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- W3019608314 abstract "This paper deals with the existence of a compact stellar object, precisely strange (quark) star, in the framework of Einstein's General Theory of Relativity with Tolman $V$ metric potential, which is one of the simplest forms of potential among his proposals. The potential is given by $e^{nu}=Kr^{2n}$, where $K$ is the constant and $n$ is a parameter [R.C. Tolman, Phys. Rev. {bf55}, 364 (1939)]. Considering charged, static, spherically symmetric, isotropic fluid sphere we have studied different physical features of some strange star candidates namely $EXO 1785-248$, $LMC X-4$, $SMC X-1$, $SAX J1808.4-3658$, $4U 1538-52$ and $Her X-1$. To represent the strange quark matter (SQM) distribution we have employed the simplest form of MIT bag equation of state (EOS), which provides a linear relationship between pressure and density of the matter through Bag constant $B$. We have done several tests for the stability criteria and the physical acceptability of the proposed model. The results show consistency with energy condition, TOV equation, adiabatic index, etc. We have calculated different physical parameters of our model for the three different consecutive values of Bag constant $B$ which are $83 MeV/fm^3$, $90 MeV/fm^3$ and $100 MeV/fm^3$. Among them with $B=90 MeV/fm^3$ we have analyzed different properties of the proposed strange star candidates." @default.
- W3019608314 created "2020-05-01" @default.
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- W3019608314 date "2020-04-22" @default.
- W3019608314 modified "2023-09-23" @default.
- W3019608314 title "Charged strange stellar model with Tolman $V$ metric potential in the Einstein-Maxwell space-time" @default.
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- W3019608314 doi "https://doi.org/10.48550/arxiv.2004.10480" @default.
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