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Related papers: Comprehensive geoneutrino analysis with Borexino

200 papers

Neutrinos emitted in the carbon, nitrogen, oxygen (CNO) fusion cycle in the Sun are a sub-dominant, yet crucial component of solar neutrinos whose flux has not been measured yet. The Borexino experiment at the Laboratori Nazionali del Gran…

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

Borexino is an organic liquid scintillator detector located in the underground Gran Sasso National Laboratory (Italy). It is devoted mainly to the real time spectroscopy of low energy solar neutrinos via the elastic scattering on electrons…

High Energy Physics - Experiment · Physics 2019-08-13 Davide D'Angelo

Roughly 40% of the Earth's total heat flow is powered by radioactive decays in the crust and mantle. Geo-neutrinos produced by these decays provide important clues about the origin, formation and thermal evolution of our planet, as well as…

Geophysics · Physics 2017-10-20 Michael Leyton , Stephen Dye , Jocelyn Monroe

We report on an improved measurement of the $^8$B solar neutrino interaction rate with the Borexino experiment at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected via their elastic scattering on electrons in a large volume of…

Geoneutrinos serve as a potent tool for comprehending the radiogenic power and composition of Earth. Although geoneutrinos have been observed in prior experiments, the forthcoming generation of experiments,such as JUNO, will be necessary…

Antineutrinos produced at nuclear reactors constitute a severe source of background for the detection of geoneutrinos, which bring to the Earth's surface information about natural radioactivity in the whole planet. In this framework we…

Instrumentation and Detectors · Physics 2015-06-23 Marica Baldoncini , Ivan Callegari , Giovanni Fiorentini , Fabio Mantovani , Barbara Ricci , Virginia Strati , Gerti Xhixha

Geo-neutrinos, electron antineutrinos from natural radioactive decays inside the Earth, bring to the surface unique information about our planet. The new techniques in neutrino detection opened a door into a completely new…

High Energy Physics - Experiment · Physics 2014-09-01 Livia Ludhova , Sandra Zavatarelli

The solar neutrino experiment Borexino, which is located in the Gran Sasso underground laboratories, is in a unique position to study muon-induced backgrounds in an organic liquid scintillator. In this study, a large sample of cosmic muons…

Borexino is a massive, calorimetric, liquid scintillator detector aimed at the detection of low energy sub-MeV solar neutrinos, installed at the Gran Sasso Laboratory. After several years of construction, data taking started in May 2007,…

High Energy Physics - Experiment · Physics 2008-10-02 G. Ranucci , Borexino Collaboration

We estimate terrestrial antineutrino and neutrino fluxes according to different models of Earth composition. We find large variations, corresponding to uncertainties on the estimated $U$, $Th$ and $K$ abundances in the mantle. Information…

Nuclear Experiment · Physics 2009-11-07 G. Fiorentini , F. Mantovani , B. Ricci

The SNO+ collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 tonne-years of new data. The measured energies of reactor antineutrino candidates were fitted to obtain the second-most precise…

