Results from Borexino on solar and geo-neutrinos

Daniele Guffanti; M. Agostini; K. Altenmüller; S. Appel; V. Atroshchenko; Z. Bagdasarian; D. Basilico; G. Bellini; Jay Burton Benziger; G. Bonfini; D. Bravo; B. Caccianiga; Frank Calaprice; A. Caminata; L. Cappelli; S. Caprioli; M. Carlini; P. Cavalcante; F. Cavanna; A. Chepurnov; K. Choi; L. Collica; D. D'Angelo; S. Davini; A. Derbin; X. F. Ding; A. Di Ludovico; L. Di Noto; I. Drachnev; K. Fomenko; A. Formozov; D. Franco; F. Gabriele; C. Galbiati; M. Gschwender; C. Ghiano; M. Giammarchi; A. Goretti; M. Gromov; D. Guffanti; T. Houdy; E. Hungerford; Aldo Ianni; Andrea Ianni; A. Jany; D. Jeschke; S. Kumaran; V. Kobychev; G. Korga; T. Lachenmaier; M. Laubenstein; E. Litvinovich; P. Lombardi; L. Ludhova; G. Lukyanchenko; L. Lukyanchenko; I. MacHulin; G. Manuzio; S. Marcocci; J. Maricic; J. Martyn; E. Meroni; M. Meyer; L. Miramonti; M. Misiaszek; V. Muratova; B. Neumair; M. Nieslony; L. Oberauer; V. Orekhov; F. Ortica; M. Pallavicini; L. Papp; Penek; L. Pietrofaccia; N. Pilipenko; A. Pocar; A. Porcelli; G. Raikov; G. Ranucci; A. Razeto; A. Re; M. Redchuk; A. Romani; N. Rossi; S. Rottenanger; S. Schönert; D. Semenov; M. Skorokhvatov; O. Smirnov; A. Sotnikov; L. F.F. Stokes; Y. Suvorov; R. Tartaglia; G. Testera; J. Thurn; E. Unzhakov; A. Vishneva; R. B. Vogelaar; F. Von Feilitzsch; S. Weinz; M. Wojcik; M. Wurm; O. Zaimidoroga; S. Zavatarelli; K. Zuber; G. Zuzel

Results from Borexino on solar and geo-neutrinos

Daniele Guffanti, M. Agostini, K. Altenmüller, S. Appel, V. Atroshchenko, Z. Bagdasarian, D. Basilico, G. Bellini, Jay Burton Benziger, G. Bonfini, D. Bravo, B. Caccianiga, Frank Calaprice, A. Caminata, L. Cappelli, S. Caprioli, M. Carlini, P. Cavalcante, F. Cavanna, A. ChepurnovK. Choi, L. Collica, D. D'Angelo, S. Davini, A. Derbin, X. F. Ding, A. Di Ludovico, L. Di Noto, I. Drachnev, K. Fomenko, A. Formozov, D. Franco, F. Gabriele, C. Galbiati, M. Gschwender, C. Ghiano, M. Giammarchi, A. Goretti, M. Gromov, D. Guffanti, T. Houdy, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, D. Jeschke, S. Kumaran, V. Kobychev, G. Korga, T. Lachenmaier, M. Laubenstein, E. Litvinovich, P. Lombardi, L. Ludhova, G. Lukyanchenko, L. Lukyanchenko, I. MacHulin, G. Manuzio, S. Marcocci, J. Maricic, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, M. Nieslony, L. Oberauer, V. Orekhov, F. Ortica, M. Pallavicini, L. Papp, Penek, L. Pietrofaccia, N. Pilipenko, A. Pocar, A. Porcelli, G. Raikov, G. Ranucci, A. Razeto, A. Re, M. Redchuk, A. Romani, N. Rossi, S. Rottenanger, S. Schönert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, L. F.F. Stokes, Y. Suvorov, R. Tartaglia, G. Testera, J. Thurn, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. Von Feilitzsch, S. Weinz, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel

