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Solar Neutrino Measurements,
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Theoretical neutrino physics,
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Astrophysical Neutrino Telescopes,
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Neutrino Mixing,
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Neutrino Masses and Mixing: Evidence and Implications,
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The solar neutrino problem and its oscillation solution,
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Nuclear spin isospin responses for low-energy neutrinos,
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Solar neutrinos,
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Solar fusion cross-sections,
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Standard Solar Composition,
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The Solar interior,
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Particle physics confronts the solar neutrino problem,
Palash B. Pal,
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The Solar neutrino problem and the neutrino magnetic moment,
Joao Pulido,
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Neutrino oscillations in matter,
T. K. Kuo, James Pantaleone,
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Resonance oscillations of neutrinos in matter,
S. P. Mikheev, A. Yu. Smirnov,
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Experimental and theoretical nuclear astrophysics: the quest for the origin of the elements,
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Solar Neutrino Experiments,
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The Internal Constitution of the Stars,
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Solar Neutrino Measurements,
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XXXVIII International Symposium on Physics in Collision, Bogota, Colombia, 11-15 september 2018.
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Helioseismology and solar neutrinos,
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4th Azarquiel School of Astronomy, June 2017, Porto Paolo di Capo Passero, Syracuse (Italy).
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Current State of Astrophysical Opacities: A White Paper,
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Second Workshop on Astrophysical Opacities, Kalamazoo, Michigan, USA: 2017 August 1st - 4th.
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Francesco Vissani,
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arXiv:1706.05435.
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Neutrino Astrophysics,
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52th Winter School of Theoretical Physics, Ladek Zdroj, 14-21 February 2016.
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arXiv:1601.08234.
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Neutrino Oscillation Workshop, 2014.
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An Experimental Review of Solar Neutrinos,
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Everything Under the Sun: A Review of Solar Neutrino,
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Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data,
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14th ICATPP Conference on Astroparticle, Particle, Space Physics and Detectors for Physics Applications (Villa Olmo, Como - September 2013).
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Solar Neutrinos in 2011,
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Lino Miramonti,
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XXII Int. Conf. on Neutrino Physics and Astrophysics, Santa Fe, 13-19 June 2006.
[Gavrin:2007wc] - [3-28]
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Nuclear Astrophysics: CIPANP 2006,
W. C. Haxton,
870
arXiv:nucl-th/0609006.
CIPANP 2006.
[Haxton:2006ae] - [3-29]
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Global fits to neutrino oscillation data,
Thomas Schwetz,
T127
arXiv:hep-ph/0606060.
SNOW2006 workshop, Stockholm, 2-6 May 2006.
[Schwetz:2006dh] - [3-30]
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Solar Neutrinos,
R.G.H. Robertson,
57
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.
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Helioseismology, Neutrinos and Radiative Zones,
S. Turck-Chieze, S. Couvidat, L. Piau,
17
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.
[Turck-Chieze:2005qdb] - [3-32]
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Neutrino oscillations: Current status and prospects,
Thomas Schwetz,
B36
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.
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Status of the Standard Solar Model Prediction of Solar Neutrino Fluxes,
Moshe Gai,
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arXiv:nucl-ex/0510081.
Fifth International Conferenceon Non-Accelerator New Physics, Dubna, June 20-25, 2005.
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Review of Solar and Reactor Neutrinos,
A.W.P. Poon,
A21
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).
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Neutrino mass and mixing parameters: A short review,
G.L. Fogli et al.,
arXiv:hep-ph/0506307,
40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005.
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-
Solar Models and Solar Neutrinos: Current Status,
John N. Bahcall,
T121
arXiv:hep-ph/0412068.
Nobel Symposium 2004, Enkoping, Sweden, August 19-24, 2004.
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Evidence for Neutrino Mass: A Decade of Discovery,
K.M. Heeger,
arXiv:hep-ex/0412032,
SEESAW25: International Conference on the Seesaw Mechanism and Neutrino Mass, Paris, France, 10-11 June 2004.
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Three-flavour effects and CP- and T-violation in neutrino oscillations,
Evgeny Akhmedov,
T121
arXiv:hep-ph/0412029.
Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
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Recent Results of non-accelarator-based neutrino experiments,
Yifang Wang,
A20
arXiv:hep-ex/0411028.
'32nd International Conference on High Energy Physics', Aug. 16-22, 2004, Beijing, P.R. China.
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The solar chemical composition,
Martin Asplund, Nicolas Grevesse, Jacques Sauval,
A777
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.
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Physics of Massive Neutrinos,
J. W. F. Valle,
149
arXiv:hep-ph/0410103.
Sixth International Conf. on Neutrino Factories and SuperBeams (NuFact04) Osaka, Japan, July 26-August 1, 2004.
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Neutrino 2004: Concluding Talk,
Guido Altarelli,
143
arXiv:hep-ph/0410101.
Neutrino 2004, Paris, 14-19 June 2004.
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Global Analysis of Neutrino Data,
M. C. Gonzalez-Garcia,
T121
arXiv:hep-ph/0410030.
Nobel Symposium on Neutrino Physics, Haga Slott, Enkoping, Sweden.
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Solar Neutrino Oscillation - An Overview,
D. P. Roy,
arXiv:hep-ph/0409336,
Xth International Symposium on Particles, Strings and Cosmology (PASCOS), Boston, 16-22 August 2004.
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Solar Neutrino Oscillation Parameters in Experiments with Reactor Anti-Neutrinos,
Sandhya Choubey,
arXiv:hep-ph/0402288,
2nd International Workshop on Neutrino oscillations in Venice (NOVE), December 3-5, 2003, Venice, Italy.
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Neutrinos: '...annus mirabilis',
A. Yu. Smirnov,
arXiv:hep-ph/0402264,
2nd Int. Workshop on Neutrino oscillations in Venice (NOVE) December 3-5, 2003, Venice, Italy.
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Global analysis of neutrino oscillation,
S. Goswami,
Neutrino 2004, 13-19 June 2004, Paris, France.
http://neutrino2004.in2p3.fr/slides/tuesday/goswami.pdf.
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Neutrino physics, recent results,
E. Lisi,
IFAE-2004, 14-16 April 2004, Torino, Italy.
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Review of Solar Neutrino Experiments,
Alain Bellerive,
A19
arXiv:hep-ex/0312045.
XXI International Symposium on Lepton and Photon Interactions at High Energies, Fermilab, USA, 11-16 August 2003.
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Solar neutrino oscillation phenomenology,
S. Goswami,
62
arXiv:hep-ph/0307224.
9th International Symposium on Particles, Strings and Cosmology (PASCOS 03), Mumbai, India, 3-8 Jan 2003.
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Neutrino masses twenty-five years later,
J. W. F. Valle,
687
arXiv:hep-ph/0307192.
MRST'03 (Joe-Fest), Syracuse, NY, May 2003.
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Neutrino oscillations in the framework of the tree-neutrino mixing,
S. M. Bilenky,
arXiv:hep-ph/0307186,
Ist Yamada Symposium Om neutrinos and Dark Matter in Nuclear Physics, June 9-14, 2003, Nara, Japan.
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Neutrino Physics after KamLAND,
A. Yu. Smirnov,
arXiv:hep-ph/0306075,
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.
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Status of Neutrino Fits,
C. Giunti,
arXiv:hep-ph/0305139,
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.
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The MSW effect and Solar Neutrinos,
A. Yu. Smirnov,
arXiv:hep-ph/0305106,
11th workshop on Neutrino Telescopes, Venice, March 11- 14, 2003.
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Solar Fusion and The Coulomb Dissociation of 8B; What Have We Learned and Where Do We Go From Here?,
Moshe Gai,
21
arXiv:nucl-ex/0303009.
19th Winter Workshop on Nuclear Dynamics, Breckenridge, Colorado, 9-15 Feb 2003.
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Neutrino Physics: Experimental Status,
T. Kajita,
19th International Workshop on Weak Interactions and Neutrinos, WIN2003, October 6-11, Lake Geneva, Wisconsin, USA.
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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.].
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Neutrino Masses and Mixing: Where We Stand and Where We are Going,
M. C. Gonzalez-Garcia,
arXiv:hep-ph/0211054,
10th International Conference on Supersymmetry and Unification of Fundamental Interactions, SUSY02 (June 17-23, 2002, DESY, Hamburg).
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Theory of Neutrino Masses and Mixing,
M. C. Gonzalez-Garcia,
117
arXiv:hep-ph/0210359.
31st international conference on high energy physics (ICHEP 2002), Amsterdam, 24-31 July 2002.
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Current Status of Neutrino Masses and Mixings,
C. Giunti,
117
arXiv:hep-ph/0209103.
31st International Conference on High Energy Physics 'ICHEP02', 24-31 July 2002, Amsterdam.
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Global analysis of solar neutrinos,
S. Choubey,
Fourth NuFact '02 Workshop on Neutrino Factories based on Muon Storage Rings, Imperial College, London, 1-6 July 2002.
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Actuality and potentiality of neutrino mixing,
C. Giunti,
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.
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Solar Neutrinos,
K. Nishikawa,
Topical Seminar on Frontier of Particle Physics 2002: Neutrinos and Cosmology, 20-25 August 2002, Beijing, China.
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Review of solar models and helioseismology,
S. Turck-Chieze,
91
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Solar flare observations with the Radio Neutrino Observatory Greenland (RNO-G),
S. Agarwal et al.,
arXiv:2404.14995,
[Agarwal:2024tat] - [4-2]
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A Measurement of Solar $pp$ Neutrino Flux using PandaX-4T Electron Recoil Data,
Xiaoying Lu et al.
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arXiv:2401.07045,
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Solar neutrino measurements using the full data period of Super-Kamiokande-IV,
K. Abe et al.
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arXiv:2312.12907,
[Super-Kamiokande:2023jbt] - [4-4]
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Search for Periodic Time Variations of the Solar $^8$B Neutrino Flux Between 1996 and 2018 in Super-Kamiokande,
K. Abe et al.,
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Final results of Borexino on CNO solar neutrinos,
D. Basilico et al.,
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Searching for neutrinos from solar flares across solar cycles 23 and 24 with the Super-Kamiokande detector,
K. Okamoto et al.
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arXiv:2210.12948,
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A First Search for Solar $^8$B Neutrino in the PandaX-4T Experiment using Neutrino-Nucleus Coherent Scattering,
Wenbo Ma et al.
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130
arXiv:2207.04883.
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Improved measurement of solar neutrinos from the Carbon-Nitrogen-Oxygen cycle by Borexino and its implications for the Standard Solar Model,
S. Appel et al.
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129
arXiv:2205.15975.
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Independent determination of the Earth's orbital parameters with solar neutrinos in Borexino,
S. Appel et al.
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145
arXiv:2204.07029.
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Testing Non-Standard Interactions Between Solar Neutrinos and Quarks with Super-Kamiokande,
P. Weatherly et al.
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arXiv:2203.11772,
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First Directional Measurement of sub-MeV Solar Neutrinos with Borexino,
M. Agostini et al.
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arXiv:2112.11816.
[BOREXINO:2021efb] - [4-12]
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First demonstration of directional measurement of sub-MeV solar neutrinos in a liquid scintillator detector with Borexino,
M. Agostini et al.
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105
arXiv:2109.04770.
[BOREXINO:2021xzc] - [4-13]
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Search for Solar Flare Neutrinos with the KamLAND detector,
S. Abe et al.
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924
arXiv:2105.02458.
[KamLAND:2021sda] - [4-14]
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Search for GeV Neutrino Emission During Intense Gamma-Ray Solar Flares with the IceCube Neutrino Observatory,
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D103
arXiv:2101.00610.
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Search for solar electron anti-neutrinos due to spin-flavor precession in the Sun with Super-Kamiokande-IV,
K. Abe et al.
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139
arXiv:2012.03807.
[Super-Kamiokande:2020frs] - [4-16]
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A search for $hep$ solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory,
B. Aharmim et al.
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D102
arXiv:2007.08018.
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First Direct Experimental Evidence of CNO neutrinos,
M. Agostini et al.
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arXiv:2006.15115.
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Sensitivity to neutrinos from the solar CNO cycle in Borexino,
M. Agostini et al.
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C80
arXiv:2005.12829.
