Gravitationally collapsing stars in $f(R)$ gravity
General Relativity and Quantum Cosmology
2021-04-05 v3 High Energy Physics - Theory
Abstract
The gravitational dynamics of a collapsing matter configuration which is simultaneously radiating heat flux is studied in gravity. Three particular functional forms in gravity are considered to show that it is possible to envisage boundary conditions such that the end state of the collapse has a weak singularity and that the matter configuration radiates away all of its mass before collapsing to reach the central singularity.
Cite
@article{arxiv.2102.08717,
title = {Gravitationally collapsing stars in $f(R)$ gravity},
author = {Ayan Chatterjee and Suresh C. Jaryal},
journal= {arXiv preprint arXiv:2102.08717},
year = {2021}
}
Comments
23 pages, 35 figures