Abstract
We show that on the future horizon of a certain type of 4-dimensional, stationary, pseudo-Riemannian spacetime, Hawking radiation will generally be produced, with a temperature proportional to the surface gravity at the horizon. The Hawking radiations of the Schwarzschild, Reissner-Nordstrom and Kerr-Mewman black-holes and the de Sitter universe appear as particular instances of our proof. Unlike a uniformly accelerated detector, a uniformly rotating detector cannot detect Rindler radiation
Sign-in/Register to access full text options 
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.
