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Related papers: A geoneutrino experiment at Homestake

200 papers

Geo-neutrinos, electron anti-neutrinos produced in beta decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet's interior. We report the first observation at more than 3$\sigma$ C.L. of…

High Energy Physics - Experiment · Physics 2012-08-27 Borexino Collaboration

We comment on the first indication of geo-neutrino events from KamLAND and on the prospects for understanding Earth energetics. Practically all models of terrestrial heat production are consistent with data within the presently limited…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Fiorentini , T. Lasserre , M. Lissia , B. Ricci , S. Schonert

Geo-reactor models suggest the existence of natural nuclear reactors at different deep-earth locations with loosely defined output power. Reactor fission products undergo beta decay with the emission of electron antineutrinos, which…

Nuclear Experiment · Physics 2010-02-09 S. T. Dye

Order of magnitude estimates of radiogenic heat and antineutrino production are given, using the San Marco cathedral as an example. Prospects of determining the radiogenic contribution to terrestrial heat by detection of antineutrinos from…

Geophysics · Physics 2007-05-23 G. Fiorentini , M. Lissia , F. Mantovani , B. Ricci

The paper focuses on a proposal for an underground antineutrino antenna to further develop the dectection of these particles as a tool to map the distribution of radiogenic heat sources, such as the natural radionuclides and a hypothetical…

Geophysics · Physics 2007-05-23 R. J. de Meijer , E. R. van der Graaf , K. P. Jungmann

Earth neutrino tomography is a realistic possibility with current and future neutrino detectors, complementary to geophysics methods. The two main approaches are based on either partial absorption of the neutrino flux as it propagates…

High Energy Physics - Phenomenology · Physics 2024-08-05 Rasmi Hajjar , Olga Mena , Sergio Palomares-Ruiz

Geo-neutrinos emitted by heat-producing elements (U, Th and K) represent a unique probe of the Earth interior. The characterization of their fluxes is subject, however, to rather large and highly correlated uncertainties. The geochemical…

Geophysics · Physics 2009-11-13 G. L. Fogli , E. Lisi , A. Palazzo , A. M. Rotunno

More than 40 years ago, neutrinos where conceived as a way to test the validity of the solar models which tell us that stars are powered by nuclear fusion reactions. The first measurement of the neutrino flux, in 1968 in the Homestake mine…

High Energy Physics - Experiment · Physics 2009-05-12 Lino Miramonti

We predict geoneutrino fluxes in a reference model based on a detailed description of Earth's crust and mantle and using the best available information on the abundances of uranium, thorium, and potassium inside Earth's layers. We estimate…

High Energy Physics - Phenomenology · Physics 2011-01-04 Fabio Mantovani , Luigi Carmignani , Gianni Fiorentini , Marcello Lissia

Geothermal energy is the key to drive the plate tectonics and interior thermodynamics of the Earth. The surface heat flux, as measured in boreholes, provide limited insights into the relative contributions of primordial versus radiogenic…

Geophysics · Physics 2020-01-08 Ruohan Gao , Zhiwei Li , Ran Han , Andong Wang , Yu-Feng Li , Yufei Xi , Jingao Liu , Xin Mao , Yao Sun , Ya Xu

The connection between geoneutrino registration and the Earth theory test is discussed. We compare standard theory of lithosphere plates and hypothesis of hydride Earth. Last hypothesis adds additional neutrino source $-$ planet core in…

High Energy Physics - Phenomenology · Physics 2010-07-16 V. V. Sinev

The terrestrial distribution of U, Th, and K abundances governs the thermal evolution, traces the differentiation, and reflects the bulk composition of the earth. Comparing the bulk earth composition to chondritic meteorites estimates the…

Geophysics · Physics 2015-05-19 Steve Dye

Estimated masses of fissioning and non-fissioning radioactive elements and their respective distributions within the Earth are presented, based upon the fundamental identity of the components of the interior 82% of the Earth, the…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. Marvin Herndon , Dennis A. Edgerley

The deepest hole that has ever been dug is about 12 km deep. Geochemists analyze samples from the Earth's crust and from the top of the mantle. Seismology can reconstruct the density profile throughout all Earth, but not its composition. In…

Geophysics · Physics 2008-11-26 Gianni Fiorentini , Marcello Lissia , Fabio Mantovani

