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A Type II Supernovae Constraint on $\nu_e$-$\nu_s$

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arxiv hep-ph/9312247 v1 pith:O5ZNDFA2 submitted 1993-12-08 hep-ph astro-ph

Xiangdong Shi , Guenter Sigl This is my paper · ORCID
classification hep-phastro-ph
keywords mixingsupernovaabilityaboveargumentscalculatedconcludedconstraint
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abstract

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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