Present Status of Spin Flavor Precession

Details Present Status of Spin Flavor Precession Present Status of Spin Flavor Precession

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1258m&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

Present status of spin flavor precession (SFP) in the Sun is reviewed. Using the recent solar neutrino data it is shown that this mechanism is disfavored as a leading solution to the solar neutrino problem. The case of SFP as a sub-leading solution is also discussed. In this case, it is shown that the recent KamLAND constraint on solar anti-neutrino flux provides a stringent constraint on the neutrino magnetic moment down to μν ≤ few × 10-12.

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