The unknown constituents of the interior of our home planet have provoked the human imagination and driven scientific exploration. We herein demonstrate that large neutrino detectors could be used in the near future to significantly improve…

Geophysics · Physics 2015-10-23 Carsten Rott , Akimichi Taketa , Debanjan Bose

This paper presents a geoneutrino measurement using 3262.74 days of data taken with the Borexino detector at LNGS in Italy. By observing $52.6 ^{+9.4}_{-8.6} ({\rm stat}) ^{+2.7}_{-2.1}({\rm sys})$ geoneutrinos (68% interval) from $^{238}$U…

High Energy Physics - Experiment · Physics 2020-02-18 M. Agostini , K. Altenmüller , S. Appel , V. Atroshchenko , Z. Bagdasarian , D. Basilico , G. Bellini , J. Benziger , D. Bick , G. Bonfini , D. Bravo , B. Caccianiga , F. Calaprice , A. Caminata , L. Cappelli , P. Cavalcante , F. Cavanna , A. Chepurnov , K. Choi , D. D'Angelo , S. Davini , A. Derbin , A. Di Giacinto , V. Di Marcello , X. F. Ding , A. Di Ludovico , L. Di Noto , I. Drachnev , G. Fiorentini , A. Formozov , D. Franco , F. Gabriele , C. Galbiati , M. Gschwender , C. Ghiano , M. Giammarchi , A. Goretti , M. Gromov , D. Guffanti , C. Hagner , E. Hungerford , Aldo Ianni , Andrea Ianni , A. Jany , D. Jeschke , S. Kumaran , V. Kobychev , G. Korga , T. Lachenmaier , T. Lasserre , M. Laubenstein , E. Litvinovich , P. Lombardi , I. Lomskaya , L. Ludhova , G. Lukyanchenko , L. Lukyanchenko , I. Machulin , F. Mantovani , G. Manuzio , S. Marcocci , J. Maricic , J. Martyn , E. Meroni , M. Meyer , L. Miramonti , M. Misiaszek , M. Montuschi , V. Muratova , B. Neumair , M. Nieslony , L. Oberauer , A. Onillon , V. Orekhov , F. Ortica , M. Pallavicini , L. Papp , Ö. Penek , L. Pietrofaccia , N. Pilipenko , A. Pocar , G. Raikov , M. T. Ranalli , G. Ranucci , A. Razeto , A. Re , M. Redchuk , B. Ricci , A. Romani , N. Rossi , S. Rottenanger , S. Schönert , D. Semenov , M. Skorokhvatov , O. Smirnov , A. Sotnikov , V. Strati , Y. Suvorov , R. Tartaglia , G. Testera , J. Thurn , E. Unzhakov , A. Vishneva , M. Vivier , R. B. Vogelaar , F. von Feilitzsch , M. Wojcik , M. Wurm , O. Zaimidoroga , S. Zavatarelli , K. Zuber , G. Zuzel

A measurement of the absorption of neutrinos with energies in excess of 10 TeV when traversing the Earth is capable of revealing its density distribution. Unfortunately, the existence of beams with sufficient luminosity for the task has…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. C. Gonzalez-Garcia , Francis Halzen , Michele Maltoni , Hiroyuki K. M. Tanaka

Energy spectra of antineutrinos coming from $^{232}$Th and $^{233}$U neutron-induced fission are calculated, relevant inverse beta decay $\bar{{\nu}_e}+p \to n + e^{+}$ positron spectra and total cross sections are found. This study is…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Domogatski , V. Kopeikin , L. Mikaelyan , V. Sinev

Every second greater than $10^{25}$ antineutrinos radiate to space from Earth, shining like a faint antineutrino star. Underground antineutrino detectors have revealed the rapidly decaying fission products inside nuclear reactors, verified…

Instrumentation and Detectors · Physics 2016-02-04 Shawn M. Usman , Glenn R. Jocher , Stephen T. Dye , William F. McDonough , John G. Learned

Geoneutrinos, the electron (anti)neutrinos generated in decays or decay chains of the radioactive elements within the Earth, primarily K-40, U-238, and Th-232, serve as a unique probe for the inner chemical composition of the Earth. A…

High Energy Physics - Experiment · Physics 2026-04-02 Haozhe Sun , Zhe Wang , Shaomin Chen