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Main Authors: Yan, Hao-Peng, Zhang, Zeng-Yi, Yue, Xiao-Jun, Li, Xiang-Qian
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2511.21205
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author Yan, Hao-Peng
Zhang, Zeng-Yi
Yue, Xiao-Jun
Li, Xiang-Qian
author_facet Yan, Hao-Peng
Zhang, Zeng-Yi
Yue, Xiao-Jun
Li, Xiang-Qian
contents We present a unified investigation of black hole shadows, quasinormal modes (QNMs), and greybody factors (GBFs) for a static, spherically symmetric black hole within a composite environment of a modified Chaplygin-like dark fluid (MCDF) and a cloud of strings (CoS). We examine the structure of critical photon orbits and the corresponding optical appearance under spherical accretion. Using the Wentzel-Kramers-Brillouin (WKB) approximation, we compute the quasinormal frequencies and greybody spectra, and explore their correspondence with the black hole shadows in the eikonal limit. A systematic parameter study demonstrates that the CoS intensity has the primary influence on the shadows, QNMs and GBFs, while the MCDF parameters introduce more complex but characterizable modifications to each. Our results demonstrate that these environmental components imprint distinct yet interrelated signatures on key observables, offering specific predictions for probing exotic black hole environments.
format Preprint
id arxiv_https___arxiv_org_abs_2511_21205
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Black holes immersed in modified Chaplygin-like dark fluid and cloud of strings: shadows, quasinomal modes and greybody factors
Yan, Hao-Peng
Zhang, Zeng-Yi
Yue, Xiao-Jun
Li, Xiang-Qian
General Relativity and Quantum Cosmology
We present a unified investigation of black hole shadows, quasinormal modes (QNMs), and greybody factors (GBFs) for a static, spherically symmetric black hole within a composite environment of a modified Chaplygin-like dark fluid (MCDF) and a cloud of strings (CoS). We examine the structure of critical photon orbits and the corresponding optical appearance under spherical accretion. Using the Wentzel-Kramers-Brillouin (WKB) approximation, we compute the quasinormal frequencies and greybody spectra, and explore their correspondence with the black hole shadows in the eikonal limit. A systematic parameter study demonstrates that the CoS intensity has the primary influence on the shadows, QNMs and GBFs, while the MCDF parameters introduce more complex but characterizable modifications to each. Our results demonstrate that these environmental components imprint distinct yet interrelated signatures on key observables, offering specific predictions for probing exotic black hole environments.
title Black holes immersed in modified Chaplygin-like dark fluid and cloud of strings: shadows, quasinomal modes and greybody factors
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2511.21205