[BOREXINO:2020hox] - [4-19]
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Search for exotic neutrino-electron interactions using solar neutrinos in XMASS-I,
K. Abe et al.
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arXiv:2005.11891.
[XMASS:2020zke] - [4-20]
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Measurement of the $^8$B Solar Neutrino Flux in SNO+ with Very Low Backgrounds,
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D99
arXiv:1812.03355.
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Constraints on Neutrino Lifetime from the Sudbury Neutrino Observatory,
B. Aharmim et al.
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D99
arXiv:1812.01088.
[SNO:2018pvg] - [4-22]
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Tests of Lorentz invariance at the Sudbury Neutrino Observatory,
B. Aharmim et al.
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D98
arXiv:1811.00166.
[SNO:2018mge] - [4-23]
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Improved measurement of 8B solar neutrinos with 1.5 kt y of Borexino exposure,
M. Agostini et al.
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D101
arXiv:1709.00756.
[Borexino:2017uhp] - [4-24]
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First Simultaneous Precision Spectroscopy of $pp$, $^7$Be, and $pep$ Solar Neutrinos with Borexino Phase-II,
M. Agostini et al.
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D100
arXiv:1707.09279.
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Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino,
M. Agostini et al.
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arXiv:1701.07970.
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Solar Neutrino Measurements in Super-Kamiokande-IV,
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D94
arXiv:1606.07538.
[Super-Kamiokande:2016yck] - [4-27]
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Measurement of neutrino flux from the primary proton-proton fusion process in the Sun with Borexino detector,
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47
arXiv:1507.02432.
[Borexino:2015axw] - [4-28]
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7Be Solar Neutrino Measurement with KamLAND,
A. Gando et al.
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C92
arXiv:1405.6190.
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Neutrinos from the primary proton-proton fusion process in the Sun,
G. Bellini et al.
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512
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First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation,
A. Renshaw et al.
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112
arXiv:1312.5176.
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New limits on heavy sterile neutrino mixing in ${^{8}\rm{B}}$-decay obtained with the Borexino detector,
G. Bellini et al.
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072010
arXiv:1311.5347.
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Final results of Borexino Phase-I on low energy solar neutrino spectroscopy,
G. Bellini et al.
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D89
arXiv:1308.0443.
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First evidence of pep solar neutrinos by direct detection in Borexino,
G. Bellini et al.
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108
arXiv:1110.3230.
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Combined Analysis of all Three Phases of Solar Neutrino Data from the Sudbury Neutrino Observatory,
B. Aharmim et al.
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C88
arXiv:1109.0763.
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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.
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C87
arXiv:1107.2901.
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Measurement of the 8B Solar Neutrino Flux with KamLAND,
S. Abe et al.
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C84
arXiv:1106.0861.
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Absence of day-night asymmetry of 862 keV $^7\text{Be}$ solar neutrino rate in Borexino and MSW oscillation parameters,
G. Bellini et al.
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B707
arXiv:1104.2150.
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Precision measurement of the $^7\text{Be}$ solar neutrino interaction rate in Borexino,
G. Bellini et al.
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107
arXiv:1104.1816.
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Solar neutrino results in Super-Kamiokande-III,
K. Abe et al.
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D83
arXiv:1010.0118.
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Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS,
G. Bellini
(Borexino),
B696
arXiv:1010.0029.
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Reanalysis of the GALLEX solar neutrino flux and source experiments,
F. Kaether, W. Hampel, G. Heusser, J. Kiko, T. Kirsten,
B685
arXiv:1001.2731.
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Low Energy Threshold Analysis of the Phase I and Phase II Data Sets of the Sudbury Neutrino Observatory,
B. Aharmim et al.
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C81
arXiv:0910.2984.
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Searches for High Frequency Variations in the $^8\text{B}$ Solar Neutrino Flux at the Sudbury Neutrino Observatory,
B. Aharmim et al.
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710
arXiv:0910.2433.
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Measurement of the solar neutrino capture rate with Gallium metal, Part III,
J. N. Abdurashitov et al.
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C80
arXiv:0901.2200.
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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.
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D82
arXiv:0808.2868.
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The Borexino detector at the Laboratori Nazionali del Gran Sasso,
G. Alimonti et al.
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A600
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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.
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101
arXiv:0806.0989.
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New results on solar neutrino fluxes from 192 days of Borexino data,
C. Arpesella et al.
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Solar neutrino measurements in Super-Kamiokande-II,
J.P. Cravens et al.
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D78
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.
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First real time detection of ${}^{7}\text{B}$ solar neutrinos by Borexino,
C. Arpesella et al.
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B658
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Measurement of the $\nu_e$ and Total ${}^{8}\text{B}$ Solar Neutrino Fluxes with the Sudbury Neutrino Observatory Phase I Data Set,
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C75
arXiv:nucl-ex/0610020.
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A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory,
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653
arXiv:hep-ex/0607010.
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Search for electron antineutrino interactions with the Borexino Counting Test Facility at Gran Sasso,
M. Balata et al.
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C47
arXiv:hep-ex/0602027.
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The SAGE@LNGS experiment: Measurement of solar neutrinos at LNGS using gallium from SAGE,
J. N. Abdurashitov et al.,
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arXiv:nucl-ex/0509031.
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Solar neutrino measurements in Super-Kamiokande-I,
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D73
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A Search for Periodicities in the $^8\text{B}$ Solar Neutrino Flux Measured by the Sudbury Neutrino Observatory,
B. Aharmim et al.
(SNO),
D72
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.
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Complete results for five years of GNO solar neutrino observations,
M. Altmann et al.
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B616
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C72
arXiv:nucl-ex/0502021.
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Electron Antineutrino Search at the Sudbury Neutrino Observatory,
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D70
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Limit On the Neutrino Magnetic Moment Using 1496 Days of Super-Kamiokande-I Solar Neutrino Data,
D. W. Liu et al.
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arXiv:hep-ex/0402015.
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Precise Measurement of the Solar Neutrino Day/Night and Seasonal Variation in Super-Kamiokande-I,
M. B. Smy et al.
(Super-Kamiokande),
D69
arXiv:hep-ex/0309011.
[Super-Kamiokande:2003yed] - [4-62]
-
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),
92
arXiv:nucl-ex/0309004.
[SNO:2003bmh] - [4-63]
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A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I,
J. Yoo et al.
(Super-Kamiokande),
D68
arXiv:hep-ex/0307070.
[Super-Kamiokande:2003snd] - [4-64]
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Search for $\bar\nu_e$ from the sun at Super-Kamiokande-I,
Y. Gando et al.
(Super-Kamiokande),
90
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.
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Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data,
S. Fukuda et al.
(Super-Kamiokande),
B539
arXiv:hep-ex/0205075.
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-
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),
95
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.
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Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters,
Q. R. Ahmad et al.
(SNO),
89
arXiv:nucl-ex/0204009.
http://www.sno.phy.queensu.ca/sno/results_04_02/DayNight.
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Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory,
Q. R. Ahmad et al.
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89
arXiv:nucl-ex/0204008.
http://www.sno.phy.queensu.ca/sno/results_04_02/NC.
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Search for radiative decays of solar neutrinos during a solar eclipse,
G. Giacomelli, V. Popa,
arXiv:hep-ex/0110013,
[Giacomelli:2001zb] - [4-70]
-
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),
87
arXiv:nucl-ex/0106015.
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Solar $^8\mathrm{B}$ and $hep$ neutrino measurements from 1258 days of Super-Kamiokande data,
S. Fukuda et al.
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86
arXiv:hep-ex/0103032.
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Measurement of the solar neutrino capture rate by SAGE and implications for neutrino oscillations in vacuum,
J. N. Abdurashitov et al.
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83
arXiv:astro-ph/9907131.
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Measurement of the solar neutrino capture rate with gallium metal,
J. N. Abdurashitov et al.
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C60
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GALLEX solar neutrino observations: Results for GALLEX IV,
W. Hampel et al.
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B447
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Measurement of the solar neutrino energy spectrum using neutrino electron scattering,
Y. Fukuda et al.
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82
arXiv:hep-ex/9812011.
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Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super- Kamiokande,
Y. Fukuda et al.
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82
arXiv:hep-ex/9812009.
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Measurements of the solar neutrino flux from Super- Kamiokande's first 300 days,
Y. Fukuda et al.
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81
arXiv:hep-ex/9805021.
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Measurement of the solar electron neutrino flux with the Homestake chlorine detector,
B. T. Cleveland et al.
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496
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Measuring Solar Neutrinos in the SNO+ Detector,
Daniel Cookman,
arXiv:2403.19532,
NuPhys2023.
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The Low Polonium Field of Borexino and its significance for the CNO neutrino detection,
S. Kumaran et al.,
arXiv:2105.13209,
2021 Neutrinos session of the 55th Rencontres de Moriond.
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First detection of CNO neutrinos with Borexino,
G. Settanta et al.,
arXiv:2105.09211,
2021 Neutrinos session of the 55th Rencontres de Moriond.
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Recent results on pp-chain solar neutrinos with the Borexino detector,
Lino Miramonti
(Borexino),
arXiv:1901.09965,
NuPhys2018 (London, 19-21 December 2018).
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Solar Neutrino Physics with Borexino,
A. Pocar et al.
(BOREXINO),
1
arXiv:1810.12967.
15th International Workshop on Tau Lepton Physics (TAU2018): Amsterdam, Netherlands, September 24-28, 2018.
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The Main Results of the Borexino Experiment,
A. Derbin et al.,
arXiv:1605.06795,
Third Annual Large Hadron Collider Physics Conference, St. Petersburg, Russia, 2015.
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Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun,
P. Mosteiro et al.,
265-266
arXiv:1508.05379.
NOW (Neutrino Oscillation Workshop) 2014.
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Solar neutrino with Borexino: results and perspectives,
O. Smirnov et al.
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46
arXiv:1410.0779.
International Workshop on Prospects of Particle Physics, 'Neutrino Physics and Astrophysics', Valday, Russia, January 26 - February 02, 2014.
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Recent Borexino results and prospects for the near future,
D. D'Angelo et al.
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126
arXiv:1405.7919.
Rencontres de Moriond EW 2014.
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Solar Neutrino Results from Super-Kamiokande,
Andrew Renshaw
(Super-Kamiokande),
61
arXiv:1403.4575.
[Renshaw:2014awa] - [5-11]
-
Solar neutrino analysis of Super-Kamiokande,
Hiroyuki Sekiya
(Super-Kamiokande),
arXiv:1307.3686,
33rd International Cosmic Ray Conference, Rio De Janeiro 2013 (ICRC2013).
[Sekiya:2013hda] - [5-12]
-
Solar neutrino physics with Borexino I,
L. Ludhova et al.
(BOREXINO),
arXiv:1205.2989,
Moriond 2012 EW session.
[BOREXINO:2012vbs] - [5-13]
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Low Energy Neutrino Astronomy in Super-Kamiokande,
Michael Smy,
arXiv:1110.0012,
DPF 2011.
[Smy:2011tm] - [5-14]
-
The Recent Results of the Solar Neutrino Measurement in Borexino,
Yusuke Koshio
(Borexino),
arXiv:1106.3055,
Recontres de Moriond EW session 2011.
[Koshio:2011vq] - [5-15]
-
Results from the solar neutrino experiment BOREXINO,
Lothar Oberauer
(Borexino),
203
[Oberauer:2010zz] - [5-16]
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Solar neutrino results from Borexino and main future perspectives,
M. Pallavicini
(Borexino),
A630
arXiv:0910.3367.
RICAP 2009.
[Pallavicini:2009ph] - [5-17]
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Solar Neutrino Measurement at SK-III,
B.S. Yang
(Super-Kamiokande),
arXiv:0909.5469,
DPF-2009, Detroit, MI, July 2009.
[Yang:2009hp] - [5-18]
-
Searching for hep Neutrinos using the Sudbury Neutrino Observatory,
Chris Howard
(SNO),
arXiv:0906.0040,
[Howard:2009uz] - [5-19]
-
Results from the Neutral Current Detector phase of the Sudbury Neutrino Observatory,
Ryan Martin
(SNO),
arXiv:0905.4907,
Lake Louise Winter Institute 2009.
[Martin:2009pb] - [5-20]
-
Results from the Borexino Experiment,
Timo Lewke
(Borexino),
arXiv:0905.2526,
Moriond 2009 EW session.
