Relativistic strange quark stars in Lovelock gravity

Grigoris Panotopoulos, ANGEL RINCON RIVERO

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We study relativistic non-rotating stars in the framework of Lovelock gravity. In particular, we consider the Gauss-Bonnet term in a five-dimensional spacetime, and we investigate the impact of the Gauss-Bonnet parameter on properties of the stars, both isotropic and anisotropic. For matter inside the star, we assume a relativistic gas of de-confined massless quarks. We integrate the modified Tolman-Oppenheimer-Volkoff equations numerically, and we obtain the mass-to-radius profile, the compactness of the star as well as the gravitational red-shift for several values of the Gauss-Bonnet parameter. The maximum star mass and radius are also reported.

Original languageEnglish
Article number472
JournalEuropean Physical Journal Plus
Volume134
Issue number9
DOIs
StatePublished - 1 Sep 2019
Externally publishedYes

Fingerprint Dive into the research topics of 'Relativistic strange quark stars in Lovelock gravity'. Together they form a unique fingerprint.

Cite this