Rotating Quark Stars in General Relativity

Rotating Quark Stars in General Relativity

We have built quasi-equilibrium models for uniformly rotating quark stars in general relativity. The conformal flatness approximation is employed and the Compact Object CALculator (cocal) code is extended to treat rotating stars with surface density discontinuity. In addition to the widely used MIT...

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Bibliographic Details
Main Authors: Enping Zhou, Antonios Tsokaros, Luciano Rezzolla, Renxin Xu, Kōji Uryū
Format: Article
Language:English
Published: MDPI AG 2018-03-01
Series:Universe
Subjects:
pulsars
quark stars
general relativity
Online Access:http://www.mdpi.com/2218-1997/4/3/48

Internet

http://www.mdpi.com/2218-1997/4/3/48

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