A Type 2 supernovae constraint on neutrinoe - neutrinos mixing

Details A Type 2 supernovae constraint on neutrinoe - neutrinos mixing A Type 2 supernovae constraint on neutrinoe - neutrinos mixing

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stin...9518746s&link_type=abstract

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Computer Science

Numerical Analysis

Big Bang Cosmology, Cool Stars, Explosions, Mixing, Solar Neutrinos, Stellar Cores, Stellar Physics, Supernovae, Cooling, Gravitational Collapse, Numerical Analysis, Stellar Evolution, Stellar Oscillations

Scientific paper

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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