Abstract
For a proposed model of decaying dark energy the deflection of light in spherically-symmetric static Gross–Perry spacetime and in Kerr–Taub–Bolt spacetime is considered. Estimates are given for the variation of the standard deflection of light in the field of the Sun.
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.
