Abstract
By virtue of a semiclassical adiabatic invariant in this paper, we quantize the horizon area of a Kerr-Newman black hole by making use of the period of the gravity system. We exploit exclusively the basic properties of the adiabatic invariant. It is found that the result produced by our method is consistent with the one obtained by calculating the adiabatic invariant step by step.
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 callDisclaimer: 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.
