Gaussian black holes in Rastall Gravity
arXiv:1709.05795 · doi:10.1142/S0218271818500037
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.
arXiv comment11 pages, 4 figures, in print on IJMPD
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