Supernova neutrino oscillation in the presence of a random magnetic field

Details Supernova neutrino oscillation in the presence of a random magnetic field Supernova neutrino oscillation in the presence of a random magnetic field

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..531..355s&link_type=abstract

PARTICLES AND FIELDS: Seventh Mexican Workshop. AIP Conference Proceedings, Volume 531, pp. 355-359 (2000).

Physics

Nuclear Physics

Neutrino Mass And Mixing, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Supernovae, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments

Scientific paper

The active-sterile neutrino conversion is studied for neutrino propagating in the axial potential generated by magnetized electron plasma in the supernova medium. We consider the effect of random magnetic field Brms on the average neutrino conversion probability and obtained the constraint on Δm2 and sin2 2θ for different strength of the random magnetic fields, inside the supernova core. Our calculation shows that, to have Δm2<~keV2, the random magnetic field Brms<~0.63×1014 Gauss is preferable. .

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