wei-Chun Tsai, Huitzu Tu, arXiv:1111.3175, 2011.
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The fluxes of CN neutrinos from the Sun in case of mixing in a spherical layer in the solar core, Anatoly Kopylov, Valery Petukhov, JCAP 1203 (2012) 003, arXiv:1110.5703.
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Solar Neutrino Matter Effects Redux, A.B. Balantekin, A. Malkus, Phys. Rev. D85 (2012) 013010, arXiv:1109.5216.
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Optimization of Neutrino Oscillation Parameters using Differential Evolution, Ghulam Mustafa, Faisal Akram, Bilal Masud, Commun.Theor.Phys. 59 (2013) 324-330, arXiv:1109.2431.
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Testing alternative theories of gravity using the Sun, Jordi Casanellas, Paolo Pani, Ilidio Lopes, Vitor Cardoso, Astrophys. J. 745 (2012) 15, arXiv:1109.0249.
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Evidence of $\vartheta_{13} > 0$ from global neutrino data analysis, G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, A. M. Rotunno, Phys. Rev. D84 (2011) 053007, arXiv:1106.6028.
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Lorentz noninvariant oscillations of massless neutrinos are excluded, Vernon Barger, Jiajun Liao, Danny Marfatia, Kerry Whisnant, Phys. Rev. D84 (2011) 056014, arXiv:1106.6023.
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Neutrinos from WIMP annihilation in the Sun : Implications of a self-consistent model of the Milky Way's dark matter halo, Susmita Kundu, Pijushpani Bhattacharjee, Phys. Rev. D85 (2012) 123533, arXiv:1106.5711.
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Testing the very-short-baseline neutrino anomalies at the solar sector, Antonio Palazzo, Phys. Rev. D83 (2011) 113013, arXiv:1105.1705.
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A step toward CNO solar neutrinos detection in liquid scintillators, F.L. Villante, A. Ianni, F. Lombardi, G. Pagliaroli, F. Vissani, Phys. Lett. B701 (2011) 336-341, arXiv:1104.1335.
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Solar neutrino-electron scattering as background limitation for double beta decay, N. F. de Barros, K. Zuber, J. Phys. G38 (2011) 105201, arXiv:1103.5757.
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Model Independent Constraints on Solar Neutrinos, Lal Singh, Bhag C. Chauhan, Ravi Dutt, K. K. Sharma, S. Dev, arXiv:1102.4917, 2011.
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Hint of non-standard MSW dynamics in solar neutrino conversion, Antonio Palazzo, Phys. Rev. D83 (2011) 101701, arXiv:1101.3875.
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Solar neutrino spectrum, sterile neutrinos and additional radiation in the Universe, P. C. de Holanda, A. Yu. Smirnov, Phys. Rev. D83 (2011) 113011, arXiv:1012.5627.
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Search for modulations of the solar Be-7 flux in the next-generation neutrino observatory LENA, Michael Wurm et al., Phys. Rev. D83 (2011) 032010, arXiv:1012.3021.
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Neutrino oscillations trigger a minimal length, Marcus Bleicher, Piero Nicolini, Martin Sprenger, Class. Quant. Grav. 28 (2011) 235019, arXiv:1011.5225.
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Solar Neutrino Observables Sensitive to Matter Effects, Hisakazu Minakata, Carlos Pena-Garay, Adv. High Energy Phys. 2012 (2012) 349686, arXiv:1009.4869.
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Solar and Atmospheric Neutrinos: Limitations for Direct Dark Matter Searches, A. Gutlein et al., Nucl. Phys.B, Proc.Suppl.229-232 2012 (2012) 536, arXiv:1009.3815.
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Improving LMA predictions with non-standard interactions: neutrino decay in solar matter?, C.R. Das, Joao Pulido, Phys. Rev. D83 (2011) 053009, arXiv:1007.2167.
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Constraints on the opacity profile of the sun from helioseismic observables and solar neutrino flux measurements, F.L. Villante, Astrophys. J. 724 (2010) 98-110, arXiv:1006.3875.
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False-alarm probability in relation to over-sampled power spectra, with application to Super-Kamiokande solar neutrino data, Peter A. Sturrock, Jeffrey D. Scargle, Astrophys. J. 718 (2010) 527-529, arXiv:1006.0546.
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Effect of low mass dark matter particles on the Sun, Marco Taoso, Fabio Iocco, Georges Meynet, Gianfranco Bertone, Patrick Eggenberger, Phys. Rev. D82 (2010) 083509, arXiv:1005.5711.
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Improving LMA predictions with non standard interactions, C.R. Das, Joao Pulido, arXiv:1003.5904, 2010.
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Solar and atmospheric neutrinos: background sources for the direct dark matter search, A. Gutlein et al., Astropart. Phys. 34 (2010) 90-96, arXiv:1003.5530.
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Extraterrestrial Solar Neutrino Physics, W-Y. Pauchy Hwang, Jen-Chieh Peng, arXiv:1003.4347, 2010.
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Three-neutrino model analysis of the world's oscillation data, D. C. Latimer, D. J. Ernst, arXiv:nucl-th/0310083, 2003.
Comment: Another junk paper in which it is claimed that solar, atmospheric and LSND data can be fitted in a three-neutrino model.
Important data (energy spectra) are omitted and the analysis is very approximate.
The claimed best-fit values of the largest $\Delta{m}^2$ are either $ 1.2 \times 10^{-3} \, \mathrm{eV}^2 $ or $ > 0.1 \, \mathrm{eV}^2 $.
The smaller value $( 1.2 \times 10^{-3} \, \mathrm{eV}^2 )$ give $P_{\bar\nu_\mu\to\bar\nu_e}=0$ in LSND. Therefore, this case is equivalent to neglect LSND.
The larger values $( > 0.1 \, \mathrm{eV}^2 )$ obviously cannot fit the energy spectra of atmospheric neutrinos, which have been omitted in the analysis.
[C.G.].

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Solar neutrinos: the SNO salt phase results and physics of conversion, P. C. de Holanda, A. Yu. Smirnov, Astropart. Phys. 21 (2004) 287, arXiv:hep-ph/0309299.
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From the abstract: Existing experiments show that the $p-p$ solar neutrino flux is $1.01 \pm 0.02\, (1\sigma)$ times the flux predicted by the BP00 standard solar model; the $^7$Be neutrino flux is $0.93 {}^{+0.25}_{-0.63}$ the predicted flux; and the $^8$B flux is $1.01 \pm 0.04$ the predicted flux. The oscillation parameters are: $\Delta m^2 = 7.3^{+0.4}_{-0.6}\times 10^{-5}~{\rm eV^2}$ and $\tan^2 \theta_{12} = 0.41 \pm 0.04$.
...
A future $^7$Be $\nu-e$ scattering experiment accurate to $\pm 10$\% can reduce the uncertainty in the experimentally determined $^7$Be neutrino flux by a factor of four and the uncertainty in the $p-p$ neutrino flux by a factor of 2.5 (to $\pm 0.8$\%). A future $p-p$ experiment must be accurate to better than $\pm 3$\% to shrink the uncertainty in $\tan^2 \theta_{12}$ by more than 15\%.

