The equation of state in nucleon and strange stars

Details The equation of state in nucleon and strange stars The equation of state in nucleon and strange stars

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..412.1007p&link_type=abstract

The sixth conference on the intersections of particle and nuclear physcis. AIP Conference Proceedings, Volume 412, pp. 1007-102

Astronomy and Astrophysics

Astrophysics

Pulsars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Quarks, Gluons, And Qcd In Nuclei And Nuclear Processes

Scientific paper

The equation of state (EOS) is an essential physical ingredient in simulations of gravitational collapse, supernovae, old and newly born neutron stars, and binary mergers of compact stars. In this talk, I will examine (1) the extent to which stringent constraints may be placed on the EOS by a comparison of calculations with the available data on some basic neutron star properties; and (2) some astrophysical consequences of the possible presence of strangeness, in the form of baryons, notably the Λ and Σ-, or as a Bose condensate, such as a K- meson condensate, or in the form of strange quarks.

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