Neutron star interiors and the equation of state of ultra-dense matter

Details Neutron star interiors and the equation of state of ultra-dense matter Neutron star interiors and the equation of state of ultra-dense matter

2006-12-05

arxiv.org/abs/astro-ph/0612132v1

AIPConf.Proc.892:515-517,2007

Astronomy and Astrophysics

Astrophysics

3 pages, 4 figures; Paper presented at the Int. Conf. on Quark Confinement and the Hadron Spectrum VII, Ponta Delgada, Acores,

Scientific paper

10.1063/1.2714458

There has been much recent progress in our understanding of quark matter,
culminating in the discovery that if such matter exists in the cores of neutron
stars it ought to be in a color superconducting state. This paper explores the
impact of superconducting quark matter on the properties (e.g., masses, radii,
surface gravity, photon emission) of compact stars.

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