Solar neutrino physics with BOREXINO i

L. Ludhova; G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; M. Buizza Avanzini; B. Caccianiga; L. Cadonati; F. Calaprice; C. Carraro; P. Cavalcante; A. Chavarria; D. D'Angelo; S. Davini; A. Derbin; A. Etenko; K. Fomenko; D. Franco; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Goger-Neff; A. Goretti; L. Grandi; E. Guardincerri; S. Hardy; Aldo Ianni; Andrea Ianni; A. Kayunov; V. Kobychev; D. Korablev; G. Korga; Y. Koshio; D. Kryn; M. Laubenstein; T. Lewke; E. Litvinovich; B. Loer; F. Lombardi; P. Lombardi; I. MacHulin; S. Manecki; W. Maneschg; G. Manuzio; Q. Meindl; E. Meroni; L. Miramonti; M. Misiaszek; D. Montanari; P. Mosteiro; V. Muratova; L. Oberauer; M. Obolenksy; F. Ortica; K. Otis; M. Pallavicini; L. Papp; L. Perasso; S. Perasso; A. Pocar; R. S. Raghavan; G. Ranucci; A. Razeto; A. Re; P. A. Romani; A. Sabelnikov; R. Saldanha; C. Salvo; S. Schonert; H. Simgen; M. Skorokhvatov; O. Smirnov; A. Sotnikov; S. Sukhotin; Y. Suvorov; R. Tartaglia; G. Testera; D. Vignaud; R. B. Vogelaar; F. Von Feilitzsch; J. Winter; M. Wojcik; A. Wright; M. Wurm; J. Xu; O. Zaimidoroga; S. Zavatarelli; G. Zuzel

Solar neutrino physics with BOREXINO i

L. Ludhova, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, P. Cavalcante, A. Chavarria, D. D'Angelo, S. Davini, A. Derbin, A. Etenko, K. Fomenko, D. Franco, C. GalbiatiS. Gazzana, C. Ghiano, M. Giammarchi, M. Goger-Neff, A. Goretti, L. Grandi, E. Guardincerri, S. Hardy, Aldo Ianni, Andrea Ianni, A. Kayunov, V. Kobychev, D. Korablev, G. Korga, Y. Koshio, D. Kryn, M. Laubenstein, T. Lewke, E. Litvinovich, B. Loer, F. Lombardi, P. Lombardi, I. MacHulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Montanari, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolenksy, F. Ortica, K. Otis, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, R. S. Raghavan, G. Ranucci, A. Razeto, A. Re, P. A. Romani, A. Sabelnikov, R. Saldanha, C. Salvo, S. Schonert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, R. B. Vogelaar, F. Von Feilitzsch, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel

Research output: Contribution to conference › Paper › peer-review

Abstract

Borexino is a large-volume liquid scintillator detector installed in the underground halls of the Laboratori Nazionali del Gran Sasso in Italy. After several years of construction, data taking started in May 2007. The Borexino phase I ended after about three years of data taking. Borexino provided the first real time measurement of the ⁷Be solar neutrino interaction rate with accuracy better than 5% and confirmed the absence of its day-night asymmetry with 1.4% precision. This latter Borexino results alone rejects the LOW region of solar neutrino oscillation parameters at more than 8.5 σ C.L. Combined with the other solar neutrino data, Borexino measurements isolate the MSW{LMA solution of neutrino oscillations with-out assuming CPT invariance in the neutrino sector. Borexino has also directly observed solar neutrinos in the 1.0-1.5 MeV energy range, leading to the first direct evidence of the pep solar neutrino signal and the strongest constraint of the CNO solar neutrino ux up to date. Borexino provided the measurement of the solar ₈B neutrino rate with 3 MeV energy threshold.

Original language	English (US)
Pages	341-346
Number of pages	6
State	Published - 2012
Event	47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012 - La Thuile, Italy Duration: Mar 3 2012 → Mar 10 2012

Conference

Conference	47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012
Country/Territory	Italy
City	La Thuile
Period	3/3/12 → 3/10/12

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Atomic and Molecular Physics, and Optics

Cite this

Ludhova, L., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Avanzini, M. B., Caccianiga, B., Cadonati, L., Calaprice, F., Carraro, C., Cavalcante, P., Chavarria, A., D'Angelo, D., Davini, S., Derbin, A., Etenko, A., Fomenko, K., Franco, D., ... Zuzel, G. (2012). Solar neutrino physics with BOREXINO i. 341-346. Paper presented at 47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012, La Thuile, Italy.

