A Type II Supernovae Constraint on $ν_e$-$ν_s$

Details A Type II Supernovae Constraint on $ν_e$-$ν_s$ A Type II Supernovae Constraint on $ν_e$-$ν_s$

1993-12-08

arxiv.org/abs/hep-ph/9312247v1

Phys.Lett.B323:360-366,1994; ERRATUM-ibid.B324:516,1994

Physics

High Energy Physics

High Energy Physics - Phenomenology

plain Tex 11 pages, 3 figures available upon request from the authors. (shi6@oddjob.uchicago.edu, sigl@oddjob)

Scientific paper

10.1016/0370-2693(94)91232-7

The role of a resonant $\nu_e$-$\nu_s$ oscillation is discussed in the event of a supernova explosion. It is concluded that a significant $\nu_e$-$\nu_s$ mixing may hinder the ability of the supernova to explode. It may also cool the proto-neutron star too quickly with respect to the observed cooling time of several seconds. The constraints on the $\nu_e$-$\nu_s$ mixing parameters based on the above arguments are calculated.

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