Comment: Figure 4 shows the allowed regions for oscillation of solar neutrinos before and after the presentation of new data at TAUP03 conference [M.L.].
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Solar and supernova neutrino physics with Sudbury Neutrino Observatory, A. B. Balantekin, F. Loreti, Phys. Rev. D45 (1992) 1059-1065.
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The Solar neutrino problem and the neutrino magnetic moment, Joao Pulido, Phys.Rept. 211 (1992) 167-199.
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Solutions of the solar neutrino problem, S. A. Bludman, D. C. Kennedy, P. G. Langacker, Nucl. Phys. B374 (1992) 373-391.
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Monte Carlo exploration of Mikheev-Smirnov-Wolfenstein solutions to the solar neutrino problem, X. Shi, D. N. Schramm, John N. Bahcall, Phys. Rev. Lett. 69 (1992) 717-720.
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The Geometrical phase in neutrino spin precession and the solar neutrino problem, A.Yu. Smirnov, Phys. Lett. B260 (1991) 161-164.
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29 - Phenomenology - Conference Proceedings

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Concerning the variability of beta-decay measurements, P.A. Sturrock, E. Fischbach, A. Parkhomov, J.D. Scargle, G. Steinitz, arXiv:1510.05996, 2015.
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Peculiar seasoning in the neutrino day-night asymmetry: where and when to look for spices?, Oleg G. Kharlanov, Andrey E. Lobanov, arXiv:1510.00985, 2015. 16th Lomonosov Conference on Elementary Particle Physics (Moscow, Russia, August 22-28, 2013).
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Sterile neutrinos in the 3+s scenario and solar data, Joao Pulido, C.R. Das, PoS EPS-HEP2013 (2014) 527, arXiv:1310.0426. EPS Conference on High Energy Physics-EPS-HEP2013, 18-24 July 2013, Stockholm, Sweden.
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The Case for a Solar Influence on Certain Nuclear Decay Rates, Peter Sturrock, Ephraim Fischbach, Daniel Javorsek II, Jere Jenkins, Robert Lee, arXiv:1301.3754, 2013. 8th Patras Workshop on Axions, WIMPs and WISPs, Chicago, July 18-22, 2012.
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Neutrino Solar Flare detection for a saving alert system of satellites and astronauts, Daniele Fargion, arXiv:1106.3750, 2011. ICRC2011.
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Evidence for Time-Varying Nuclear Decay Rates: Experimental Results and Their Implications for New Physics, Ephraim Fischbach, Jere H. Jenkins, Peter A. Sturrock, arXiv:1106.1470, 2011. Rencontres de Moriond 2011: Gravitational Waves and Experimental Gravity (20-27 March 2011), La Thuile, Aosta valley, Italy.
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NSI can improve LMA predictions: neutrino decay in solar matter?, Joao Pulido, C.R. Das, Nucl. Phys. Proc. Suppl. 217 (2011) 350-352, arXiv:1012.3842. NOW 2010, Neutrino Oscillation Workshop, Conca Specchiulla (Otranto, Lecce, Italy), September 4-11, 2010.
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Lorentz violation in solar-neutrino oscillations, Jonah E. Bernhard, arXiv:1009.4717, 2010. Fifth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 28-July 2, 2010.
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Evidence for Solar Influences on Nuclear Decay Rates, Ephraim Fischbach et al., arXiv:1007.3318, 2010. Fifth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 28-July 2, 2010.
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[29-10]
Matter Effects in Solar Neutrino Active-Sterile Oscillations, Carlo Giunti, Yu-Feng Li, Prog. Part. Nucl. Phys. 64 (2010) 213-215, arXiv:0911.3934. Erice 2009 Neutrinos in Cosmology, in Astro-, Particle- and Nuclear Physics.
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Neutrinos from CNO cycle at the present epoch of the solar neutrino research, A. Kopylov, V.Petukhov, Prog. Part. Nucl. Phys. 64 (2010) 423-425, arXiv:0910.5152. Erice School 2009 in 'Progress in Particle and Nuclear Physics'.
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Remaining inconsistencies with solar neutrinos: can spin flavour precession provide a clue?, Joao Pulido, C R Das, Marco Picariello, J. Phys. Conf. Ser. 203 (2010) 012086, arXiv:0910.0203. TAUP 2009 (Rome).
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Neutrino Dipole Moments and Solar Experiments, M. Picariello et al., arXiv:0907.0637, 2009. 44th Rencontres de Moriond in the Electroweak 09.
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[29-14]
SNO, KamLAND and neutrino oscillations: theta(13), G.L. Fogli, E. Lisi, A. Marrone, A. Palazzo, A.M. Rotunno, arXiv:0905.3549, 2009. NEUTEL 2009, XIII International Workshop on 'Neutrino Telescopes' (Venice, Italy, March 10-13, 2009).
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[29-15]
Three-flavour neutrino oscillation update and comments on possible hints for a non-zero $\theta_{13}$, Michele Maltoni, Thomas Schwetz, PoS IDM2008 (2008) 072, arXiv:0812.3161. IDM2008, Aug. 18-22, 2008, Stockholm, Sweden.
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Solar Neutrinos as Background in Direct Dark Matter Searches, J. D. Vergados, I. Giomataris, AIP Conf. Proc. 1115 (2009) 7-12, arXiv:0809.0785. DSU.
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[29-17]
Analytical description of the Day-Night neutrino asymmetry, A. D. Supanitsky, J. C. D'Olivo, G. A. Medina-Tanco, arXiv:0708.0629, 2007. 30th International Cosmic Ray Conference, Merida, Mexico, July 2007.
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SNO and solar neutrino results, J. Maneira, Nucl. Phys. Proc. Suppl. 168 (2007) 84-89.
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MSW Oscillations - LMA and Subdominant Effects, Alexander Friedland, Nucl. Phys. Proc. Suppl. 221 (2011) 79-84, arXiv:hep-ph/0612266. Neutrino 2006.
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Gallium data variability and KamLAND, Joao Pulido, Bhag Chauhan, Marco Picariello, Nucl. Phys. Proc. Suppl. 168 (2007) 137-139, arXiv:hep-ph/0611331. NOW2006, Sep.9-16, Otranto, Italy.
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[29-21]
On the Mass Eigenstate Purity of $B^8$ Solar Neutrinos, Stephen Parke, Hiroshi Nunokawa, Renata Zukanovich Funchal, AIP Conf. Proc. 842 (2006) 889-891, arXiv:hep-ph/0601208. PANIC 2005.
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On solar neutrino fluxes in radiochemical experiments, R. N. Ikhsanov, Yu. N. Gnedin, E. V. Miletsky, arXiv:hep-ph/0512094, 2005. 9th International Pulkovo Conference on Solar Physics, Saint-Petersburg, Russia, July 4-9, 2005.
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Solar Neutrinos: Spin Flavour Precession and LMA, Joao Pulido, B. C. Chauhan, R. S. Raghavan, arXiv:hep-ph/0511341, 2005. 12th Lomonosov Conference in Elementary Particle Physics, Moscow, Aug 24-31 (2005).
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The measurement of theta(13) and delta: The role of the uncertainties on the solar and atmospheric parameters, D. Meloni, Nucl. Phys. Proc. Suppl. 155 (2006) 178, arXiv:hep-ph/0509370. NUFACT'05, 21-26 June 2005, Frascati.
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Global Analysis of Neutrino Oscillation, Srubabati Goswami, Abhijit Bandyopadhyay, Sandhya Choubey, Nucl. Phys. Proc. Suppl. 143 (2005) 121, arXiv:hep-ph/0409224. 21st International Conference on Neutrino Physics and Astrophysics (Neutrino 2004), Paris, France, 14-19 June 2004.
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Discovering Tau and Muon Solar Neutrino Flares above backgrounds, D. Fargion, F. Moscato, arXiv:astro-ph/0407211, 2004. Noon 2004, Februry 2004.
