Geo-Neutrinos


References

  1 - Books

  2 - Reviews

  3 - Reviews - Conference Proceedings

  4 - Experiment

  5 - Experiment - Conference Proceedings

  6 - Experiment - Detector

  7 - Phenomenology

  8 - Phenomenology - Conference Proceedings

  9 - Theory

  10 - Geophysics

  11 - Geophysics - Models

  12 - Future Experiments

  13 - Future Experiments - Conference Proceedings

The references in each group are listed in approximate inverted chronological order.
Click on the reference label to search it in inSPIRE.


1 - Books

[1-1]
Theory of the Earth, D.L. Anderson, Blackwell Scientific Publications, 1989.[Anderson-89 BibTeX&LaTeX]


2 - Reviews

[2-1]
Antineutrino Science in KamLAND, Atsuto Suzuki, Eur.Phys.J. C74 (2014) 3094, arXiv:1409.4515.[Suzuki:2014woa BibTeX&LaTeX]
[2-2]
Geo-neutrinos, Livia Ludhova, Sandra Zavatarelli, arXiv:1310.3961, 2013.[Ludhova:2013hna BibTeX&LaTeX]
[2-3]
Geo-neutrinos, G. Bellini, A. Ianni, L. Ludhova, F. Mantovani, W.F. McDonough, Prog.Part.Nucl.Phys. 73 (2013) 1-34, arXiv:1310.3732.[Bellini:2013wsa BibTeX&LaTeX]
[2-4]
Geo-neutrinos as indicators of the origin and thermal history of the Earth, Steve Dye, Rev. Geophys. 50 (2012) 3007, arXiv:1111.6099.[Dye:2011mc BibTeX&LaTeX]
[2-5]
Geo-neutrinos and Earth's interior, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Phys. Rept. 453 (2007) 117-172, arXiv:0707.3203.[Fiorentini:2007te BibTeX&LaTeX]
[2-6]
Journey to the centre of the Earth, Gianni Fiorentini, Alessandro Pascolini, CERN Cour. 43N8 (2003). http://www.cerncourier.com/main/article/43/8/12.[Fiorentini-CERN-2004 BibTeX&LaTeX]


3 - Reviews - Conference Proceedings

[3-1]
Low-energy neutrinos, Livia Ludhova, arXiv:1601.08234, 2016. TAUP 2015, 7-11 September 2015, Torino (Italy).[Ludhova:2016wbn BibTeX&LaTeX]
[3-2]
Geo-neutrinos: recent developments, Steve Dye, arXiv:1412.3520, 2014. NOW 2014.[Dye:2014zfa BibTeX&LaTeX]
[3-3]
Geo-neutrinos: A short review, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Riccardo Vannucci, Nucl. Phys. Proc. Suppl. 143 (2005) 53, arXiv:hep-ph/0409152.[Fiorentini:2004xk BibTeX&LaTeX]


4 - Experiment

[4-1]
Spectroscopy of geo-neutrinos from 2056 days of Borexino data, M. Agostini et al. (Borexino), Phys. Rev. D92 (2015) 031101, arXiv:1506.04610.[Agostini:2015cba BibTeX&LaTeX]
[4-2]
Measurement of geo-neutrinos from 1353 days of Borexino, G. Bellini et al. (Borexino), Phys.Lett. B722 (2013) 295-300, arXiv:1303.2571.[Bellini:2013nah BibTeX&LaTeX]
[4-3]
Observation of Geo-Neutrinos, G. Bellini et al. (Borexino), Phys. Lett. B687 (2010) 299-304, arXiv:1003.0284.[Bellini:2010hy BibTeX&LaTeX]
[4-4]
Experimental investigation of geologically produced antineutrinos with KamLAND, T. Araki et al. (KamLAND), Nature 436 (2005) 499-503. http://www.nature.com/nature/journal/v436/n7050/abs/nature03980.html;jsessionid=2B54E1F6E002C96A8C0F0275FB860964.
From the abstract: Assuming a Th/U mass concentration ratio of 3.9, the 90 per cent confidence interval for the total number of geoneutrinos detected is 4.5 to 54.2. This result is consistent with the central value of 19 predicted by geophysical models.
From the article: ... a 'rate only' analysis gives $ 25 {}^{+19}_{-18} $ geoneutrino candidates from the $^{238}\text{U}$ and $^{232}\text{Th}$ decay chains. Dividing by the detection efficiency, live-time, and number of target protons, the total geoneutrino detected rate obtained is $ 5.1 {}^{+3.9}_{-3.6} \times 10^{-31} $ $\bar\nu_e$ per target proton per year.
...
The 99\% confidence upper limit obtained on the total detected $^{238}\text{U}$ and $^{232}\text{Th}$ geoneutrino rate is $ 1.45 \times 10^{-30} $ $\bar\nu_e$ per target proton per year, corresponding to a flux at KamLAND of $ 1.62 \times 10^7 \, \text{cm}^{-2} \, \text{s}^{-1}$. On the basis of our reference model, this corresponds to an upper limit on the radiogenic power from $^{238}\text{U}$ and $^{232}\text{Th}$ decay of 60 TW.
[KamLAND-Nature436-499-2005 BibTeX&LaTeX]
[4-5]
First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 90 (2003) 021802, arXiv:hep-ex/0212021.[Eguchi:2002dm BibTeX&LaTeX]


