Abstract
In a general curved space–time, the requirements that the Feynman Green’s function be symmetric and have the Hadamard form are shown to result in specific constraints on the local behavior of the function. These constraints are solved yielding a general form for the function.
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.
