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- W1567731093 abstract "The evolution of a stellar core is studied during itsfinal quasi-hydrostatic contraction. The core structure and the(poorly known) properties of neutron rich matter are parametrizedto include most plausible cases. It is found that thedensity-temperature trajectory of the material in the centralpart of the core (the core-center) is insensitive to nearly allreasonable parameter variations. The central density at theonset of the dynamic phase of the collapse (when the core-centerbegins to fall away from the rest of the star) and thefraction of the emitted neutrinos which are trapped in thecollapsing core-center depend quite sensitively on the propertiesof neutron rich matter. We estimate that the amount of energyE_(cm); which is imparted to the core-mantle by the neutrinoswhich escape from the imploded core-center can span alarge range of values. For plausible choices of nuclear andmodel parameters E_(cm) can be large enough to yield a supernovaevent." @default.
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- W1567731093 date "1979-05-01" @default.
- W1567731093 modified "2023-10-16" @default.
- W1567731093 title "Collapsing Stellar Cores and Supernovae" @default.
- W1567731093 hasPublicationYear "1979" @default.
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