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Open AccessArticle
Thin Accretion Disk Around Bardeen Black Hole Surrounded by Perfect Fluid Dark Matter
by
Dan-Dan Cui
Dan-Dan Cui and
Haiyuan Feng
Haiyuan Feng *
School of Physics and Electronic Engineering, Shanxi Normal University, Taiyuan 030031, China
*
Author to whom correspondence should be addressed.
Universe 2026, 12(1), 8; https://doi.org/10.3390/universe12010008 (registering DOI)
Submission received: 11 November 2025
/
Revised: 18 December 2025
/
Accepted: 25 December 2025
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Published: 29 December 2025
Abstract
We investigate the thin accretion disk around Bardeen black hole (BH) surrounded by perfect fluid dark matter (PFDM), focusing on how the magnetic charge g and dark matter (DM) parameter b affect its radiative properties. The results show that increasing g slightly enhances the energy flux, radiation temperature, luminosity, and efficiency, while shifting the innermost stable circular orbit () inward. Additionally, the influence of b is found to be dominant, making it a key parameter in distinguishing PFDM-surrounded Bardeen BH from their Schwarzschild counterparts.
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MDPI and ACS Style
Cui, D.-D.; Feng, H.
Thin Accretion Disk Around Bardeen Black Hole Surrounded by Perfect Fluid Dark Matter. Universe 2026, 12, 8.
https://doi.org/10.3390/universe12010008
AMA Style
Cui D-D, Feng H.
Thin Accretion Disk Around Bardeen Black Hole Surrounded by Perfect Fluid Dark Matter. Universe. 2026; 12(1):8.
https://doi.org/10.3390/universe12010008
Chicago/Turabian Style
Cui, Dan-Dan, and Haiyuan Feng.
2026. "Thin Accretion Disk Around Bardeen Black Hole Surrounded by Perfect Fluid Dark Matter" Universe 12, no. 1: 8.
https://doi.org/10.3390/universe12010008
APA Style
Cui, D.-D., & Feng, H.
(2026). Thin Accretion Disk Around Bardeen Black Hole Surrounded by Perfect Fluid Dark Matter. Universe, 12(1), 8.
https://doi.org/10.3390/universe12010008
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