Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

P. Mosteiro; G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; B. Caccianiga; L. Cadonati; F. Calaprice; A. Caminata; P. Cavalcante; Chavarría; A. Chepurnov; D. D'Angelo; S. Davini; A. Derbin; A. Empl; A. Etenko; K. Fomenko; D. Franco; F. Gabriele; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Göger-Neff; A. Goretti; M. Gromov; C. Hagner; E. Hungerford; Al Ianni; An Ianni; V. Kobychev; D. Korablëv; G. Korga; D. Kryn; M. Laubenstein; B. Lehnert; T. Lewke; E. Litvinovich; F. Lombardi; P. Lombardi; L. Ludhova; G. Lukyanchenko; I. Machulin; S. Manecki; W. Maneschg; S. Marcocci; Q. Meindl; E. Meroni; M. Meyer; L. Miramonti; M. Misiaszek; M. Montuschi; V. Muratova; L. Oberauer; M. Obolensky; F. Ortica; K. Otis; M. Pallavicini; L. Papp; L. Perasso; A. Pocar; G. Ranucci; A. Razeto; A. Re; A. Romani; N. Rossi; R. Saldanha; C. Salvo; S. Schönert; H. Simgen; M. Skorokhvatov; O. Smirnov; A. Sotnikov; S. Sukhotin; Y. Suvorov; R. Tartaglia; G. Testera; D. Vignaud; R. B. Vogelaar; F. von Feilitzsch; H. Wang; J. Winter; M. Wojcik; A. Wright; M. Wurm; O. Zaimidoroga; S. Zavatarelli; K. Zuber; G. Zuzel

doi:10.1016/j.nuclphysbps.2015.06.023

Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

P. Mosteiro, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, L. Cadonati, F. Calaprice, A. Caminata, P. Cavalcante, Chavarría, A. Chepurnov, D. D'Angelo, S. Davini, A. Derbin, A. Empl, A. Etenko, K. Fomenko, D. FrancoF. Gabriele, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Göger-Neff, A. Goretti, M. Gromov, C. Hagner, E. Hungerford, Al Ianni, An Ianni, V. Kobychev, D. Korablëv, G. Korga, D. Kryn, M. Laubenstein, B. Lehnert, T. Lewke, E. Litvinovich, F. Lombardi, P. Lombardi, L. Ludhova, G. Lukyanchenko, I. Machulin, S. Manecki, W. Maneschg, S. Marcocci, Q. Meindl, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, M. Montuschi, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, A. Pocar, G. Ranucci, A. Razeto, A. Re, A. Romani, N. Rossi, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R. B. Vogelaar, F. von Feilitzsch, H. Wang, J. Winter, M. Wojcik, A. Wright, M. Wurm, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel

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Abstract

The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as well as further validation of the LMA-MSW model of neutrino oscillations.

Original language	English (US)
Pages (from-to)	87-92
Number of pages	6
Journal	Nuclear and Particle Physics Proceedings
Volume	265-266
DOIs	https://doi.org/10.1016/j.nuclphysbps.2015.06.023
State	Published - Aug 2015

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.1016/j.nuclphysbps.2015.06.023

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Mosteiro, P., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarría, Chepurnov, A., D'Angelo, D., Davini, S., Derbin, A., Empl, A., Etenko, A., Fomenko, K., ... Zuzel, G. (2015). Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun. Nuclear and Particle Physics Proceedings, 265-266, 87-92. https://doi.org/10.1016/j.nuclphysbps.2015.06.023

@article{6a4c9077f7d44bc5819b59fd462e0068,

title = "Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun",

abstract = "The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as well as further validation of the LMA-MSW model of neutrino oscillations.",

author = "P. Mosteiro and G. Bellini and J. Benziger and D. Bick and G. Bonfini and D. Bravo and B. Caccianiga and L. Cadonati and F. Calaprice and A. Caminata and P. Cavalcante and Chavarr{\'i}a and A. Chepurnov and D. D'Angelo and S. Davini and A. Derbin and A. Empl and A. Etenko and K. Fomenko and D. Franco and F. Gabriele and C. Galbiati and S. Gazzana and C. Ghiano and M. Giammarchi and M. G{\"o}ger-Neff and A. Goretti and M. Gromov and C. Hagner and E. Hungerford and Al Ianni and An Ianni and V. Kobychev and D. Korabl{\"e}v and G. Korga and D. Kryn and M. Laubenstein and B. Lehnert and T. Lewke 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 Q. Meindl and E. Meroni and M. Meyer and L. Miramonti and M. Misiaszek and M. Montuschi and V. Muratova and L. Oberauer and M. Obolensky and F. Ortica and K. Otis 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 N. Rossi and R. Saldanha and C. Salvo and S. Sch{\"o}nert and H. Simgen and M. Skorokhvatov and O. Smirnov and A. Sotnikov and S. Sukhotin and Y. Suvorov and R. Tartaglia and G. Testera and D. Vignaud and Vogelaar, {R. B.} and {von Feilitzsch}, F. and H. Wang and J. Winter and M. Wojcik and A. Wright and M. Wurm and O. Zaimidoroga and S. Zavatarelli and K. Zuber and G. Zuzel",