@conference{d3915fd8cc664d17a1ec14744e83feba,

title = "Solar neutrino physics with BOREXINO i",

abstract = "Borexino is a large-volume liquid scintillator detector installed in the underground halls of the Laboratori Nazionali del Gran Sasso in Italy. After several years of construction, data taking started in May 2007. The Borexino phase I ended after about three years of data taking. Borexino provided the first real time measurement of the 7Be solar neutrino interaction rate with accuracy better than 5% and confirmed the absence of its day-night asymmetry with 1.4% precision. This latter Borexino results alone rejects the LOW region of solar neutrino oscillation parameters at more than 8.5 σ C.L. Combined with the other solar neutrino data, Borexino measurements isolate the MSW{LMA solution of neutrino oscillations with-out assuming CPT invariance in the neutrino sector. Borexino has also directly observed solar neutrinos in the 1.0-1.5 MeV energy range, leading to the first direct evidence of the pep solar neutrino signal and the strongest constraint of the CNO solar neutrino ux up to date. Borexino provided the measurement of the solar 8B neutrino rate with 3 MeV energy threshold.",

author = "L. Ludhova and G. Bellini and J. Benziger and D. Bick and G. Bonfini and D. Bravo and Avanzini, {M. Buizza} and B. Caccianiga and L. Cadonati and F. Calaprice and C. Carraro and P. Cavalcante and A. Chavarria and D. D'Angelo and S. Davini and A. Derbin and A. Etenko and K. Fomenko and D. Franco and C. Galbiati and S. Gazzana and C. Ghiano and M. Giammarchi and M. Goger-Neff and A. Goretti and L. Grandi and E. Guardincerri and S. Hardy and Aldo Ianni and Andrea Ianni and A. Kayunov and V. Kobychev and D. Korablev and G. Korga and Y. Koshio and D. Kryn and M. Laubenstein and T. Lewke and E. Litvinovich and B. Loer and F. Lombardi and P. Lombardi and I. MacHulin and S. Manecki and W. Maneschg and G. Manuzio and Q. Meindl and E. Meroni and L. Miramonti and M. Misiaszek and D. Montanari and P. Mosteiro and V. Muratova and L. Oberauer and M. Obolenksy and F. Ortica and K. Otis and M. Pallavicini and L. Papp and L. Perasso and S. Perasso and A. Pocar and Raghavan, {R. S.} and G. Ranucci and A. Razeto and A. Re and Romani, {P. A.} and A. Sabelnikov and R. Saldanha and C. Salvo and S. Schonert 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 J. Winter and M. Wojcik and A. Wright and M. Wurm and J. Xu and O. Zaimidoroga and S. Zavatarelli and G. Zuzel",

note = "Funding Information: The Borexino program is made possible by funding from INFN (Italy), NSF (USA), BMBF, DFG, and MPG (Germany), NRC Kurchatov Institute (Russia), and MNiSW (Poland). We acknowledge the generous support of the Laboratori Nazionali del Gran Sasso (LNGS). Publisher Copyright: {\textcopyright} EW 2012.; 47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012 ; Conference date: 03-03-2012 Through 10-03-2012",

year = "2012",

language = "English (US)",

pages = "341--346",

}

Ludhova, L, Bellini, G, Benziger, J, Bick, D, Bonfini, G, Bravo, D, Avanzini, MB, Caccianiga, B, Cadonati, L, Calaprice, F, Carraro, C, Cavalcante, P, Chavarria, A, D'Angelo, D, Davini, S, Derbin, A, Etenko, A, Fomenko, K, Franco, D, Galbiati, C, Gazzana, S, Ghiano, C, Giammarchi, M, Goger-Neff, M, Goretti, A, Grandi, L, Guardincerri, E, Hardy, S, Ianni, A, Ianni, A, Kayunov, A, Kobychev, V, Korablev, D, Korga, G, Koshio, Y, Kryn, D, Laubenstein, M, Lewke, T, Litvinovich, E, Loer, B, Lombardi, F, Lombardi, P, MacHulin, I, Manecki, S, Maneschg, W, Manuzio, G, Meindl, Q, Meroni, E, Miramonti, L, Misiaszek, M, Montanari, D, Mosteiro, P, Muratova, V, Oberauer, L, Obolenksy, M, Ortica, F, Otis, K, Pallavicini, M, Papp, L, Perasso, L, Perasso, S, Pocar, A, Raghavan, RS, Ranucci, G, Razeto, A, Re, A, Romani, PA, Sabelnikov, A, Saldanha, R, Salvo, C, Schonert, S, Simgen, H, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvorov, Y, Tartaglia, R, Testera, G, Vignaud, D, Vogelaar, RB, Von Feilitzsch, F, Winter, J, Wojcik, M, Wright, A, Wurm, M, Xu, J, Zaimidoroga, O, Zavatarelli, S & Zuzel, G 2012, 'Solar neutrino physics with BOREXINO i', Paper presented at 47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012, La Thuile, Italy, 3/3/12 - 3/10/12 pp. 341-346.

TY - CONF

T1 - Solar neutrino physics with BOREXINO i

AU - Ludhova, L.

AU - Bellini, G.

AU - Benziger, J.

AU - Bick, D.

AU - Bonfini, G.

