Gravitational lensing in the Simpson-Visser black-bounce spacetime in a strong deflection limit
arXiv:2011.03932 · doi:10.1103/PhysRevD.103.024033
Abstract
A Simpson-Visser spacetime has two nonnegative parameters and and its metric is correspond with (i) a Schwarzschild metric for and , (ii) a regular black hole metric for , (iii) a one-way traversable wormhole metric for , (vi) a two-way traversable wormhole metric for , and (v) an Ellis-Bronnikov wormhole metric for and . The spacetime is one of the most useful spacetimes for the purpose of comprehensively understanding gravitational lensing of light rays reflected by a photon sphere of black holes and wormholes. We have investigated gravitational lensing in the Simpson-Visser spacetime in a strong deflection limit in all the nonnegative parameters of and . In a case of , two photon spheres and an antiphoton sphere at the throat degenerate into a marginally unstable photon sphere. The deflection angle of the light rays reflected by the marginally unstable photon sphere at the throat diverges nonlogarithmically in the strong deflection limit.
arXiv comment13 pages, 6 figures, minor correction, references added, accepted for publication in Physical Review D
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