https://doi.org/10.1140/epjc/s10052-024-12812-8
Regular Article - Theoretical Physics
Analysis of Dyonic ModMax black hole through accretion disk
1
Department of Mathematics, Bahauddin Zakariya University, Vehari Campus, 61100, Vehari, Pakistan
2
Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur, Pakistan
3
Department of Mathematics, Zhejiang Normal University, 321004, Jinhua, Zhejiang, China
4
Department of Mathematics, King Abdulaziz University, 21589, Jeddah, Saudi Arabia
5
Department of Mathematics and Statistics, University of South Florida, 33620-5700, Tampa, FL, USA
6
School of Mathematical and Statistical Sciences, North-West University, Mafikeng Campus, Mahikeng, South Africa
Received:
2
March
2024
Accepted:
30
March
2024
Published online:
4
May
2024
In the present study, we probe the geodesic motion and accretion of particles around the spherically symmetric Dyonic ModMax black hole using isothermal fluid. The geodesic motion of the particles around the black hole leads to the formation of disk like structure during the accretion process. We compute the radiant temperature, radioactive efficiency, radiant flux energy, circular orbits and observe the behavior of particles within stable circular orbits in the equatorial plane. We examine how the particles are perturbed during the process by using restoring forces and the oscillatory behavior of the particles surrounding a compact object and also investigate the fluid’s critical flow and maximum accretion rate. Our findings demonstrate how the black hole parameter 
and charge Q affect the circular geodesic of particles as well as the maximum accretion rate of the Dyonic ModMax black hole.
© The Author(s) 2024
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Funded by SCOAP3.
