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

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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 \(\alpha \), 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 6th-order WKB method. We tabulate values of quasinormal frequencies for various values of \(\alpha \), angular momentum \(\ell \), and overtone number n. We also graphically show the dependence of real and imaginary parts of quasinormal frequency on \(\alpha \) and \(\ell \). Additionally, We study the convergence of the WKB method for various values of pair \((n,\ell )\). Finally, we shed light on the dependence of the Hawking temperature on the parameter \(\alpha \) and the dependence of greybody bounds on \(\alpha \) and \(\ell \).

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    Sohan Kumar Jha

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Jha, S.K. Photonsphere, shadow, quasinormal modes, and greybody bounds of non-rotating Simpson–Visser black hole. Eur. Phys. J. Plus 138, 757 (2023). https://doi.org/10.1140/epjp/s13360-023-04384-5

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