[Lewke:2009ry] - [5-21]
-
The first year of Borexino,
Borexino
(Borexino),
arXiv:0905.1044,
Heavy Quarks and Leptons, Melbourne, 2008.
[Borexino:2009awt] - [5-22]
-
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,
ICHEP08.
[Jamieson:2008wd] - [5-23]
-
Recent Results from Super-Kamiokande,
H. Sekiya et al.
(Super-Kamiokande),
arXiv:0810.0595,
ICHEP08, Philadelphia, USA, July 2008.
[Sekiya:2008nb] - [5-24]
-
Results and perspectives of the solar neutrino experiment Borexino,
G. Ranucci
(Borexino),
arXiv:0810.0176,
ICHEP08, Philadelphia, USA, July 2008.
[Borexino:2008omw] - [5-25]
-
Search for possible solar neutrino radiative decays during total solar eclipses,
S. Cecchini et al.,
arXiv:hep-ex/0606037,
SPSE2006, Waw an Namos, Libya, 27-29 March 2006.
[Cecchini:2006fz] - [5-26]
-
Integral Fluxes, Day-Night, and Spectrum Results from SNO's 391-Day Salt Phase,
Juergen Wendland et al.
(SNO),
arXiv:hep-ex/0507058,
Lake Louise Winter Institute: Fundamental Interactions, Lake Louise, Alberta, Canada, Feb 20-26 2005.
[Wendland:2005kj] - [5-27]
-
Results from the Salt Phase of SNO,
K. Miknaitis
(SNO),
arXiv:hep-ex/0505071,
XXXXth Rencontres de Moriond: Electroweak Interactions and Unified Theories, La Thuile, Italy, March 5-12, 2005.
[Miknaitis:2005rw] - [5-28]
-
Measurement of the SAGE Response to Neutrinos from Ar37 Source,
V.N. Gavrin
(SAGE),
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] - [5-29]
-
Sudbury Neutrino Observatory Results,
A.B. McDonald et al.
(SNO),
T121
arXiv:hep-ex/0412060.
Nobel Symposium 129, August 19-24, 2004, Enkoping, Sweden.
[McDonald:2004rx] - [5-30]
-
Super Kamiokande results: atmospheric and solar neutrinos,
M.Ishitsuka
(Super-Kamiokande),
arXiv:hep-ex/0406076,
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] - [5-31]
-
High Sensitivity Anti-Neutrino Detection by KamLAND,
S. Hatakeyama et al.
(KamLAND),
arXiv:hep-ex/0405001,
Moriond EW04.
[Hatakeyama:2004gm] - [5-32]
-
Search for neutrino radiative decays during a total solar eclipse,
V. Popa,
AHEP2003
arXiv:hep-ex/0402014.
AHEP2003, Valencia.
[Popa:2003mjo] - [5-33]
-
Results from radiochemical solar neutrino experiments,
C. Cattadori,
Neutrino 2004, 13-19 June 2004, Paris, France.
http://neutrino2004.in2p3.fr/slides/monday/cattadori.ppt.
[Cattadori-Nu2004] - [5-34]
-
KamLAND: updated results,
K. Inoue,
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] - [5-35]
-
SuperKamiokande's solar neutrino results,
M. Nakahata
(Super-Kamiokande),
Neutrino 2004, 13-19 June 2004, Paris, France.
http://neutrino2004.in2p3.fr/slides/monday/nakahata.pdf.
[Nakahata-Nu2004] - [5-36]
-
The Sudbury Neutrino Observatory,
J. Wilkerson
(SNO),
Neutrino 2004, 13-19 June 2004, Paris, France.
http://neutrino2004.in2p3.fr/slides/monday/wilkerson.pdf.
[Wilkerson-Nu2004] - [5-37]
-
Recent Results from the Sudbury Neutrino Observatory,
A. W. P. Poon
(SNO),
C33
arXiv:hep-ex/0312002.
International Europhysics Conference on High Energy Physics (EPS2003).
[Poon:2003xx] - [5-38]
-
Recent Results from KamLAND,
J. Detwiler
(KamLAND),
C0307282
arXiv:hep-ex/0311007.
SLAC Summer Institute, July 2003.
[Detwiler:2003fb] - [5-39]
-
The Solar Neutrino Day/Night Effect in Super-Kamiokande,
M. B. Smy
(Super-Kamiokande),
138
arXiv:hep-ex/0310064.
TAUP 2003.
[Smy:2003sb] - [5-40]
-
Latest News from SNO,
K. Graham
(SNO),
C030626
arXiv:hep-ex/0310039.
XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Graham:2003pu] - [5-41]
-
A study of short-time periodic variation of the B8 solar neutrino flux at Super-Kamiokande,
J. Yoo
(Super-Kamiokande),
C030626
arXiv:hep-ex/0309048.
XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Yoo:2003ky] - [5-42]
-
KamLAND results,
K. Inoue
(Kamland),
arXiv:hep-ex/0307030,
XXXVIIIth Recontres de Moriond Electroweak Interactions and Unified Theories.
[Inoue:2003qs] - [5-43]
-
The recent results of solar neutrino measurements in Super-Kamiokande,
Y. Koshio
(Super-Kamiokande),
arXiv:hep-ex/0306002,
XXXVIIIth Recontres de Moriond Electroweak Interactions and Unified Theories.
[Koshio:2003py] - [5-44]
-
The Gallium Neutrino Observatory (GNO),
E. Bellotti
(GNO),
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] - [5-45]
-
KamLAND Results,
K. Inoue
(Kamland),
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] - [5-46]
-
Results from SNO and Other Solar Neutrino Experiments,
R. Robertson,
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] - [5-47]
-
Solar Neutrino Observations at the Sudbury Neutrino Observatory,
A. W. P. Poon
(SNO),
C020805
arXiv:hep-ex/0211013.
SLAC Summer Institute Topical Conference (SSI02-TTh01), 2002.
[SNO:2002fbv] - [5-48]
-
Solar Neutrinos,
A. B. McDonald,
C020620
arXiv:hep-ex/0209056.
Physics in Collision Conference, Stanford, California, June, 2002.
[McDonald:2002fx] - [5-49]
-
Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data,
M. B. Smy
(Super-Kamiokande),
118
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] - [5-50]
-
Five Years of Neutrino Physics with Super-Kamiokande,
M. B. Smy
(Super-Kamiokande),
arXiv:hep-ex/0206016,
XXXVII Rencontres de Moriond: Electroweak Interactions and Unified Theories.
[Smy:2002hr] - [5-51]
-
An update on progress at KamLAND,
S. A. Dazeley
(KamLAND),
arXiv:hep-ex/0205041,
[Dazeley:2002yf] - [5-52]
-
First Results from KamLAND: Evidence for $\bar{\nu}_e$ disappearance,
G. Gratta
(Kamland),
SLAC Colloquium, December 2002.
http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.
[Gratta:SLAC2002] - [5-53]
-
The Sudbury Neutrino Observatory,
A. Hallin
(SNO),
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] - [5-54]
-
KamLAND: Examination of the LMA solution with reactor neutrinos,
A. Suzuki
(Kamland),
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]
- [6-1]
-
Deep Probabilistic Direction Prediction in 3D with Applications to Directional Dark Matter Detectors,
Majd Ghrear, Peter Sadowski, Sven Einar Vahsen,
arXiv:2403.15949,
[Ghrear:2024rku] - [6-2]
-
Method to Reduce Noise for Measurement of $^7$Be and $^8$B Solar Neutrinos on Gallium-71,
Jonathan Folkerts, Nick Solomey, Brooks Hartsock, Gregory Pawloski,
arXiv:2312.10157,
[Folkerts:2023svx] - [6-3]
-
Discrimination of pp solar neutrinos and $^{14}$C pile-up events in a large scale LS detector,
Guo-Ming Chen, Xin Zhang, Ze-Yuan Yu, Si-Yuan Zhang, Yu Xu, Wen-Jie Wu, Yao-Guang Wang, Yong-Bo Huang,
34
arXiv:2303.08512.
[Chen:2023xhj] - [6-4]
-
Slow-Fluor Scintillator for Low Energy Solar Neutrinos and Neutrinoless Double Beta Decay,
Jack Dunger, Edward J. Leming, Steven D. Biller,
105
arXiv:2203.01147.
[Dunger:2022gif] - [6-5]
-
A new method of energy reconstruction for large spherical liquid scintillator detectors,
Wenjie Wu, Miao He, Xiang Zhou, Haoxue Qiao,
14
arXiv:1812.01799.
[Wu:2018zwk] - [6-6]
-
Calibration of liquid argon and neon detectors with $^{83}Kr^m$,
W.H. Lippincott et al.,
C81
arXiv:0911.5453.
[Lippincott:2009ea] - [6-7]
-
Self-Calibration of Neutrino Detectors using characteristic Backgrounds,
Joachim Kopp, Manfred Lindner, Alexander Merle,
A582
arXiv:hep-ph/0703055.
[Kopp:2007us] - [6-8]
-
Reconstruction of Composite Events in Neutrino Telescopes,
Mathieu Ribordy,
A574
arXiv:astro-ph/0611604.
[Ribordy:2006qd] - [6-9]
-
THE ANALYSIS OF RADIOACTIVE DECAY WITH A SMALL NUMBER OF COUNTS BY THE METHOD OF MAXIMUM LIKELIHOOD,
B. T. Cleveland,
214
[Cleveland:1983sd] - [6-10]
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V. A. Kuzmin,
22
[Zh. Eksp. Teor. Fiz. 49 (1965) 1532].
[Kuzmin-Ga-65]
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Study on cosmogenic activation in germanium detectors for future tonne-scale CDEX experiment,
J. L. Ma et al.,
62
arXiv:1802.09327.
[Ma:2018tdv] - [7-2]
-
Study of the Production of Radioactive Isotopes through Cosmic Muon Spallation in KamLAND,
S. Abe et al.
(KamLAND),
C81
arXiv:0907.0066.
[KamLAND:2009zwo]
- [8-1]
-
Status of Direct Determination of Solar Neutrino Fluxes after Borexino,
M. C. Gonzalez-Garcia, Michele Maltoni, Joao Paulo Pinheiro, Aldo M. Serenelli,
02
arXiv:2311.16226.
[Gonzalez-Garcia:2023kva] - [8-2]
-
Solar models with convective overshoot, the solar-wind mass loss, and a PMS disk accretion: helioseismic quantities, Li depletion and neutrino fluxes,
Qian-Sheng Zhang, Yan Li, Jorgen Christensen-Dalsgaard,
arXiv:1907.02166,
[Zhang:2019xxs] - [8-3]
-
The effects of a revised $^7$Be e$^-$-capture rate on solar neutrino fluxes,
D. Vescovi, L. Piersanti, S. Cristallo, M. Busso, F. Vissani, S. Palmerini, S. Simonucci, S. Taioli,
623
arXiv:1902.01826.
[Vescovi:2019vjd] - [8-4]
-
Solar neutrinos at keV energies: thermal flux,
Edoardo Vitagliano, Javier Redondo, Georg Raffelt,
1342
arXiv:1709.02811.
[Vitagliano:2017ona] - [8-5]
-
A new Generation of Standard Solar Models,
Nuria Vinyoles et al.,
835
arXiv:1611.09867.
[Vinyoles:2016djt] - [8-6]
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Solar models with new low-metal abundances,
Wuming Yang,
arXiv:1603.01666,
[1603.01666] - [8-7]
-
Generalised form factor dark matter in the Sun,
Aaron C. Vincent, Aldo Serenelli, Pat Scott,
1508
arXiv:1504.04378.
[Vincent:2015gqa] - [8-8]
-
Astrophysical implications of the proton-proton cross section updates,
E. Tognelli, S. Degl'Innocenti, L. E. Marcucci, P.G. Prada Moroni,
B742
arXiv:1411.5480.
[Tognelli:2014axa] - [8-9]
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The estimation of neutrino flux produced by $\mathbf{pep}$ reactions in the Sun,
B.F. Irgaziev, V.B. Belyaev, Jameel-Un Nabi,
89
arXiv:1408.4532.