AU - Bravo, D.

AU - Avanzini, M. Buizza

AU - Caccianiga, B.

AU - Cadonati, L.

AU - Calaprice, F.

AU - Carraro, C.

AU - Cavalcante, P.

AU - Chavarria, A.

AU - D'Angelo, D.

AU - Davini, S.

AU - Derbin, A.

AU - Etenko, A.

AU - Fomenko, K.

AU - Franco, D.

AU - Galbiati, C.

AU - Gazzana, S.

AU - Ghiano, C.

AU - Giammarchi, M.

AU - Goger-Neff, M.

AU - Goretti, A.

AU - Grandi, L.

AU - Guardincerri, E.

AU - Hardy, S.

AU - Ianni, Aldo

AU - Ianni, Andrea

AU - Kayunov, A.

AU - Kobychev, V.

AU - Korablev, D.

AU - Korga, G.

AU - Koshio, Y.

AU - Kryn, D.

AU - Laubenstein, M.

AU - Lewke, T.

AU - Litvinovich, E.

AU - Loer, B.

AU - Lombardi, F.

AU - Lombardi, P.

AU - MacHulin, I.

AU - Manecki, S.

AU - Maneschg, W.

AU - Manuzio, G.

AU - Meindl, Q.

AU - Meroni, E.

AU - Miramonti, L.

AU - Misiaszek, M.

AU - Montanari, D.

AU - Mosteiro, P.

AU - Muratova, V.

AU - Oberauer, L.

AU - Obolenksy, M.

AU - Ortica, F.

AU - Otis, K.

AU - Pallavicini, M.

AU - Papp, L.

AU - Perasso, L.

AU - Perasso, S.

AU - Pocar, A.

AU - Raghavan, R. S.

AU - Ranucci, G.

AU - Razeto, A.

AU - Re, A.

AU - Romani, P. A.

AU - Sabelnikov, A.

AU - Saldanha, R.

AU - Salvo, C.

AU - Schonert, 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 - Winter, J.

AU - Wojcik, M.

AU - Wright, A.

AU - Wurm, M.

AU - Xu, J.

AU - Zaimidoroga, O.

AU - Zavatarelli, S.

AU - Zuzel, G.

N1 - Funding Information: The Borexino program is made possible by funding from INFN (Italy), NSF (USA), BMBF, DFG, and MPG (Germany), NRC Kurchatov Institute (Russia), and MNiSW (Poland). We acknowledge the generous support of the Laboratori Nazionali del Gran Sasso (LNGS). Publisher Copyright: © EW 2012.

PY - 2012

Y1 - 2012

N2 - Borexino is a large-volume liquid scintillator detector installed in the underground halls of the Laboratori Nazionali del Gran Sasso in Italy. After several years of construction, data taking started in May 2007. The Borexino phase I ended after about three years of data taking. Borexino provided the first real time measurement of the 7Be solar neutrino interaction rate with accuracy better than 5% and confirmed the absence of its day-night asymmetry with 1.4% precision. This latter Borexino results alone rejects the LOW region of solar neutrino oscillation parameters at more than 8.5 σ C.L. Combined with the other solar neutrino data, Borexino measurements isolate the MSW{LMA solution of neutrino oscillations with-out assuming CPT invariance in the neutrino sector. Borexino has also directly observed solar neutrinos in the 1.0-1.5 MeV energy range, leading to the first direct evidence of the pep solar neutrino signal and the strongest constraint of the CNO solar neutrino ux up to date. Borexino provided the measurement of the solar 8B neutrino rate with 3 MeV energy threshold.

AB - Borexino is a large-volume liquid scintillator detector installed in the underground halls of the Laboratori Nazionali del Gran Sasso in Italy. After several years of construction, data taking started in May 2007. The Borexino phase I ended after about three years of data taking. Borexino provided the first real time measurement of the 7Be solar neutrino interaction rate with accuracy better than 5% and confirmed the absence of its day-night asymmetry with 1.4% precision. This latter Borexino results alone rejects the LOW region of solar neutrino oscillation parameters at more than 8.5 σ C.L. Combined with the other solar neutrino data, Borexino measurements isolate the MSW{LMA solution of neutrino oscillations with-out assuming CPT invariance in the neutrino sector. Borexino has also directly observed solar neutrinos in the 1.0-1.5 MeV energy range, leading to the first direct evidence of the pep solar neutrino signal and the strongest constraint of the CNO solar neutrino ux up to date. Borexino provided the measurement of the solar 8B neutrino rate with 3 MeV energy threshold.

UR - http://www.scopus.com/inward/record.url?scp=85088888861&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85088888861&partnerID=8YFLogxK

M3 - Paper

AN - SCOPUS:85088888861

SP - 341

EP - 346

T2 - 47th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2012

Y2 - 3 March 2012 through 10 March 2012

ER -

Solar neutrino physics with BOREXINO i

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