Neutron Star Matter with In-Medium Meson Mass

Details Neutron Star Matter with In-Medium Meson Mass Neutron Star Matter with In-Medium Meson Mass

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..387h&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

We investigate the properties of the neutron star matter with the relativistic mean field models. We incorporate in quantum hadrodynamics and quark-meson coupling models a possible reduction of meson masses in nuclear matter. The equation of state for neutron star matter is calculated at the matter densities up to 4 times the nuclear saturation density. We find that the equation of state and the composition of the matter are sensitive to the behavior of meson masses in medium.

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