Gravitational lensing by $k-n$ generalized black-bounce space-times
Gravitational lensing by $k-n$ generalized black-bounce space-times
We study gravitational lensing by $k-n$ generalized black-bounce space-times both in regimes of weak and strong field approximations. These metrics interpolate between regular black holes and one-way or traversable wormholes. First, we investigate the light-like geodesic trajectories and derive an analytical expression for the deflection angle in terms of the bounce parameter in the weak-field gravitational regime. We then turn to the strong-field gravitational regime and display the behavior of the bending angle as a function of both the impact parameter and the bounce parameter. Next, using the lens equations, we analyze how the observables for \textit{Sagittarius} A* behave concerning the bounce parameter. We obtain the shadow's radii for some black-bounce metrics and plot the graph of their sizes, comparing them with the Schwarzschild one.
C. Furtado、A. L. A. Moreira、J. R. Nascimento、A. Yu. Petrov、P. J. Porfirio
物理学天文学
C. Furtado,A. L. A. Moreira,J. R. Nascimento,A. Yu. Petrov,P. J. Porfirio.Gravitational lensing by $k-n$ generalized black-bounce space-times[EB/OL].(2025-04-28)[2025-05-19].https://arxiv.org/abs/2504.19920.点此复制
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