Rapidly rotating strange stars for a new equation of state of strange quark matter

Details Rapidly rotating strange stars for a new equation of state of strange quark matter Rapidly rotating strange stars for a new equation of state of strange quark matter

2000-09-20

arxiv.org/abs/astro-ph/0009328v1

Astrophys.J. 541 (2000) L71

Astronomy and Astrophysics

Astrophysics

Two figures, uses psbox.tex and emulateapj5.sty

Scientific paper

10.1086/312897

For a new equation of state of strange quark matter, we construct equilibrium sequences of rapidly rotating strange stars in general relativity. The sequences are the normal and supramassive evolutionary sequences of constant rest mass. We also calculate equilibrium sequences for a constant value of $\Omega$ corresponding to the most rapidly rotating pulsar PSR 1937 + 21. In addition to this, we calculate the radius of the marginally stable orbit and its dependence on $\Omega$, relevant for modeling of kilo-Hertz quasi-periodic oscillations in X-ray binaries.

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