High Energy Physics - Experiment · Physics 2025-09-18 SNO+ Collaboration , : , M. Abreu , V. Albanese , A. Allega , R. Alves , M. R. Anderson , S. Andringa , L. Anselmo , J. Antunes , E. Arushanova , S. Asahi , M. Askins , D. M. Asner , D. J. Auty , A. R. Back , S. Back , A. Bacon , T. Baltazar , F. Barão , Z. Barnard , A. Barr , N. Barros , D. Bartlett , R. Bayes , C. Beaudoin , E. W. Beier , G. Berardi , T. S. Bezerra , A. Bialek , S. D. Biller , E. Blucher , A. Boeltzig , R. Bonventre , M. Boulay , D. Braid , E. Caden , E. J. Callaghan , J. Caravaca , J. Carvalho , L. Cavalli , D. Chauhan , M. Chen , S. Cheng , O. Chkvorets , K. J. Clark , B. Cleveland , C. Connors , D. Cookman , J. Corning , I. T. Coulter , M. A. Cox , D. Cressy , X. Dai , C. Darrach , S. DeGraw , R. Dehghani , J. Deloye , M. M. Depatie , F. Descamps , C. Dima , J. Dittmer , K. H. Dixon , F. Di Lodovico , A. Doxtator , N. Duhaime , F. Duncan , J. Dunger , A. D. Earle , M. S. Esmaeilian , D. Fabris , E. Falk , A. Farrugia , N. Fatemighomi , C. Felber , V. Fischer , E. Fletcher , R. Ford , K. Frankiewicz , N. Gagnon , A. Gaur , J. Gauthier , A. Gibson-Foster , K. Gilje , O. I. González-Reina , D. Gooding , P. Gorel , K. Graham , C. Grant , J. Grove , S. Grullon , E. Guillian , R. L. Hahn , S. Hall , A. L. Hallin , D. Hallman , S. Hans , J. Hartnell , P. Harvey , C. Hearns , M. R. Hebert , M. Hedayatipour , W. J. Heintzelman , J. Heise , R. L. Helmer , C. Hewitt , B. Hodak , M. Hodak , M. Hood , D. Horne , M. Howe , B. Hreljac , J. Hu , P. Huang , R. Hunt-Stokes , T. Iida , A. S. Inácio , C. M. Jackson , N. A. Jelley , C. J. Jillings , C. Jones , P. G. Jones , S. Kaluzienski , K. Kamdin , T. Kaptanoglu , J. Kaspar , K. Keeter , C. Kefelian , P. Khaghani , L. Kippenbrock , J. Kladnik , J. R. Klein , R. Knapik , J. Kofron , L. L. Kormos , S. Korte , B. Krar , C. Kraus , C. B. Krauss , T. Kroupová , K. Labe , F. Lafleur , C. Lake , I. Lam , C. Lan , B. J. Land , R. Lane , S. Langrock , P. Larochelle , S. Larose , A. LaTorre , I. Lawson , L. Lebanowski , J. Lee , C. Lefebvre , G. M. Lefeuvre , E. J. Leming , A. Li , O. Li , J. Lidgard , B. Liggins , P. Liimatainen , Y. H. Lin , X. Liu , Y. Liu , V. Lozza , M. Luo , S. Maguire , A. Maio , K. Majumdar , S. Manecki , J. Maneira , R. D. Martin , E. Marzec , A. Mastbaum , A. Mathewson , N. McCauley , A. B. McDonald , K. McFarlane , P. Mekarski , M. Meyer , C. Miller , C. Mills , G. Milton , M. Mlejnek , E. Mony , B. Morissette , D. Morris , I. Morton-Blake , M. J. Mottram , M. Mubasher , S. Nae , S. Naugle , M. Newcomer , M. Nirkko , L. J. Nolan , V. M. Novikov , H. M. O'Keeffe , E. O'Sullivan , G. D. Orebi Gann , S. Ouyang , J. Page , S. Pal , K. Paleshi , W. Parker , M. J. Parnell , J. Paton , S. J. M. Peeters , T. Pershing , Z. Petriw , J. Petzoldt , L. J. Pickard , D. Pracsovics , G. Prior , J. C. Prouty , B. Quenallata , S. Quirk , P. Ravi , S. Read , A. Reichold , M. Reinhard , S. Riccetto , M. Rigan , I. Ritchie , A. Robertson , B. C. Robertson , J. Rose , R. Rosero , P. M. Rost , J. Rumleskie , A. Sörensen , P. Schrock , M. A. Schumaker , M. H. Schwendener , D. Scislowski , J. Secrest , M. Seddighin , L. Segui , S. Seibert , I. Semenec , F. Shaker , T. Shantz , M. K. Sharma , J. Shen , T. M. Shokair , L. Sibley , J. Simms , J. R. Sinclair , K. Singh , P. Skensved , M. Smiley , T. Sonley , M. St-Amant , R. Stainforth , S. Stankiewicz , M. Strait , M. I. Stringer , A. Stripay , R. Svoboda , S. Tacchino , R. Tafirout , B. Tam , C. Tanguay , J. Tatar , L. Tian , N. Tolich , J. Tseng , H. W. C. Tseung , E. Turner , E. Vázquez-Jáuregui , S. Valder , R. Van Berg , J. G. C. Veinot , C. J. Virtue , B. von Krosigk , J. M. G. Walker , M. Walker , J. Wallig , S. C. Walton , F. Wang , J. Wang , M. Ward , J. Waterfield , J. J. Weigand , R. F. White , J. F. Wilkerson , J. R. Wilson , J. D. Wilson , T. J. Winchester , P. Woosaree , A. Wright , S. Yang , K. Yazigi , Z. Ye , M. Yeh , S. Yu , T. Zhang , Y. Zhang , T. Zhao , K. Zuber , A. Zummo

Borexino is a massive calorimetric liquid scintillation detector whose installation has been completed in the underground Gran Sasso Laboratory. The focus of the experiment is on the direct and real time measurement of the flux of neutrinos…

High Energy Physics - Experiment · Physics 2007-05-23 Lino Miramonti

High flux of geoantineutrinos $^{40}$K and geoneutrinos $^{40}$K ($^{40}$K-geo-($\bar{\nu} + \nu$)) can be obtained from reanalysis of the Borexino Phase III data. Large amounts of $^{40}$K should produce a significant heat flow that should…

High Energy Physics - Phenomenology · Physics 2026-02-18 Ivan Karpikov

The review is conceived to help the reader to interpret present geoneutrino results in the framework of Earth's energetics and composition. Starting from the comprehension of antineutrino production, propagation, and detection, the status…

In the heart of the Creighton Mine near Sudbury (Canada), the SNO+ detector is foreseen to observe almost in equal proportion electron antineutrinos produced by U and Th in the Earth and by nuclear reactors. SNO+ will be the first long…

Geophysics · Physics 2016-07-21 M Baldoncini , V Strati , S A Wipperfurth , G Fiorentini , F Mantovani , W F McDonough , B Ricci

Borexino is a solar neutrino experiment running at the Laboratori Nazionali del Gran Sasso, Italy. The radioactive background levels in the liquid scintillator target meet or even exceed design goals, opening unanticipated opportunities.…

Solar and Stellar Astrophysics · Physics 2019-08-13 M. Pallavicini

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

Geoneutrinos are electron antineutrinos ($\bar\nu_e$) generated by the beta-decays of radionuclides naturally occurring inside the Earth, in particular $^{238}$U, $^{232}$Th, and $^{40}$K. Measurement of these neutrinos provides powerful…

High Energy Physics - Experiment · Physics 2017-03-08 Linyan Wan , Ghulam Hussain , Zhe Wang , Shaomin Chen