Geo-Neutrinos


References

  1 - Books

  2 - Reviews

  3 - Reviews - Conference Proceedings

  4 - Experiment

  5 - Experiment - Conference Proceedings

  6 - Phenomenology

  7 - Phenomenology - Conference Proceedings

  8 - Theory

  9 - Geophysics

  10 - Geophysics - Models

  11 - Future Experiments

  12 - 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.[BibTeX&LaTeX]


2 - Reviews

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


3 - Reviews - Conference Proceedings

[3-1]
Geo-neutrinos: A short review, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Riccardo Vannucci, Nucl. Phys. Proc. Suppl. 143 (2005) 53, arXiv:hep-ph/0409152.[BibTeX&LaTeX]


4 - Experiment

[4-1]
Measurement of geo-neutrinos from 1353 days of Borexino, G. Bellini et al. (Borexino), Phys.Lett. B722 (2013) 295-300, arXiv:1303.2571.[BibTeX&LaTeX]
[4-2]
Observation of Geo-Neutrinos, G. Bellini et al. (Borexino), Phys. Lett. B687 (2010) 299-304, arXiv:1003.0284.[BibTeX&LaTeX]
[4-3]
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.
[BibTeX&LaTeX]
[4-4]
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.[BibTeX&LaTeX]


5 - Experiment - Conference Proceedings

[5-1]
Recent Borexino results and prospects for the near future, D. D'Angelo et al. (Borexino Collaboration), arXiv:1405.7919, 2014. Rencontres de Moriond EW 2014.[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.[BibTeX&LaTeX]


