Abstract

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.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.