Research output: Contribution to journal › Conference article › peer-review

Abstract

Borexino is running at the INFN Gran Sasso National Laboraries, Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the foundation for the outstanding achievements accumulated by this experiment. In this contribution, after recalling the main features of the detector, the impressive solar data gathered so far by Borexino will be summarized. Special emphasis will be given to the illustration of the recent release of the fluxes as stemming from the simultaneous real time spectroscopy of the neutrinos from the entire pp nuclear fusion chain in the Sun, opening with the remarkable 2.7% accuracy of the ⁷Be flux the era of precision measurements also in the realm of the sub-MeV solar neutrinos. Such results put Borexino in the unique situation of being the only detector able to perform solar neutrino spectroscopy over the entire solar spectrum; the counterpart of this peculiar status, in the flavor conversion interpretation of the solar neutrino data, is the capability of Borexino alone to perform the full validation across the solar energy range of the MSW-LMA paradigm. This contribution will be concluded with an account of the Borexino accomplishments in the geo-neutrino field, marked by the detection of the geo-neutrino signal with a significance as high as 5:9σ.

Original language	English (US)
Article number	007
Journal	Proceedings of Science
Volume	340
State	Published - 2019
Event	39th International Conference on High Energy Physics, ICHEP 2018 - Seoul, Korea, Republic of Duration: Jul 4 2018 → Jul 11 2018

All Science Journal Classification (ASJC) codes

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Cite this

Guffanti, D., Agostini, M., Altenmüller, K., Appel, S., Atroshchenko, V., Bagdasarian, Z., Basilico, D., Bellini, G., Benziger, J. B., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cappelli, L., Caprioli, S., Carlini, M., Cavalcante, P., Cavanna, F., ... Zuzel, G. (2019). Results from Borexino on solar and geo-neutrinos. Proceedings of Science, 340, Article 007.

@article{df4372d7de9749f5aec8b50d78f5a176,

title = "Results from Borexino on solar and geo-neutrinos",

abstract = "Borexino is running at the INFN Gran Sasso National Laboraries, Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the foundation for the outstanding achievements accumulated by this experiment. In this contribution, after recalling the main features of the detector, the impressive solar data gathered so far by Borexino will be summarized. Special emphasis will be given to the illustration of the recent release of the fluxes as stemming from the simultaneous real time spectroscopy of the neutrinos from the entire pp nuclear fusion chain in the Sun, opening with the remarkable 2.7% accuracy of the 7Be flux the era of precision measurements also in the realm of the sub-MeV solar neutrinos. Such results put Borexino in the unique situation of being the only detector able to perform solar neutrino spectroscopy over the entire solar spectrum; the counterpart of this peculiar status, in the flavor conversion interpretation of the solar neutrino data, is the capability of Borexino alone to perform the full validation across the solar energy range of the MSW-LMA paradigm. This contribution will be concluded with an account of the Borexino accomplishments in the geo-neutrino field, marked by the detection of the geo-neutrino signal with a significance as high as 5:9σ.",

author = "Daniele Guffanti and M. Agostini and K. Altenm{\"u}ller and S. Appel and V. Atroshchenko and Z. Bagdasarian and D. Basilico and G. Bellini and Benziger, {Jay Burton} and G. Bonfini and D. Bravo and B. Caccianiga and Frank Calaprice and A. Caminata and L. Cappelli and S. Caprioli and M. Carlini and P. Cavalcante and F. Cavanna and A. Chepurnov and K. Choi and L. Collica and D. D'Angelo and S. Davini and A. Derbin and Ding, {X. F.} and {Di Ludovico}, A. and {Di Noto}, L. and I. Drachnev and K. Fomenko and A. Formozov and D. Franco and F. Gabriele and C. Galbiati and M. Gschwender and C. Ghiano and M. Giammarchi and A. Goretti and M. Gromov and D. Guffanti and T. Houdy and E. Hungerford and Aldo Ianni and Andrea Ianni and A. Jany and D. Jeschke and S. Kumaran and V. Kobychev and G. Korga and T. Lachenmaier and M. Laubenstein and E. Litvinovich and P. Lombardi and L. Ludhova and G. Lukyanchenko and L. Lukyanchenko and I. MacHulin and G. Manuzio and S. Marcocci and J. Maricic and J. Martyn and E. Meroni and M. Meyer and L. Miramonti and M. Misiaszek and V. Muratova and B. Neumair and M. Nieslony and L. Oberauer and V. Orekhov and F. Ortica and M. Pallavicini and L. Papp and Penek and L. Pietrofaccia and N. Pilipenko and A. Pocar and A. Porcelli and G. Raikov and G. Ranucci and A. Razeto and A. Re and M. Redchuk and A. Romani and N. Rossi and S. Rottenanger and S. Sch{\"o}nert and D. Semenov and M. Skorokhvatov and O. Smirnov and A. Sotnikov and Stokes, {L. F.F.} and Y. Suvorov and R. Tartaglia and G. Testera and J. Thurn and E. Unzhakov and A. Vishneva and Vogelaar, {R. B.} and {Von Feilitzsch}, F. and S. Weinz and M. Wojcik and M. Wurm and O. Zaimidoroga and S. Zavatarelli and K. Zuber and G. Zuzel",

