Correlation between solar neutrino flux and solar magnetic activity for Majorana neutrinos

Details Correlation between solar neutrino flux and solar magnetic activity for Majorana neutrinos Correlation between solar neutrino flux and solar magnetic activity for Majorana neutrinos

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..243..389l&link_type=abstract

Physics Letters B, Volume 243, Issue 4, p. 389-395.

Physics

23

Scientific paper

We study the interplay between solar neutrino event rates and solar magnetic field in both the Kamiokande-II and the 37Cl experiments, in a framework with resonant spin-flavor precession. An interesting difference in the correlation in these two experiments arises especially due to the presence of νe-->νμ-->νe for Majorana neutrinos. The conversion rate is sizable for parameters, Δm2<10-7 eV2, sin22θ> 0.5 and the Zeeman energy μB>10-10 (μB.1 kG) with μB b being the Bohr magneton. The detection of characteristic ve signals in the Kamiokande-II is also discussed.

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