Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1217r&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
super-Kamiokande(SK) and SNO detectors detected recoil electron energy spectrum from νe + e- → νe + e- .Analysing statistically recoil electron energy spectrum from SK and SNO detectors we find that recoil energy spectrum from > 10 MeV is higher than the recoil electron energy spectrum from 5 MeV to 10 MeV with > 95% C.L. This finding indicates that recoil energy spectrum is distorted which is due to disturb ed nature of the solar core.We suggest that both SK and SNO detectors detected neutrino flux from 3 H e+p neutrinos apart from 8 bneutrinos.We have calculated the neutrino flux from 3 H e+p neutrinos and is found to be(1 ˜ 1.5) × 105 cm-2 sec-1 which is higher than the observed upper limit reported by SK's 1496 day data. We suggest that the contribution of 3 H e+p and 8 bneutrino flux from 5 to 20 MeV is reflected in both the detectors due to distortion of neutrino flux.The recoil electron energy spectrum is fitted with the sum of several Gaussian curves indicating the sto chastic nature of the solar core.
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