Author/Authors :
Testera، نويسنده , , G. and Bellini، نويسنده , , G. and Benziger، نويسنده , , J. and Bick، نويسنده , , D. and Bonetti، نويسنده , , S. and Bonfini، نويسنده , , G. and Caccianiga، نويسنده , , B. and Cadonati، نويسنده , , L. and Calaprice، نويسنده , , F. and Carraro، نويسنده , , C. and Chavarria، نويسنده , , A. and DʹAngelo، نويسنده , , D. and Derbin، نويسنده , , A. and Etenko، نويسنده , , A. and Fomenko، نويسنده , , K. and Franco، نويسنده , , D.، نويسنده ,
Abstract :
We report the direct measurement of the 7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso and the search for a day–night asymmetry of this interaction rate. The interaction rate of the 0.862 MeV 7Be neutrinos is 46 ± 1.6 ( stat ) − 1.6 + 1.5 ( syst ) counts/(day · 100 ton). The hypothesis of no oscillation for this solar neutrinos is inconsistent with our measurement at the 5.8 σ C.L. Our result is the first direct measurement of solar neutrinos with an accuracy better than 5%. We report the survival probability for solar ν e in the transition region between matter-enhanced and vacuum-driven oscillations. The measured day night asymmetry is A dn = 0.001 ± 0.012 (stat)±0.007 (syst), in agreement with the predicition of MSW–LMA neutrino [13] oscillations. This result discourages MSW oscillations with mixing parameters in the LOW region at more than 8.5 σ , meaning that this region is, for the first time, strongly rejected without the assumption of CPT symmetry. The result can also be used to constrain some neutrino oscillation scenarios involving new physics.
Keywords :
Solar neutrinos , Neutrino oscillations , Low background detectors , Liquid scintillators