Equation of state of stellar nuclear matter in the temperature-dependent extended Thomas-Fermi formalism

Details Equation of state of stellar nuclear matter in the temperature-dependent extended Thomas-Fermi formalism Equation of state of stellar nuclear matter in the temperature-dependent extended Thomas-Fermi formalism

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvc..55.3139o&link_type=abstract

Physical Review C (Nuclear Physics), Volume 55, Issue 6, June 1997, pp.3139-3148

Physics

Nuclear Physics

10

Nuclear Matter, Forces In Hadronic Systems And Effective Interactions, Nuclear Structure Models And Methods, Nuclear Matter Aspects Of Neutron Stars

Scientific paper

Using the full temperature-dependent extended Thomas-Fermi formalism, we calculate the equation of state of inhomogeneous nuclear matter for a force that has been fitted to essentially all nuclear masses, and has the correct properties of neutron matter. Both droplet and bubble phases are considered, under the conditions appropriate to a collapsing star. We examine the relevance of the choice of effective mass to the temperature.

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