[Irgaziev:2014hfa] - [8-10]
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The mixing in the solar core and the neutrino fluxes,
Anatoly Kopylov, Valery Petukhov,
arXiv:1209.3719,
[Kopylov:2012bc] - [8-11]
-
Solar models with accretion. I. Application to the solar abundance problem,
Aldo M. Serenelli, Wick C. Haxton, Carlos Pena-Garay,
743
arXiv:1104.1639.
Comment: SHP11.
[Serenelli:2011py] - [8-12]
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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,
715
arXiv:1004.1657.
[Turck-Chieze:2010fxx] - [8-13]
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New Solar Composition: The Problem With Solar Models Revisited,
Aldo Serenelli, Sarbani Basu, Jason W. Ferguson, Martin Asplund,
705
arXiv:0909.2668.
[Serenelli:2009yc] - [8-14]
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Solar neutrinos and the solar composition problem,
Carlos Pena-Garay, Aldo Serenelli,
arXiv:0811.2424,
[Pena-Garay:2008cyw] - [8-15]
-
10,000 Standard Solar Models: a Monte Carlo Simulation,
John N. Bahcall, Aldo M. Serenelli, Sarbani Basu,
165
arXiv:astro-ph/0511337.
[Bahcall:2005va] - [8-16]
-
What Is The Neon Abundance Of The Sun?,
John N. Bahcall, Sarbani Basu, Aldo M. Serenelli,
631
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] - [8-17]
-
New solar opacities, abundances, helioseismology, and neutrino fluxes,
John N. Bahcall, Aldo M. Serenelli, Sarbani Basu,
621
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] - [8-18]
-
How do Uncertainties in the Surface Chemical Abundances of the Sun Affect the Predicted Solar Neutrino Fluxes?,
John N. Bahcall, Aldo M. Serenelli,
626
arXiv:astro-ph/0412096.
[Bahcall:2004mq] - [8-19]
-
Surprising Sun,
S. Turck-Chieze et al.,
93
arXiv:astro-ph/0407176.
[Turck-Chieze:2004jqb] - [8-20]
-
What do we (not) know theoretically about solar neutrino fluxes?,
John N. Bahcall, M. H. Pinsonneault,
92
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] - [8-21]
-
Solar seismic models and the neutrino predictions,
S. Couvidat, Sylvaine Turck-Chieze, A.G. Kosovichev,
599
[Couvidat:2002gvk] - [8-22]
-
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,
583
arXiv:astro-ph/0210127.
[Boothroyd:2002qw] - [8-23]
-
Solar models: Current epoch and time dependences, neutrinos, and helioseismological properties,
J. N. Bahcall, M. H. Pinsonneault, S. Basu,
555
arXiv:astro-ph/0010346.
Comment: BP00.
[Bahcall:2000nu] - [8-24]
-
How uncertain are solar neutrino predictions?,
J. N. Bahcall, S. Basu, M. H. Pinsonneault,
B433
arXiv:astro-ph/9805135.
Comment: BP98.
[Bahcall:1998wm] - [8-25]
-
Gallium solar neutrino experiments: Absorption cross sections, neutrino spectra, and predicted event rates,
John N. Bahcall,
C56
arXiv:hep-ph/9710491.
[Bahcall:1997eg] - [8-26]
-
Are standard solar models reliable?,
J. N. Bahcall, M. H. Pinsonneault, S. Basu, J. Christensen-Dalsgaard,
78
arXiv:astro-ph/9610250.
[Bahcall:1996qw] - [8-27]
-
Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes,
N. Itoh, H. Hayashi, A. Nishikawa, Y. Kohyama,
102
[1996ApJS..102..411I] - [8-28]
-
Solar models with helium and heavy element diffusion,
J. N. Bahcall, M. H. Pinsonneault,
67
arXiv:hep-ph/9505425.
Comment: BP95.
[Bahcall:1995bt] - [8-29]
-
The Be-7 solar neutrino line: A Reflection of the central temperature distribution of the sun,
J. N. Bahcall,
D49
[Bahcall:1994cf] - [8-30]
-
Toward a unified classical model of the sun: On the sensitivity of neutrinos and helioseismology to the microscopic physics,
S. Turck-Chieze, I. Lopes,
408
[Turck-Chieze:1993dw] - [8-31]
-
Standard solar models, with and without helium diffusion and the solar neutrino problem,
J. N. Bahcall, M. H. Pinsonneault,
64
Comment: BP92.
[Bahcall:1992hn] - [8-32]
-
Solar models, neutrino experiments and helioseismology,
J. N. Bahcall, Roger K. Ulrich,
60
Comment: BU88.
[Bahcall:1988jc] - [8-33]
-
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,
54
[Bahcall:1982zh] - [8-34]
-
Present status of the theoretical predictions for the Cl-36 solar neutrino experiment,
John N. Bahcall, Neta A. Bahcall, G. Shaviv,
20
[Bahcall:1968hc] - [8-35]
-
Solar neutrinos. I: Theoretical,
J. N. Bahcall,
12
[Bahcall:1964gx] - [8-36]
-
J. N. Bahcall, W. A. Fowler, I. Iben, R. L. Sears,
137
[Bahcall-63] - [8-37]
-
E. M. Burbidge, G. R Burbidge, W. A. Fowler, F. Hoyle,
29
[Burbidge-Burbidge-Fowler-Hoyle-RMP-29-547-1957] - [8-38]
-
Nuclear Reactions in Stars and Nucleogenesis,
A. G. W. Cameron,
69
[Cameron-PASP-69-201-1957] - [8-39]
-
Energy Production in Stars,
H. A. Bethe,
55
[Bethe-PR-55-434-1939]
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New Results on Standard Solar Models,
Aldo M. Serenelli,
328
arXiv:0910.3690.
Synergies between solar and stellar modelling, Rome, June 2009.
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Progress report on solar age calibration,
G. Houdek, D.O. Gough,
A78
arXiv:0807.3443.
The Art of Modelling Stars in the 21st Century, Proc. IAU Symp. No. 252.
[Houdek:2008rw] - [9-3]
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Solar Models and Solar Neutrinos,
John N. Bahcall,
C030626
arXiv:astro-ph/0310030.
XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Bahcall:2003jg]
- [10-1]
-
In-depth analysis of solar models with high-metallicity abundances and updated opacity tables,
G. Buldgen et al.,
arXiv:2404.10478,
[Buldgen:2024aak] - [10-2]
-
Higher metal abundances do not solve the solar problem,
G. Buldgen, P. Eggenberger, A. Noels, R. Scuflaire, A. M. Amarsi, N. Grevesse, S. Salmon,
669
arXiv:2212.06473.
[Buldgen:2022nso] - [10-3]
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Rotating Solar Models in Agreement with Helioseismic Results and Updated Neutrino Fluxes,
Wuming Yang,
939
arXiv:2209.13483.
[Yang:2022dsq] - [10-4]
-
Theoretical evaluation of solar proton-proton fusion reaction rate and its uncertainties,
Hilla De-Leon, Doron Gazit,
844
arXiv:2207.10176.
[De-Leon:2022omx] - [10-5]
-
Core overshoot constrained by the absence of a solar convective core and some solar-like stars,
Qian-Sheng Zhang, Jorgen Christensen-Dalsgaard, Yan Li,
arXiv:2203.08686,
[2203.08686] - [10-6]
-
Observational constraints on the origin of the elements. IV: The standard composition of the Sun,
Ekaterina Magg, Maria Bergemann, Aldo Serenelli, Manuel Bautista, Bertrand Plez, Ulrike Heiter, Jeffrey M. Gerber, Hans-Gunter Ludwig, Sarbani Basu, Jason W. Ferguson, Helena Carvajal Gallego, Sebastien Gamrath, Patrick Palmeri, Pascal Quinet,
arXiv:2203.02255,
[2203.02255] - [10-7]
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Search for solar atmospheric neutrinos with the ANTARES neutrino telescope,
A. Albert et al.
(ANTARES),
06
arXiv:2201.11642.
[ANTARES:2022azv] - [10-8]
-
667
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Standard solar models: a perspective from updated solar neutrino fluxes and the gravity-mode period spacing,
Sebastien Salmon, Gael Buldgen, Arlette Noels, Patrick Eggenberger, Richard Scuflaire, Georges Meynet,
651
arXiv:2105.00911.
[Salmon:2021rar] - [10-10]
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The impact of composition choices on solar evolution: age, helio- and asteroseismology, and neutrinos,
Diogo Capelo, Ilidio Lopes,
498
arXiv:2010.01686.
[Capelo:2020lha] - [10-11]
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On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram,
Ebraheem Farag, F.X. Timmes, Morgan Taylor, Kelly M. Patton, R. Farmer,
893
arXiv:2003.05844.
[Farag:2020nll] - [10-12]
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Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances,
Wuming Yang,
873
arXiv:1901.11290.
[Yang:2019jip] - [10-13]
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Astrophysical S-factor of the $^{14}\textrm{N(p,}\gamma\textrm{)}^{15}\textrm{O}$ reaction at 0.4 - 1.3\,MeV,
L. Wagner et al.,
C97
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[Wagner:2017vpz] - [10-14]
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Potential approach to astrophysical $^{3}{\rm He}(\alpha, \gamma)^{7}{\rm Be}$ and $^{3}{\rm H}(\alpha,\gamma)^{7}{\rm Li}$ direct capture reactions,
E.M. Tursunov, S.A. Turakulov, A.S. Kadyrov,
C97
arXiv:1707.05948.
[Tursunov:2017zlg] - [10-15]
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The effect of ionic correlations on radiative properties in the solar interior and terrestrial experiments,
Menahem Krief, Yair Kurzweil, Alexander Feigel, Doron Gazit,
856
arXiv:1611.09339.
[Krief:2016vyp] - [10-16]
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Magnetic helicity estimations in models and observations of the solar magnetic field. Part I: Finite volume methods,
Gherardo Valori et al.,
arXiv:1610.02193,
[1610.02193] - [10-17]
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Bayesian Estimation of Thermonuclear Reaction Rates,
Christian Iliadis, Kevin Anderson, Alain Coc, Frank Timmes, Sumner Starrfield,
831
arXiv:1608.05853.
[Iliadis:2016vkw] - [10-18]
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Reconstruction of Solar Subsurfaces by Local Helioseismology,
Alexander G. Kosovichev, Junwei Zhao,
arXiv:1607.05681,
[1607.05681] - [10-19]
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Model description of non-Maxwellian nuclear processes in the solar interior,
Victor T. Voronchev, Yasuyuki Nakao, Yukinobu Watanabe,
arXiv:1606.00612,
[1606.00612] - [10-20]
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Implications of solar wind measurements for solar models and composition,
Aldo Serenelli et al.,
463
arXiv:1604.05318.
[Serenelli:2016nms] - [10-21]
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A successful solar model using new solar composition data,
Sunny Vagnozzi, Katherine Freese, Thomas H. Zurbuchen,
839
arXiv:1603.05960.
[Vagnozzi:2016cmr] - [10-22]
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Line broadening and the solar opacity problem,
M. Krief, A. Feigel, D. Gazit,
arXiv:1603.01153,
[1603.01153] - [10-23]
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Sunspot Numbers from ISOON: A Ten-Year Data Analysis,
K. S. Balasubramaniam, T. W. Henry,
arXiv:1602.07741,
[1602.07741] - [10-24]
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Chameleon fields and solar physics,
Andrea Zanzi, Barbara Ricci,
A30
arXiv:1405.1581.
[Zanzi:2014aia] - [10-25]
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The chemical composition of the Sun from helioseismic and solar neutrino data,
F.L. Villante, A.M. Serenelli, F. Delahaye, M.H. Pinsonneault,
787
arXiv:1312.3885.
[Villante:2013mba] - [10-26]
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Planetary influence on the young Sun's evolution: the solar neutrino probe,
Ilidio Lopes, Joseph Silk,
435
arXiv:1309.7571.
[Lopes:2013iia] - [10-27]
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What have we learned from helioseismology, what have we really learned, and what do we aspire to learn?,
Douglas Gough,
287
arXiv:1210.0820.
[Gough:2012tb] - [10-28]
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Analytical results connecting stellar structure parameters and extended reaction rates,
H.J. Haubold, D. Kumar,
2014
arXiv:1109.5613.
[Haubold:2011kk] - [10-29]
-
The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos,
Sylvaine Turck-Chieze, Laurent Piau, Sebastien Couvidat,
731
arXiv:1103.2620.
