Gravitational time advancement and its possible detection

Abstract

The gravitational time advancement is a natural but a consequence of curve space-time geometry. In the present work the expressions of gravitational time advancement have been obtained for geodesic motions. The situation when the distance of signal travel is small in comparison to the distance of closest approach has also been considered. The possibility of experimental detection of time advancement effect has been explored.

5 pages, 4 figures, a part of the work has been changed in the revised version

References in corpus (3)

• General post-Minkowskian expansion of time transfer functions
• The Laser Astrometric Test of Relativity (LATOR) Mission
• The Laser Astrometric Test of Relativity Mission

Cited by in corpus (9)

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• Times of arrival (TOA) of signals in the Kerr-MOG black hole
• Vacuum Brans-Dicke theory in the Jordan and Einstein frames: can they be distinguished by lensing?
• Probing dark matter and dark energy through Gravitational Time Advancement
• Gravitational time advancement effect in Bumblebee gravity for Earth bound systems
• Is it possible to distinguish between different black hole solutions using the Shapiro time delay?
• Can a regular black hole be observationally distinguished from singular black holes as spinning lens partner in PSR-BH binaries?