4.8 Article

Precision Measurement of the 7Be Solar Neutrino Interaction Rate in Borexino

期刊

PHYSICAL REVIEW LETTERS
卷 107, 期 14, 页码 -

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AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.107.141302

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资金

  1. INFN (Italy)
  2. NSF (USA)
  3. BMBF (Germany)
  4. DFG (Germany)
  5. MPG (Germany)
  6. NRC Kurchatov Institute (Russia)
  7. MNiSW (Poland)
  8. Direct For Mathematical & Physical Scien
  9. Division Of Physics [0802114] Funding Source: National Science Foundation
  10. Division Of Physics
  11. Direct For Mathematical & Physical Scien [0902140, 1103987] Funding Source: National Science Foundation

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The rate of neutrino-electron elastic scattering interactions from 862 keV Be-7 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 nu(e)-equivalent Be-7 solar neutrino flux of (3.10 +/- 0.15) x 10(9) cm(-2) s(-1) and, under the assumption of nu(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 sigma. A global solar neutrino analysis with free fluxes determines Phi(pp) = 6.06(-0.66)(+0.02) x 10(10) cm(-2) s(-1) and Phi(CNO) < 1.3 x 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.

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