We report the direct measurement of the 7 Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV Be-7 neutrinos is 49 +/- 3(stat) +/- 4(syst) counts/(day . 100 ton). The hypothesis of no oscillation for Be-7 solar neutrinos is inconsistent with our measurement at the 4 sigma C.L. Our result is the first direct measurement of the survival probability for solar P, in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of Be-7, pp, and CNO solar v(e) and the limit on the effective neutrino magnetic moment using solar neutrinos.

Direct measurement of the Be-7 solar neutrino flux with 192 days of Borexino data

DE BARI, ANTONIO;
2008-01-01

Abstract

We report the direct measurement of the 7 Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV Be-7 neutrinos is 49 +/- 3(stat) +/- 4(syst) counts/(day . 100 ton). The hypothesis of no oscillation for Be-7 solar neutrinos is inconsistent with our measurement at the 4 sigma C.L. Our result is the first direct measurement of the survival probability for solar P, in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of Be-7, pp, and CNO solar v(e) and the limit on the effective neutrino magnetic moment using solar neutrinos.
2008
The Physics category includes resources of a broad, general nature that contain materials from all areas of physics, The category also includes resources specifically concerned with the following physics sub-fields: mathematical physics, particle and nuclear physics, physics of fluids and plasmas, quantum physics, and theoretical physics.
Esperti anonimi
Inglese
Internazionale
STAMPA
101
9
091302-1
091302-6
6
The Borexino program was made possible by funding from INFN (Italy), NSF (U.S.), BMBF, DFG and MPG (Germany), Rosnauka (Russia), and MNiSW (Poland). We acknowledge the generous support of the Laboratori Nazionali del Gran Sasso (LNGS). This work has been supported by the ILIAS integrating activity (Contract No. RII3-CT-2004-506222) as part of the EU FP6 programme. O. Smirnov aknowledges the support of Fondazione Cariplo.
BE-7; SOLAR NEUTRINO FLUX; BOREXINO; MAGNETIC MOMENTS; TESTING FACILITY; GAUGE THEORIES; DETECTOR; OSCILLATIONS; MUON; SCINTILLATOR; ABUNDANCE; LEPTON; MATTER
133
info:eu-repo/semantics/article
262
Arpesella, C.; Back, H. O.; Balata, M.; Bellini, G.; Benziger, J.; Bonetti, S.; Brigatti, A.; Caccianiga, B.; Cadonati, L.; Calaprice, F.; Carraro, C....espandi
1 Contributo su Rivista::1.1 Articolo in rivista
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11571/141997
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