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Efficient solar anti-neutrino production in random magnetic fields, O. G. Miranda, T. I. Rashba, A. I. Rez, J. W. F. Valle, PoS AHEP2003 (2003) AHEP2003/072, arXiv:hep-ph/0405107. International Workshop on Astroparticle and High Energy Physics (AHEP-2003), Valencia, Spain, 14-18 October 2003.
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Problem of neutrino handedness in weak interactions, S. Ciechanowicz, W. Sobkow, M. Misiaszek, Acta Phys. Polon. B35 (2004) 1961, arXiv:astro-ph/0405066. Epiphany Conference on Astroparticle Physics, 8-11 January 2004, Cracow, Poland.
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Muon and Tau Neutrinos Spectra from Solar Flares, D. Fargion, F. Moscato, Chin. J. Astron. Astrophys. 3 (2003) S75, arXiv:astro-ph/0405039. Vulcano Conference 2003.
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[29-30]
Constraining neutrino magnetic moment with solar and reactor neutrino data, M. A. Tortola, PoS AHEP2003 (2003) 022, arXiv:hep-ph/0401135. International Workshop on Astroparticle and High Energy Physics (AHEP-2003), Valencia, Spain, 14-18 October 2003.
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Constraints on neutrino mixing parameters with the SNO data, Alain Bellerive (SNO), ECONF C030908 (2003) TUIT003, arXiv:hep-ex/0401018. PHYSTAT2003, SLAC, Stanford, Ca, USA, 8-11 Sep 2003. http://www.slac.stanford.edu/econf/C030908/papers/TUIT003.pdf.
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What can we learn on solar models from future solar neutrino experiments?, C. Pena-Garay, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/pena-garay.ppt.
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Physics Potential of Solar Neutrino Experiments, A.B. Balantekin, H. Yuksel, Nucl. Phys. Proc. Suppl. 138 (2005) 347, arXiv:hep-ph/0312281. TAUP 2003, 8th Int. Workshop on Topics in Astroparticle and Underground Physics, September 5 - 9, 2003 University of Washington, Seattle, Washington USA.
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Solar Neutrino Oscillation Parameters after KamLAND, Srubabati Goswami, Abhijit Bandyopadhyay, Sandhya Choubey, Phys. Atom. Nucl. 67 (2004) 1076, arXiv:hep-ph/0312028. 4th International Conference on Nonaccelerator New Physics (NANP 03), Dubna, Russia, 23-28 June 2003.
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[29-35]
Neutrino transition magnetic moments and the solar magnetic field from the Kamland evidence, V.Antonelli et al., arXiv:hep-ph/0310262, 2003. TAUP 2003.
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[29-36]
Neutrino Oscillations: A Global Analysis, G.L. Fogli et al., eConf C030626 (2003) THAT05, arXiv:hep-ph/0310012. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
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[29-37]
KamLAND and Solar Antineutrino Spectrum, Bhag C. Chauhan, Joao Pulido, E. Torrente-Lujan, Phys. Atom. Nucl. 67 (2004) 1151, arXiv:hep-ph/0309068. NANP'03, JINR Dubna, Russia, June 2003.
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Solar Neutrino Experiments: An Overview, Srubabati Goswami, Proc.Indian Natl.Acad.Sci. (2003), arXiv:hep-ph/0303075. Indian National Academy of Sciences, on Neutrino Physics.
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Magnus Expansion and Three-Neutrino Oscillations in Matter, Alexis A. Aguilar-Arevalo, L. G. Cabral-Rosetti, J. C. D'Olivo, J. Phys. Conf. Ser. 37 (2006) 161, arXiv:hep-ph/0302017. Mexican School of Astrophysics (EMA), Guanajuato, Mexico, July 31 - August 7, 2002.
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Neutrino Oscillations: Global Fits, T. Schwetz, 2003. MPI-TUM Ringberg Workshop on Neutrinos and Astroparticle Physics, July 24-25, 2003, Ringberg Castle, Tegernsee, Germany. http://www1.physik.tu-muenchen.de/~sfb375/Server/ringberg_2003/schwetz.pdf.
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Solar neutrino problem and KamLAND, S. Goswami, 2003. IV International conference on non-accelerator new physics - NANP 2003 - Dubna, Russia, June 23-28, 2003. http://nanp.dubna.ru/talks/goswami.pdf.
[Goswami:Nanp03]
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Solar and reactor neutrino analysis: Results and desiderata, E. Lisi, 2003. 4th Workshop on 'Neutrino Oscillations and their Origin' (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Lisi.pdf.
[Lisi:NOON2003]
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After Sno and Before Kamland: Present and Future of Solar and Reactor Neutrino Physics, P. Aliani et al., Aip Conf. Proc. 655 (2003) 103, arXiv:hep-ph/0211062. Third Tropical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology (Puerto Rico, August 2002).
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Standard and Non-Standard Physics in Neutrino Oscillations, M. Maltoni, Nucl. Phys. Proc. Suppl. 114 (2003) 191-196, arXiv:hep-ph/0210111. XXX International Meeting on Fundamental Physics (Jaca, Spain, 28/01-1/02/2002).
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[29-45]
Solar Neutrinos: Interpretation of Results, A. Smirnov, Nucl. Phys. Proc. Suppl. 118 (2003) 87, arXiv:hep-ph/0209131. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/smirnov.
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Standard and non-standard neutrino properties, J. W. F. Valle, Nucl. Phys. Proc. Suppl. 118 (2003) 255, arXiv:hep-ph/0209047. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/valle.
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[29-47]
The solar neutrino puzzle: present situation and future scenarios, E.Torrente-Lujan P. Aliani, V.Antonelli, R. Ferrari, M.Picariello, arXiv:hep-ph/0206308, 2002. Les Rencontres de Physique de la Vallee d'Aoste, February 2002.
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[29-48]
Solving the solar neutrino problem with kamLAND and BOREXINO, P. Aliani, V. Antonelli, R. Ferrari, M. Picariello, E. Torrente-Lujan, arXiv:hep-ph/0205061, 2002. 37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002.
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[29-49]
Analysis of solar neutrino induced double beta processes for several nuclei, P. Domin S. V. Semenov, Yu. V. Gaponov, F. Simkovic, Phys. Atom. Nucl. 65 (2002) 2184, arXiv:hep-ph/0205003. International Workhop on Non-Accelerator New Physics (NANP'01), Dubna, Russia, June 2001.
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Status of the Borexino experiment, Tristan J. Beau, arXiv:hep-ex/0204035, 2002. Rencontres de Moriond conference, Electroweak and Unified Theories session, 2002.
[Beau:2002hn]
[29-51]
A Unique Oscillation Solution to the Solar Neutrino Problem?, M. B. Smy, arXiv:hep-ex/0202020, 2002. NOON 2001 workshop.
[Smy:2002fs]
[29-52]
A Place in the Sun for Neutrinos, H. Robertson (SNO), 2002. 18th International Workshop on Weak Interactions and Neutrinos, WIN 2002, Christchurch, New Zealand, January 21 - 26, 2002. http://www.anta.canterbury.ac.nz/neutrino/overheads/H_Robertson.pdf.
[Robertson-WIN2002]
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Neutrino oscillations - global analyses, E. Lisi, 2002. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/lisi.
[Lisi-Nu2002]
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After the SNO NC result, C. Pena-Garay, 2002. Muon Week at CERN, 12 june 2002. http://muonstoragerings.web.cern.ch/muonstoragerings/Events/20020610/pena.pdf.
[Pena-CERN-02-12-06]
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Recent Progress in Neutrino Astrophysics, Steen Hannestad, arXiv:hep-ph/0112167, 2001.
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[29-56]
Solar neutrino experiments and Borexino perspectives, P. Aliani, V. Antonelli, M. Picariello, E. Torrente-Lujan, Nucl. Phys. Proc. Suppl. 110 (2002) 361-363, arXiv:hep-ph/0112101. TAUP 2001.
[Aliani:2001ba]
[29-57]
Solar neutrino results from the Sudbury Neutrino Observatory, Joshua R. Klein (SNO), Int. J. Mod. Phys. A17 (2002) 3378-3392, arXiv:hep-ex/0111040.
