Neutron star properties and the relativistic equation of state of asymmetric nuclear matter

Details Neutron star properties and the relativistic equation of state of asymmetric nuclear matter Neutron star properties and the relativistic equation of state of asymmetric nuclear matter

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvc..50.1287h&link_type=abstract

Physical Review C (Nuclear Physics), Volume 50, Issue 3, September 1994, pp.R1287-R1291

Physics

Nuclear Physics

24

Nuclear Matter, Hypernuclei, Lagrangian And Hamiltonian Approach, Pulsars

Scientific paper

We calculate the equation of state of asymmetric nuclear matter in
generalized chemical equilibrium in the relativistic
Brueckner-Hartree-Fock approximation, and study its impact on the
properties of (rapidly) rotating neutron stars by solving the stellar
structure equations in the framework of general relativity theory.

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