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- W1983995807 abstract "The theory of core-collapse models for type II supernovae now encompasses the concept that apparently small differences in stellar evolution models can have dramatic effects on the predictions of the final outcome, bearing on the question as to whether a neutron star forms in a type II supernova explosion or the collapse continues to form a black hole. This sensitivity is primarily due to the inefficiency of the conversion of the proto-neutron star's gravitational binding energy into outward momentum by a hydrodynamical shock wave, and by long neutrino diffusion times, which do not allow efficient use of the thermal energy stored in leptons. The supernova stellar structure, the core mass, and the entropy determine whether or not the shock is sufficiently strong for mass ejection. 74 references." @default.
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- W1983995807 date "1984-03-01" @default.
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- W1983995807 title "Core-Collapse Models of Type II Supernova Explosions and Neutron Star Formation" @default.
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- W1983995807 doi "https://doi.org/10.1111/j.1749-6632.1984.tb23354.x" @default.
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