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Update on solar and atmospheric four-neutrino oscillations, M. C. Gonzalez-Garcia, M. Maltoni, Carlos Pena-Garay, PoS HEP2001 (2001) hep2001/191, arXiv:hep-ph/0108073.
[GonzalezGarcia:2001zi]
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Solar Neutrino Results from Super-Kamiokande, M. B. Smy (Super-Kamiokande), arXiv:hep-ex/0106064, 2001. XXXVI th Rencontres de Moriond 'Electroweak Interactions and Unified Theories', Les Arcs, France, 10-17 Mar 2001.
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A new fit to solar neutrinos using extra dimensions, David O. Caldwell, arXiv:hep-ph/0105275, 2001.
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Statistical analysis of solar neutrino data, M. V. Garzelli, C. Giunti, arXiv:hep-ph/0104085, 2001. 5th Topical Workshop at the Gran Sasso Laboratory: Solar Neutrinos: Where are the Oscillations?, Gran Sasso, Italy, 12-14 Mar 2001.
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Testing large mixing MSW solutions of the solar neutrino problem through earth regeneration effects, Antonio Palazzo, Nucl. Phys. Proc. Suppl. 100 (2001) 55-57, arXiv:hep-ph/0103027.
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Solar neutrino oscillations in the quasi-vacuum regime, Daniele Montanino, Nucl. Phys. Proc. Suppl. 100 (2001) 51-54, arXiv:hep-ph/0102076.
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Solar neutrino problem accounting for self-consistent magnetohydrodynamics solution for solar magnetic fields, T. I. Rashba, O. G. Miranda, Carlos Pena-Garay, V. B. Semikoz, J. W. F. Valle, Nucl. Phys. Proc. Suppl. 95 (2001) 123-129, arXiv:hep-ph/0101207.
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Neutrinos, large extra dimensions and solar neutrino puzzle, D. O. Caldwell, R. N. Mohapatra, S. J. Yellin, arXiv:hep-ph/0101043, 2001.
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Updated solution to the solar neutrino problem based on non-standard neutrino interactions, M. M. Guzzo, P. C. de Holanda, H. Nunokawa, Nucl. Phys. Proc. Suppl. 100 (2001) 62-64.
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Solar neutrino results from SAGE, V. N. Gavrin (SAGE), Nucl. Phys. Proc. Suppl. 91 (2001) 36-43.
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[29-68]
Solutions to the solar neutrino problem, P. Krastev, Nucl. Phys. Proc. Suppl. 100 (2001) 83-86.
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Solar Neutrino Results from Super-Kamiokande, Y. Suzuki, Nucl. Phys. Proc. Suppl. 91 (2001) 29-35.
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Solar neutrino results (from radio-chemical and water Cherenkov detectors), Y. Suzuki, Nucl. Phys. Proc. Suppl. 100 (2001) 14-23.
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Experiments with Solar and Atmospheric Neutrinos: Evidence for Neutrino Masses and Lepton Mixing. Experimental status and Future Projects, S. Schoenert, 2001. Astroparticle Physics Workshop, DESY - Zeuten, 19-21 June 2001. http://www.desy.de/desy-hs/zeuthen2001/presentations/main/schoenert.pdf.
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Solar neutrinos and gravity, T. K. Kuo, Nucl. Phys. Proc. Suppl. 100 (2001) 65-67.
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Solar Neutrinos, A.B. McDonald, 2001. TAUP2001 - Topics in Astroparticle and Underground Physics, LNGS, Italy (September 8-12, 2001). http://taup2001.lngs.infn.it/f2/f2.pdf.
[McDonald-TAUP2001]
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Statistical analysis of solar neutrino data, M. V. Garzelli, C. Giunti, Nucl. Phys. Proc. Suppl. 100 (2001) 77-79, arXiv:hep-ph/0012247. Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Ita, 9-16 Sep 2000.
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Helioseismology and solar neutrinos: An update, G. Fiorentini, B. Ricci, F. L. Villante, Nucl. Phys. Proc. Suppl. 95 (2001) 116-122, arXiv:astro-ph/0012239.
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Neutrino magnetic moment solution for the solar neutrino problem and the SNO experiment, Joao Pulido, Nucl. Phys. Proc. Suppl. 100 (2001) 71-73, arXiv:hep-ph/0012059. Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Ita, 9-16 Sep 2000.
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A frequentist analysis of solar neutrino data, M. V. Garzelli, C. Giunti, Nucl. Phys. Proc. Suppl. 95 (2001) 146-149, arXiv:hep-ph/0012044. EURESCO Conference on Frontiers in Particle Astrophysics and Cosmology, San Feliu de Guixols, Spain, 30 Sep - 5 Oct 2000.
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Elastic $\nu-e^-$ scattering of solar neutrinos with electromagnetic moments, W. Grimus, T. Schwetz, Nucl. Phys. Proc. Suppl. 95 (2001) 169-172, arXiv:hep-ph/0011169.
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Solar and atmospheric neutrino oscillations, M. C. Gonzalez-Garcia, Phys. Scripta T93 (2001) 26-31, arXiv:hep-ph/0010136.
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Experimental results on neutrino oscillations using atmospheric, solar and accelerator beams, D. Kielczewska (Super-Kamiokande and K2K), Acta Phys. Polon. B31 (2000) 1181-1207.
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Pseudo-Dirac scenario for neutrino oscillations, C. S. Lim, 2000. Workshop on Neutrino Oscillations and Their Origin, Fujiyoshida, Japan, 11-13 Feb 2000.
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Mixed MSW and vacuum solutions of solar neutrino problem, Q. Y. Liu, arXiv:hep-ph/9708308, 1997. 4th International Solar Neutrino Conference, Heidelberg, Germany, 8-11 Apr 1997.
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The Neutrino magnetic moment and time variations of the solar neutrino flux, Evgeny K. Akhmedov, arXiv:hep-ph/9705451, 1997.
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A Model independent approach to future solar neutrino experiments, S. M. Bilenky, C. Giunti, arXiv:hep-ph/9501241, 1995. Proceedings of the $4^{\mathrm{th}}$ \textit{International Conference on Physics Beyond the Standard Model}, Lake Tahoe, California, 13-18 Dec 1994, pag. 567-569.
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A Model independent analysis of solar neutrino data, S. M. Bilenky, C. Giunti, Nucl. Phys. Proc. Suppl. 43 (1994) 71-74, arXiv:hep-ph/9412296.
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[29-86]
A Model independent approach to solar neutrino experiments, S. M. Bilenky, C. Giunti, arXiv:hep-ph/9411373, 1994. Proceedings of the \textit{The First Artic Workshop on Future Physics and Accelerators}, Saariselka, Finland, 21-26 Aug 1994, pag. 170-192.
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Future solar neutrino experiments and neutrino spin flavor precession, S. M. Bilenky, C. Giunti, arXiv:hep-ph/9312211, 1993. Proceedings of the $6^{\mathrm{th}}$ \textit{International Workshop on Neutrino Telescopes}, Venezia, 22-24 February 1994, pag. 293-301.
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[29-88]
Neutrino mixing and future solar neutrino experiments, S. M. Bilenky, C. Giunti, Nucl. Phys. Proc. Suppl. 35 (1994) 430-432, arXiv:hep-ph/9310352.
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[29-89]
Pseudo-Dirac neutrinos and the solar neutrino problem, C. W. Kim, 1992. 4th International Symposium on Neutrino Telescopes, Venice, Italy, 10-13 Mar 1992.
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Pseudo-Dirac neutrinos and the solar neutrino problem, Hisakazu Minakata, Hiroshi Nunokawa, Phys. Rev. D45 (1992) 3316-3320.
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Pseudo-Dirac solar neutrinos?, Utpal Sarkar, Phys. Rev. D35 (1987) 1528.
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The solar neutrino puzzle, the Mikheev-Smirnov-Wolfenstein mechanism and the pseudo-Dirac neutrino, S. Toshev, Phys. Lett. B180 (1986) 285-289.
[Toshev:1986yp]