5 - Experiment - Conference Proceedings

[5-1]
Recent Borexino results and prospects for the near future, D. D'Angelo et al. (Borexino), arXiv:1405.7919, 2014. Rencontres de Moriond EW 2014.[D'Angelo:2014vgk BibTeX&LaTeX]
[5-2]
KamLAND results, K. Inoue, arXiv:hep-ex/0307030, 2003. XXXVIII Rencontres de Moriond on Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003.[Inoue:2003qs BibTeX&LaTeX]


6 - Experiment - Detector

[6-1]
Directional Antineutrino Detection, Benjamin R. Safdi, Burkhant Suerfu, Phys.Rev.Lett. 114 (2015) 071802, arXiv:1410.8530.[Safdi:2014hwa BibTeX&LaTeX]


7 - Phenomenology

[7-1]
On the implementation of CVC in weak charged-current proton-neutron transitions, C. Giunti, arXiv:1602.00215, 2016.[Giunti:2016vlh BibTeX&LaTeX]
[7-2]
Improved estimate of the cross section for inverse beta decay, Artur M. Ankowski, arXiv:1601.06169, 2016.[Ankowski:2016oyj BibTeX&LaTeX]
[7-3]
Web Application for Modeling Global Antineutrinos, Andrew Barna, Steve Dye, arXiv:1510.05633, 2015.[Barna:2015rza BibTeX&LaTeX]
[7-4]
Potential of Geo-neutrino Measurements at JUNO, Ran Han, Yu-Feng Li, Liang Zhan, William F McDonough, Jun Cao, arXiv:1510.01523, 2015.[Han:2015roa BibTeX&LaTeX]
[7-5]
AGM2015: Antineutrino Global Map 2015, Shawn M. Usman, Glenn R. Jocher, Stephen T. Dye, William F. McDonough, John G. Learned, Sci. Rep. 5 (2015) 13945, arXiv:1509.03898.[Usman:2015yda BibTeX&LaTeX]
[7-6]
Could Geoneutrinos Interact With the Geomagnetic Field?, C.A.B. Quintero, J.A. Helayel Neto, arXiv:1508.03493, 2015.[Quintero:2015oha BibTeX&LaTeX]
[7-7]
Expected geoneutrino signal at JUNO, Virginia Strati et al., arXiv:1412.3324, 2014.[Strati:2014kaa BibTeX&LaTeX]
[7-8]
A reference worldwide model for antineutrinos from reactors, Marica Baldoncini et al., Phys.Rev. D91 (2015) 065002, arXiv:1411.6475.[Baldoncini:2014vda BibTeX&LaTeX]
[7-9]
Geoneutrinos and Hydridic Earth (or primordially Hydrogen-Rich Planet), L. Bezrukov, V. Sinev, Phys.Part.Nucl. 46 (2015) 182-185, arXiv:1405.3161.[Bezrukov:2014rja BibTeX&LaTeX]
[7-10]
Looking for antineutrino flux from $^{40}$K with large liquid scintillator detector, V. V. Sinev et al., Phys.Part.Nucl. 46 (2015) 186-189, arXiv:1405.3140.[Sinev:2014jaa BibTeX&LaTeX]
[7-11]
Regional study of the Archean to Proterozoic crust at the Sudbury Neutrino Observatory (SNO+), Ontario: Predicting the geoneutrino flux, Yu Huang et al., Geochem.Geophys.Geosyst. 15 (2014) 3925, arXiv:1404.6692.[Huang:2014dpa BibTeX&LaTeX]
[7-12]
Terracentric Nuclear Fission Reactor: Background, Basis, Feasibility, Structure, Evidence, and Geophysical Implications, J. Marvin Herndon, arXiv:1308.5934, 2013.[Herndon:2013eta BibTeX&LaTeX]
[7-13]
Geoneutrino and Hydridic Earth model, Leonid Bezrukov, arXiv:1308.4163, 2013.[Bezrukov:2013qwa BibTeX&LaTeX]
[7-14]
Theoretical Antineutrino Detection, Direction and Ranging at Long Distances, G. R. Jocher et al., Phys.Rept. 527 (2013) 131-204, arXiv:1307.2832.[Jocher:2013gta BibTeX&LaTeX]
[7-15]
A reference Earth model for the heat producing elements and associated geoneutrino flux, Yu Huang, Viacheslav Chubakov, Fabio Mantovani, Roberta L. Rudnick, William F. McDonough, arXiv:1301.0365, 2013.[1301.0365 BibTeX&LaTeX]
[7-16]
