Observational appearances of an inner extremal regular black hole illuminated by various accretion flows
Year: 2025
Type: article
Abstract: This paper investigates the observational appearances of an inner extremal regular black hole (IERBH) illuminated by various types of accretion models. The study reveals that when the BH is illuminated by specific accretion flows, the effects of quantum gravity become more pronounced, significantly impacting key observational features such as the shadow radius, photon ring, and total observed intensity. Specifically, the introduction of a more realistic radially infalling spherical accretion flow further accentuates these differences. This dynamic flow results in a darker central region in the BH image due to the Doppler effect, which modulates the observed intensity based on the relative motion of the infalling matter. The shadow radius and total observed intensity are notably affected by the quantum correction parameters, providing additional signatures that distinguish regular BHs from their classical counterparts.
Source: The European Physical Journal C
Authors: Dan Zhang, Guoyang Fu, Xi-Jing Wang, Qiyuan Pan, Xiao-Mei Kuang, Jian-Pin Wu
Institutions: Yangzhou University, Wuhan University, Hunan Normal University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: diamond
OpenAlex ID: W4414435167