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Analysis of accretion disk around the Euler-Heisenberg Anti-de Sitter Black Hole

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arxiv 2309.03236 v1 pith:XNDKDQ6N submitted 2023-09-06 gr-qc

G. Abbas , H. Rehman This is my paper · ORCID
classification gr-qc
keywords blackholespecificangularcircularsitteraccretionorbits
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We demonstrate the investigation of thin accretion disc surrounding the Einstein- Euler-Heisenberg-Anti-de Sitter black hole. Additionally, we analyze the black hole event horizons and compute their effective potential and equations of motion. The specific energy, specific angular momentum, and specific angular velocity of the particles that move in circular orbits above the thin accretion disk are obtained. Also, the effects of parameters of the Einstein- Euler-Heisenberg-Anti de sitter black hole on specific angular velocity, specific heat energy, and specific angular momentum, have been discussed in detail. We display the positions of the innermost stable circular orbits and illustrate the effective potential. Furthermore, the circular orbits of black hole are obtained numerically and locates the position of the innermost stable circular orbit and event horizon. Also, we study the Gamma ray burst emitted from the Einstein Euler-Heisenberg Anti de sitter black hole.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Purely Electric, Magnetic, and Dyonic Black Holes in Einstein-Euler-Heisenberg Theory

    gr-qc 2026-07 conditional novelty 6.0 of 10

    In Einstein-Euler-Heisenberg theory, purely magnetic and mixed electric-magnetic black holes can have three horizons, one outer and two inner, for weak QED coupling.

  2. Investigating QED Effects on the Thin Accretion Disk Properties Around Rotating Euler-Heisenberg Black Holes

    gr-qc 2025-06 reject novelty 4.0 of 10

    For a charged rotating Euler-Heisenberg black hole, the ISCO radius is larger than in Kerr and grows with spin, while higher charge moves it inward and heats the disk.

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