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General Relativity and Quantum Cosmology

arXiv:2412.18651 (gr-qc)
[Submitted on 24 Dec 2024 (v1) , last revised 21 Feb 2025 (this version, v2)]

Title: Quasinormal modes of black holes embedded in halos of matter

Title: 嵌入物质晕中的黑洞的准正模

Authors:Laura Pezzella, Kyriakos Destounis, Andrea Maselli, Vitor Cardoso
Abstract: We investigate the (axial) quasinormal modes of black holes embedded in generic matter profiles. Our results reveal that the axial QNMs experience a redshift when the black hole is surrounded by various matter environments, proportional to the compactness of the matter halo. Our calculations demonstrate that for static black holes embedded in galactic matter distributions, there exists a universal relation between the matter environment and the redshifted vacuum quasinormal modes. In particular, for dilute environments the leading order effect is a redshift $1+U$ of frequencies and damping times, with $U \sim -{\cal C}$ the Newtonian potential of the environment at its center, which scales with its compactness ${\cal C}$.
Abstract: 我们研究了嵌入通用物质分布中的黑洞的(轴向)准正规模式。 我们的结果显示,当黑洞被各种物质环境包围时,轴向准正规模式的频率会发生红移,且该红移与物质晕的致密性成正比。 我们的计算表明,对于嵌入星系物质分布中的静态黑洞,物质环境和红移的真空准正规模式之间存在一个普适关系。 特别是,在稀疏环境中,主导效应是对频率和阻尼时间的红移 $1+U$,其中 $U \sim -{\cal C}$ 是环境中心的牛顿势,它随环境的致密性 ${\cal C}$ 而变化。
Comments: 12 pages, 8 figures, accepted for publication in PRD
Subjects: General Relativity and Quantum Cosmology (gr-qc) ; Astrophysics of Galaxies (astro-ph.GA); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
Cite as: arXiv:2412.18651 [gr-qc]
  (or arXiv:2412.18651v2 [gr-qc] for this version)
  https://doi.org/10.48550/arXiv.2412.18651
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. D 111, 064026 (2025)
Related DOI: https://doi.org/10.1103/PhysRevD.111.064026
DOI(s) linking to related resources

Submission history

From: Laura Pezzella [view email]
[v1] Tue, 24 Dec 2024 19:00:01 UTC (255 KB)
[v2] Fri, 21 Feb 2025 13:49:03 UTC (1,888 KB)
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