We develop here a new procedure within Einstein's theory of gravity to generate equilibrium configurations that result as the final state of gravitational collapse from regular initial …
M Sharif, Z Yousaf - Astrophysics and space science, 2014 - Springer
We study the factors affecting the stability of a locally isotropic spherical self-gravitating systems in f (R, T) gravity, where R is the Ricci curvature invariant and T is the trace of stress …
G Leon, EN Saridakis - Journal of Cosmology and Astroparticle …, 2015 - iopscience.iop.org
We investigate the cosmological behavior of mimetic F (R) gravity. This scenario is the F (R) extension of usual mimetic gravity classes, which are based on re-parametrizations of the …
XX Zeng, YW Han, DY Chen - Chinese Physics C, 2019 - iopscience.iop.org
As a charged fermion drops into a BTZ black hole, the laws of thermodynamics and the weak cosmic censorship conjecture are investigated in both the normal and extended phase …
We study spherically symmetric gravitational collapse of a homogeneous perfect fluid in Rastall gravity. Considering a linear equation of state (EoS) for the fluid profiles, we examine …
Z Yousaf, M Bhatti, U Farwa - Mon. Not. R. Astron. Soc., 2017 - academia.edu
This manuscript explores the unstable/stable regimes of self-gravitating matter configuration of spherical star due to the impact of modification in gravity model as studied in f (R, T …
M Sharif, Z Yousaf - Astrophysics and Space Science, 2015 - Springer
In this paper, we discuss dynamical properties of dissipative collapsing cylindrical self- gravitating systems with account of f (R)= R+ γR 2+ β 1 R 3 gravity model. In this perspective …
M Sharif, Z Yousaf - Monthly Notices of the Royal Astronomical …, 2014 - academic.oup.com
This paper performs stability analysis of an adiabatic anisotropic cylindrical collapsing system in metric f (R) gravity. We construct general collapse equation from the dynamical …
In this paper, we study the effects of modification of gravity on the problem of dynamical instability of the spherical relativistic anisotropic interiors. We have considered non-zero …