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Entropy 2015, 17(8), 5145-5156; doi:10.3390/e17085145

Scale-Invariant Rotating Black Holes in Quadratic Gravity

1,2,†
,
1,2,†,* and 1,2,†
1
Dipartimento di Fisica, Università di Trento, Via Sommarive 14, 38123 Trento, Italy
2
INFN-TIFPA, Via Sommarive 14, 38123 Trento, Italy
These authors contributed equally to this work.
*
Author to whom correspondence should be addressed.
Academic Editor: Remo Garattini
Received: 23 June 2015 / Revised: 15 July 2015 / Accepted: 20 July 2015 / Published: 23 July 2015
(This article belongs to the Special Issue Entropy in Quantum Gravity and Quantum Cosmology)
View Full-Text   |   Download PDF [213 KB, uploaded 23 July 2015]

Abstract

Black hole solutions in pure quadratic theories of gravity are interesting since they allow the formulation of a set of scale-invariant thermodynamics laws. Recently, we have proven that static scale-invariant black holes have a well-defined entropy, which characterizes equivalent classes of solutions. In this paper, we generalize these results and explore the thermodynamics of rotating black holes in pure quadratic gravity. View Full-Text
Keywords: rotating black holes; modified gravity; thermodynamics rotating black holes; modified gravity; thermodynamics
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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MDPI and ACS Style

Cognola, G.; Rinaldi, M.; Vanzo, L. Scale-Invariant Rotating Black Holes in Quadratic Gravity. Entropy 2015, 17, 5145-5156.

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