Geometry of the thermodynamics of the black holes in Ho řava-Lifshitz gravity

Details Geometry of the thermodynamics of the black holes in Ho řava-Lifshitz gravity Geometry of the thermodynamics of the black holes in Ho řava-Lifshitz gravity

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011gregr..43...41b&link_type=abstract

General Relativity and Gravitation, Volume 43, Issue 1, pp.41-50

Computer Science

4

Thermodynamics, Black Hole, Phase Transition

Scientific paper

Recently, a non-relativistic renormalizable theory of gravity has been proposed by Ho řava. This theory is essentially a field theoretic model for a UV complete theory of gravity and it reduces to Einstein's general relativity at large distances. Subsequently, Cai and his collaborators have obtained black hole solution in this gravity theory and studied the thermodynamic properties of the black hole solutions. In present work, we investigate the geometric thermodynamics of the above black hole solutions and examine the possibilities of any phase transition.

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