English

Modified Black Hole Potentials and Their Korteweg-de Vries Integrals: Instabilities and Beyond

General Relativity and Quantum Cosmology 2025-11-18 v2 High Energy Astrophysical Phenomena High Energy Physics - Theory Exactly Solvable and Integrable Systems

Abstract

Black Hole (BH) Quasi-Normal Modes (QNMs) and Greybody Factors (GBFs) are key signatures of BH dynamics that are crucial for testing fundamental physics via gravitational waves. Recent studies of the BH pseudospectrum have revealed instabilities in QNMs. Here, we introduce a new perspective using hidden symmetries in the BH dynamics, specifically the Korteweg-de Vries (KdV) integrals - an infinite series of conserved quantities. By analyzing modified BH potentials, we find strong evidence that KdV integrals are valuable indicators for detecting instabilities in QNMs and GBFs.

Keywords

Cite

@article{arxiv.2509.01500,
  title  = {Modified Black Hole Potentials and Their Korteweg-de Vries Integrals: Instabilities and Beyond},
  author = {Michele Lenzi and Arnau Montava Agudo and Carlos F. Sopuerta},
  journal= {arXiv preprint arXiv:2509.01500},
  year   = {2025}
}

Comments

Submitted to the Proceedings of the 24th International Conference on General Relativity and Gravitation & 16th Edoardo Amaldi Conference on Gravitational Waves. 3 pages. JPCS style