Quark stars admitting a one-parameter group of conformal motions

Abstract

An exact analytical solution describing the interior of a charged strange quark star is found under the assumption of spherical symmetry and the existence of a one-parameter group of conformal motions. The solution describes a unique static charged configuration of quark matter with radius $R=9.46$ km and total mass $M=2.86M_{\odot }$.

arXiv comment5 pages, no figures, to appear in IJMPD

References in corpus (2)

• Conversion of neutron stars to strange stars as an origin of gamma-ray bursts
• Fast rotation of strange stars

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