30 - Phenomenology - Models

[30-1]
Solar neutrinos, helicity effects and new affine gravity with torsion II, David Alvarez-Castillo, Diego Julio Cirilo-Lombardo, Jilberto Zamora-Saa, JHEAp 13 (2017) 14, arXiv:1611.02137.
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[30-2]
A model for large non-standard interactions of neutrinos leading to the LMA-Dark solution, Yasaman Farzan, Phys. Lett. B748 (2015) 311-315, arXiv:1505.06906.
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[30-3]
Discrete flavour symmetries for degenerate solar neutrino pair and their predictions, Anjan S. Joshipura, Ketan M. Patel, Phys. Rev. D90 (2014) 036005, arXiv:1405.6106.
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[30-4]
Relating large $U_{e3}$ to the ratio of neutrino mass-squared differences, Werner Rodejohann, Morimitsu Tanimoto, Atsushi Watanabe, Phys. Lett. B710 (2012) 636-640, arXiv:1201.4936.
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[30-5]
Isospin-Violating Dark Matter and Neutrinos From the Sun, Shao-Long Chen, Yue Zhang, Phys. Rev. D84 (2011) 031301, arXiv:1106.4044.
[Chen:2011vda]
[30-6]
Light WIMPs in the Sun: Constraints from Helioseismology, Daniel T. Cumberbatch, Joyce. A. Guzik, Joseph Silk, L. Scott Watson, Stephen M. West, Phys. Rev. D82 (2010) 103503, arXiv:1005.5102.
[Cumberbatch:2010hh]
[30-7]
Asymmetric dark matter and the Sun, Mads T. Frandsen, Subir Sarkar, Phys. Rev. Lett. 105 (2010) 011301, arXiv:1003.4505.
[Frandsen:2010yj]
[30-8]
Neutrino oscillation phase dynamically induced by f(R)-gravity, S. Capozziello, M. De Laurentis, D. Vernieri, Mod. Phys. Lett. A25 (2010) 1163-1168, arXiv:1001.4173.
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[30-9]
Golden Ratio Prediction for Solar Neutrino Mixing, Adisorn Adulpravitchai, Alexander Blum, Werner Rodejohann, New J. Phys. 11 (2009) 063026, arXiv:0903.0531.
[Adulpravitchai:2009bg]
[30-10]
Possible scenario for MaVaN's as the only neutrino flavor conversion mechanism in the Sun, Pedro Cunha de Holanda, JCAP 0907 (2009) 024, arXiv:0811.0567.
[deHolanda:2008nn]
[30-11]
CN-Cycle Solar Neutrinos and Sun's Primordial Core Metalicity, W. C. Haxton, A. M. Serenelli, Astrophys. J. 687 (2008) 678-691, arXiv:0805.2013.
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[30-12]
The golden ratio prediction for the solar neutrino mixing, Yuji Kajiyama, Martti Raidal, Alessandro Strumia, Phys. Rev. D76 (2007) 117301, arXiv:0705.4559.
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[30-13]
Lowering solar mixing angle in inverted hierarchy without charged lepton corrections, N.Nimai Singh, Monisa Rajkhowa, Abhijit Borah, J. Phys. G34 (2007) 345-352, arXiv:hep-ph/0603154.
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[30-14]
Fixing the Solar Parameters with Sterile Neutrinos, J.C. Gomez-Izquierdo, A. Perez-Lorenzana, Phys. Rev. D74 (2006) 013005, arXiv:hep-ph/0601223.
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[30-15]
Reply to 'Is U(e3) really related to the solar neutrino solutions?', Evgeny K. Akhmedov, G.C. Branco, M.N. Rebelo, arXiv:hep-ph/0007029, 2000.
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[30-16]
Is U(e3) really related to the solar neutrino solutions?, N. Haba, Tomoharu Suzuki, Mod.Phys.Lett. A15 (2000) 2257-2264, arXiv:hep-ph/0006281.
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[30-17]
Linking solar and long baseline terrestrial neutrino experiments, E. K. Akhmedov, G. C. Branco, M. N. Rebelo, Phys. Rev. Lett. 84 (2000) 3535, arXiv:hep-ph/9912205.
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Solar neutrinos and grand unification, K. S. Babu, Q. Y. Liu, A. Yu. Smirnov, Phys. Rev. D57 (1998) 5825-5835, arXiv:hep-ph/9707457.
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Decaying Dirac neutrinos, A. Acker, S. Pakvasa, James T. Pantaleone, Phys. Rev. D45 (1992) 1-4.
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31 - Phenomenology - Slides

[31-1]
Active-Sterile Solar Neutrino Oscillation, H. Long, 2014. Padua University, 27 October 2014. http://www.pd.infn.it/~laveder/unbound/seminari/fisica-neutrino/Long_Padova_2014.pdf.
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[31-2]
The antineutrino anomaly: implications for the solar neutrino sector, A. Palazzo, 2011. Rencontres de Moriond EW 2011, 13-20 March 2011, La Thuile, Italy. http://indico.in2p3.fr/getFile.py/access?contribId=39&sessionId=7&resId=0&materialId=slides&confId=4403.
[Palazzo2011]

32 - Phenomenology - Background

[32-1]
Measuring the Cosmic Ray Muon-Induced Fast Neutron Spectrum by (n,p) Isotope Production Reactions in Underground Detectors, Cristiano Galbiati, John. F. Beacom, Phys. Rev. C72 (2005) 025807, arXiv:hep-ph/0504227.
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33 - Phenomenology - Gallium Anomaly

[33-1]
The Reactor Antineutrino Anomaly, G. Mention et al., Phys. Rev. D83 (2011) 073006, arXiv:1101.2755.
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Statistical Significance of the Gallium Anomaly, Carlo Giunti, Marco Laveder, Phys. Rev. C83 (2011) 065504, arXiv:1006.3244.
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[33-3]
Gallium experiments with artificial neutrino sources as a tool for investigation of transition to sterile states, V. N. Gavrin, V. V. Gorbachev, E. P. Veretenkin, B. T. Cleveland, arXiv:1006.2103, 2010.
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Short-Baseline Electron Neutrino Disappearance, Tritium Beta Decay and Neutrinoless Double-Beta Decay, Carlo Giunti, Marco Laveder, Phys. Rev. D82 (2010) 053005, arXiv:1005.4599.
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[33-5]
VSBL Electron Neutrino Disappearance, Carlo Giunti, Marco Laveder, Phys. Rev. D80 (2009) 013005, arXiv:0902.1992.
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[33-6]
Limits on $\nu_e$ and $\bar\nu_e$ disappearance from Gallium and reactor experiments, Mario A. Acero, Carlo Giunti, Marco Laveder, Phys. Rev. D78 (2008) 073009, arXiv:0711.4222.
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[33-7]
$\nu_e$ Disappearance in MiniBooNE, Carlo Giunti, Marco Laveder, Phys. Rev. D77 (2008) 093002, arXiv:0707.4593.
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[33-8]
Short-Baseline Active-Sterile Neutrino Oscillations?, Carlo Giunti, Marco Laveder, Mod. Phys. Lett. A22 (2007) 2499-2509, arXiv:hep-ph/0610352.
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34 - Phenomenology - Gallium Anomaly - Conference Proceedings

[34-1]
The Gallium and reactor neutrinos anomaly, Mario A. Acero, Carlo Giunti, Marco Laveder, Nucl. Phys. Proc. Suppl. 188 (2009) 211-213. NOW 2008: Neutrino Oscillation Workshop, Conca Specchiulla (Otranto), Lecce, Italy, 6-13 Sep 2008.
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Unbound neutrino roadmaps, Marco Laveder, Nucl. Phys. Proc. Suppl. 168 (2007) 344-346. Workshop on Neutrino Oscillation Physics (NOW 2006), Otranto, Lecce, Italy, 9-16 Sep 2006.
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35 - Theory

