Forward-Peaked νe-e Scattering and the Solar-Neutrino Problem

Details Forward-Peaked νe-e Scattering and the Solar-Neutrino Problem Forward-Peaked νe-e Scattering and the Solar-Neutrino Problem

Oct 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvd...8.2261c&link_type=abstract

Physical Review D, vol. 8, Issue 7, pp. 2261-2263

Physics

13

Scientific paper

The possibility that multiple νe-e scattering within the sun can account for the low solar-neutrino counting rates is considered. In the absence of νe-e scattering data, bounds are imposed from ν¯e-e data, introducing a requirement for strong forward peaking. Generalized four-fermion interactions calculated to first order are found to be inadequate. Electromagnetic νe-e interactions with a finite neutrino magnetic moment are found to be satisfactory, but require a seemingly unphysical neutrino form factor corresponding to a mean neutrino radius of r¯ν>7×10-10 cm.

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