Neutron star equation of state

Details Neutron star equation of state Neutron star equation of state

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010newar..54..101l&link_type=abstract

New Astronomy Reviews, Volume 54, Issue 3-6, p. 101-109.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

New observations of neutron stars from sources such as radio pulsars, X-ray binaries, quasi-periodic oscillators, X-ray bursters and thermally-emitting isolated neutron stars, can ultimately constrain the dense matter equation of state. Observable quantities include neutron star masses, radii, rotation rates, radiation radii, redshifts, moments of inertia, temperatures and ages. Several ways in which these quantities can lead to theoretical limits are discussed.

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