Gravitational Aharonov-Bohm effect and gravitational lensing
A. Tartaglia
Abstract
Considering the spacetime around a rotating massif body it is seen that the time of flight of a light ray is different whether it travels on one side of the source or on the other. The difference is proportional to the angular momentum of the body. In the case that a compact rapidly rotating object is the source of a gravitational lensing effect, the contribution coming from the above mentioned gravitational Aharonov-Bohm effect should be added to the other causes of phase difference between light rays coming from different images of the same object.
Create a lesson
Related papers
Constraining the Progenitor Orbits of Sequential Black-Hole Mergers in Hierarchical Triples: Peters-Based Estimates
Felix M. Heinze, Zhoujian Cao
Cubic Quasinormal Modes in the Black-Hole Ringdown
Neev Khera, Huan Yang
Separation of variables for coupled radiative perturbations of Kerr-Newman-de Sitter black holes
Daisuke Yoshida
An extension principle for Einstein-Maxwell-charged scalar field system with finite Doppler exponent
Xinliang An, Haoyang Chen, Taoran He
A Scale-Critical μ<38 Extension Principle for Spherically Symmetric Einstein-Scalar Field System
Xinliang An, Haoyang Chen, Jaydeep Singh
Analytical Time-Domain Waveforms for Black-Hole Scattering in the Post-Minkowskian Expansion
Stefano De Angelis, Vincent F. He, Julio Parra-Martinez