B. K. Guha

Relativistic compact stars in

We provide a set of exact spherically symmetric solutions describing the interior of a relativistic star under f(T)

f(T)

f(T)

gravity admitting conformal motion

modified gravity. To tackle the problem with lucidity we also assume the existence of a conformal Killing vector field within this f(T)

Anisotropic stars with non-static conformal symmetry

f(T)

Compact stars in f(R,\mathcal {T}) gravity

gravity. We study several cases of interest to explore physically valid features of the solutions.

Relativistic model for anisotropic strange stars

We propose a model for relativistic compact star with anisotropy and analytically obtain exact spherically symmetric solutions which describe interior of the dense star admitting non-static conformal symmetry. Several features of the solutions, including drawbacks of the model, have been explored and discussed. For this purpose we have provided the energy conditions, TOV equation and other physical requirements and thus thoroughly have investigated stability, mass-radius relation and surface redshift of the model. It is observed that most of the features are well matched with the compact strange stars.

Strange stars in f(R,) gravity

In the present paper we generate a set of solutions describing the interior of a compact star under

Compact stars in

f(R,T)

f(R,T)

theory of gravity which admits conformal motion. We consider the equation of state (EOS)

gravity

p=\omega\rho