paper

Quark Stars in Gravity

arXiv:1701.04761 · doi:10.1140/epjc/s10052-017-4637-8

Abstract

We derive a working model for the Tolman-Oppenheimer-Volkoff equation for quark star systems within the modified -gravity class of models. We consider -gravity for a static spherically symmetric space-time. In this instance the metric is built from a more fundamental tetrad vierbein from which the metric tensor can be derived. We impose a linear parameter parameter, namely taking and investigate the behavior of a linear energy-momentum tensor trace, . We also outline the restrictions which modified -gravity imposes upon the coupling parameters. Finally we incorporate the MIT bag model in order to derive the mass-radius and mass-central density relations of the quark star within -gravity.

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