Anisotropic charged strange stars in Krori-Barua spacetime under f (R, T) gravity
We present spherically symmetric anisotropic charged strange stars under the framework of f
(R, T) gravity. For this we consider that the Lagrangian density is a linear function of R and T
where R is the Ricci Scalar and T represents the trace of the energy–momentum tensor.
These stars are considered to be built with Strange Quark Matter (SQM) distribution. To
describe this SQM distribution inside the stellar bodies, we incorporate the simplest form of
phenomenological MIT bag model equation of state (EOS) pr= 1 3 (ρ− 4 B g), where pr is the …
(R, T) gravity. For this we consider that the Lagrangian density is a linear function of R and T
where R is the Ricci Scalar and T represents the trace of the energy–momentum tensor.
These stars are considered to be built with Strange Quark Matter (SQM) distribution. To
describe this SQM distribution inside the stellar bodies, we incorporate the simplest form of
phenomenological MIT bag model equation of state (EOS) pr= 1 3 (ρ− 4 B g), where pr is the …
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