[Turck-Chieze:2011iru] - [10-30]
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Radioactivities in Low- and Intermediate-Mass Stars,
Maria Lugaro, Alessandro Chieffi,
218
arXiv:1010.1304.
[Lugaro:2010ia] - [10-31]
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The Extreme Energies Lines in the Solar Neutrino Spectrum,
B.I. Goryachev,
arXiv:1005.3458,
[Goryachev:2010am] - [10-32]
-
Fresh insights on the structure of the solar core,
Sarbani Basu, William J. Chaplim, Yvonne Elsworth, Roger New, Aldo M. Serenelli,
699
arXiv:0905.0651.
[Basu:2009mi] - [10-33]
-
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,
490
arXiv:0808.0422.
[Lefebvre:2008am] - [10-34]
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Bayesian Analysis of Solar Oscillations,
M. S. Marsh, J. Ireland, T. Kucera,
681
arXiv:0804.1447.
[Marsh:2008qm] - [10-36]
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Update on g-mode research,
R.A. Garcia et al.,
329
arXiv:0802.4296.
[Garcia:2008mi] - [10-37]
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Are solar cycles predictable?,
Manfred Schuessler,
328
arXiv:0712.1917.
[Schuessler:2007rq] - [10-38]
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The energy of high frequency waves in the low solar Chromosphere,
Aleksandra Andic,
242
arXiv:astro-ph/0703721.
[Andic:2007wy] - [10-39]
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Modeling the (upper) solar atmosphere including the magnetic field,
H. Peter,
39
arXiv:astro-ph/0703575.
[Peter:2007yx] - [10-40]
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The solar oxygen crisis: Probably not the last word,
H. Socas-Navarro, A. A. Norton,
arXiv:astro-ph/0702162.
[Socas-Norton:2007fbo] - [10-41]
-
Probing the internal solar magnetic field through g-modes,
Timur I. Rashba, V. B. Semikoz, S. Turck-Chieze, J. W. F. Valle,
377
arXiv:astro-ph/0611728.
[Rashba:2006jp] - [10-42]
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Low abundances of heavy elements in the solar outer layers: comparisons of solar models with helioseismic inversions,
M. Castro, S. Vauclair, O. Richard,
463
arXiv:astro-ph/0611619.
[Castro:2006qu] - [10-43]
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Solar Atmospheric Oscillations and the Chromospheric Magnetic Topology,
A. Vecchio et al.,
461
arXiv:astro-ph/0611206.
[Vecchio:2006yi] - [10-44]
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Origin of solar torsional oscillations,
Matthias Rempel,
655
arXiv:astro-ph/0610221.
[Rempel:2006zu] - [10-45]
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Solar abundances and helioseismology: fine structure spacings and separation ratios of low-degree p modes,
Sarbani Basu et al.,
655
arXiv:astro-ph/0610052.
To appear in ApJ.
[Basu:2006vh] - [10-46]
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Local helioseismology and correlation tracking analysis of surface structures in realistic simulations of solar convection,
Dali Georgobiani et al.,
657
arXiv:astro-ph/0608204.
[Georgobiani:2006ty] - [10-47]
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Damping and excitation variations of the solar acoustic modes using LOWL observations,
D. Salabert, S.J. Jiménez-Reyes,
650
arXiv:astro-ph/0607346.
[Salabert:2006td] - [10-48]
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A Comparative Study on Lithium Abundances in Solar-Type Stars With and Without Planets,
Y. Q. Chen, G. Zhao,
131
arXiv:astro-ph/0607295.
[Chen:2006fr] - [10-49]
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Neon Abundances in B-Stars of the Orion Association: Solving the Solar Model Problem?,
Katia Cunha, Ivan Hubeny, Thierry Lanz,
647
arXiv:astro-ph/0606738.
[Cunha:2006jf] - [10-50]
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Long-term Variability in the Length of the Solar Cycle,
Michael L. Rogers, Mercedes T. Richards, Donald St.P. Richards,
arXiv:astro-ph/0606426,
[Rogers:2006bg] - [10-51]
-
Can Galactic Cosmic Rays Account for Solar 6Li Without Overproducing Gamma Rays?,
T. Prodanovic, B. D. Fields,
645
arXiv:astro-ph/0605675.
[Prodanovic:2006fm] - [10-52]
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The Sun's Interior Metallicity Constrained by Neutrinos,
Guillermo Gonzalez,
370
arXiv:astro-ph/0605647.
[Gonzalez:2006zd] - [10-53]
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Determining solar abundances using helioseismology,
H.M. Antia, Sarbani Basu,
644
arXiv:astro-ph/0603001.
[Antia:2006zy] - [10-54]
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Total Solar Irradiance Variability and the Solar Activity Cycle,
Probhas Raychaudhuri,
arXiv:astro-ph/0601335,
[Raychaudhuri:2006zc] - [10-55]
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The Solar Heavy Element Abundances: I. Constraints from Stellar Interiors,
Franck Delahaye, Marc Pinsonneault,
649
arXiv:astro-ph/0511779.
[Delahaye:2005ed] - [10-56]
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Angular Momentum Transport by Gravity Waves in the Solar Interior,
Tamara M. Rogers, Gary A. Glatzmaier,
653
arXiv:astro-ph/0511739.
[Rogers:2005yz] - [10-57]
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Radiative zone solar magnetic fields and g-modes,
Timur I. Rashba, V. B. Semikoz, J. W. F. Valle,
370
arXiv:astro-ph/0511708.
[Rashba:2005uj] - [10-59]
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The solar model problem resurrected,
M. Asplund, N. Grevesse, M. Guedel, A.J. Sauval,
436
arXiv:astro-ph/0510377.
[Asplund:2005js] - [10-60]
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The Ne/O abundance ratio in the quiet Sun,
P.R. Young,
arXiv:astro-ph/0510264.
[Young:2005ke] - [10-61]
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Neon Lights Up a Controversy: the Solar Ne/O Abundance,
J.T. Schmelz et al.,
634
arXiv:astro-ph/0510230.
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Solar Neutron Events of October-November 2003,
K. Watanabe et al.,
636
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[Watanabe:2005pd] - [10-63]
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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,
361
arXiv:astro-ph/0506286.
[Monteiro:2005cb] - [10-64]
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The Solar Model Problem Solved by the Abundance of Neon in Stars of the Local Cosmos,
Jeremy J. Drake Paola Testa, Paola Testa,
436
arXiv:astro-ph/0506182.
[Drake:2005hn] - [10-65]
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Can Enhanced Diffusion Improve Helioseismic Agreement for Solar Models with Revised Abundances?,
J. Guzik, L. S. Watson, A. Cox,
627
arXiv:astro-ph/0502364.
[Guzik:2005db] - [10-66]
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The discrepancy between solar abundances and helioseismology,
H. M. Antia, Sarbani Basu,
620
arXiv:astro-ph/0501129.
[Antia:2005mg] - [10-67]
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Does solar structure vary with solar magnetic activity?,
Sarbani Basu, Anna Mandel,
617
arXiv:astro-ph/0411427.
[Basu:2004kq] - [10-68]
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Helioseismological Implications of Recent Solar Abundance Determinations,
John N. Bahcall, Sarbani Basu, Marc Pinsonneault, Aldo M. Serenelli,
618
arXiv:astro-ph/0407060.
[Bahcall:2004yr] - [10-69]
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Determination of S17(0) from published data,
R. H. Cyburt, B. Davids, B. K. Jennings,
C70
arXiv:nucl-th/0406011.
[Cyburt:2004jp] - [10-70]
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How Accurately Can We Calculate the Depth of the Solar Convective Zone?,
John N. Bahcall, Aldo M. Serenelli, Marc Pinsonneault,
614
arXiv:astro-ph/0403604.
[Bahcall:2004aq] - [10-71]
-
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,
B590
arXiv:astro-ph/0312559.
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How Accurately Do We Know the Formation of Solar 8B?,
Moshe Gai,
arXiv:nucl-ex/0312003,
[Gai:2003ef] - [10-73]
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On Solar Radius Variation with Magnetic Field,
A. R. Choudhuri, P. Chatterjee,
arXiv:astro-ph/0311028,
[Choudhuri:2003we] - [10-74]
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A Millennium Scale Sunspot Number Reconstruction: Evidence For an Unusually Active Sun Since the 1940's,
I. G. Usoskin et al.,
91
arXiv:astro-ph/0310823.
[Usoskin:2003au] - [10-75]
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Helioseismic Probing of Solar Variability: The Formalism and Simple Assessments,
W.A. Dziembowski, P.R. Goode,
600
arXiv:astro-ph/0310095.
[Dziembowski:2003vb] - [10-76]
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Towards a Solution to the Early Faint Sun Paradox: A Lower Cosmic Ray Flux from a Stronger Solar Wind,
N. J. Shaviv,
A108
arXiv:astro-ph/0306477.
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Precise measurement of cross section of 3He(3He,2p)4He by using He-3 doubly charged beam,
Nobuyuki Kudomi et al.,
C69
arXiv:astro-ph/0306454.
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Resonant origin for density fluctuations deep within the Sun: helioseismology and magneto-gravity waves,
C. P. Burgess et al.,
348
arXiv:astro-ph/0304462.
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Bounds on the Magnetic Fields in the Radiative Zone of the Sun,
Alexander Friedland, Andrei Gruzinov,
601
arXiv:astro-ph/0211377.
[Friedland:2002is] - [10-80]
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Possible in situ Tests of the Evolution of Elemental and Isotopic Abundances in the Solar Convection Zone,
S. Turcotte, R. F. Wimmer-Schweingruber,
A107
arXiv:astro-ph/0210219.
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Our Sun. V. A Bright Young Sun Consistent with Helioseismology and Warm Temperatures on Ancient Earth and Mars,
I.-J. Sackmann, A. I. Boothroyd,
583
arXiv:astro-ph/0210128.
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Screened thermonuclear reactions in astrophysical plasmas: Improving Salpeter's and Mitler's models,
Theodore E. Liolios,
A18
arXiv:nucl-th/0210031.
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The State Be7 in the Core of the Sun and the Solar Neutrino Flux,
G. Shaviv N. J. Shaviv,
341
arXiv:astro-ph/0209253.
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Constraints on proton-proton fusion from helioseismology,
D.B. Guenther K.I.T. Brown, M.N. Butler,
arXiv:nucl-th/0207008,
[Brown:2002ih] - [10-85]
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Seismic test of solar models, solar neutrinos and implications for metal-rich accretion,
R. A. Winnick, Pierre Demarque, Sarbani Basu, D. B. Guenther,
576
arXiv:astro-ph/0111096.
[Winnick:2001uc] - [10-86]
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A possible solution to the solar neutrino problem: Relativistic corrections to the Maxwellian velocity distribution,
Jian-Miin Liu,
arXiv:physics/0110002,
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Velocity distribution of high-energy particles and the solar neutrino problem,
Jian-Miin Liu,
arXiv:astro-ph/0108304,
[Liu:2001rm] - [10-88]
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J. N. Bahcall,
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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,
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Influence of protons on the capture of electrons by the nuclei of 7Be in the Sun,
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Scattering of $^{7}\text{Be}$ and $^{8}\text{B}$ and the astrophysical $S_{17}$ factor,
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Is There a Significant Difference Between the Results of the Coulomb Dissociation of 8B and the Direct Capture 7Be(p,g)8B Reaction?,
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C74
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Astrophysical $S_{17}(0)$ factor from a measurement of $d({}^{7}\text{Be},{}^{8}\text{B})n$ reaction at $E_{c.m.} = 4.5 MeV$,
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The ${}^{8}\text{B}$ neutrino spectrum,
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Determination of $S_{17}(0)$ from published data,
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Precise measurement of the $^7\mathrm{Be}(p,gamma)^8\mathrm{B}$ S-factor,
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Precise measurement of cross section of 3He(3He,2p)4He by using He-3 doubly charged beam,
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Electromagnetic dissociation of ${}^{8}\text{B}$ and the astrophysical $S$ factor for ${}^{7}\text{Be}(p,gamma){}^{8}\text{B}$,
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C68
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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 [8-23] $S_{17}(0) = 19 {}^{+2.7}_{-1.3} \, \text{eV} \, \text{b}$ (see [25-1]), taken from [2-81].
