Abstract
Introduction/purpose: Starting from general relativity, black hole generation and effects are investigated. Method: Einstein's equation and its Schwarzschild solution are employed to study black holes. Quantum mechanics is used to obtain Hawking's radiation. Results: Black holes are actually not completely black - they radiate energy during their lifetime. Conclusions: Black holes could evaporate and this effect is observable if their mass is sufficiently small. Their entropy scales differently with respect to their mass from that of other objects in thermodynamics.
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.
