Neutron Stars and Massive Quark Matter

Details Neutron Stars and Massive Quark Matter Neutron Stars and Massive Quark Matter

1995-05-26

arxiv.org/abs/nucl-th/9505037v1

Phys. Lett. B380 (1996) 13

Physics

Nuclear Physics

Nuclear Theory

8 pages, Revtex style, 4 uuencoded figures appended

Scientific paper

10.1016/0370-2693(96)00479-0

Using the Color-Dielectric model to describe quark confinement, including
strange quarks and accounting for beta--equilibrium, we get masses for a static
neutron star in the range $1.3\leq M/M_{\odot}\leq 1.54 $ for a radius
$R\approx 9$ km. Rapid cooling through the direct URCA mechanism is obtained.
The implications for the composition of neutron stars is discussed.

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