The phase transitions of superdense matter and supernova explosions

Details The phase transitions of superdense matter and supernova explosions The phase transitions of superdense matter and supernova explosions

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119...45t&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

5

Density Distribution, Equations Of State, Gravitational Collapse, Phase Transformations, Supernovae, Adiabatic Conditions, Energy Dissipation, Stellar Cores, Stellar Models

Scientific paper

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).

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