Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector

O. Yu 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

doi:10.1134/S106377961606023X

Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector

O. Yu 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

Joint Inst. for Nuclear Research
Cluster of Excellence E-conversion
University of Milan
Department of Chemical Engineering
Universität Hamburg
Laboratori Nazionali del Gran Sasso
Virginia Polytechnic Institute and State University
Princeton University
Istituto Nazionale per la Fisica della Materia
Moscow State University
University of Hawaii
Gran Sasso Science Institute
Petersburg Nuclear Phys. Inst.
Center for Nuclear Receptors and Cell Signaling, University of Houston
National Research Centre "Kurchatov Institute"
Université Paris Diderot
Jagiellonian University
Institute for Nuclear Research
Technische Universität Dresden
National Research Nuclear University MEPhI
Max-Planck-Institut für Kernphysik
INFN Sezione di Perugia
University of Massachusetts Amherst
University of California at Los Angeles
Johannes Gutenberg University

Research output: Contribution to journal › Article › peer-review

10 Scopus citations

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 10⁵ 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.

Original language	English
Pages (from-to)	995-1002
Number of pages	8
Journal	Physics of Particles and Nuclei
Volume	47
Issue number	6
DOIs	https://doi.org/10.1134/S106377961606023X
State	Published - 1 Nov 2016
Externally published	Yes

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10.1134/S106377961606023X

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Smirnov, O. Y., Agostini, M., Appel, S., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chepurnov, A., Choi, K., D’Angelo, D., Davini, S., Derbin, A., Di Noto, L., Drachnev, I., ... Zuzel, G. (2016). Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector. Physics of Particles and Nuclei, 47(6), 995-1002. https://doi.org/10.1134/S106377961606023X

@article{dff7d12f9a414311a4d6b362dbdb63ac,

title = "Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector",

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 105 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.",

author = "Smirnov, \{O. Yu\} and M. Agostini and S. Appel and G. Bellini and J. Benziger and D. Bick and G. Bonfini and D. Bravo and B. Caccianiga and F. Calaprice and A. Caminata and P. Cavalcante and A. Chepurnov and K. Choi and D. D{\textquoteright}Angelo and S. Davini and A. Derbin and \{Di Noto\}, L. and I. Drachnev and A. Empl and A. Etenko and K. Fomenko and D. Franco and F. Gabriele and C. Galbiati and C. Ghiano and M. Giammarchi and M. Goeger-Neff and A. Goretti and M. Gromov and C. Hagner and E. Hungerford and Aldo Ianni and Andrea Ianni and K. Jedrzejczak and M. Kaiser and V. Kobychev and D. Korablev and G. Korga and D. Kryn and M. Laubenstein and B. Lehnert and E. Litvinovich and F. Lombardi and P. Lombardi and L. Ludhova and G. Lukyanchenko and I. Machulin and S. Manecki and W. Maneschg and S. Marcocci and E. Meroni and M. Meyer and L. Miramonti and M. Misiaszek and P. Mosteiro and V. Muratova and B. Neumair and L. Oberauer and M. Obolensky and F. Ortica and K. Otis and L. Pagani and M. Pallavicini and L. Papp and L. Perasso and A. Pocar and G. Ranucci and A. Razeto and A. Re and A. Romani and R. Roncin and N. Rossi and S. Sch{\"o}nert and D. Semenov and H. Simgen and M. Skorokhvatov and A. Sotnikov and S. Sukhotin and Y. Suvorov and R. Tartaglia and G. Testera and J. Thurn and M. Toropova and E. Unzhakov and Vogelaar, \{R. B.\} and \{von Feilitzsch\}, F. and H. Wang and S. Weinz and J. Winter and M. Wojcik and M. Wurm and Z. Yokley and O. Zaimidoroga and S. Zavatarelli and K. Zuber and G. Zuzel",

