Terminal stages of stellar evolution in quantum chromodynamics

Details Terminal stages of stellar evolution in quantum chromodynamics Terminal stages of stellar evolution in quantum chromodynamics

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phlb...69..257k&link_type=abstract

Physics Letters B, Volume 69, Issue 2, p. 257-260.

Physics

3

Scientific paper

The characteristics of matter undergoing gravitational collapse are described using the modern strong interaction theory, quantum chromodynamics (QCD). We show that (a) there is a small range of densities from about 4 × 1014 to about 3 × 1015 g/cm3, in which a collapsing stellar core of less than 3.5 ? will undergo hydrodynamic bounce; (b) there is a new source of energy release from the hyperonization of normal matter. Energies of O(1053) erg or greater are involved in both mechanisms. Processes (a), (b) are thus serious mechanisms for supernovae generation.
Present address: Ames Laboratory-ERDA, Ames, Iowa 50011, USA.

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