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Particle acceleration and thermodynamics of the rotating Simpson–Visser black hole

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Abstract

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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Acknowledgements

This research is partly supported by Research Grant F-FA-2021-510 of the Uzbekistan Ministry for Innovative Development.

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Authors and Affiliations

  1. National University of Uzbekistan, 100174, Tashkent, Uzbekistan

    Abdurakhmon Nosirov & Ahmadjon Abdujabbarov

  2. Ulugh Beg Astronomical Institute, Astronomy St 33, 100052, Tashkent, Uzbekistan

    Abdurakhmon Nosirov & Ahmadjon Abdujabbarov

  3. New Uzbekistan University, Mustaqillik ave. 54, 100007, Tashkent, Uzbekistan

    Farruh Atamurotov

  4. Central Asian University, Milliy Bog’ Street 264, 111221, Tashkent, Uzbekistan

    Farruh Atamurotov

  5. Inha University in Tashkent, Ziyolilar 9, 100170, Tashkent, Uzbekistan

    Farruh Atamurotov

  6. Institute of Fundamental and Applied Research, National Research University TIIAME, Kori Niyoziy 39, 100000, Tashkent, Uzbekistan

    Farruh Atamurotov

  7. Tashkent State Technical University, 100095, Tashkent, Uzbekistan

    Gulzoda Rakhimova & Ahmadjon Abdujabbarov

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  1. Abdurakhmon Nosirov
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Nosirov, A., Atamurotov, F., Rakhimova, G. et al. Particle acceleration and thermodynamics of the rotating Simpson–Visser black hole. Eur. Phys. J. Plus 138, 846 (2023). https://doi.org/10.1140/epjp/s13360-023-04501-4

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