An Exact Anisotropic Quark Star Model

Details An Exact Anisotropic Quark Star Model An Exact Anisotropic Quark Star Model

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002chjaa...2..248m&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 2, p. 248-259

Astronomy and Astrophysics

Astrophysics

19

Stars, Quark: Interior Solution: Anisotropy

Scientific paper

We present an exact analytical solution of the gravitational field equations describing a static spherically symmetric anisotropic quark matter distribution. The radial pressure inside the star is assumed to obey a linear equation of state, while the tangential pressure is a complicated function of the radial coordinate. In order to obtain the general solution of the field equations a particular density profile inside the star is also assumed. The anisotropic pressure distribution leads to an increase in the maximum radius and mass of the quark star, which in the present model is around three solar masses.

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