note = "Publisher Copyright: {\textcopyright} 2016, Pleiades Publishing, Ltd.",

year = "2016",

month = nov,

day = "1",

doi = "10.1134/S106377961606023X",

language = "English",

volume = "47",

pages = "995--1002",

journal = "Physics of Particles and Nuclei",

issn = "1063-7796",

publisher = "Pleiades Publishing",

number = "6",

}

Smirnov, OY, Agostini, M, Appel, S, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Caccianiga, B, Calaprice, F, Caminata, A, Cavalcante, P, Chepurnov, A, Choi, K, D’Angelo, D, Davini, S, Derbin, A, Di Noto, L, Drachnev, I, Empl, A, Etenko, A, Fomenko, K, Franco, D, Gabriele, F, Galbiati, C, Ghiano, C, Giammarchi, M, Goeger-Neff, M, Goretti, A, Gromov, M, Hagner, C, Hungerford, E, Ianni, A, Ianni, A, Jedrzejczak, K, Kaiser, M, Kobychev, V, Korablev, D, Korga, G, Kryn, D, Laubenstein, M, Lehnert, B, Litvinovich, E, Lombardi, F, Lombardi, P, Ludhova, L, Lukyanchenko, G, Machulin, I, Manecki, S, Maneschg, W, Marcocci, S, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Mosteiro, P, Muratova, V, Neumair, B, Oberauer, L, Obolensky, M, Ortica, F, Otis, K, Pagani, L, Pallavicini, M, Papp, L, Perasso, L, Pocar, A, Ranucci, G, Razeto, A, Re, A, Romani, A, Roncin, R, Rossi, N, Schönert, S, Semenov, D, Simgen, H, Skorokhvatov, M, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Thurn, J, Toropova, M, Unzhakov, E, Vogelaar, RB, von Feilitzsch, F, Wang, H, Weinz, S, Winter, J, Wojcik, M, Wurm, M, Yokley, Z, Zaimidoroga, O, Zavatarelli, S, Zuber, K & Zuzel, G 2016, 'Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector', Physics of Particles and Nuclei, vol. 47, no. 6, pp. 995-1002. https://doi.org/10.1134/S106377961606023X

TY - JOUR

T1 - Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector

AU - Smirnov, O. Yu

AU - Agostini, M.

AU - Appel, S.

AU - Bellini, G.

AU - Benziger, J.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Caccianiga, B.

AU - Calaprice, F.

AU - Caminata, A.

AU - Cavalcante, P.

AU - Chepurnov, A.

AU - Choi, K.

AU - D’Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Di Noto, L.

AU - Drachnev, I.

AU - Empl, A.

AU - Etenko, A.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goeger-Neff, M.

AU - Goretti, A.

AU - Gromov, M.

AU - Hagner, C.

AU - Hungerford, E.

AU - Ianni, Aldo

AU - Ianni, Andrea

AU - Jedrzejczak, K.

AU - Kaiser, M.

AU - Kobychev, V.

AU - Korablev, D.

AU - Korga, G.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lehnert, B.

AU - Litvinovich, E.

AU - Lombardi, F.

AU - Lombardi, P.

AU - Ludhova, L.

AU - Lukyanchenko, G.

AU - Machulin, I.

AU - Manecki, S.

AU - Maneschg, W.

AU - Marcocci, S.

AU - Meroni, E.

AU - Meyer, M.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Mosteiro, P.

AU - Muratova, V.

AU - Neumair, B.

AU - Oberauer, L.

AU - Obolensky, M.

AU - Ortica, F.

AU - Otis, K.

AU - Pagani, L.

AU - Pallavicini, M.

AU - Papp, L.

AU - Perasso, L.

AU - Pocar, A.

AU - Ranucci, G.

AU - Razeto, A.

AU - Re, A.

AU - Romani, A.

AU - Roncin, R.

AU - Rossi, N.

AU - Schönert, S.

AU - Semenov, D.

AU - Simgen, H.

AU - Skorokhvatov, M.

AU - Sotnikov, A.

AU - Sukhotin, S.

AU - Suvorov, Y.

AU - Tartaglia, R.

AU - Testera, G.

AU - Thurn, J.

AU - Toropova, M.

AU - Unzhakov, E.

AU - Vogelaar, R. B.

AU - von Feilitzsch, F.

AU - Wang, H.

AU - Weinz, S.

AU - Winter, J.

AU - Wojcik, M.

AU - Wurm, M.

AU - Yokley, Z.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuber, K.

AU - Zuzel, G.

PY - 2016/11/1

Y1 - 2016/11/1

N2 - 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 105 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.

AB - 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 105 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.

UR - https://www.scopus.com/pages/publications/85013949281

U2 - 10.1134/S106377961606023X

DO - 10.1134/S106377961606023X

M3 - Article

AN - SCOPUS:85013949281

SN - 1063-7796

VL - 47

SP - 995

EP - 1002

JO - Physics of Particles and Nuclei

JF - Physics of Particles and Nuclei

IS - 6

ER -

Measurement of neutrino flux from the primary proton–proton fusion process in the Sun with Borexino detector

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