Potential of a Neutrino Detector in the ANDES Underground Laboratory for Geophysics and Astrophysics of Neutrinos, P. A. N. Machado, T. Muhlbeier, H. Nunokawa, R. Zukanovich Funchal, Phys. Rev. D86 (2012) 125001, arXiv:1207.5454.[Machado:2012ee BibTeX&LaTeX]
[7-17]
Geophysical and geochemical constraints on geoneutrino fluxes from Earth's mantle, Ondrej Sramek et al., Earth Planet. Sci. Lett. 361 (2013) 356-366, arXiv:1207.0853.[Sramek:2012nk BibTeX&LaTeX]
[7-18]
Comment on 'Observation of electron-antineutrino disappearance at Daya Bay', V.D. Rusov, V.A. Tarasov, S.A. Chernegenko, V.P. Smolyar, arXiv:1204.5974, 2012.[Rusov:2012nq BibTeX&LaTeX]
[7-19]
Mantle geoneutrinos in KamLAND and Borexino, G. Fiorentini, G. L. Fogli, E. Lisi, F. Mantovani, A. M. Rotunno, Phys. Rev. D86 (2012) 033004, arXiv:1204.1923.[Fiorentini:2012yk BibTeX&LaTeX]
[7-20]
U and Th content in the Central Apennines continental crust: a contribution to the determination of the geo-neutrinos flux at LNGS, M. Coltorti, R. Boraso, F. Mantovani, M. Morsilli, G. Fiorentini et al., Geochim.Cosmochim.Acta 75 (2011) 2271, arXiv:1102.1335.[Coltorti:2011gr BibTeX&LaTeX]
[7-21]
The KamLAND-experiment and Soliton-like Nuclear Georeactor. Part 1. Comparison of Theory with Experiment, V.D. Rusov et al., arXiv:1011.3568, 2010.[Rusov:2010bk BibTeX&LaTeX]
[7-22]
Geoneutrinos and the Earth inner parts structure, V.V. Sinev, arXiv:1007.2526, 2010.[Sinev:2010bk BibTeX&LaTeX]
[7-23]
Combined analysis of KamLAND and Borexino neutrino signals from Th and U decays in the Earth's interior, G.L. Fogli, E. Lisi, A. Palazzo, A.M. Rotunno, Phys. Rev. D82 (2010) 093006, arXiv:1006.1113.[Fogli:2010vx BibTeX&LaTeX]
[7-24]
Nuclear physics for geo-neutrino studies, Gianni Fiorentini et al., Phys. Rev. C81 (2010) 034602, arXiv:0908.3433.[Fiorentini:2009bv BibTeX&LaTeX]
[7-25]
Neutrino Mixing Discriminates Geo-reactor Models, S. T. Dye, Phys. Lett. B679 (2009) 15-18, arXiv:0905.0523.[Dye:2009jp BibTeX&LaTeX]
[7-26]
Neutrino geophysics with KamLAND and future prospects, S. Enomoto, E. Ohtani, K. Inoue, A. Suzuki, arXiv:hep-ph/0508049, 2005.[Enomoto:2005mb BibTeX&LaTeX]
[7-27]
KamLAND results and the radiogenic terrestrial heat, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Barbara Ricci, Phys. Lett. B629 (2005) 77, arXiv:hep-ph/0508048.[Fiorentini:2005ma BibTeX&LaTeX]
[7-28]
Geo-neutrinos: a new probe of Earth's interior, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Riccardo Vannucci, Earth Planet.Sci.Lett. 238 (2005) 235-247, arXiv:physics/0508019.[Fiorentini:2005mr BibTeX&LaTeX]
[7-29]
KamLAND neutrino spectra in energy and time: Indications for reactor power variations and constraints on the georeactor, G. L. Fogli, E. Lisi, A. Palazzo, A. M. Rotunno, Phys. Lett. B623 (2005) 80, arXiv:hep-ph/0505081.[Fogli:2005qa BibTeX&LaTeX]
[7-30]
Contribution of Ue3 to geo-neutrino flux, Subhendra Mohanty, arXiv:hep-ph/0502241, 2005.[Mohanty:2005fd BibTeX&LaTeX]
[7-31]
Background for Terrestrial Antineutrino Investigations: Radionuclide Distribution, Georeactor Fission Events, and Boundary Conditions on Fission Power Production, J. Marvin Herndon, Dennis A. Edgerley, Proc.Roy.Soc.Lond.A Math.Phys.Eng.Sci. (2005), arXiv:hep-ph/0501216.[Herndon:2005zq BibTeX&LaTeX]
[7-32]
