Borexino results on neutrinos from the Sun and Earth,
Sindhujha Kumaran, Livia Ludhova, Omer Penek, Giulio Settanta,
Universe 7 (2021) 231,arXiv:2105.13858.
[Kumaran:2021lvv]
Experimental Aspects of Geoneutrino Detection: Status and Perspectives,
Oleg Smirnov,
Prog.Part.Nucl.Phys. 109 (2019) 103712,arXiv:1910.09321.
[Smirnov:2019pnj]
Abundances of uranium and thorium elements in Earth estimated by geoneutrino spectroscopy,
S. Abe et al.(KamLAND),
arXiv:2205.14934, 2022. [KamLAND:2022vbm]
Spectroscopy of geo-neutrinos from 2056 days of Borexino data,
M. Agostini et al.(Borexino),
Phys. Rev. D92 (2015) 031101,arXiv:1506.04610.
[Borexino:2015ucj]
Measurement of geo-neutrinos from 1353 days of Borexino,
G. Bellini et al.(Borexino),
Phys.Lett. B722 (2013) 295-300,arXiv:1303.2571.
[Borexino:2013tnm]
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]
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.
[KamLAND:2002uet]
Recent Borexino results and prospects for the near future,
D. D'Angelo et al.(Borexino),
EPJ Web Conf. 126 (2016) 02008,arXiv:1405.7919.
Rencontres de Moriond EW 2014. [Borexino:2014lrx]
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]
A new method of energy reconstruction for large spherical liquid scintillator detectors,
Wenjie Wu, Miao He, Xiang Zhou, Haoxue Qiao,
JINST 14 (2019) P03009,arXiv:1812.01799.
[Wu:2018zwk]
Measurement of Trace Elements in Volcanic Materials: Consequences for the Cretaceous-Tertiary Mass Extinction, Geoneutrinos and the Origin of the Hawaii's Archipelago,
Pedro V. Guillaumon, Iuda D. Goldman, Eric B. Norman, Keenan J. Thomas, Paulo R. Pascholati, Ross E. Meyer, Jordan L. Sabella, Alan R. Smith,
arXiv:2503.19921, 2025. [2503.19921]
The indication for $^{40}$K geo-antineutrino flux with Borexino phase-III data,
L. B. Bezrukov, I. S. Karpikov, V. V. Sinev,
arXiv:2304.02747, 2023. [Bezrukov:2023dwb]
Antineutrino sensitivity at THEIA,
Stephane Zsoldos, Zara Bagdasarian, Gabriel D. Orebi Gann, Andrew Barna, Stephen Dye,
Eur.Phys.J.C 82 (2022) 1151,arXiv:2204.12278.
[Zsoldos:2022mre]
On first detection of solar neutrinos from CNO cycle with Borexino,
L.B. Bezrukov, I.S. Karpikov, A.S. Kurlovich, A.K. Mezhokh, S.V.Silaeva, V.V. Sinev, V.P. Zavarzina,
Bull.Russ.Acad.Sci.Phys. 85 (2021) 430-432,arXiv:2007.07371.
[Bezrukov:2020aqv]
On the contribution of the $^{40}$K geo-antineutrino to single Borexino events,
L.B. Bezrukov, I.S. Karpikov, A.S. Kurlovich, A.K. Mezhokh, S.V. Silaeva, V.V. Sinev, V.P. Zavarzina,
arXiv:2004.02533, 2020. [Bezrukov:2020rwx]
Radiogenic power and geoneutrino luminosity of the Earth and other terrestrial bodies through time,
William F. McDonough, Ondrej Sramek, Scott A. Wipperfurth,
arXiv:1912.04655, 2019. [McDonough:2019pih]
Reference Models for Lithospheric Geoneutrino Signal,
Scott A. Wipperfurth, Ondrej Sramek, William F. McDonough,
arXiv:1907.12184, 2019. [Wipperfurth:2019idn]
JULOC: A Local 3-D Refined Crust Model for the Geoneutrino Measurement at JUNO,
Ruohan Gao, Zhiwei Li, Ran Han, Andong Wang, Yu-Feng Li, Yufei Xi, Jingao Liu, Xin Mao, Yao Sun, Ya Xu,
Physics of the Earth and Planetary Interiors 299 (2020) 106409,arXiv:1903.11871.
[Gao:2019pvi]
GIGJ: a crustal gravity model of the Guangdong Province for predicting the geoneutrino signal at the JUNO experiment,
M. Reguzzoni et al.,
J.Geophys.Res.Solid Earth 124 (2019) 4231-4249,arXiv:1901.01945.
[Reguzzoni:2019tir]
Geoneutrinos in Large Direct Detection Experiments,
Graciela B. Gelmini, Volodymyr Takhistov, Samuel J. Witte,
Phys.Rev. D99 (2019) 093009,arXiv:1812.05550.
