Gaussian black holes in Rastall Gravity
General Relativity and Quantum Cosmology
2018-01-18 v1 High Energy Physics - Theory
Abstract
In this short note we present the solution of Rastall gravity equations sourced by a Gaussian matter distribution. We find that the black hole metric shares all the common features of other regular, General Relativity BH solutions discussed in the literature: there is no curvature singularity and the Hawking radiation leaves a remnant at zero temperature in the form of a massive ordinary particle.
Cite
@article{arxiv.1709.05795,
title = {Gaussian black holes in Rastall Gravity},
author = {Euro Spallucci and Anais Smailagic},
journal= {arXiv preprint arXiv:1709.05795},
year = {2018}
}
Comments
11 pages, 4 figures, in print on IJMPD