How much Uranium is in the Earth? Predictions for geo- neutrinos at KamLAND, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Riccardo Vannucci, Phys. Rev. D72 (2005) 033017, arXiv:hep-ph/0501111.[Fiorentini:2005cu BibTeX&LaTeX]
[7-33]
Can Radiogenic Heat Sources Inside the Earth be located by their Antineutrino incoming Directions?, G. Domogatsky, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 69 (2006) 1894-1898, arXiv:hep-ph/0411163.[Domogatsky:2004be BibTeX&LaTeX]
[7-34]
Neutrino Geophysics at Baksan (Part II): Possible Studies of Antineutrino- and Radiogenic Heat Sources in Earth Interior, G. Domogatski, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys.Atom.Nucl. (2004), arXiv:hep-ph/0409069.[Domogatsky:2004pm BibTeX&LaTeX]
[7-35]
Background for Terrestrial Antineutrino Investigations: Scientific Basis of Knowledge on the Composition of the Deep Interior of the Earth, J. Marvin Herndon, Curr.Sci. (2004), arXiv:hep-ph/0407148.[Herndon:2004dj BibTeX&LaTeX]
[7-36]
Imaging the Earth's Interior: the Angular Distribution of Terrestrial Neutrinos, Brian D. Fields, Kathrin A. Hochmuth, Earth Moon Planets 99 (2006) 155-181, arXiv:hep-ph/0406001.[Fields:2004tf BibTeX&LaTeX]
[7-37]
Inverse beta decay reaction in $^{232}\mathrm{Th}$ and $^{233}\mathrm{U}$ fission antineutrino flux, G. Domogatski, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 68 (2005) 234-236, arXiv:hep-ph/0403155.[Domogatski:2005cw BibTeX&LaTeX]
[7-38]
Geoantineutrino Spectrum and Slow Nuclear Burning on the Boundary of the Liquid and Solid Phases of the Earth's core, V.D. Rusov et al., arXiv:hep-ph/0402039, 2004.[Rusov:2004dp BibTeX&LaTeX]
[7-39]
Neutrino Geophysics at Baksan I: Possible Detection of Georeactor Antineutrinos, G. Domogatski, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 68 (2005) 69-72, arXiv:hep-ph/0401221.[Domogatski:2004gs BibTeX&LaTeX]
[7-40]
Antineutrino Spectrum of the Earth and the Problem of Oscillating Geoantineutrino Deficit, V.D. Rusov et al., arXiv:hep-ph/0312296, 2003.[Rusov:2003sx BibTeX&LaTeX]
[7-41]
Antineutrinos from the earth: the reference model and its uncertainties, Fabio Mantovani, Luigi Carmignani, Gianni Fiorentini, Marcello Lissia, Phys. Rev. D69 (2004) 013001, arXiv:hep-ph/0309013.[Mantovani:2003yd BibTeX&LaTeX]
[7-42]
Discriminating among Earth composition models using geo-antineutrinos, H. Nunokawa, W. J. C. Teves, R. Zukanovich Funchal, JHEP 0311 (2003) 020, arXiv:hep-ph/0308175.[Nunokawa:2003dd BibTeX&LaTeX]
[7-43]
Determination of the age of the earth from Kamland measurement of geo-neutrinos, Subhendra Mohanty, arXiv:hep-ph/0302060, 2003.[Mohanty:2003zb BibTeX&LaTeX]
[7-44]
KamLAND, terrestrial heat sources and neutrino oscillations, G. Fiorentini et al., Phys. Lett. B558 (2003) 15, arXiv:hep-ph/0301042.[Fiorentini:2003ww BibTeX&LaTeX]
[7-45]
Neutrinos and Energetics of the Earth, G. Fiorentini, F. Mantovani, B. Ricci, Phys. Lett. B557 (2003) 139, arXiv:nucl-ex/0212008.[Fiorentini:2002bp BibTeX&LaTeX]
[7-46]
Electron neutrino sources from the core of the Earth, A. Widom, E. Sassaroli, Y. N. Srivastava, arXiv:hep-ph/9812284, 1998.[Widom:1998uh BibTeX&LaTeX]
[7-50]
Geophysics by neutrinos, G. Marx, Czech. J. Phys. B19 (1969) 1471-1479.[BibTeX&LaTeX]
[7-51]
Terrestrial neutrinos, G. Eder, Nucl. Phys. 78 (1966) 657-662.[BibTeX&LaTeX]


