Spin-flavour conversions of neutrinos in collapsing stars

Details Spin-flavour conversions of neutrinos in collapsing stars Spin-flavour conversions of neutrinos in collapsing stars

1999-02-02

arxiv.org/abs/hep-ph/9902222v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

5 pages, Latex (uses sprocl.sty), No figures, Talk presented at Second Meeting on New Worlds in Astroparticle Physics (NW 98),

Scientific paper

I discuss in some detail the spin-flavour conversions of neutrinos in the almost isotopically neutral region of collapsing stars along with the resulting experimental signatures. In particular, I show that for realistic magnetic field strength, the observable effects may exist for neutrino magnetic moment, $\mu \sim (2-3)\times 10^{-14}\mu_B$ ($\mu_B$ is the Bohr magneton) with relevant neutrino mass squared difference, $\Delta m^2 \sim (10^{-9}-10^{-8}) eV^2$.

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