Literature DB >> 22107184

Precision measurement of the (7)Be solar neutrino interaction rate in Borexino.

G Bellini1, J Benziger, D Bick, S Bonetti, G Bonfini, 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 Goeger-Neff, A Goretti, L Grandi, E Guardincerri, S Hardy, Aldo Ianni, Andrea Ianni, V Kobychev, D Korablev, G Korga, Y Koshio, D Kryn, M Laubenstein, T Lewke, E Litvinovich, B Loer, F Lombardi, P Lombardi, L Ludhova, 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 Obolensky, F Ortica, M Pallavicini, L Papp, C Peña-Garay, L Perasso, S Perasso, A Pocar, R S Raghavan, G Ranucci, A Razeto, A Re, A Romani, A Sabelnikov, 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, J Winter, M Wojcik, A Wright, M Wurm, J Xu, O Zaimidoroga, S Zavatarelli, G Zuzel.   

Abstract

The rate of neutrino-electron elastic scattering interactions from 862 keV (7)Be solar neutrinos in Borexino is determined to be 46.0±1.5(stat)(-1.6)(+1.5)(syst) counts/(day·100  ton). This corresponds to a ν(e)-equivalent (7)Be solar neutrino flux of (3.10±0.15)×10(9)  cm(-2) s(-1) and, under the assumption of ν(e) transition to other active neutrino flavours, yields an electron neutrino survival probability of 0.51±0.07 at 862 keV. The no flavor change hypothesis is ruled out at 5.0 σ. A global solar neutrino analysis with free fluxes determines Φ(pp)=6.06(-0.06)(+0.02)×10(10)  cm(-2) s(-1) and Φ(CNO)<1.3×10(9)  cm(-2) s(-1) (95% C.L.). These results significantly improve the precision with which the Mikheyev-Smirnov-Wolfenstein large mixing angle neutrino oscillation model is experimentally tested at low energy.

Entities:  

Year:  2011        PMID： 22107184     DOI： 10.1103/PhysRevLett.107.141302

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN： 0031-9007            Impact factor:   9.161


  7 in total

1.  Neutrinos reveal final secret of Sun's nuclear fusion.

Authors:  Davide Castelvecchi
Journal:  Nature       Date:  2020-07       Impact factor: 49.962

2.  Neutrinos from the primary proton-proton fusion process in the Sun.

Authors: 
Journal:  Nature       Date:  2014-08-28       Impact factor: 49.962

3.  Neutrino physics: What makes the Sun shine.

Authors:  Wick Haxton
Journal:  Nature       Date:  2014-08-28       Impact factor: 49.962

4.  Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun.

Authors: 
Journal:  Nature       Date:  2020-11-25       Impact factor: 49.962

5.  Theoretical study of structure and stability of small gadolinium carboxylate complexes in liquid scintillator solvents.

Authors:  Pin-Wen Huang
Journal:  J Mol Model       Date:  2014-09-10       Impact factor: 1.810

6.  Prospects for beyond the Standard Model physics searches at the Deep Underground Neutrino Experiment: DUNE Collaboration.

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Journal:  Eur Phys J C Part Fields       Date:  2021-04-16       Impact factor: 4.590

7.  Selective inhibition of soluble tumor necrosis factor signaling reduces abdominal aortic aneurysm progression.

Authors:  Silke Griepke; Emilie Grupe; Jes Sanddal Lindholt; Elizabeth Hvitfeldt Fuglsang; Lasse Bach Steffensen; Hans Christian Beck; Mia Dupont Larsen; Sissel Karoline Bang-Møller; Martin Overgaard; Lars Melholt Rasmussen; Kate Lykke Lambertsen; Jane Stubbe
Journal:  Front Cardiovasc Med       Date:  2022-09-16
  7 in total

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