Towards the equation of state for dense stellar matter

Details Towards the equation of state for dense stellar matter Towards the equation of state for dense stellar matter

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jphcs.202a2003b&link_type=abstract

Journal of Physics: Conference Series, Volume 202, Issue 1, pp. 012003 (2010).

Physics

Scientific paper

The thermal nuclear multifragmentation reaction can be used to investigate the nuclear liquid-gas phase coexistence region and its relation to the astrophysical processes such as the collapse of massive stars, and the supernova type-II explosions. We have performed some calculations to estimate stellar equation of state (EOS) on the basis of statistical multifragmentation model.

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