2016/02/18 by Abdul Jawad, M. Umair Shahzad
Physics and Astronomy · #Accretion (finance) #Accretion disc #Astrophysical Phenomena and Observations #Binary black hole #Black Holes and Theoretical Physics #Black hole (networking) #Gamma-ray burst progenitors #Intermediate-mass black hole #Nonlinear system #Quantum Electrodynamics and Casimir Effect #Sonic black hole #Stellar black hole #gr-qc
paper · pdf · doi:10.1140/epjc/s10052-016-3967-2
published as Eur. Phys. J. C 76(2016) 123 · 25 pages, 7 figures, Accepted for publication in Eur. Phys. J. C
arxiv created 2016/02/18 · openalex publication_date 2016/03/01 · openalex created_date 2016/06/24 · arxiv updated 2016/10/28 · openalex updated_date 2026/08/05
In this work, we discuss the accretion onto static spherically symmetric regular black holes for specific choices of the equation of state parameter. The underlying regular black holes are charged regular black holes using the Fermi–Dirac distribution, logistic distribution, nonlinear electrodynamics, respectively, and Kehagias–Sftesos asymptotically flat regular black holes. We obtain the critical radius, critical speed, and squared sound speed during the accretion process near the regular black holes. We also study the behavior of radial velocity, energy density, and the rate of change of the mass for each of the regular black holes.