note = "Publisher Copyright: {\textcopyright} 2015 Elsevier B.V.",

year = "2015",

month = aug,

doi = "10.1016/j.nuclphysbps.2015.06.023",

language = "English (US)",

volume = "265-266",

pages = "87--92",

journal = "Nuclear and Particle Physics Proceedings",

issn = "2405-6014",

publisher = "Elsevier B.V.",

}

Mosteiro, P, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Caccianiga, B, Cadonati, L, Calaprice, F, Caminata, A, Cavalcante, P, Chavarría, Chepurnov, A, D'Angelo, D, Davini, S, Derbin, A, Empl, A, Etenko, A, Fomenko, K, Franco, D, Gabriele, F, Galbiati, C, Gazzana, S, Ghiano, C, Giammarchi, M, Göger-Neff, M, Goretti, A, Gromov, M, Hagner, C, Hungerford, E, Ianni, A, Ianni, A, Kobychev, V, Korablëv, D, Korga, G, Kryn, D, Laubenstein, M, Lehnert, B, Lewke, T, Litvinovich, E, Lombardi, F, Lombardi, P, Ludhova, L, Lukyanchenko, G, Machulin, I, Manecki, S, Maneschg, W, Marcocci, S, Meindl, Q, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Montuschi, M, Muratova, V, Oberauer, L, Obolensky, M, Ortica, F, Otis, K, Pallavicini, M, Papp, L, Perasso, L, Pocar, A, Ranucci, G, Razeto, A, Re, A, Romani, A, Rossi, N, Saldanha, R, Salvo, C, Schönert, S, Simgen, H, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Vignaud, D, Vogelaar, RB, von Feilitzsch, F, Wang, H, Winter, J, Wojcik, M, Wright, A, Wurm, M, Zaimidoroga, O, Zavatarelli, S, Zuber, K & Zuzel, G 2015, 'Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun', Nuclear and Particle Physics Proceedings, vol. 265-266, pp. 87-92. https://doi.org/10.1016/j.nuclphysbps.2015.06.023

TY - JOUR

T1 - Low-energy (anti)neutrino physics with Borexino

T2 - Neutrinos from the primary proton-proton fusion process in the Sun

AU - Mosteiro, P.

AU - Bellini, G.

AU - Benziger, J.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Caccianiga, B.

AU - Cadonati, L.

AU - Calaprice, F.

AU - Caminata, A.

AU - Cavalcante, P.

AU - Chavarría,

AU - Chepurnov, A.

AU - D'Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Empl, A.

AU - Etenko, A.

AU - Fomenko, K.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Gazzana, S.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Göger-Neff, M.

AU - Goretti, A.

AU - Gromov, M.

AU - Hagner, C.

AU - Hungerford, E.

AU - Ianni, Al

AU - Ianni, An

AU - Kobychev, V.

AU - Korablëv, D.

AU - Korga, G.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lehnert, B.

AU - Lewke, T.

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 - Meindl, Q.

AU - Meroni, E.

AU - Meyer, M.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Montuschi, M.

AU - Muratova, V.

AU - Oberauer, L.

AU - Obolensky, M.

AU - Ortica, F.

AU - Otis, K.

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 - Rossi, N.

AU - Saldanha, R.

AU - Salvo, C.

AU - Schönert, S.

AU - Simgen, H.

AU - Skorokhvatov, M.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Sukhotin, S.

AU - Suvorov, Y.

AU - Tartaglia, R.

AU - Testera, G.

AU - Vignaud, D.

AU - Vogelaar, R. B.

AU - von Feilitzsch, F.

AU - Wang, H.

AU - Winter, J.

AU - Wojcik, M.

AU - Wright, A.

AU - Wurm, M.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuber, K.

AU - Zuzel, G.

PY - 2015/8

Y1 - 2015/8

N2 - The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as well as further validation of the LMA-MSW model of neutrino oscillations.

AB - The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as well as further validation of the LMA-MSW model of neutrino oscillations.

UR - http://www.scopus.com/inward/record.url?scp=84947573644&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84947573644&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2015.06.023

DO - 10.1016/j.nuclphysbps.2015.06.023

M3 - Article

AN - SCOPUS:84947573644

SN - 2405-6014

VL - 265-266

SP - 87

EP - 92

JO - Nuclear and Particle Physics Proceedings

JF - Nuclear and Particle Physics Proceedings

ER -

Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

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