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26 April 2024

» arxiv » 1507.2432

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Measurement of neutrino flux from the primary proton--proton fusion process in the Sun with Borexino detector
O. Y. Smirnov ; M. Agostini ; S. Appel ; G. Bellini ; J. Benziger ; D. Bick ; G. Bonfini ; D. Bravo ; B. Caccianiga ; F. Calaprice ; A. Caminata ; P. Cavalcante ; A. Chepurnov ; K. Choi ; D. D'Angelo ; S. Davini ; A. Derbin ; L. Di Noto ; I. Drachnev ; A. Empl ; A. Etenko ; K. Fomenko ; D. Franco ; F. Gabriele ; C. Galbiati ; C. Ghiano ; M. Giammarchi ; M. Goeger-Neff ; A. Goretti ; M. Gromov ; C. Hagner ; E. Hungerford ; Aldo Ianni ; Andrea Ianni ; K. Jedrzejczak ; M. Kaiser ; V. Kobychev ; D. Korablev ; G. Korga ; D. Kryn ; M. Laubenstein ; B. Lehnert ; E. Litvinovich ; F. Lombardi ; P. Lombardi ; L. Ludhova ; G. Lukyanchenko ; I. Machulin ; S. Manecki ; W. Maneschg ; S. Marcocci ; E. Meroni ; M. Meyer ; L. Miramonti ; M. Misiaszek ; P. Mosteiro ; V. Muratova ; B. Neumair ; L. Oberauer ; M. Obolensky ; F. Ortica ; K. Otis ; L. Pagani ; M. Pallavicini ; L. Papp ; L. Perasso ; A. Pocar ; G. Ranucci ; A. Razeto ; A. Re ; A. Romani ; R. Roncin ; N. Rossi ; S. Schönert ; D. Semenov ; H. Simgen ; M. Skorokhvatov ; A. Sotnikov ; S. Sukhotin ; Y. Suvorov ; R. Tartaglia ; G. Testera ; J. Thurn ; M. Toropova ; E. Unzhakov ; R. B. Vogelaar ; F. von Feilitzsch ; H. Wang ; S. Weinz ; J. Winter ; M. Wojcik ; M. Wurm ; Z. Yokley ; O. Zaimidoroga ; S. Zavatarelli ; K. Zuber ; G. Zuzel ;
Date:	9 Jul 2015
Abstract:	Neutrino produced in a chain of nuclear reactions in the Sun starting from the fusion of two protons, for the first time has been detected in a real-time detector in spectrometric mode. The unique properties of the Borexino detector provided an oppurtunity to disentangle pp-neutrino spectrum from the background components. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10$^{5}$ years time scale, and sets a strong limit on the power production in the unknown energy sources in the Sun of no more than 4\% of the total energy production at 90\% C.L.
Source:	arXiv, 1507.2432
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