Incompressibility of hot nuclear matter and general relativistic stellar collapse

Details Incompressibility of hot nuclear matter and general relativistic stellar collapse Incompressibility of hot nuclear matter and general relativistic stellar collapse

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...237...97m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 237, no. 1, Oct. 1990, p. 97-102. Research supported by CICYT.

Astronomy and Astrophysics

Astrophysics

2

Condensed Matter Physics, Gravitational Collapse, Nuclear Astrophysics, Relativistic Effects, Stellar Evolution, Mass Distribution, Stellar Mass, Stellar Models, Supernova Remnants, Hydrodynamics, Stars: Collapsed, Supernovae And Supernovae Remnants: General, Dense Matter

Scientific paper

We have made a series of hydrodynamic calculations of core collapsing models to examine the effects of temperature dependence of nuclear compressibility. With this aim we have focused on the influence of the equation of state derived by Viñas et al. for two extreme types of nuclear interactions. A Multigroup Trapping Scheme for neutrino transport is used. Results show that we can reach a maximum central density in the range to 1.5ρ0 to 2.5ρ0, depending on the particular force used.

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