The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …

In the context of $ f (R)= R+\alpha R^{2} $ gravity, we study the existence of neutron and
quark stars for various α with no intermediate approximation in the system of equations …

In this paper, we present charged dilatonic black holes in gravity's rainbow. We study the
geometric and thermodynamic properties of black hole solutions. We also investigate the …

In this paper, we consider a spherical symmetric metric to extract the hydrostatic equilibrium
equation of stars in (3+ 1)-dimensional gravity's rainbow in the presence of cosmological …

In the context of f (R) gravity theories, we show that the apparent mass of a neutron star as
seen from an observer at infinity is numerically calculable but requires careful matching, first …

Motivated by the recent interests in spin− 2 massive gravitons, we study the structure of
neutron star in the context of massive gravity. The modifications of TOV equation in the …

Motivated by low energy effective action of string theory and numerous applications of BTZ
black holes, we will consider minimal coupling between dilaton and nonlinear …

This paper is devoted to an investigation of nonlinearly charged dilatonic black holes in the
context of gravity's rainbow with two cases:(1) by considering the usual entropy,(2) in the …

We apply quadratic f (R)= R+ epsilon R 2 field equations, where epsilon has a dimension [L
2], to static spherical stellar model. We assume the interior configuration is determined by …

As we know, the effect of strong magnetic field causes the anisotropy for the magnetized
compact objects. Therefore, in this paper, we have studied the structure properties of …