Non-dynamical contributions to left-right transitions in the solar neutrino problem

Details Non-dynamical contributions to left-right transitions in the solar neutrino problem Non-dynamical contributions to left-right transitions in the solar neutrino problem

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..249..473v&link_type=abstract

Physics Letters B, Volume 249, Issue 3-4, p. 473-477.

Physics

32

Scientific paper

The conditions under which the adiabatic phases can produce a reduction in the solar neutrino flux are studied for a realistic model of the solar magnetic field. Within the adiabatic approximation, it is found that μ > 10-13 μBohr will produce a sensible decrease in the flux. The possible correlations with the solar cycle, as well as the corrections to the adiabatic approximation are briefly considered.

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