[35-1]
Analytical description of quasivacuum oscillations of solar neutrinos, E. Lisi, A. Marrone, D. Montanino, A. Palazzo, S. T. Petcov, Phys. Rev. D63 (2001) 093002, arXiv:hep-ph/0011306.
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On the evolution of the neutrino state inside the sun, Alexander Friedland, Phys. Rev. D64 (2001) 013008, arXiv:hep-ph/0010231.
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Solar neutrinos and the MSW effect for three neutrino mixing, X. Shi, David N. Schramm, Phys. Lett. B283 (1992) 305-312.
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Anti-neutrinos from the sun, E. Kh. Akhmedov, Phys. Lett. B255 (1991) 84-88.
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Oscillation-assisted resonance spin-flavor precession and time variations of the solar neutrino flux, E. Kh. Akhmedov, Phys. Lett. B257 (1991) 163-167.
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Solar weak currents, neutrino oscillations and time variations, W. C. Haxton, W. M. Zhang, Phys. Rev. D43 (1991) 2484-2494.
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Resonant spin flavor precession of neutrinos and the solar neutrino problem, E. Kh. Akhmedov, O. V. Bychuk, Sov. Phys. JETP 68 (1989) 250-257.
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Resonant spin-flavor precession of solar and supernova neutrinos, Chong-Sa Lim, William J. Marciano, Phys. Rev. D37 (1988) 1368.
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Resonance enchancement of the neutrino spin precession in matter and the solar neutrino problem, E. Kh. Akhmedov, Sov. J. Nucl. Phys. 48 (1988) 382-383.
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Resonant amplification of neutrino spin rotation in matter and the solar-neutrino problem, E. Kh. Akhmedov, Phys. Lett. B213 (1988) 64.
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Nonadiabatic resonant conversion of solar neutrinos in three generations, C. W. Kim, S. Nussinov, W. K. Sze, Phys. Lett. B184 (1987) 403.
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Neutrino oscillations and the solar neutrino problem, A. Dar, A. Mann, Y. Melina, D. Zajfman, Phys. Rev. D35 (1987) 3607.
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Three neutrino oscillations and the solar neutrino experiments, T. K. Kuo, James Pantaleone, Phys. Rev. D35 (1987) 3432.
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Effect of transmission through the earth on neutrino oscillations, A. J. Baltz, J. Weneser, Phys. Rev. D35 (1987) 528.
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Analytic treatments of matter enhanced solar neutrino oscillations, W. C. Haxton, Phys. Rev. D35 (1987) 2352.
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Nonadiabatic level crossing in resonant neutrino oscillations, Stephen J. Parke, Phys. Rev. Lett. 57 (1986) 1275-1278.
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On the electric dipole moment of neutrino, L. B. Okun, Sov. J. Nucl. Phys. 44 (1986) 546.
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Adiabatic conversion of solar neutrinos, W. C. Haxton, Phys. Rev. Lett. 57 (1986) 1271-1274.
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Neutrino magnetic moment and time variation of solar neutrino flux, M. B. Voloshin, M. I. Vysotsky, Sov. J. Nucl. Phys. 44 (1986) 544.
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Resonant solar neutrino oscillation experiments, Stephen J. Parke, Terry P. Walker, Phys. Rev. Lett. 57 (1986) 2322.
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Matter effects for solar neutrino oscillations, J. Bouchez et al., Z. Phys. C32 (1986) 499.
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The solar neutrino problem and three neutrino oscillations, T. K. Kuo, James Pantaleone, Phys. Rev. Lett. 57 (1986) 1805-1808.
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Resonant amplification of neutrino oscillations in matter and solar neutrino spectroscopy, S. P. Mikheev, A. Yu. Smirnov, Nuovo Cim. C9 (1986) 17-26.
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Possible explanation of the solar-neutrino puzzle, H. A. Bethe, Phys. Rev. Lett. 56 (1986) 1305.
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Neutrino electrodynamics and possible consequences for solar neutrinos, L. B. Okun, M. B. Voloshin, M. I. Vysotsky, Sov. Phys. JETP 64 (1986) 446-452.
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Electromagnetic properties of neutrino and possible semiannual variation cycle of the solar neutrino flux, L. B. Okun, M. B. Voloshin, M. I. Vysotsky, Sov. J. Nucl. Phys. 44 (1986) 440.
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MSW regeneration of solar electron-neutrino in the earth, M. Cribier, W. Hampel, J. Rich, D. Vignaud, Phys. Lett. B182 (1986) 89.
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Resonance enhancement of oscillations in matter and solar neutrino spectroscopy, S. P. Mikheev, A. Yu. Smirnov, Sov. J. Nucl. Phys. 42 (1985) 913-917.
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Effect of neutrino magnetic moment on solar neutrino observations, Arturo Cisneros, Astrophys. Space Sci. 10 (1971) 87-92.
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36 - Future Experiments

[36-1]
Design and analysis of a 1-ton prototype of the Jinping Neutrino Experiment, Zongyi Wang, Yuanqing Wang, Zhe Wang, Shaomin Chen, Xinxi Du, Tianxiong Zhang, Ziyi Guo, Huanxin Yuan, Nucl. Instrum. Meth. A855 (2017) 81, arXiv:1703.01478.
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[36-2]
Letter of Intent: Jinping Neutrino Experiment, Jinping Neutrino Experiment group (Jinping), Chin.Phys. C41 (2017) 023002, arXiv:1602.01733.
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[36-3]
Solar neutrino detection in a large volume double-phase liquid argon experiment, D. Franco et al., JCAP 1608 (2016) 017, arXiv:1510.04196.
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[36-4]
Solar neutrino physics with low-threshold dark matter detectors, J. Billard, L. Strigari, E. Figueroa-Feliciano, Phys. Rev. D91 (2015) 095023, arXiv:1409.0050.
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[36-5]
Neutrino physics with multi-ton scale liquid xenon detectors, L. Baudis et al., JCAP 1401 (2014) 044, arXiv:1309.7024.
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[36-6]
Hyper-Kamiokande Physics Opportunities, E. Kearns et al. (Hyper-Kamiokande Working Group), arXiv:1309.0184, 2013.
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[36-7]
Future large-scale water-Cherenkov detector, L. Agostino et al. (MEMPHYS), Phys. Rev. ST Accel. Beams 16, 061001 (2013) 061001, arXiv:1306.6865.
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[36-8]
XMASS detector, K. Abe et al., Nucl.Instrum.Meth. A716 (2013) 78-85, arXiv:1301.2815.
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[36-9]
Study of the performance of a large scale water-Cherenkov detector (MEMPHYS), L. Agostino et al. (MEMPHYS), JCAP 1301 (2013) 024, arXiv:1206.6665.
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[36-10]
Letter of Intent: The Hyper-Kamiokande Experiment - Detector Design and Physics Potential, K. Abe et al., arXiv:1109.3262, 2011.
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[36-11]
Real-time spectroscopy of solar pp neutrinos using $^{150}$Nd, K. Zuber, Phys. Lett. B709 (2012) 6-8, arXiv:1108.2529.
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[36-12]
Studies of a three-stage dark matter and neutrino observatory based on multi-ton combinations of liquid xenon and liquid argon detectors, K. Arisaka et al., Astropart. Phys. 36 (2012) 93-122, arXiv:1107.1295.