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The solar neutrino problem: Low energy measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ cross section,
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Indirect measurements of the solar neutrino production reaction ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$,
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Precision measurements of the ${}^7\mathrm{Be}(p,\gamma){}^8\mathrm{B}$ reaction with radioactive beams and the $^8\mathrm{B}$ solar neutrino flux,
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Constraining electron number density in the Sun via Earth-based neutrino flavor data,
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Generalized Lomb-Scargle Analysis of 22 years of Super-Kamiokande solar $^8$B neutrino data,
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Light vector mediators at direct detection experiments,
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The Sun and core-collapse supernovae are leading probes of the neutrino lifetime,
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Exploring Solar Neutrino Oscillation Parameters with LCS at Yemilab and JUNO,
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Statistically improved Analysis of Neutrino Oscillation Data with the latest KamLAND result,
P. Aliani, V. Antonelli M. Picariello, E. Torrente-Lujan,
arXiv:hep-ph/0511071,
[Aliani:2005se] - [16-248]
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Likelihood scan of the Super-Kamiokande I time series data,
Gioacchino Ranucci,
D73
arXiv:hep-ph/0511026.
[Ranucci:2005ep] - [16-249]
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$^7$Be Neutrino Signal Variation in KamLAND,
Bhag C. Chauhan,
0602
arXiv:hep-ph/0510415.
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Solving Solar Neutrino Puzzle via LMA MSW Conversion,
Q. Y. Liu et al.,
44
arXiv:hep-ph/0509182.
[Liu:2005rh] - [16-251]
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An approximate solution for solar and supernova neutrino oscillation in matter,
Rui Luo,
arXiv:hep-ph/0506020,
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-
Do solar neutrinos probe neutrino electromagnetic properties?,
Alexander Friedland,
arXiv:hep-ph/0505165,
[Friedland:2005xh] - [16-253]
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Time Series Analysis Methods Applied to the Super-Kamiokande I Data,
Gioacchino Ranucci,
arXiv:hep-ph/0505062,
[Ranucci:2005jr] - [16-254]
-
Coherent lunar effect on solar neutrino,
K. Ishikawa, T. Shimomura,
arXiv:hep-ph/0505057,
[Ishikawa:2005jk] - [16-255]
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Constraints on Weakly Mixed Sterile Neutrinos in the Light of SNO Salt Phase and 766.3 Ty KamLAND Data,
S. Dev, Sanjeev Kumar,
A20
arXiv:hep-ph/0504237.
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Random magnetic fields inducing solar neutrino spin-flavor precession in a three generation context,
M. M. Guzzo, P. C. de Holanda, O. L. G. Peres,
D72
arXiv:hep-ph/0504185.
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Low Energy Solar Neutrinos and Spin Flavour Precession,
Bhag C. Chauhan, Joao Pulido, R. S. Raghavan,
0507
arXiv:hep-ph/0504069.
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Do two flavour oscillations explain both KamLAND data and the Solar Neutrino Spectrum?,
Bipin Singh Koranga, Mohan Narayan, S. Uma Sankar,
50
arXiv:hep-ph/0503092.
[SinghKoranga:2005ty] - [16-259]
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Mass Varying Neutrinos in the Sun,
Marco Cirelli, M. C. Gonzalez-Garcia, Carlos Pena-Garay,
B719
arXiv:hep-ph/0503028.
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The Polarized electron target as a new solar-neutrino detector,
Marcin Misiaszek, S. Ciechanowicz, W. Sobkow,
B734
arXiv:astro-ph/0502522.
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Solar mass-varying neutrino oscillations,
V. Barger, Patrick Huber, Danny Marfatia,
95
arXiv:hep-ph/0502196.
[Barger:2005mn] - [16-262]
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Geotomography with solar and supernova neutrinos,
E. Kh. Akhmedov, M. A. Tortola, J. W. F. Valle,
0506
arXiv:hep-ph/0502154.
[Akhmedov:2005yt] - [16-263]
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Neutrinos in a fluctuating plasma and the solar neutrino puzzle,
Archil Kobakhidze,
arXiv:hep-ph/0501249,
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Testing the LMA solution with solar neutrinos independently of solar models,
V. Barger, D. Marfatia, K. Whisnant,
B617
arXiv:hep-ph/0501247.
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Power-Spectrum Analyses of Super-Kamiokande Solar Neutrino Data: Variability and its Implications for Solar Physics and Neutrino Physics,
P.A. Sturrock, D.O. Caldwell, J.D. Scargle, M.S. Wheatland,
D72
arXiv:hep-ph/0501205.
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Evidence for solar neutrino flux variability and its implications,
David O. Caldwell, P. A. Sturrock,
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Solar neutrinos and 1-3 leptonic mixing,
Srubabati Goswami, Alexei Yu. Smirnov,
D72
arXiv:hep-ph/0411359.
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Does the neutrino magnetic moment have an impact on solar physics?,
A. B. Balantekin, C. Volpe,
D72
arXiv:hep-ph/0411148.
[Balantekin:2004tk] - [16-269]
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About the sign of $\Delta m_{12}^2$,
Anatoly Kopylov,
arXiv:hep-ph/0411031,
[Kopylov:2004cy] - [16-270]
-
High Precision Measurements of $\theta_{\odot}$ in Solar and Reactor Neutrino Experiments,
Abhijit Bandyopadhyay, Sandhya Choubey, Srubabati Goswami, S.T. Petcov,
D72
arXiv:hep-ph/0410283.
[Bandyopadhyay:2004cp] - [16-271]
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Constraints on the Neutrino Parameters from the `Rise-up' in the Boron Neutrino Spectrum at Low Energies,
S. Dev, Sanjeev Kumar,
A20
arXiv:hep-ph/0409325.
[Dev:2004sc] - [16-272]
-
Power spectrum analysis of the Gallex and GNO solar neutrino data,
P.A. Sturrock, D.O. Caldwell,
26
arXiv:hep-ph/0409064.
[Sturrock:2004jv] - [16-273]
-
Review of methods of power-spectrum analysis as applied to Super-Kamiokande solar neutrino data,
P. A. Sturrock,
D72
arXiv:hep-ph/0408017.
[Sturrock:2004vv] - [16-274]
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Possible neutrino gravitoelectric dipole moments and atmospheric and solar neutrino anomalies,
An. S. Kuznetsov,
arXiv:hep-ph/0407031,
[Kuznetsov:2004xn] - [16-275]
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Update of the solar neutrino oscillation analysis with the 766 Ty KamLAND spectrum,
Abhijit Bandyopadhyay et al.,
B608
arXiv:hep-ph/0406328.
[Bandyopadhyay:2004da] - [16-276]
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Probing New Physics by Comparing Solar and KamLAND Data,
Andre de Gouvea, Carlos Pena-Garay,
D71
arXiv:hep-ph/0406301.
[deGouvea:2004va] - [16-277]
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Solar neutrinos before and after Neutrino 2004,
John N. Bahcall, M. C. Gonzalez-Garcia, Carlos Pena-Garay,
08
arXiv:hep-ph/0406294.
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-
Are solar neutrino oscillations robust?,
O. G. Miranda, M. A. Tortola, J. W. F. Valle,
10
arXiv:hep-ph/0406280.
[Miranda:2004nb] - [16-279]
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Search for time modulations in the Gallex/GNO solar neutrino data,
L. Pandola,
22
arXiv:hep-ph/0406248.
[Pandola:2004gz] - [16-280]
-
SNO, SuperKamiokande data, antineutrinos and sterile neutrinos,
Bhag C. Chauhan, J. Pulido,
0412
arXiv:hep-ph/0406227.
[Chauhan:2004xz] - [16-281]
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Analysis of Neutrino oscillation data with the recent KamLAND results,
P. Aliani et al.,
arXiv:hep-ph/0406182,
[Aliani:2004bf] - [16-282]
-
Enhanced solar anti-neutrino flux in random magnetic fields,
O. G. Miranda, T. I. Rashba, A. I. Rez, J. W. F. Valle,
D70
arXiv:hep-ph/0406066.
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Physics from future SNO and KamLAND data,
A. B. Balantekin et al.,
B613
arXiv:hep-ph/0405019.
[Balantekin:2004hi] - [16-284]
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A simple analytic three-flavour description of the day-night effect in the solar neutrino flux,
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0405
arXiv:hep-ph/0404083.
[Akhmedov:2004rq] - [16-285]
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Toward precision measurements in solar neutrinos,
P.C. de Holanda, Wei Liao, A. Yu. Smirnov,
B702
arXiv:hep-ph/0404042.
[deHolanda:2004fd] - [16-286]
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Comment on 'Search for periodic modulations of the solar neutrino flux in Super-Kamiokande' by J. Yoo et al,
P.A. Sturrock et al.,
arXiv:hep-ph/0403246,
[Sturrock:2004hx] - [16-287]
-
Probing oscillations into sterile neutrinos with cosmology, astrophysics and experiments,
Marco Cirelli, Guido Marandella, Alessandro Strumia, Francesco Vissani,
B708
arXiv:hep-ph/0403158.
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Effects of non-standard neutrino interactions on MSW-LMA solution,
M. M. Guzzo, P. C. de Holanda, O. L. G. Peres,
B591
arXiv:hep-ph/0403134.
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Implications of SNO and BOREXINO results on Neutrino Oscillations and Majorana Magnetic Moments,
Sin Kyu Kang, C. S. Kim,
B584
arXiv:hep-ph/0403059.
[Kang:2004tx] - [16-290]
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Unbinned test of time-dependent signals in real-time neutrino oscillation experiments,
E. Lisi, A. Palazzo, A.M. Rotunno,
21
arXiv:hep-ph/0403036.
[Lisi:2004jw] - [16-291]
-
Equalization of Response Functions of SK and SNO,
Faisal Akram, Haris Rashid,
arXiv:hep-ph/0403006,
[Akram:2004xq] - [16-292]
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Solar neutrinos as probes of neutrino-matter interactions,
Alexander Friedland, Cecilia Lunardini, Carlos Pena-Garay,
B594
arXiv:hep-ph/0402266.
[Friedland:2004pp] - [16-293]
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LMA and sterile neutrinos: a case for resonance spin flavour precession?,
Bhag C. Chauhan, Joao Pulido,
0406
arXiv:hep-ph/0402194.
[Chauhan:2004sf] - [16-294]
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Search for possible neutrino radiative decays during the 2001 total solar eclipse,
S. Cecchini et al.,
21
arXiv:hep-ex/0402008.
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Neutrino magnetic moments and photo-disintegration of deuterium,
J. A. Grifols, Eduard Masso, Subhendra Mohanty,
B587
arXiv:hep-ph/0401144.
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Solar Neutrino Constraints on the BBN Production of Li,
Richard H. Cyburt, Brian D. Fields, Keith A. Olive,
D69
arXiv:astro-ph/0312629.
[Cyburt:2003ae] - [16-297]
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Neutrino flux variations and solar activity,
R.N. Ikhsanov, E.V. Miletsky,
arXiv:astro-ph/0312581,
[Ikhsanov:2003rh] - [16-298]
-
Neutrino oscillations, fluctuations and solar magneto- gravity waves,
C. P. Burgess N. S. Dzhalilov et al.,
AHEP2003
arXiv:hep-ph/0312345.
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Detecting Solar Neutrino Flares and Flavors,
D. Fargion,
0406
arXiv:hep-ph/0312011.
[Fargion:2003yq] - [16-300]
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Neutrino oscillations in the Sun probe long-range leptonic forces,
J. A. Grifols, E. Masso,
B579
arXiv:hep-ph/0311141.
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Day-Night Effect in Solar Neutrino Oscillations with Three Flavors,
M. Blennow, T. Ohlsson, H. Snellman,
D69
arXiv:hep-ph/0311098.
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The effect of very low energy solar neutrinos on the MSW mechanism,
S. Esposito,
A19
arXiv:hep-ph/0311093.
[Esposito:2003xr] - [16-303]
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Constraining the neutrino magnetic moment with anti-neutrinos from the Sun,
O. G. Miranda, T. I. Rashba, A. I. Rez, J. W. F. Valle,
93
arXiv:hep-ph/0311014.