6 - Phenomenology

[6-1]
Geoneutrinos and Hydridic Earth (or primordially Hydrogen-Rich Planet), L. Bezrukov, V. Sinev, arXiv:1405.3161, 2014.[BibTeX&LaTeX]
[6-2]
Looking for antineutrino flux from $^{40}$K with large liquid scintillator detector, V. V. Sinev et al., arXiv:1405.3140, 2014.[BibTeX&LaTeX]
[6-3]
Regional study of the Archean to Proterozoic crust at the Sudbury Neutrino Observatory (SNO+), Ontario: Predicting the geoneutrino flux, Yu Huang et al., arXiv:1404.6692, 2014.[BibTeX&LaTeX]
[6-4]
Terracentric Nuclear Fission Reactor: Background, Basis, Feasibility, Structure, Evidence, and Geophysical Implications, J. Marvin Herndon, arXiv:1308.5934, 2013.[BibTeX&LaTeX]
[6-5]
Geoneutrino and Hydridic Earth model, Leonid Bezrukov, arXiv:1308.4163, 2013.[BibTeX&LaTeX]
[6-6]
Theoretical Antineutrino Detection, Direction and Ranging at Long Distances, G. R. Jocher et al., Phys.Rept. 527 (2013) 131-204, arXiv:1307.2832.[BibTeX&LaTeX]
[6-7]
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.[BibTeX&LaTeX]
[6-8]
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.[BibTeX&LaTeX]
[6-9]
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.[BibTeX&LaTeX]
[6-10]
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.[BibTeX&LaTeX]
[6-11]
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.[BibTeX&LaTeX]
[6-12]
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., arXiv:1102.1335, 2011.[BibTeX&LaTeX]
[6-13]
The KamLAND-experiment and Soliton-like Nuclear Georeactor. Part 1. Comparison of Theory with Experiment, V.D. Rusov et al., arXiv:1011.3568, 2010.[BibTeX&LaTeX]
[6-14]
Geoneutrinos and the Earth inner parts structure, V.V. Sinev, arXiv:1007.2526, 2010.[BibTeX&LaTeX]
[6-15]
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.[BibTeX&LaTeX]
[6-16]
Nuclear physics for geo-neutrino studies, Gianni Fiorentini et al., Phys. Rev. C81 (2010) 034602, arXiv:0908.3433.[BibTeX&LaTeX]
[6-17]
Neutrino Mixing Discriminates Geo-reactor Models, S. T. Dye, Phys. Lett. B679 (2009) 15-18, arXiv:0905.0523.[BibTeX&LaTeX]
[6-18]
Neutrino geophysics with KamLAND and future prospects, S. Enomoto, E. Ohtani, K. Inoue, A. Suzuki, arXiv:hep-ph/0508049, 2005.[BibTeX&LaTeX]
[6-19]
KamLAND results and the radiogenic terrestrial heat, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Barbara Ricci, Phys. Lett. B629 (2005) 77, arXiv:hep-ph/0508048.[BibTeX&LaTeX]
[6-20]
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.[BibTeX&LaTeX]
[6-21]
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.[BibTeX&LaTeX]
[6-22]
Contribution of Ue3 to geo-neutrino flux, Subhendra Mohanty, arXiv:hep-ph/0502241, 2005.[BibTeX&LaTeX]
[6-23]
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.[BibTeX&LaTeX]
[6-24]
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.[BibTeX&LaTeX]
[6-25]
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.[BibTeX&LaTeX]
[6-26]
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.[BibTeX&LaTeX]
[6-27]
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.[BibTeX&LaTeX]
[6-28]
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.[BibTeX&LaTeX]
[6-29]
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.[BibTeX&LaTeX]
[6-30]
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.[BibTeX&LaTeX]
[6-31]
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]
[6-32]
Antineutrino Spectrum of the Earth and the Problem of Oscillating Geoantineutrino Deficit, V.D. Rusov et al., arXiv:hep-ph/0312296, 2003.[BibTeX&LaTeX]
[6-33]
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.[BibTeX&LaTeX]
[6-34]
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.[BibTeX&LaTeX]
[6-35]
Determination of the age of the earth from Kamland measurement of geo-neutrinos, Subhendra Mohanty, arXiv:hep-ph/0302060, 2003.[BibTeX&LaTeX]
[6-36]
KamLAND, terrestrial heat sources and neutrino oscillations, G. Fiorentini et al., Phys. Lett. B558 (2003) 15, arXiv:hep-ph/0301042.[BibTeX&LaTeX]
[6-37]
Neutrinos and Energetics of the Earth, G. Fiorentini, F. Mantovani, B. Ricci, Phys. Lett. B557 (2003) 139, arXiv:nucl-ex/0212008.[BibTeX&LaTeX]
[6-38]
Electron neutrino sources from the core of the Earth, A. Widom, E. Sassaroli, Y. N. Srivastava, arXiv:hep-ph/9812284, 1998.[BibTeX&LaTeX]
[6-39]
Measuring the global radioactivity in the earth by multidetector anti-neutrino spectroscopy, R. S. Raghavan et al., Phys. Rev. Lett. 80 (1998) 635-638.[BibTeX&LaTeX]
[6-40]
Antineutrino Geophysics with Liquid Scintillator Detectors, Casey G. Rothschild, Mark C. Chen, Frank P. Calaprice, Geophys. Res. Lett. 25 (1998) 1083, arXiv:nucl-ex/9710001.[BibTeX&LaTeX]
[6-41]
The Earth as an antineutrino star, Masao Kobayashi, Yoshio Fukao, Geophys. Res. Lett. 18 (1991) 633-636.[BibTeX&LaTeX]
[6-42]
Antineutrino astronomy and geophysics, Lawrence M. Krauss, Sheldon L. Glashow, David N. Schramm, Nature 310 (1984) 191-198.[BibTeX&LaTeX]
[6-43]
The Earth as a source of anti-neutrinos, C. Avilez, G. Marx, B. Fuentes, Phys. Rev. D23 (1981) 1116.[BibTeX&LaTeX]
[6-44]
Geophysics by neutrinos, G. Marx, Czech. J. Phys. B19 (1969) 1471-1479.[BibTeX&LaTeX]
[6-45]
Terrestrial neutrinos, G. Eder, Nucl. Phys. 78 (1966) 657-662.[BibTeX&LaTeX]