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[36-13]
The next-generation liquid-scintillator neutrino observatory LENA, Michael Wurm et al. (LENA), Astropart. Phys. 35 (2012) 685-732, arXiv:1104.5620.
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[36-14]
Research of the natural neutrino fluxes by use of large volume scintillation detector at Baksan, I. R. Barabanov, G. Ya. Novikova, V. V. Sinev, E. A. Yanovich, arXiv:0908.1466, 2009.
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[36-15]
XAX: a multi-ton, multi-target detection system for dark matter, double beta decay and pp solar neutrinos, K. Arisaka et al., Astropart. Phys. 31 (2009) 63-74, arXiv:0808.3968.
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[36-16]
Potential for Precision Measurement of Solar Neutrino Luminosity by HERON, Y. H. Huang et al., Astropart. Phys. 30 (2008) 1-11, arXiv:0711.4095.
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[36-17]
Low energy tracking and particles identification in the MUNU Time Projection Chamber at 1 bar. Possible application in low energy solar neutrino spectroscopy, Z. Daraktchieva et al. (MUNU), J. Phys. G35 (2008) 125107, arXiv:0710.1049.
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[36-18]
Large underground, liquid based detectors for astro-particle physics in Europe: scientific case and prospects, J. Aysto et al., JCAP 0711 (2007) 011, arXiv:0705.0116.
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[36-19]
MEMPHYS: A large scale water Cerenkov detector at Frejus, A. de Bellefon et al., arXiv:hep-ex/0607026, 2006.
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[36-20]
How to observe 8B solar neutrinos in liquid scintillator detectors, A. Ianni, D. Montanino, F.L. Villante, Phys. Lett. B627 (2005) 38, arXiv:physics/0506171.
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[36-21]
Prototype scintillator cell for an In-based solar neutrino detector, Dario Motta et al., Nucl. Instrum. Meth. A547 (2005) 368, arXiv:physics/0502086.
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[36-22]
Calculations of liquid helium and neon VUV emission spectra, self-absorption and scattering for a neutrino detector, I. M. Savukov, arXiv:physics/0411215, 2004.
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[36-23]
Cosmogenic 11C production and sensitivity of organic scintillator detectors to pep and CNO neutrinos, C. Galbiati et al., Phys. Rev. C71 (2005) 055805, arXiv:hep-ph/0411002.
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Cryogenic avalanche detectors based on gas electron multipliers, A. Bondar et al., Nucl. Instrum. Meth. A524 (2004) 130, arXiv:physics/0403066.
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[36-25]
Neutrino Detection With CLEAN, D. N. McKinsey, K. J. Coakley, Astropart. Phys. 22 (2005) 355, arXiv:astro-ph/0402007.
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[36-26]
A design outline for a Cherenkoff neutrino observatory, E. P. Bonvin, S. T. Hatamian, arXiv:physics/0310160, 2003.
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[36-27]
Physics Chapter: NUSEL-Homestake Science Book, C. Aalseth et al. (Homestake), arXiv:nucl-ex/0308018, 2003.
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[36-28]
The Sensitivity of a Lithium Experiment on Solar Neutrinos to the Mixing Angle $\theta_{12}$, Anatoly Kopylov, Valery Petukhov, arXiv:hep-ph/0308004, 2003.
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[36-29]
Lithium Experiment in the Interplay of Solar and Neutrino Physics, Anatoly Kopylov, Valery Petukhov, arXiv:hep-ph/0306148, 2003.
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[36-30]
A Lithium Experiment as the Stringent Test of the Theory of Stellar Evolution, Anatoly Kopylov, Valery Petukhov, arXiv:hep-ph/0301016, 2003.
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[36-31]
Spectroscopy of low energy solar neutrinos using CdTe detectors, K. Zuber, Phys. Lett. B571 (2003) 148, arXiv:astro-ph/0206340.
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[36-32]
Cosmogenesis Backgrounds, Experiment Depth and the Solar Neutrino TPC, G. Bonvicini, A. Schreiner, Nucl. Instrum. Meth. A493 (2002) 90-98, arXiv:hep-ex/0203014.
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The HLMA project: determination of high delta-m^2 LMA mixing parameters and constraint on |U < sub > e3 < /sub > | with a new reactor neutrino experiment, Lothar Oberauer Stefan Schoenert, Thierry Lasserre, Astropart. Phys. 18 (2003) 565, arXiv:hep-ex/0203013.
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A preliminary look at the physics reach of a solar neutrino TPC: Time-independent two neutrino oscillations, G. Bonvicini et al., eConf C010630 (2001) E603, arXiv:hep-ph/0109199.
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Review of the technical issues associated with the construction of a solar neutrino TPC, G. Bonvicini, D. Naples, V. Paolone, Nucl. Instrum. Meth. A491 (2002) 402-418, arXiv:hep-ex/0109032.
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Why do solar neutrino experiments below 1-MeV?, J. N. Bahcall, arXiv:hep-ex/0106086, 2001.
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p p solar neutrino spectroscopy: Return of the indium detector, R. S. Raghavan, Phys. Rev. Lett. (2001), arXiv:hep-ex/0106054.
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LANNDD: A massive liquid argon detector for proton decay, supernova and solar neutrino studies, and a neutrino factory detector, David B. Cline, Franco Sergiampietri, John G. Learned, Kirk McDonald, Nucl. Instrum. Meth. A503 (2003) 136, arXiv:astro-ph/0105442.
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KamLAND: A reactor neutrino experiment testing the solar neutrino anomaly, A. Piepke (KamLAND), Nucl. Phys. Proc. Suppl. 91 (2001) 99-104.
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Bulk GaAs as a solar neutrino detector, V. N. Gavrin et al., Nucl. Instrum. Meth. A466 (2001) 119-125.
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[36-41]
Further studies of the OMNIS supernova neutrino observatory: Optimisation of detector configuration and possible extension to solar neutrinos, P. F. Smith, Astropart. Phys. 16 (2001) 75-96.
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Some future solar neutrino experiments, H. De Kerret, Nucl. Phys. Proc. Suppl. 100 (2001) 45-47.
[deKerret:2001zk]
[36-43]
Se-75 as a new neutrino source for calibrating low- threshold detectors of solar neutrinos, V. N. Kornoukhov, Phys. Atom. Nucl. 64 (2001) 256-260.
[Kornoukhov:2001tf]
[36-44]
Future solar neutrino experiments, F. von Feilitzsch, Nucl. Phys. Proc. Suppl. 91 (2001) 66-70.
[vonFeilitzsch:2001td]
[36-45]
Perspectives on the solar neutrino experiments, G. Bellini, Nucl. Phys. Proc. Suppl. 100 (2001) 87-90.
[Bellini:2001zs]
[36-46]
Science and technology of Borexino: A real time detector for low energy solar neutrinos, G. Alimonti et al. (Borexino), Astropart. Phys. 16 (2002) 205-234, arXiv:hep-ex/0012030.
[Alimonti:2000xc]
[36-47]
Study of solar neutrinos with the 600-t liquid argon ICARUS detector, F. Arneodo et al., Nucl. Instrum. Meth. A455 (2000) 376-389.
[Arneodo:2000fa]
[36-48]
The solar neutrino project HELLAZ: Status report on the hardware and the simulation, P. Gorodetzky (HELLAZ), Nucl. Instrum. Meth. A471 (2000) 131-135.
[Gorodetzky:2000jk]
[36-49]
The solar neutrino problem and the radiochemical lithium detector, S. N. Danshin, G. T. Zatsepin, A. V. Kopylov, V. V. Petukhov, E. A. Yanovich, Phys. Part. Nucl. 28 (1997) 1-4.
[Danshin:1997wz]

