Phase transitions of regular schwarzschild-anti-desitter black holes

3Citations
Citations of this article
7Readers
Mendeley users who have this article in their library.
Get full text

Abstract

We study a solution of the Einstein’s equations generated by a selfgravitating, anisotropic, static, non-singular matter fluid. The resulting Schwarzschild like solution is regular and accounts for smearing effects of noncommutative fluctuations of the geometry.We call this solution regular Schwarzschild spacetime. In the presence of an Anti-deSitter cosmological term, the regularized metric offers an extension of the Hawking-Page transition into a van der Waals-like phase diagram. Specifically the regular Schwarzschild-Anti-deSitter geometry undergoes a first order small/large black hole transition similar to the liquid/gas transition of a real fluid. In the present analysis we have considered the cosmological constant as a dynamical quantity and its variation is included in the first law of black hole thermodynamics.

Cite

CITATION STYLE

APA

Frassino, A. M. (2016). Phase transitions of regular schwarzschild-anti-desitter black holes. In Springer Proceedings in Physics (Vol. 170, pp. 241–247). Springer Science and Business Media, LLC. https://doi.org/10.1007/978-3-319-20046-0_28

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free