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Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter

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Published 2000 September 19 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Ignazio Bombaci et al 2000 ApJ 541 L71 DOI 10.1086/312897

1538-4357/541/2/L71

Abstract

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 Ω corresponding to the most rapidly rotating pulsar PSR 1937+21. In addition, we calculate the radius of the marginally stable orbit and its dependence on Ω, relevant for modeling of kilohertz quasi-periodic oscillations in X-ray binaries.

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10.1086/312897