note = "Publisher Copyright: {\textcopyright} 2019 Sissa Medialab Srl. All rights reserved.; 39th International Conference on High Energy Physics, ICHEP 2018 ; Conference date: 04-07-2018 Through 11-07-2018",

year = "2019",

language = "English (US)",

volume = "340",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Guffanti, D, Agostini, M, Altenmüller, K, Appel, S, Atroshchenko, V, Bagdasarian, Z, Basilico, D, Bellini, G, Benziger, JB, Bonfini, G, Bravo, D, Caccianiga, B, Calaprice, F, Caminata, A, Cappelli, L, Caprioli, S, Carlini, M, Cavalcante, P, Cavanna, F, Chepurnov, A, Choi, K, Collica, L, D'Angelo, D, Davini, S, Derbin, A, Ding, XF, Di Ludovico, A, Di Noto, L, Drachnev, I, Fomenko, K, Formozov, A, Franco, D, Gabriele, F, Galbiati, C, Gschwender, M, Ghiano, C, Giammarchi, M, Goretti, A, Gromov, M, Guffanti, D, Houdy, T, Hungerford, E, Ianni, A, Ianni, A, Jany, A, Jeschke, D, Kumaran, S, Kobychev, V, Korga, G, Lachenmaier, T, Laubenstein, M, Litvinovich, E, Lombardi, P, Ludhova, L, Lukyanchenko, G, Lukyanchenko, L, MacHulin, I, Manuzio, G, Marcocci, S, Maricic, J, Martyn, J, Meroni, E, Meyer, M, Miramonti, L, Misiaszek, M, Muratova, V, Neumair, B, Nieslony, M, Oberauer, L, Orekhov, V, Ortica, F, Pallavicini, M, Papp, L, Penek, Pietrofaccia, L, Pilipenko, N, Pocar, A, Porcelli, A, Raikov, G, Ranucci, G, Razeto, A, Re, A, Redchuk, M, Romani, A, Rossi, N, Rottenanger, S, Schönert, S, Semenov, D, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Stokes, LFF, Suvorov, Y, Tartaglia, R, Testera, G, Thurn, J, Unzhakov, E, Vishneva, A, Vogelaar, RB, Von Feilitzsch, F, Weinz, S, Wojcik, M, Wurm, M, Zaimidoroga, O, Zavatarelli, S, Zuber, K & Zuzel, G 2019, 'Results from Borexino on solar and geo-neutrinos', Proceedings of Science, vol. 340, 007.

TY - JOUR

T1 - Results from Borexino on solar and geo-neutrinos

AU - Guffanti, Daniele

AU - Agostini, M.

AU - Altenmüller, K.

AU - Appel, S.

AU - Atroshchenko, V.

AU - Bagdasarian, Z.

AU - Basilico, D.

AU - Bellini, G.

AU - Benziger, Jay Burton

AU - Bonfini, G.

AU - Bravo, D.

AU - Caccianiga, B.

AU - Calaprice, Frank

AU - Caminata, A.

AU - Cappelli, L.

AU - Caprioli, S.

AU - Carlini, M.

AU - Cavalcante, P.

AU - Cavanna, F.

AU - Chepurnov, A.

AU - Choi, K.

AU - Collica, L.

AU - D'Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Ding, X. F.

AU - Di Ludovico, A.

AU - Di Noto, L.

AU - Drachnev, I.

AU - Fomenko, K.

AU - Formozov, A.

AU - Franco, D.

AU - Gabriele, F.

AU - Galbiati, C.

AU - Gschwender, M.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goretti, A.

AU - Gromov, M.

AU - Guffanti, D.

AU - Houdy, T.