37 - Future Experiments - Conference Proceedings

[37-1]
Exploring Neutrino Interactions with MicroBooNE, Tia Miceli, arXiv:1411.4572, 2014. Physics in Collisions 2014.
[Miceli:2014cga]
[37-2]
Scintillator phase of the SNO+ experiment, V. Lozza (SNO+), J. Phys. Conf. Ser. 375 (2012) 042050, arXiv:1201.6599. TAUP2011.
[Lozza:2012bf]
[37-3]
The Physics Potential of the LENA Detector, Michael Wurm et al., Acta Phys. Polon. B41 (2010) 1749-1764, arXiv:1004.3474. Cracow Epiphany Conference, 5-8 January 2010.
[Wurm:2010ny]
[37-4]
The LAGUNA design study- towards giant liquid based underground detectors for neutrino physics and astrophysics and proton decay searches, D. Angus et al. (LAGUNA), arXiv:1001.0077, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
[Angus:2010sz]
[37-5]
Giant Liquid Argon Observatory for Proton Decay, Neutrino Astrophysics and CP-violation in the Lepton Sector (GLACIER), A. Badertscher et al., arXiv:1001.0076, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
[Badertscher:2010sy]
[37-6]
R&D for Future 100 kton Scale Liquid Argon Detectors, A. Marchionni, arXiv:0912.4417, 2009. European Strategy for Future Neutrino Physics, CERN, Oct. 2009.
[Marchionni:2009tj]
[37-7]
Underground Neutrino Detectors for Particle and Astroparticle Science: the Giant Liquid Argon Charge Imaging ExpeRiment (GLACIER), A. Rubbia, J. Phys. Conf. Ser. 171 (2009) 012020, arXiv:0908.1286.
[Rubbia:2009md]
[37-8]
The SNO+ Experiment, Mark C. Chen (SNO+), arXiv:0810.3694, 2008. ICHEP08.
[Chen:2008un]
[37-9]
Perspectives to Study a Solar CNO Cycle by Means of a Lithium Detector of Neutrinos, A. Kopylov, V. Petukhov, JCAP 0810 (2008) 007, arXiv:0806.0460. International Symposium 'Physics of Massive Neutrinos' at MILOS (Greece) 19-23 May 2008.
[Kopylov:2008zz]
[37-10]
Borexino, Lino Miramonti (BOREXINO), Nucl. Phys. Proc. Suppl. 221 (2011) 375, arXiv:hep-ex/0609011. XXII International Conference on Neutrino Physics and Astrophysics. Santa Fe, New Mexico, June 13-19, 2006.
[Miramonti:2006kp]
[37-11]
Low energy neutrino astronomy with the large liquid scintillation detector LENA, T. Marrodan Undagoitia et al., Prog. Part. Nucl. Phys. 57 (2006) 283-289, arXiv:hep-ph/0605229. International School of Nuclear Physics, Neutrinos in Cosmology, in Astro, Particle and Nuclear Physics, Erice (SICILY) 16 - 24 Sept. 2005.
[MarrodanUndagoitia:2006re]
[37-12]
A lithium experiment in the program of solar neutrino research, A. Kopylov, I. Orekhov, V. Petukhov, A. Solomatin, Phys. Atom. Nucl. 69 (2006) 1829-1832, arXiv:hep-ph/0601091. 5th International Conference on Non-accelerator New Physics (NANP 05), Dubna, Russia, 20-25 June 2005.
[Kopylov:2006je]
[37-13]
Is FLARE for solar flare?, Daniele Fargion, Proc. Sci. HEP2005 (2006) 180, arXiv:astro-ph/0512181. EPS International Europhysics Conference on High Energy Physics (HEP-EPS 2005), Lisbon, Portugal, 21-27 Jul 2005.
[Fargion:2005st]
[37-14]
On the possiblity of detecting Solar pp-neutrino with a large volume liquid organic scintillator detector, A.V.Derbin, O.Yu.Smirnov, O.A.Zaimidoroga, Phys. Atom. Nucl. 67 (2004) 2066, arXiv:physics/0403030. Nonaccelerating New Neutrino Physics, NANP-2003, Dubna.
[Derbin:2004ma]
[37-15]
Future solar neutrino experiments, Y. Suzuki, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/suzuki.pdf.
[Suzuki-Nu2004]
[37-16]
Lithium Experiment on Solar Neutrinos to Weight the CNO Cycle, A. Kopylov et al., Phys. Atom. Nucl. 67 (2004) 1182, arXiv:hep-ph/0310163. NANP 2003, Dubna, Russia, June 2003.
[Kopylov:2003tj]
[37-17]
New Projects in Underground Physics, M. Goodman, arXiv:hep-ex/0307017, 2003. 10th International Workshop on Neutrino Telescopes, Venice, March 2003.
[Goodman:2003qq]
[37-18]
GENIUS - A New Underground Observatory for Non-Accelerator Particle Physics, H. V. Klapdor-Kleingrothaus, Nucl. Phys. Proc. Suppl. 110 (2002) 364-368, arXiv:hep-ph/0206249. TAUP 2001, September 8-12, 2001.
[KlapdorKleingrothaus:2002mda]
[37-19]
Search for Cold Dark Matter and Solar Neutrinos with GENIUS and GENIUS-TF, I. V. Krivosheina, Prog. Part. Nucl. Phys. 48 (2002) 283-286, arXiv:hep-ph/0206149. International School on Nuclear Physics, 23rd Course: Neutrinos in Astro, Particle and Nuclear Physics, Erice, 18-26 September 2001.
[Krivosheina:2002jh]
[37-20]
Borexino: A real time liquid scintillator detector for low energy solar neutrino study, L. Miramonti, arXiv:hep-ex/0206063, 2002. 10th International Conference on Calorimetry in High Energy Physics.
[Miramonti:2002kr]
[37-21]
Phenomenological Study of Solar-Neutrino Induced Double Beta Decay of Mo100, P. Domin, F. Simkovic, S. V. Semenov, Yu. V. Gaponov, Czech. J. Phys. 52 (2002) 451, arXiv:hep-ph/0204143. MEDEX'01 (Prague, June, 2001), to appear in Czech. J. Phys. 52 (2002).
[Domin:2002mg]
[37-22]
Solar and Reactor Neutrinos: Upcoming Experiments and Future Projects, S. Schonert, Nucl. Phys. Proc. Suppl. 110 (2002) 277-287, arXiv:hep-ex/0202021. Contribution to the proceedings of 'TAUP2001 - Topics in Astroparticle and Underground Physics', LNGS, Italy (September 8-12, 2001). http://taup2001.lngs.infn.it/l3/l3.pdf.
[Schonert:2002ft]
[37-23]
Status of XMASS, M. Nakahata, 2002. IIIrd International Workshop on Low Energy Solar Neutrinos - LowNu 2002, 22-24 May 2002, Heidelberg, Germany. http://www.mpi-hd.mpg.de/nubis/www_lownu2002/transparency/nakahata_lownu_2002.pdf.
[Nakahata-LowNu2002]
[37-24]
The HLMA project, T. Lasserre, 2002. IIIrd International Workshop on Low Energy Solar Neutrinos - LowNu 2002, 22-24 May 2002, Heidelberg, Germany. http://www.mpi-hd.mpg.de/nubis/www_lownu2002/transparency/HLMAproject_lownu2002.ppt.
[Lasserre-LowNu2002]
[37-25]
Why do solar neutrino experiments below 1 MeV?, J. N. Bahcall, 2002. IIIrd International Workshop on Low Energy Solar Neutrinos - LowNu 2002, 22-24 May 2002, Heidelberg, Germany. http://www.mpi-hd.mpg.de/nubis/www_lownu2002/transparency/bahcall_lownu_2002.pdf.
[Bahcall-LowNu2002]
[37-26]
Borexino: Status Report, B. R. Vogelaar,, 2002. International Workshop on Neutrinos and Subterranean Science - NeSS 02, Washington, DC, September 19-21, 2002. http://mocha.phys.washington.edu/~int_talk/WorkShops/Neutrino02/Working_Groups/People/Vogelaar_R/vogelaar_thurs_snsnp.pdf.
[Bruce-talk:2002a]
[37-27]
UNO: Underground Nucleon Decay and Neutrino Observatory, C. McGrew, 2002. International Workshop on Neutrinos and Subterranean Science - NeSS 02, Washington, DC, September 19-21, 2002. http://mocha.phys.washington.edu/~int_talk/WorkShops/Neutrino02/Working_Groups/People/McGrew_C/mcgrew_thurs_protondecaywg.pdf.
[McGrew-talk:2002b]
[37-28]
New underground neutrino observatory - GENIUS - in the new millenium: For solar neutrinos, dark matter and double beta decay, H. V. Klapdor-Kleingrothaus, arXiv:hep-ph/0104028, 2001. International Workshop on Low Energy Solar Neutrinos (LowNu2), December 4 and 5, 2000, Tokyo, Japan.
[KlapdorKleingrothaus:2000eq]
[37-29]
New physics in the new millennium with GENIUS: Double beta decay, dark matter, solar neutrinos, H. V. Klapdor-Kleingrothaus, Part. Nucl. Lett. 104 (2001) 20-39, arXiv:hep-ph/0102319. International Workshop on Non-Accelerator New Physics in Neutrino Observations (NANPino), Dubna, Russia, July 19-22, 2000.
[KlapdorKleingrothaus:2000rd]
[37-30]
GENIUS - A new facility of non-accelerator particle physics, H. V. Klapdor-Kleingrothaus, Nucl. Phys. Proc. Suppl. 100 (2001) 350-355, arXiv:hep-ph/0102277. Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Italy, 9-16 Sep 2000.
[KlapdorKleingrothaus:2000dh]

38 - Education

[38-1]
Solar Neutrinos: A Popular Account, John N. Bahcall, arXiv:physics/0411190, 2004.
[Bahcall:2004in]

39 - History

[39-1]
Solving the Mystery of the Missing Neutrinos, John Bahcall, arXiv:physics/0406040, 2004.
[Bahcall:2004cc]
[39-2]
Nobel Lecture: A half-century with solar neutrinos, R. Davis, Rev. Mod. Phys. 75 (2003) 985-994.
[Davis:2003kh]
[39-3]
A half-century with solar neutrinos, R. Davis, Int. J. Mod. Phys. A18 (2003) 3089-3108.
[Davis:2003xx]
[39-4]
Memories of a Nobel laureate, R. Davis, CERN Cour. 42N10 (2002) 15-17.
[Davis:2002fb]
[39-5]
The beginning of a new science, J. N. Bahcall, R. Davis, CERN Cour. 40N6 (2000) 17-21. http://www.cerncourier.com/main/article/40/6/18.
[Bahcall:2000up]
[39-6]
The evolution of neutrino astronomy, J. N. Bahcall, Raymond Davis, Publ. Astron. Soc. Pac. 112 (2000) 429-433, arXiv:astro-ph/9911486.
[Bahcall:2000rt]

40 - History - Conference Proceedings

[40-1]
Solar Models: An Historical Overview, J. N. Bahcall, AAPPS Bull. 12N4 (2002) 12, arXiv:astro-ph/0209080. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/bahcall.
[Bahcall:2002ng]
[40-2]
Astrophysical neutrinos: 20th century and beyond, J. N. Bahcall, Nucl. Phys. Proc. Suppl. 91 (2001) 9-17, arXiv:hep-ph/0009044. Neutrino 2000.
[Bahcall:2000ue]

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