paper

Photonsphere, shadow, quasinormal modes, and greybody bounds of non-rotating Simpson-Visser black hole

arXiv:2309.06454 · doi:10.1140/epjp/s13360-023-04384-5

Abstract

In this manuscript, we study photonsphere, shadow, quasinormal modes, Hawking temperature, and greybody bounds of a non-rotating Simpson-Visser black hole which is a regular black hole. We observe that though the radius of the photonsphere does depend on the Simpson-Visser parameter , the shadow radius is independent of it. The shadow radius is found to be equal to that for Schwarzschild black hole. We, then, study quasinormal frequencies of the Simpson-Visser black hole for scalar and electromagnetic perturbations with the help of th order WKB method. We tabulate values of quasinormal frequencies for various values of , angular momentum , and overtone number . We also graphically show the dependence of real and imaginary parts of quasinormal frequency on and . Additionally, We study the convergence of the WKB method for various values of pair . Finally, we shed light on the dependence of the Hawking temperature on the parameter and the dependence of greybody bounds on and .

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