Thermodynamic Geometries of Black Holes

Details Thermodynamic Geometries of Black Holes Thermodynamic Geometries of Black Holes

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1511a&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

We report outcomes from the geometrical studies (Ruppeiner and Weinhold geometries) of thermodynamics of certain black hole families in various spacetime dimensions e.g. BTZ, general relativity and higher-dimensional Einstein-Maxwell gravity. So far the most physically suggestive result occurs for the Kerr black hole in D ≥ 5 in which thermodynamic stability is found to be encoded in the curvature of the Ruppeiner metric. This is consistent with the known result in the literature.

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