Abstract
A model describing a collapsing sphere with radial heat flow is studied. Vaidya’s pure radiation field is taken as the exterior solution. The motion of the boundary surface follows from the matching conditions. In the remote part, the evolution starts with the interior and exterior Schwarzschild solution.
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.
