Observations of neutron stars and the equation of state of matter at high densities

Details Observations of neutron stars and the equation of state of matter at high densities Observations of neutron stars and the equation of state of matter at high densities

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011prpnp..66..674t&link_type=abstract

Progress in Particle and Nuclear Physics, Volume 66, Issue 3, p. 674-680.

Physics

Nuclear Physics

1

Scientific paper

We summarize the constraints on the equation of state of high-density nuclear matter derived from neutron star observations. The most stringent constraints are provided by the largest mass, the largest radius, the highest rotational frequency, and the maximum surface gravity observed for neutron stars. The combination of these constraints allows only nuclear equations of state which are quite stiff.

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