8 - Phenomenology - Conference Proceedings

[8-1]
Geo-neutrinos and Earth Models, S.T. Dye, Y. Huang, V. Lekic, W.F. McDonough, O. Sramek, Phys.Procedia 61 (2015) 310-318, arXiv:1405.0192. TAUP 2013.[BibTeX&LaTeX]
[8-2]
Reactor Antineutrinos Signal all over the world, B. Ricci et al., PoS Neutel2013 (2013) 077, arXiv:1403.4072.[BibTeX&LaTeX]
[8-3]
Neutral Current Coherent Cross Sections- Implications on Gaseous Spherical TPC's for detecting SN and Earth neutrinos, J. D. Vergados, J. Phys. Conf. Ser. 309 (2011) 012031, arXiv:1103.1107. Fifth symposium on large TPCs> (2012) 042050, arXiv:1201.6599. TAUP2011.[BibTeX&LaTeX]
[13-2]
The Physics Potential of the LENA Detector, Michael Wurm et al., Acta Phys. Polon. B41 (2010) 1749-1764, arXiv:1004.3474. Cracow Epiphany Conference, 5-8 January 2010.[BibTeX&LaTeX]
[13-3]
Hanohano: A Deep Ocean Anti-Neutrino Detector for Unique Neutrino Physics and Geophysics Studies, John G. Learned, Stephen T. Dye, Sandip Pakvasa, arXiv:0810.4975, 2008. Twelfth International Workshop on Neutrino Telescopes, Venice, March 2007.[BibTeX&LaTeX]
[13-4]
The SNO+ Experiment, Mark C. Chen (SNO+), arXiv:0810.3694, 2008. ICHEP08.[BibTeX&LaTeX]
[13-5]
Hanohano:A Deep Ocean Antineutrino Observatory, M. Batygov et al., J. Phys. Conf. Ser. 136 (2008) 042002, arXiv:0810.0564. ICHEP08, Philadelphia, USA, July 2008.[BibTeX&LaTeX]
[13-6]
Science Potential of a Deep Ocean Antineutrino Observatory, Steve Dye, Nucl. Phys. Proc. Suppl. 168 (2007) 144-146, arXiv:hep-ex/0611039. NOW 2006, Lecce, Italy.[BibTeX&LaTeX]
[13-7]
Probing the Earth's interior with the LENA detector, Kathrin A. Hochmuth et al., Earth Moon Planets 99 (2006) 253-264, arXiv:hep-ph/0610048. Neutrino Sciences 2005: Neutrino Geophysics, Honolulu, HI, 14-16 Dec 2005.[BibTeX&LaTeX]
[13-8]
A geoneutrino experiment at Homestake, N. Tolich et al., Earth Moon Planets (2006) 229-240, arXiv:physics/0607230. Neutrino Sciences 2005, submitted to Earth, Moon, and Planets.[BibTeX&LaTeX]
[13-9]
Geoneutrinos in Borexino, Marco G. Giammarchi, Lino Miramonti, arXiv:hep-ex/0604019, 2006. Neutrino Geophysics Honolulu, Hawaii December 14-16, 2005.[BibTeX&LaTeX]


