Deflection angle of photon through dark matter by black holes and wormholes using the Gauss-Bonnet theorem
arXiv:1806.05549 · doi:10.3390/universe5050115
Abstract
In this research, we use the Gibbons-Werner method (Gauss-Bonnet theorem) on the optical geometry of a black hole and wormhole, extending the calculation of the weak gravitational lensing within the Maxwell's fish eye-like profile and dark matter medium. The angle is seen as a partially topological effect and the Gibbons-Werner method can be used on any asymptotically flat Riemannian optical geometry of compact objects in dark matter medium.
Accepted to publish in a special issue of Universe "Gravitational Lensing and Optical Geometry: A Centennial Perspective" (https://www.mdpi.com/journal/universe/special_issues/gravitational_lensing_optical_geometry#info)