Abstract
In this paper, we investigate light bending in the spacetime of regular black holes with cosmic strings in weak field limits. To do so, we apply the Gauss-Bonnet theorem to the optical geometry of the black hole; and, using the Gibbons-Werner method, we obtain the deflection angle of light in the weak field limits which shows that the bending of light is a global and topological effect. Afterwards, we demonstrate the effect of a plasma medium on the deflection of light by a regular black hole with cosmic strings. We discuss that increasing cosmic string parameter μ and mass M0 will increase the bending angle.
Original language | English |
---|---|
Article number | 104075 |
Journal | Physical Review D |
Volume | 99 |
Issue number | 10 |
DOIs | |
State | Published - 15 May 2019 |