Z Yousaf - Astrophysics and Space Science, 2018 - Springer
The aim of this study is to analyze the role of modification of gravity on some dynamical properties of spherically symmetric relativistic systems. In this settings, the mathematical …
We examine, in a general manner, the role played by the initial density and velocity distributions in the gravitational collapse of a spherically symmetric inhomogeneous dust …
An outstanding problem in gravitation theory and relativistic astrophysics today is to understand the final outcome of an endless gravitational collapse. Such a continual collapse …
L Herrera, A Di Prisco, J Ibáñez - … Review D—Particles, Fields, Gravitation, and …, 2011 - APS
We consider Lemaitre-Tolman-Bondi spacetimes from the point of view of a tilted observer, ie one with respect to which the fluid is radially moving. The imperfect fluid and the …
RA Sussman - Classical and Quantum Gravity, 2013 - iopscience.iop.org
We obtain covariant expressions that generalize the growing and decaying density modes of linear perturbation theory of dust sources by means of the exact density perturbation from …
The action for a relativistic free particle of mass m receives a contribution− m R (x, y) from a path of length R (x, y) connecting the events xi and y i. Using this action in a path integral …
S Ray, A Panda, B Majumder, MR Islam… - Chinese Physics …, 2022 - iopscience.iop.org
In this study, we investigate the collapsing scenario for the k-essence emergent Vaidya spacetime in the context of massive gravity's rainbow. For this study, we consider that the …
PS Joshi, IH Dwivedi - Classical and Quantum Gravity, 1999 - iopscience.iop.org
Generalizing earlier results on the initial data and the final fate of dust collapse, we study here the relevance of the initial state of a spherically symmetric matter cloud towards …
We study fluid distributions endowed with hyperbolic symmetry, which share many common features with Lemaitre–Tolman–Bondi (LTB) solutions (eg, they are geodesic, shearing, and …