Useful Links

A reference worldwide model for antineutrinos from reactors


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We Can Put an End to Word Attachments


Authors:
Carlo Giunti / giunti@to.infn.it
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Last Update: Mon 16 Nov 2015, day 320 of the year 2015, 10:16:40 UTC me='9'>

9 - Theory

[9-1]
Geoantineutrino Spectrum, 3He/4He - ratio radial distribution and Slow Nuclear Burning on the Boundary of the Liquid and Solid Phases of the Earth's core, V.D. Rusov et al., arXiv:nucl-th/0605025, 2006.[BibTeX&LaTeX]


10 - Geophysics

[10-1]
Distribution of U and Th and Their Nuclear Fission in the Outer Core of the Earth and Their effects on the Geodynamics, Xuezhao Bao, Geol. Rev. 45 (1999) S82-92, arXiv:0903.1566.[BibTeX&LaTeX]


11 - Geophysics - Models

[11-1]
Preliminary reference earth model, A. M. Dziewonski, D. L. Anderson, Phys. Earth Planet. Interiors 25 (1981) 297-356.[BibTeX&LaTeX]


12 - Future Experiments

[12-1]
Neutrino Physics with JUNO, Fengpeng An et al. (JUNO), arXiv:1507.05613, 2015.[BibTeX&LaTeX]
[12-2]
Research of the natural neutrino fluxes by use of large volume scintillation detector at Baksan, I. R. Barabanov, G. Ya. Novikova, V. V. Sinev, E. A. Yanovich, arXiv:0908.1466, 2009.[BibTeX&LaTeX]
[12-3]
Large underground, liquid based detectors for astro-particle physics in Europe: scientific case and prospects, J. Aysto et al., JCAP 0711 (2007) 011, arXiv:0705.0116.[BibTeX&LaTeX]
[12-4]
Earth Radioactivity Measurements with a Deep Ocean Anti-neutrino Observatory, S.T. Dye et al., Earth Moon Planets 99 (2006) 241-252, arXiv:hep-ex/0609041.[BibTeX&LaTeX]
[12-5]
Search for electron antineutrino interactions with the Borexino Counting Test Facility at Gran Sasso, M. Balata et al. (Borexino), Eur. Phys. J. C47 (2006) 21-30, arXiv:hep-ex/0602027.[BibTeX&LaTeX]
[12-6]
Quest for the Nuclear Georeactor, R.J. de Meijer, E.R. van der Graaf, K.P. Jungmann, Nucl. Phys. News 14 (2004) 20, arXiv:physics/0404046.[BibTeX&LaTeX]


13 - Future Experiments - Conference Proceedings

[13-1]
Scintillator phase of the SNO+ experiment, V. Lozza (SNO+), J. Phys. Conf. Ser. 375 Neutrino Geophysics at Baksan I: Possible Detection of Georeactor Antineutrinos, G. Domogatski, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 68 (2005) 69-72, arXiv:hep-ph/0401221.[BibTeX&LaTeX]
[7-38]
Antineutrino Spectrum of the Earth and the Problem of Oscillating Geoantineutrino Deficit, V.D. Rusov et al., arXiv:hep-ph/0312296, 2003.[BibTeX&LaTeX]