https://doi.org/10.1140/epjp/s13360-023-04501-4
Regular Article
Particle acceleration and thermodynamics of the rotating Simpson–Visser black hole
1
National University of Uzbekistan, 100174, Tashkent, Uzbekistan
2
Ulugh Beg Astronomical Institute, Astronomy St 33, 100052, Tashkent, Uzbekistan
3
New Uzbekistan University, Mustaqillik ave. 54, 100007, Tashkent, Uzbekistan
4
Central Asian University, Milliy Bog’ Street 264, 111221, Tashkent, Uzbekistan
5
Inha University in Tashkent, Ziyolilar 9, 100170, Tashkent, Uzbekistan
6
Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, 100000, Tashkent, Uzbekistan
7
Tashkent State Technical University, 100095, Tashkent, Uzbekistan
Received:
21
June
2023
Accepted:
15
September
2023
Published online:
25
September
2023
We have considered a time-like geodesics in the background of rotating Simpson–Visser (SV) black hole (BH) to examine structure of the horizon and ergosphere. The innermost stable circular orbits (ISCO) and the effective potential, which controls the particle’s motion in spacetime, have been studied for different values of parameters in SV BH. Center-of-mass (CM) energy of two colliding particles near the horizon has been investigated for both extremal and non-extremal cases. Furthermore, thermodynamic properties of SV black hole have been also investigated in detail.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
