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PreprintarXiv licencearXiv

Ruling out matter-induced bumps in black-hole effective potentials

Abstract

Matter fields localized around black holes can produce small secondary bumps in the effective potentials governing black-hole perturbations, potentially leading to quasinormal-mode spectral instabilities and late-time echoes. Considering physically motivated models of anisotropic fluids surrounding a spherically symmetric black hole, we show that the appearance of such a secondary bump is accompanied by either singular matter profiles or divergent characteristic speeds in the fluid. These features indicate that the corresponding matter configurations are unphysical. We further demonstrate that a secondary bump in the effective potential does not necessarily imply the existence of additional light rings in the spacetime.

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BibTeX
@misc{rocca2026ruling,
  title = {{Ruling out matter-induced bumps in black-hole effective potentials}},
  author = {Matteo Della Rocca and Romeo Felice Rosato and Paolo Pani},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.09284},
  eprint = {2609.09284},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.09284},
}
RIS
TY  - UNPB
TI  - Ruling out matter-induced bumps in black-hole effective potentials
AU  - Matteo Della Rocca
AU  - Romeo Felice Rosato
AU  - Paolo Pani
PY  - 2026
DA  - 2026/09/08
PB  - arXiv
DO  - 10.48550/arxiv.2609.09284
UR  - https://arxiv.org/abs/2609.09284
AB  - Matter fields localized around black holes can produce small secondary bumps in the effective potentials governing black-hole perturbations, potentially leading to quasinormal-mode spectral instabilities and late-time echoes. Considering physically motivated models of anisotropic fluids surrounding a spherically symmetric black hole, we show that the appearance of such a secondary bump is accompanied by either singular matter profiles or divergent characteristic speeds in the fluid. These features indicate that the corresponding matter configurations are unphysical. We further demonstrate that a secondary bump in the effective potential does not necessarily imply the existence of additional light rings in the spacetime.
ER  -