7 - Phenomenology - Conference Proceedings

[7-1]
Geo-neutrinos and Earth Models, S.T. Dye, Y. Huang, V. Lekic, W.F. McDonough, O. Sramek, arXiv:1405.0192, 2014. TAUP 2013.[BibTeX&LaTeX]
[7-2]
Reactor Antineutrinos Signal all over the world, B. Ricci et al., PoS Neutel2013 (2013) 077, arXiv:1403.4072.[BibTeX&LaTeX]
[7-3]
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 for low energy rare event detection and workshop on neutrinos from Supernovae, Paris Dec. 14-18, 2010.[BibTeX&LaTeX]
[7-4]
Considerations For a Dedicated Geoneutrino Detector For Geosciences, P. Ila, W. Gosnold, P. Jagam, G. I. Lykken (GRAFG), arXiv:0902.3607, 2009. AGU 2008.[BibTeX&LaTeX]
[7-5]
Nuclear physics inputs needed for geo-neutrino studies, G. Bellini et al., J. Phys. Conf. Ser. 120 (2008) 052007, arXiv:0712.0298. International Conference on Topics in Astroparticle and Underground Physics (TAUP) 2007, Sendai, Japan, September 11-15, 2007.[BibTeX&LaTeX]
[7-6]
Geo-neutrinos: A systematic approach to uncertainties and correlations, G.L. Fogli, E. Lisi, A. Palazzo, A.M. Rotunno, arXiv:physics/0608025, 2006. Neutrino Science 2005 (Honolulu, Hawaii, Dec. 2005).[BibTeX&LaTeX]
[7-7]
Geoneutrino Analysis in KamLAND: Input and Desiderata, G.L. Fogli, E. Lisi, A. Palazzo, A.M. Rotunno, arXiv:hep-ph/0405139, 2004. 39th Rencontres de Moriond on Electronweack Interactions and Unified Theories, La Thuile, Italy, 21-28 Mar 2004.[BibTeX&LaTeX]
[7-8]
Geo-neutrinos, mantle circulation and silicate earth, Gianni Fiorentini, Marcello Lissia, Fabio Mantovani, Riccardo Vannucci, PoS AHEP2003 (2003) AHEP2003/035, arXiv:hep-ph/0401085. International Workshop on Astroparticle and High-Energy Physics (AHEP-2003), Valencia, Spain, 14-18 Oct 2003.[BibTeX&LaTeX]
[7-9]
Geoneutrinos, G. Fiorentini, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/fiorentini.pdf.[BibTeX&LaTeX]
[7-10]
Neutrinos and (anti)neutrinos from supernovae and from the earth in the Borexino detector, Lino Miramonti, arXiv:hep-ex/0307029, 2003. 1st Yamada Symposium on Neutrinos and Dark Matter in Nuclear Physics June 9-14, 2003, Nara, Japan.[BibTeX&LaTeX]
[7-11]
Neutrinos from San Marco and Below, G. Fiorentini, M. Lissia, F. Mantovani, B. Ricci, arXiv:physics/0305075, 2003. Tenth International Workshop on Neutrino Telescopes, March 11-14, 2003, Venice.[BibTeX&LaTeX]
[7-12]
Neutrinos and Geology, G. Fiorentini, 2003. Seminar at Padua University, February 2003. http://www.fe.infn.it/~fiorenti/scientific%20seminars/geology.ppt.[BibTeX&LaTeX]
[7-13]
Neutrino induced charged lepton oscillations and neutrinos from the core of the earth, A. Widom, Y. Srivastava, E. Sassaroli, 1999. 8th International Workshop on Neutrino Telescopes, Venice, Italy, 23-26 Feb 1999.[BibTeX&LaTeX]


8 - Theory

[8-1]
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]


9 - Geophysics

[9-1]
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]


10 - Geophysics - Models

[10-1]
Preliminary reference earth model, A. M. Dziewonski, D. L. Anderson, Phys. Earth Planet. Interiors 25 (1981) 297-356.[BibTeX&LaTeX]


11 - Future Experiments

[11-1]
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]
[11-2]
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]
[11-3]
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]
[11-4]
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]
[11-5]
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]


12 - Future Experiments - Conference Proceedings

[12-1]
Scintillator phase of the SNO+ experiment, V. Lozza (SNO+), J. Phys. Conf. Ser. 375 (2012) 042050, arXiv:1201.6599. TAUP2011.[BibTeX&LaTeX]
[12-2]
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]
[12-3]
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]
[12-4]
The SNO+ Experiment, Mark C. Chen (SNO+), arXiv:0810.3694, 2008. ICHEP08.[BibTeX&LaTeX]
[12-5]
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]
[12-6]
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]
[12-7]
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]
[12-8]
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]
[12-9]
Geoneutrinos in Borexino, Marco G. Giammarchi, Lino Miramonti, arXiv:hep-ex/0604019, 2006. Neutrino Geophysics Honolulu, Hawaii December 14-16, 2005.[BibTeX&LaTeX]


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Authors:
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Mon 1 Sep 2014, day 244 of the year 2014, 08:29:41 UTC