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Bibliographic Details
Main Authors: Jiang, Yu-Hao, Wang, Towe
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2408.10150
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author Jiang, Yu-Hao
Wang, Towe
author_facet Jiang, Yu-Hao
Wang, Towe
contents A relativistic model of geometrically thin and optically thick accretion disks is worked out for a class of magnetically charged black holes, which are solutions to the Einstein-Maxwell-dilaton theory with a dilaton-coupled Euler-Heisenberg correction. Constraints on black hole parameters are derived from the subextremality condition and energy conditions. The Keplerian orbits, the time-averaged energy flux, the local temperature, the specific luminosity and the conversion efficiency of accreting mass into radiation are obtained and compared with Schwarzschild and Gibbons-Maeda-Garfinkle-Horowitz-Strominger black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2408_10150
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Accretion disks around magnetically charged black holes in string theory with an Euler-Heisenberg correction
Jiang, Yu-Hao
Wang, Towe
General Relativity and Quantum Cosmology
A relativistic model of geometrically thin and optically thick accretion disks is worked out for a class of magnetically charged black holes, which are solutions to the Einstein-Maxwell-dilaton theory with a dilaton-coupled Euler-Heisenberg correction. Constraints on black hole parameters are derived from the subextremality condition and energy conditions. The Keplerian orbits, the time-averaged energy flux, the local temperature, the specific luminosity and the conversion efficiency of accreting mass into radiation are obtained and compared with Schwarzschild and Gibbons-Maeda-Garfinkle-Horowitz-Strominger black holes.
title Accretion disks around magnetically charged black holes in string theory with an Euler-Heisenberg correction
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2408.10150