https://doi.org/10.1140/epjc/s10052-023-12033-5
Regular Article - Theoretical Physics
Matter accretion onto the magnetically charged Euler–Heisenberg black hole with scalar hair
1
Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur, Pakistan
2
National Astronomical Observatories, Chinese Academy of Sciences, 100101, Beijing, People’s Republic of China
3
Institute for Theoretical Physics and Cosmology, Zhejiang University of Technology, 310023, Hangzhou, People’s Republic of China
4
United Center for Gravitational Wave Physics (UCGWP), Zhejiang University of Technology, 310023, Hangzhou, People’s Republic of China
5
Department of Physics, Zhejiang Normal University, 321004, Jinhua, People’s Republic of China
6
New Uzbekistan University, Mustaqillik Ave. 54, 100007, Tashkent, Uzbekistan
Received:
30
July
2023
Accepted:
12
September
2023
Published online:
25
September
2023
This paper deals with astrophysical accretion onto the magnetically charged Euler–Heisenberg black holes with scalar hair. We examine the accretion process of a variety of perfect fluids, including polytropic and isothermal fluids of the ultra-stiff, ultra-relativistic, and sub-relativistic forms, when fluid is accreting in the vicinity of the black hole. By using the Hamiltonian dynamical approach, we can find the sonic or critical points numerically for the various types of fluids that are accreting onto the black hole. Furthermore, for several types of fluids, the solution is provided in closed form, expressing phase diagram curves. We compute the mass accretion rate of a magnetically charged Euler–Heisenberg black hole with scalar hair. We observe that the maximum accretion rate is attained for small values of the black hole parameters. We may be able to understand the physical mechanism of accretion onto black holes using the outcomes of this investigation.
© The Author(s) 2023
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