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Cornering Solar Radiative-Zone Fluctuations with KamLAND and SNO Salt,
C. P. Burgess et al.,
0401
arXiv:hep-ph/0310366.
[Burgess:2003su] - [16-305]
-
Three-neutrino model analysis of the world's oscillation data,
D. C. Latimer, D. J. Ernst,
arXiv:nucl-th/0310083,
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,
21
arXiv:hep-ph/0309299.
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-
Solar Neutrinos from CNO Electron Capture,
L. C. Stonehill, J. A. Formaggio, R. G. H. Robertson,
C69
arXiv:hep-ph/0309266.
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Analysis of Super-Kamiokande 5-day Measurements of the Solar Neutrino Flux,
P. A. Sturrock,
605
arXiv:hep-ph/0309239.
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-
On the Measurement of Solar Neutrino Oscillation Parameters with KamLAND,
Abhijit Bandyopadhyay, Sandhya Choubey, Srubabati Goswami, S.T. Petcov,
B581
arXiv:hep-ph/0309236.
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Constraints on neutrino oscillation parameters from the SNO salt phase data,
Abhijit Bandyopadhyay et al.,
B583
arXiv:hep-ph/0309174.
[Bandyopadhyay:2003pk] - [16-311]
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The Neutrino mass matrix after Kamland and SNO salt enhanced results,
P. Aliani, V. Antonelli, M. Picariello, E. Torrente-Lujan,
arXiv:hep-ph/0309156,
[Aliani:2003ns] - [16-312]
-
Status of three-neutrino oscillations after the SNO-salt data,
M. Maltoni, T. Schwetz, M.A. Tortola, J.W.F. Valle,
D68
arXiv:hep-ph/0309130.
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Monte Carlo simulation of an experiment looking for radiative solar neutrino decays,
S. Cecchini et al.,
21
arXiv:hep-ph/0309107.
[Cecchini:2003ye] - [16-314]
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Evidence for Mikheyev-Smirnov-Wolfenstein effects in solar neutrino flavor transitions,
G.L. Fogli, E. Lisi, A. Marrone, A Palazzo,
B583
arXiv:hep-ph/0309100.
[Fogli:2003vj] - [16-315]
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Constraints on Neutrino Parameters from Neutral-Current Solar Neutrino Measurements,
A.B. Balantekin, H. Yuksel,
D68
arXiv:hep-ph/0309079.
[Balantekin:2003jm] - [16-316]
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Addendum to: Solar neutrino oscillation parameters after first KamLAND results,
G.L. Fogli et al.,
D69
arXiv:hep-ph/0308055.
[Fogli:2003am] - [16-317]
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Neutrino Oscillations, Solar Antineutrinos and the Solar Magnetic Fields,
S. Dev, Sanjeev Kumar,
arXiv:hep-ph/0308054,
[Dev:2003ak] - [16-318]
-
Homestake result, sterile neutrinos and low energy solar neutrino experiments,
P. C. de Holanda, A. Yu. Smirnov,
D69
arXiv:hep-ph/0307266.
[deHolanda:2003tx] - [16-319]
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Constraints on axial two-body currents from solar neutrino data,
A. B. Balantekin, H. Yuksel,
C68
arXiv:hep-ph/0307227.
[Balantekin:2003ep] - [16-320]
-
New Interpretation on the Solar Neutrino Flux with Flavor Mixing and Majorana Magnetic Moment,
Sin Kyu Kang, C. S. Kim,
arXiv:hep-ph/0306210,
[Kang:2003zs] - [16-321]
-
Precision Neutrino Oscillation Physics with an Intermediate Baseline Reactor Neutrino Experiment,
Sandhya Choubey, S.T. Petcov, M. Piai,
D68
arXiv:hep-ph/0306017.
[Choubey:2003qx] - [16-322]
-
Three neutrino mixing after the first results from K2K and KamLAND,
M. C. Gonzalez-Garcia, Carlos Pena-Garay,
D68
arXiv:hep-ph/0306001.
[Gonzalez-Garcia:2003myw] - [16-323]
-
Further Evidence for Neutrino Flux Variability from Super- Kamiokande Data,
D. O. Caldwell, P. A. Sturrock,
arXiv:hep-ph/0305303.
[Caldwell:2003yg] - [16-324]
-
Global analyses as a road map to solar neutrino fluxes and oscillation parameters,
John N. Bahcall, Carlos Pena-Garay,
0311
arXiv:hep-ph/0305159.
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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-
A new model of solar neutrinos in manifest violation of CPT invariance,
R. S. Raghavan,
0308
arXiv:astro-ph/0304331.
[Raghavan:2003du] - [16-326]
-
KamLAND, solar antineutrinos and the solar magnetic field,
Bhag C. Chauhan, Joao Pulido, E. Torrente-Lujan,
D68
arXiv:hep-ph/0304297.
[Chauhan:2003wr] - [16-327]
-
Possible Observation of Nuclear Reactor Neutrinos Near the Oscillation Absolute Minimum,
C.Bouchiat,
arXiv:hep-ph/0304253,
[Bouchiat:2003jj] - [16-328]
-
Joint Time-Series Analysis of Homestake and GALLEX-GNO Solar Neutrino Data: Evidence for Rieger-Type Periodicities and their Interpretation as R-Mode Oscillations,
P. A. Sturrock,
arXiv:hep-ph/0304106.
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Time-Series Analysis of Super-Kamiokande Measurements of the Solar Neutrino Flux,
P.A. Sturrock,
594
arXiv:hep-ph/0304073.
[Sturrock:2003ep] - [16-330]
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Limits on charge non-conservation from possible seasonal variations of the solar neutrino experiments,
Manuel Torres, Hector Vucetich,
A19
arXiv:astro-ph/0303588.
[Torres:2003ei] - [16-331]
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Large mixing angle solution to the solar neutrino problem and random matter density perturbations,
M. M. Guzzo, P. C. de Holanda, N. Reggiani,
B569
arXiv:hep-ph/0303203.
[Guzzo:2003xk] - [16-332]
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Do the KamLAND and Solar Neutrino Data Rule out Solar Density Fluctuations?,
A. B. Balantekin, H. Yuksel,
D68
arXiv:hep-ph/0303169.
[Balantekin:2003qm] - [16-333]
-
Exploring the sensitivity of current and future experiments to $\theta_{\odot}$,
Abhijit Bandyopadhyay, Sandhya Choubey, Srubabati Goswami,
D67
arXiv:hep-ph/0302243.
[Bandyopadhyay:2003du] - [16-334]
-
Maximum likelihood analysis of the first KamLAND results,
A. Ianni,
G29
arXiv:hep-ph/0302230.
[Ianni:2003xy] - [16-335]
-
KamLAND Bounds on Solar Antineutrinos and neutrino transition magnetic moments,
E. Torrente-Lujan,
0304
arXiv:hep-ph/0302082.
[Torrente-Lujan:2003xfu] - [16-336]
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A Search for Periodicity in the Super-Kamiokande Solar Neutrino Flux Data,
A. Milsztajn,
arXiv:hep-ph/0301252,
[Milsztajn:2003af] - [16-337]
-
Global Analysis of Solar Neutrino and KamLAND Data,
A.B. Balantekin, H. Yuksel,
G29
arXiv:hep-ph/0301072.
[Balantekin:2003dc] - [16-338]
-
Does the Sun Shine by pp or CNO Fusion Reactions?,
J. N. Bahcall, M. C. Gonzalez-Garcia, C. Penya-Garay,
90
arXiv:astro-ph/0212331.
[Bahcall:2002jt] - [16-339]
-
LMA MSW solution of the solar neutrino problem and first KamLAND results,
P. C. de Holanda, A. Yu. Smirnov,
0302
arXiv:hep-ph/0212270.
[deHolanda:2002iv] - [16-340]
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Neutrino mass parameters from Kamland, SNO and other solar evidence,
P. Aliani, V. Antonelli, M. Picariello, E. Torrente-Lujan,
D69
arXiv:hep-ph/0212212.
[Aliani:2002na] - [16-341]
-
Determining the oscillation parameters by Solar neutrinos and KamLAND,
H. Nunokawa, W. J. C. Teves, R. Zukanovich Funchal,
B562
arXiv:hep-ph/0212202.
[Nunokawa:2002mq] - [16-342]
-
Solar Neutrinos Before and After KamLAND,
J. N. Bahcall, M. C. Gonzalez-Garcia, Carlos Pena-Garay,
0302
arXiv:hep-ph/0212147.
[Bahcall:2002ij] - [16-343]
-
The Solar Neutrino Problem after the first results from Kamland,
Abhijit Bandyopadhyay et al.,
B559
arXiv:hep-ph/0212146.
[Bandyopadhyay:2002en] - [16-344]
-
Implications of the KamLAND Measurement on the Lepton Flavor Mixing Matrix and the Neutrino Mass Matrix,
W.-L. Guo, Z.-Z. Xing,
D67
arXiv:hep-ph/0212142.
[Guo:2002ei] - [16-345]
-
Combining first KamLAND results with solar neutrino data,
M. Maltoni, T. Schwetz, J.W.F. Valle,
D67
arXiv:hep-ph/0212129.
[Maltoni:2002aw] - [16-346]
-
Solar neutrino oscillation parameters after first KamLAND results,
G.L. Fogli et al.,
D67
arXiv:hep-ph/0212127.
[Fogli:2002au] - [16-347]
-
KamLAND and solar neutrino data eliminate the LOW solution,
V. Barger, D. Marfatia,
B555
arXiv:hep-ph/0212126.
[Barger:2002at] - [16-348]
-
Super-Kamiokande hep neutrino best fit: A possible signal of nonmaxwellian solar plasma,
Massimo Coraddu, Marcello Lissia, Giuseppe Mezzorani, Piero Quarati,
A326
arXiv:hep-ph/0212054.
[Coraddu:2002qt] - [16-349]
-
Implications on neutrino oscillation plus decay from recent solar neutrino data,
D. Indumathi,
arXiv:hep-ph/0212038,
[Indumathi:2002qb] - [16-350]
-
Critical review of the results of the Homestake solar neutrino experiment,
Paolo Walter Cattaneo,
arXiv:astro-ph/0211534,
Comment: The data are reanalyzed and a new ratio $\mathrm{DATA/BP00} = 0.40 \pm 0.03$ has been found. (M.L.).
[Cattaneo:2002vj] - [16-351]
-
Solar neutrino oscillations and indications of matter effects in the Sun,
G.L. Fogli, E. Lisi, A. Palazzo, A.M. Rotunno,
D67
arXiv:hep-ph/0211414.
[Fogli:2002hb] - [16-352]
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Status of a Supersymmetric Flavour Violating Solution to the Solar Neutrino Puzzle with Three Generations,
H. K. Dreiner, G. Moreau,
D67
arXiv:hep-ph/0211354.
[Dreiner:2002ne] - [16-353]
-
Analysis of solar neutrino problem by means of Notzold and Nakagawa's approach including the interference term- Hyperbolic-tangent profile for electron density in the sun and exact solution -,
Masahiro Kaneyama, Minoru Biyajima,
arXiv:hep-ph/0211273,
[Kaneyama:2002mj] - [16-354]
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Testing the solar LMA region with KamLAND data,
Abhijit Bandyopadhyay et al.,
G29
arXiv:hep-ph/0211266.
[Bandyopadhyay:2002mc] - [16-355]
-
Searches for sterile component with solar neutrinos and KamLAND,
P. C. de Holanda, A. Yu. Smirnov,
arXiv:hep-ph/0211264,
[deHolanda:2002ma] - [16-356]
-
Active neutrino Oscillations and the SNO neutral Current measurement,
A. A. Aguilar-Arevalo, J.C. Dolivo,
D66
arXiv:hep-ph/0211091.
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arXiv:hep-ph/0208089.
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Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data,
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B643
arXiv:hep-ph/0207157.
From the abstract: ... all four-neutrino descriptions of the LSND anomaly, both in (2+2) as well as (3+1) realizations, are highly disfavoured. Our analysis brings the LSND hint to a more puzzling status.
From the article: The exclusion of four-neutrino oscillation schemes of the (2+2)-type is based on the improved sensitivity of solar and atmospheric neutrino experiments to oscillations into a sterile neutrino, thanks to recent experimental data. This is a very robust result, independent of whether the LSND experiment is confirmed or disproved. The exclusion of (3+1) schemes depends somehow on the used LSND data. Furthermore, it heavily relies on the results of negative SBL experiments, especially on the Bugey and CDHS disappearance experiments.
