Abstract
Using the thin film brick-wall model and WKBapproximation, the entropy of the Dirac field in the non-stationary andslowly changing Reissner-Nordström (R-N) black hole is calculated. Theresult shows that the entropy of the R-N black hole is still proportional toits surface area if we choose proper cut-off.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
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.