[Gelmini:2018gqa]
Testing a proposed 'second continent' beneath eastern China using geoneutrino measurements,
Bedrich Roskovec, Ondrej Sramek, William F. McDonough,
arXiv:1810.10914, 2018. [Roskovec:2018qxg]
Perceiving the crust in 3D: a model integrating geological, geochemical, and geophysical data,
Virginia Strati, Scott A. Wipperfurth, Marica Baldoncini, William F. McDonough, Fabio Mantovani,
arXiv:1712.04676, 2017. [Strati:2017rkj]
Exploring the hidden interior of the Earth with directional neutrino measurements,
Michael Leyton, Stephen Dye, Jocelyn Monroe,
Nature Commun. 8 (2017) 15989,arXiv:1710.06724.
[Leyton:2017tza]
Potential of Geo-neutrino Measurements at JUNO,
Ran Han, Yu-Feng Li, Liang Zhan, William F McDonough, Jun Cao,
Chin. Phys. C40 (2016) 033003,arXiv:1510.01523.
[Han:2015roa]
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]
A reference worldwide model for antineutrinos from reactors,
Marica Baldoncini et al.,
Phys. Rev. D91 (2015) 065002,arXiv:1411.6475.
[Baldoncini:2014vda]
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]
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]
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]
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]
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]
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]
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]
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]
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]
The KamLAND-experiment and Soliton-like Nuclear Georeactor. Part 1. Comparison of Theory with Experiment,
V.D. Rusov et al.,
J.Mod.Phys. 4 (2013) 528-550,arXiv:1011.3568.
[Rusov:2010bk]
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]
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]
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]
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]
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]
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]
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]
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]
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:2004nvt]
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]
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]
Antineutrino Spectrum of the Earth and the Problem of Oscillating Geoantineutrino Deficit,
V.D. Rusov et al.,
arXiv:hep-ph/0312296, 2003. [Rusov:2003sx]
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]
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]
KamLAND, terrestrial heat sources and neutrino oscillations,
G. Fiorentini et al.,
Phys. Lett. B558 (2003) 15,arXiv:hep-ph/0301042.
[Fiorentini:2003ww]
Measuring the global radioactivity in the earth by multidetector anti-neutrino spectroscopy,
R. S. Raghavan et al.,
Phys. Rev. Lett. 80 (1998) 635-638. [Raghavan:1997gw]
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.
[Rothschild:1997dd]
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. [Vergados:2011ym]
Considerations For a Dedicated Geoneutrino Detector For Geosciences,
P. Ila, W. Gosnold, P. Jagam, G. I. Lykken(GRAFG),
arXiv:0902.3607, 2009.AGU 2008. [Ila:2009cm]
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. [Bellini:2007wj]
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. [Fogli:2004vb]
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. [Miramonti:2003hw]
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. [Fiorentini:2003pq]
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. [Widom:1999my]
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. [Rusov:2006pu]
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.
[Bao:1999baf]
A newly developed multi-kilo-channel high-speed and precision waveform digitization system for neutrino experiments,
H. Yang et al.,
Nucl.Instrum.Meth.A 1072 (2025) 170211,arXiv:2404.10373.
[Yang:2024zwm]
Probing Earth's Missing Potassium using the Unique Antimatter Signature of Geoneutrinos,
A. Cabrera et al.(LiquidO Consortium),
arXiv:2308.04154, 2023. [LiquidOConsortium:2023bqe]
Performance of the 1-ton Prototype Neutrino Detector at CJPL-I,
Yiyang Wu et al.,
Nucl.Instrum.Meth.A 1054 (2023) 168400,arXiv:2212.13158.
[Wu:2022oxo]
Measurement of Muon-induced Neutron Production at China Jinping Underground Laboratory,
Lin Zhao et al.,
Chin.Phys.C 46 (2022) 085001,arXiv:2108.04010.
[JNE:2021cyb]
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. [Barabanov:2009rk]
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.
[Autiero:2007zj]
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.
[Dye:2006gx]
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.
[Borexino:2006qmb]
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.
[deMeijer:2004wq]
New methods of neutrino and anti-neutrino detection from 0.115 to 105 MeV,
Nickolas Solomey et al.,
arXiv:2411.05615, 2024.25th International Workshop on Neutrinos from Accelerators. [Solomey:2024cgv]
Geoneutrinos and reactor antineutrinos at SNO+,
M Baldoncini et al.,
J. Phys. Conf. Ser. 718 (2016) 062003,arXiv:1607.05959.
XIV International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015). [Baldoncini:2016mbp]
The Physics Potential of the LENA Detector,
Michael Wurm et al.,
Acta Phys. Polon. B41 (2010) 1749-1764,arXiv:1004.3474.
Cracow Epiphany Conference, 5-8 January 2010. [Wurm:2010ny]
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. [Learned:2007zz]
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. [Batygov:2008mr]
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. [Dye:2006hg]
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. [Hochmuth:2006gz]
A geoneutrino experiment at Homestake,
N. Tolich et al.,
Earth Moon Planets (2006) 229-240,arXiv:physics/0607230.
Neutrino Sciences 2005: Neutrino Geophysics, Honolulu, HI, 14-16 Dec 2005. [Tolich:2006nr]
Geoneutrinos in Borexino,
Marco G. Giammarchi, Lino Miramonti,
arXiv:hep-ex/0604019, 2006.Neutrino Geophysics Honolulu, Hawaii December 14-16, 2005. [Giammarchi:2006up]
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