General properties of neutrino spin precession in magnetic field and their possible implication for solar neutrinos

Details General properties of neutrino spin precession in magnetic field and their possible implication for solar neutrinos General properties of neutrino spin precession in magnetic field and their possible implication for solar neutrinos

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..293..378m&link_type=abstract

Physics Letters B, Volume 293, Issue 3-4, p. 378-382.

Physics

3

Scientific paper

We consider the problem of the spin (or spin-flavour) precession of the solar electron neutrinos veL, possessing a nonzero magnetic moment (or transition moment of magnetic dipole type) μν, in the magnetic field B of the sun, including the case when B twists continuously along the neutrino path. A lower bound on the product of μv and the absolute value of the transverse (with respect to the neutrino momentum) component of B, needed to induce a veL-->vR transition with a given probability, vR being a right-handed neutrino, is derived.

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