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説明
Effects of the phase transitions of superdense matter on supernova explosions are investigated with the aid of an idealized equation of state on the assumptions of adiabatic collapse. It is found that in the case of strong phase transitions explosions become weaker, while in the case of weak phase transitions explosions become stronger. However, the increment of the ejected energy is not so large as suggested by Migdal et al. (1979).
収録刊行物
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- Astrophysics and Space Science
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Astrophysics and Space Science 119 45-49, 1986-01-01
Springer Science and Business Media LLC