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Does Solar Physics Provide Constraints to Weakly Interacting Massive Particles?,
A. Bottino et al.,
D66
arXiv:hep-ph/0206211.
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D66
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Getting the most from the statistical analysis of solar neutrino oscillations,
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D66
arXiv:hep-ph/0206162.
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B549
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Which solar neutrino data favour the LMA solution?,
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B541
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Before and after: How has the SNO neutral current measurement changed things?,
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Bounds on neutrino magnetic moment tensor from solar neutrinos,
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D66
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B537
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If sterile neutrinos exist, how can one determine the total B-8 and Be-7 solar neutrino fluxes?,
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C66
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Neutrino decay confronts the SNO data,
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B555
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D65
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D66
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Addendum to: Model-dependent and -independent implications of the first Sudbury Neutrino Observatory results,
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D65
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Has Super-Kamiokande observed antineutrinos from the Sun?,
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Implications of recent solar neutrino observations: an analysis of charged current data,
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D65
arXiv:hep-ph/0201031.
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Matter Effects of Thin Layers: Detecting Oil by Oscillations of Solar Neutrinos,
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Solar neutrino zenith angle distribution and uncertainty in earth matter density,
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The LMA MSW solution of the solar neutrino problem, inverted neutrino mass hierarchy and reactor neutrino experiments,
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B634
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The solar neutrino spectrum derived from electron scattering and charged current interactions,
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Model independent information on solar neutrino oscillations,
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D65
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Robust signatures of solar neutrino oscillation solutions,
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Large solar neutrino mixing and radiative neutrino mechanism,
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Which solar neutrino experiment after KamLAND and Borexino?,
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arXiv:hep-ph/0109172.
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Energy independent solution to the solar neutrino anomaly including the SNO data,
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D65
arXiv:hep-ph/0109017.
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Bayesian view of solar neutrino oscillations,
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arXiv:hep-ph/0108191.
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Global analysis with SNO: Toward the solution of the solar neutrino problem,
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Obtaining the large angle MSW solution to the solar neutrino problem in models,
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Exact analysis of the combined data of SNO and Super-Kamiokande,
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arXiv:hep-ph/0108166.
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How many sigma's is the solar neutrino effect?,
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C65
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A non-resonant dark-side solution to the solar neutrino problem,
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B521
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Electron neutrino survival probability from solar-neutrino data,
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B521
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SN1987A and the status of oscillation solutions to the solar neutrino problem,
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D65
arXiv:hep-ph/0108100.
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Implications for solar neutrino oscillations from Super- Kamiokande and SNO data,
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Are there $\nu_\mu$ or $\nu_\tau$ in the flux of solar neutrinos on Earth?,
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D65
arXiv:hep-ph/0107310.
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Solving the solar neutrino puzzle with KamLAND and solar data,
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D64
arXiv:hep-ph/0107186.
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Neutrinoless double beta decay, solar neutrinos and mass scales,
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B520
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Violation of the equivalence principle in the light of the SNO and SK solar neutrino results,
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D65
arXiv:hep-ph/0107022.
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Probing an extended region of $\Delta{m}^2$ with rapidly oscillating $^7\mathrm{Be}$ solar neutrinos,
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D65
arXiv:hep-ph/0106339.
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Global analysis of solar neutrino oscillations including SNO CC measurement,
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arXiv:hep-ph/0106258.
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Model-dependent and independent implications of the first Sudbury Neutrino Observatory results,
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D64
arXiv:hep-ph/0106247.
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Is right-handed neutrino degeneracy compatible with the solar and atmospheric neutrino data?,
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arXiv:hep-ph/0106226.
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Unknowns after the SNO charged-current measurement,
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arXiv:hep-ph/0106207.
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Global analysis of solar neutrinos with magnetic moment and solar field profiles,
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Global oscillation analysis of solar neutrino data with helioseismically constrained fluxes,
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D64
arXiv:hep-ph/0106168.
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Solar neutrino results from super-Kamiokande,
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Status of the Gribov-Pontecorvo solution to the solar neutrino problem,
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B517
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Solar and atmospheric four-neutrino oscillations,
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D64
arXiv:hep-ph/0105269.
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A new three flavor oscillation solution of the solar neutrino deficit in R-parity violating supersymmetry,
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Solutions of the atmospheric, solar and LSND neutrino anomalies from TeV scale quark lepton unification,
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arXiv:hep-ph/0105101.
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Quasiaveraged solar neutrino oscillations,
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D65
arXiv:hep-ph/0105080.
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Exotic solutions to the solar neutrino problem and some implications for low energy solar neutrino experiments,
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Atmospheric, solar, and CHOOZ neutrinos: A global three generation analysis,
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Three flavor neutrino oscillations, LSND, SNA and ANA,
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Earth regeneration of solar neutrinos at SNO and Super-Kamiokande,
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D64
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Comparative analysis of {GALLEX-GNO} solar neutrino data and {SOHO/MDI} helioseismology data: Further evidence for rotational modulation of the solar neutrino flux,
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Constraints on neutrino oscillations using 1258 days of Super-Kamiokande solar neutrino data,
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Solar neutrino event spectra: Tuning SNO to equalize super- Kamiokande,
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D64
arXiv:hep-ph/0102279.
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QED corrections to the scattering of solar neutrinos and electrons,
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Can three flavor oscillations solve the solar neutrino problem?,
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MSW mediated neutrino decay and the solar neutrino problem,
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Status of the solution to the solar neutrino problem based on non-standard neutrino interactions,
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Exotic solutions to the solar neutrino anomaly,
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Zenith angle distributions at super-Kamiokande and SNO and the solution of the solar neutrino problem,
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Violation of equivalence principle and solar neutrinos,
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On the massless 'just-so' solution to the solar neutrino problem,
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Limits on radiative decays of solar neutrinos from a measurement during a solar eclipse,
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Is the LMA solar neutrino solution ruled out by SN1987A data?,
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The sign of the day-night asymmetry for solar neutrinos,
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Reply to 'Is U(e3) really related to the solar neutrino solutions?',
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Is U(e3) really related to the solar neutrino solutions?,
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Solar Neutrinos: Spin Flavour Precession and LMA,
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The measurement of theta(13) and delta: The role of the uncertainties on the solar and atmospheric parameters,
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Global Analysis of Neutrino Oscillation,
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Discovering Tau and Muon Solar Neutrino Flares above backgrounds,
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Neutrino Oscillations: A Global Analysis,
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Solving the solar neutrino problem with kamLAND and BOREXINO,
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Analysis of solar neutrino induced double beta processes for several nuclei,
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Neutrino oscillations - global analyses,
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After the SNO NC result,
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A Place in the Sun for Neutrinos,
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A new fit to solar neutrinos using extra dimensions,
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Experiments with Solar and Atmospheric Neutrinos: Evidence for Neutrino Masses and Lepton Mixing. Experimental status and Future Projects,
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Measuring the Cosmic Ray Muon-Induced Fast Neutron Spectrum by (n,p) Isotope Production Reactions in Underground Detectors,
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GENIUS - A New Underground Observatory for Non-Accelerator Particle Physics,
H. V. Klapdor-Kleingrothaus,
110
arXiv:hep-ph/0206249.
TAUP 2001, September 8-12, 2001.
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Search for Cold Dark Matter and Solar Neutrinos with GENIUS and GENIUS-TF,
I. V. Krivosheina,
48
arXiv:hep-ph/0206149.
International School on Nuclear Physics, 23rd Course: Neutrinos in Astro, Particle and Nuclear Physics, Erice, 18-26 September 2001.
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Borexino: A real time liquid scintillator detector for low energy solar neutrino study,
L. Miramonti,
arXiv:hep-ex/0206063,
10th International Conference on Calorimetry in High Energy Physics.
[Miramonti:2002kr] - [22-25]
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Phenomenological Study of Solar-Neutrino Induced Double Beta Decay of Mo100,
P. Domin, F. Simkovic, S. V. Semenov, Yu. V. Gaponov,
52
arXiv:hep-ph/0204143.
MEDEX'01 (Prague, June, 2001), to appear in Czech. J. Phys. 52 (2002).
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Solar and Reactor Neutrinos: Upcoming Experiments and Future Projects,
S. Schonert,
110
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.
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Why do solar neutrino experiments below 1 MeV?,
J. N. Bahcall,
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.
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Borexino: Status Report,
B. R. Vogelaar,,
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.
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The HLMA project,
T. Lasserre,
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.
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UNO: Underground Nucleon Decay and Neutrino Observatory,
C. McGrew,
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] - [22-31]
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Status of XMASS,
M. Nakahata,
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.
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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,
International Workshop on Low Energy Solar Neutrinos (LowNu2), December 4 and 5, 2000, Tokyo, Japan.
[Klapdor-Kleingrothaus:2000mnz] - [22-33]
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New physics in the new millennium with GENIUS: Double beta decay, dark matter, solar neutrinos,
H. V. Klapdor-Kleingrothaus,
104
arXiv:hep-ph/0102319.
International Workshop on Non-Accelerator New Physics in Neutrino Observations (NANPino), Dubna, Russia, July 19-22, 2000.
[Klapdor-Kleingrothaus:2000gfm] - [22-34]
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GENIUS - A new facility of non-accelerator particle physics,
H. V. Klapdor-Kleingrothaus,
100
arXiv:hep-ph/0102277.
Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Italy, 9-16 Sep 2000.
[Klapdor-Kleingrothaus:2000nps]
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Solar Neutrinos: A Popular Account,
John N. Bahcall,
arXiv:physics/0411190,
[Bahcall:2004in] - [23-2]
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How the sun shines,
John N. Bahcall,
31N1
arXiv:astro-ph/0009259.
[Bahcall:2000xc]
- [24-1]
-
Solving the Mystery of the Missing Neutrinos,
John Bahcall,
arXiv:physics/0406040,
[Bahcall:2004cc] - [24-2]
-
Nobel Lecture: A half-century with solar neutrinos,
R. Davis,
75
[Davis:2003kh] - [24-3]
-
A half-century with solar neutrinos,
R. Davis,
A18
[Davis:2003xx] - [24-4]
-
Memories of a Nobel laureate,
R. Davis,
42N10
[Davis:2002fb] - [24-5]
-
The beginning of a new science,
J. N. Bahcall, R. Davis,
40N6
http://www.cerncourier.com/main/article/40/6/18.
[Bahcall:2000up] - [24-6]
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The evolution of neutrino astronomy,
J. N. Bahcall, Raymond Davis,
112
arXiv:astro-ph/9911486.
[Bahcall:2000rt]
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Solar Models: An Historical Overview,
J. N. Bahcall,
12N4
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.
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Astrophysical neutrinos: 20th century and beyond,
J. N. Bahcall,
91
arXiv:hep-ph/0009044.
Neutrino 2000.
[Bahcall:2000ue]
Solar Neutrino Experiments - Bahcall et al. Standard Solar Models: BU88, BP92, BP95, BP98, BP00, BP04, BS05.
- Software and Data by J. Bahcall. New (June 2002): 7Be line shape data, from Phys. Rev. D 49 (1994) 3923. Has some effect in the BOREXino predictions for some part of the space of parameters (Carlos Peña Garay). The damping of oscillations due to the 7Be line shape is more important than averaging over the radial distribution of neutrino production in the Sun (John Bahcall). See: Fogli, Lisi, Montanino, Palazzo, PRD 62, 113004 (2000), hep-ph/0005261, Sec. VI and Fig. 5, and Lisi, Marrone, Montanino, Palazzo, Petcov, PRD 63, 093002 (2001), hep-ph/0011306, Fig. 8 and related comments.
- Super-Kamiokande-I Solar Neutrino Data
- Tables and Figures of Neutrino (Anti-Neutrino) Deuteron Reactions Cross Sections
- Living Reviews in Solar Physics
- Solar Physics (NASA's Marshall Space Flight Center)
- Solar Physics Glossary
- The Solar and Heliospheric Observatory (SOHO)
- APS Neutrino Study: Solar and Atmospheric Neutrino Experiments Working Group
- NASA Astronomy Picture of the Day (5 June 1998): Neutrinos in the Sun
