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.
Gaussian black holes in Rastall gravity / Spallucci, Euro; Smailagic, Anais. - In: INTERNATIONAL JOURNAL OF MODERN PHYSICS D. - ISSN 0218-2718. - 27:2(2018), pp. 1850003.1-1850003.11. [10.1142/S0218271818500037]
Gaussian black holes in Rastall gravity
Spallucci, Euro;
2018-01-01
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.File in questo prodotto:
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