Nuclear Physics and Atomic Energy

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Nuclear Physics and Atomic Energy

  ISSN: 1818-331X (Print), 2074-0565 (Online)
  Publisher: Institute for Nuclear Research of the National Academy of Sciences of Ukraine
  Languages: Ukrainian, English, Russian
  Periodicity: 4 times per year

  Open access peer reviewed journal


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Nucl. Phys. At. Energy 2017, volume 18, issue 4, pages 303-312.
Section: Nuclear Physics.
Received: 27.09.2017; Accepted: 28.12.2017; Published online: 20.02.2018.
PDF Full text (en)
https://doi.org/10.15407/jnpae2017.04.303

Joint analysis of Borexino and SNO solar neutrino data and reconstruction of the survival probability

Francesco Vissani1,2*

1 INFN - Laboratori Nazionali del Gran Sasso, Assergi (AQ), Italy
2 Gran Sasso Science Institute, L’Aquila (AQ), Italy


*Corresponding author. E-mail address: francesco.vissani@lngs.infn.it

Abstract: Solar neutrino oscillations are supported by KamLAND’s antineutrino measurements, but certain solar neutrino data – the observed shape of the 8B flux and the difference between day and night counting rates measured in Super-K – do not fit well with the ensuing oscillation pattern. Interestingly, other solar neutrino data allow independent tests of the survival probability. Thanks to the new measurements of Borexino at low-energies along with the standard solar model and to the results of SNO at high-energies, four values of the neutrino survival probability are known. We build and study a likelihood based only on these solar neutrino data. The results agree well with the standard oscillation pattern and in particular with KamLAND findings. A related and straightforward procedure permits to reconstruct the survival probability of solar neutrinos and to assess its uncertainties, for all solar neutrino energies.

Keywords: solar neutrinos, neutrino oscillations, nuclear astrophysics, pp neutrinos, pep neutrinos, 7Be neutrinos, 8B neutrinos.

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