AU - Hungerford, E.

AU - Ianni, Aldo

AU - Ianni, Andrea

AU - Jany, A.

AU - Jeschke, D.

AU - Kumaran, S.

AU - Kobychev, V.

AU - Korga, G.

AU - Lachenmaier, T.

AU - Laubenstein, M.

AU - Litvinovich, E.

AU - Lombardi, P.

AU - Ludhova, L.

AU - Lukyanchenko, G.

AU - Lukyanchenko, L.

AU - MacHulin, I.

AU - Manuzio, G.

AU - Marcocci, S.

AU - Maricic, J.

AU - Martyn, J.

AU - Meroni, E.

AU - Meyer, M.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Muratova, V.

AU - Neumair, B.

AU - Nieslony, M.

AU - Oberauer, L.

AU - Orekhov, V.

AU - Ortica, F.

AU - Pallavicini, M.

AU - Papp, L.

AU - Penek,

AU - Pietrofaccia, L.

AU - Pilipenko, N.

AU - Pocar, A.

AU - Porcelli, A.

AU - Raikov, G.

AU - Ranucci, G.

AU - Razeto, A.

AU - Re, A.

AU - Redchuk, M.

AU - Romani, A.

AU - Rossi, N.

AU - Rottenanger, S.

AU - Schönert, S.

AU - Semenov, D.

AU - Skorokhvatov, M.

AU - Smirnov, O.

AU - Sotnikov, A.

AU - Stokes, L. F.F.

AU - Suvorov, Y.

AU - Tartaglia, R.

AU - Testera, G.

AU - Thurn, J.

AU - Unzhakov, E.

AU - Vishneva, A.

AU - Vogelaar, R. B.

AU - Von Feilitzsch, F.

AU - Weinz, S.

AU - Wojcik, M.

AU - Wurm, M.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuber, K.

AU - Zuzel, G.

PY - 2019

Y1 - 2019

N2 - Borexino is running at the INFN Gran Sasso National Laboraries, Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the foundation for the outstanding achievements accumulated by this experiment. In this contribution, after recalling the main features of the detector, the impressive solar data gathered so far by Borexino will be summarized. Special emphasis will be given to the illustration of the recent release of the fluxes as stemming from the simultaneous real time spectroscopy of the neutrinos from the entire pp nuclear fusion chain in the Sun, opening with the remarkable 2.7% accuracy of the 7Be flux the era of precision measurements also in the realm of the sub-MeV solar neutrinos. Such results put Borexino in the unique situation of being the only detector able to perform solar neutrino spectroscopy over the entire solar spectrum; the counterpart of this peculiar status, in the flavor conversion interpretation of the solar neutrino data, is the capability of Borexino alone to perform the full validation across the solar energy range of the MSW-LMA paradigm. This contribution will be concluded with an account of the Borexino accomplishments in the geo-neutrino field, marked by the detection of the geo-neutrino signal with a significance as high as 5:9σ.

AB - Borexino is running at the INFN Gran Sasso National Laboraries, Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the foundation for the outstanding achievements accumulated by this experiment. In this contribution, after recalling the main features of the detector, the impressive solar data gathered so far by Borexino will be summarized. Special emphasis will be given to the illustration of the recent release of the fluxes as stemming from the simultaneous real time spectroscopy of the neutrinos from the entire pp nuclear fusion chain in the Sun, opening with the remarkable 2.7% accuracy of the 7Be flux the era of precision measurements also in the realm of the sub-MeV solar neutrinos. Such results put Borexino in the unique situation of being the only detector able to perform solar neutrino spectroscopy over the entire solar spectrum; the counterpart of this peculiar status, in the flavor conversion interpretation of the solar neutrino data, is the capability of Borexino alone to perform the full validation across the solar energy range of the MSW-LMA paradigm. This contribution will be concluded with an account of the Borexino accomplishments in the geo-neutrino field, marked by the detection of the geo-neutrino signal with a significance as high as 5:9σ.

UR - http://www.scopus.com/inward/record.url?scp=85084108585&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85084108585&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85084108585

SN - 1824-8039

VL - 340

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 007

T2 - 39th International Conference on High Energy Physics, ICHEP 2018

Y2 - 4 July 2018 through 11 July 2018

ER -

Results from Borexino on solar and geo-neutrinos

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