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Bound States of the Schwarzschild Black Hole

Sebastian H. Völkel*

  • *Contact author: sebastian.voelkel@aei.mpg.de

Phys. Rev. Lett. 134, 241401 – Published 17 June, 2025

DOI: https://doi.org/10.1103/tbm2-gzv9

Abstract

Understanding the physical significance and spectral stability of black hole quasinormal modes is fundamental to high-precision spectroscopy with future gravitational wave detectors. Inspired by Mashhoon’s idea of relating quasinormal modes of black holes with their equivalent bound states in an inverted potential, we investigate, for the first time, energy levels and eigenfunctions of the Schwarzschild black hole quantitatively. While quasinormal modes describe the characteristic damped oscillations of a black hole, the bound states of the inverted potential are qualitatively more similar to those of the hydrogen atom. Although the physical interpretation of these states may initially be of more academic interest, it furthers our understanding of open problems related to quasinormal modes in a similar spirit to Maggiore’s interpretation of the Schwarzschild quasinormal mode spectrum. One surprising insight from the explicit calculation of bound states is that eigenfunctions corresponding to quasinormal mode overtones become rapidly delocalized and extremely loosely bound. This observation raises immediate questions about the common interpretation of quasinormal modes as excitations of the light ring region. Closely related, as a second application, we also explore the spectral stability of bound states and demonstrate that they can provide complementary insights into the quasinormal mode spectrum.

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References (65)

  1. O. Dreyer, B. J. Kelly, B. Krishnan, L. S. Finn, D. Garrison, and R. Lopez-Aleman, Black hole spectroscopy: Testing general relativity through gravitational wave observations, Classical Quantum Gravity 21, 787 (2004).
  2. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Observation of gravitational waves from a binary black hole merger, Phys. Rev. Lett. 116, 061102 (2016).
  3. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Tests of general relativity with GW150914, Phys. Rev. Lett. 116, 221101 (2016); 121, 129902(E) (2018).
  4. M. Dafermos, G. Holzegel, and I. Rodnianski, The linear stability of the Schwarzschild solution to gravitational perturbations, Acta Math. 222, 1 (2019).
  5. E. Berti, K. Yagi, H. Yang, and N. Yunes, Extreme gravity tests with gravitational waves from compact binary coalescences: (II) Ringdown, Gen. Relativ. Gravit. 50, 49 (2018).
  6. V. Cardoso and P. Pani, Testing the nature of dark compact objects: A status report, Living Rev. Relativity 22, 4 (2019).
  7. N. Franchini and S. H. Völkel, Testing General Relativity with Black Hole Quasi-normal Modes, in Recent Progress on Gravity Tests, Springer Series in Astrophysics and Cosmology (Springer, Singapore, 2024), 10.1007/978-981-97-2871-8_9.
  8. S. Hod, Bohr’s correspondence principle and the area spectrum of quantum black holes, Phys. Rev. Lett. 81, 4293 (1998).
  9. K. D. Kokkotas and B. G. Schmidt, Quasinormal modes of stars and black holes, Living Rev. Relativity 2, 2 (1999).
  10. H.-P. Nollert, Topical review: Quasinormal modes: The characteristic ‘sound’ of black holes and neutron stars, Classical Quantum Gravity 16, R159 (1999).
  11. E. Berti, V. Cardoso, and A. O. Starinets, Quasinormal modes of black holes and black branes, Classical Quantum Gravity 26, 163001 (2009).
  12. R. A. Konoplya and A. Zhidenko, Quasinormal modes of black holes: From astrophysics to string theory, Rev. Mod. Phys. 83, 793 (2011).
  13. T. Regge and J. A. Wheeler, Stability of a Schwarzschild singularity, Phys. Rev. 108, 1063 (1957).
  14. F. J. Zerilli, Effective potential for even parity Regge-Wheeler gravitational perturbation equations, Phys. Rev. Lett. 24, 737 (1970).
  15. S. Chandrasekhar and S. L. Detweiler, The quasi-normal modes of the Schwarzschild black hole, Proc. R. Soc. A 344, 441 (1975).
  16. H.-P. Nollert, Quasinormal modes of Schwarzschild black holes: The determination of quasinormal frequencies with very large imaginary parts, Phys. Rev. D 47, 5253 (1993).
  17. S. Chandrasekhar, V. Ferrari, and J. E. Enderby, On the non-radial oscillations of a star. III. A reconsideration of the axial modes, Proc. R. Soc. A 434, 449 (1991).
  18. K. D. Kokkotas, Axial modes for relativistic stars, Mon. Not. R. Astron. Soc. 268, 1015 (1994).
  19. M. Maggiore, The physical interpretation of the spectrum of black hole quasinormal modes, Phys. Rev. Lett. 100, 141301 (2008).
  20. J. D. Bekenstein, The quantum mass spectrum of the Kerr black hole, Lett. Nuovo Cimento 11, 467 (1974).
  21. V. F. Mukhanov, Are black holes quantized?, JETP Lett. 44, 63 (1986), https://ui.adsabs.harvard.edu/abs/1986ZhPmR..44...50M/abstract.
  22. B. Mashhoon, Quasinormal modes of a black hole, in Proceedings of the 3rd Marcel Grossmann Meeting on the Recent Developments of General Relativity (1982).
  23. H.-J. Blome and B. Mashhoon, Quasi-normal oscillations of a Schwarzschild black hole, Phys. Lett. 100A, 231 (1984).
  24. V. Ferrari and B. Mashhoon, Oscillations of a black hole, Phys. Rev. Lett. 52, 1361 (1984).
  25. V. Ferrari and B. Mashhoon, New approach to the quasinormal modes of a black hole, Phys. Rev. D 30, 295 (1984).
  26. S. H. Völkel, Quasinormal modes from bound states: The numerical approach, Phys. Rev. D 106, 124009 (2022).
  27. Y. Hatsuda, Quasinormal modes of black holes and Borel summation, Phys. Rev. D 101, 024008 (2020).
  28. G. Aminov, A. Grassi, and Y. Hatsuda, Black hole quasinormal modes and Seiberg-Witten theory, Ann. Henri Poincare 23, 1951 (2022).
  29. M. G. Richarte, J. C. Fabris, and A. Saa, Quasinormal modes and the analytical continuation of non-self-adjoint operators, arXiv:2409.00857.
  30. C. Burgess and F. Koenig, Hyperboloidal method for quasinormal modes of non-relativistic operators, Front. Phys. 12, 1457543 (2024).
  31. K. D. Kokkotas, Normal modes of the Kerr black hole, Classical Quantum Gravity 8, 2217 (1991).
  32. H. Liu and B. Mashhoon, On the spectrum of oscillations of a Schwarzschild black hole, Classical Quantum Gravity 13, 233 (1996).
  33. A. Buonanno and T. Damour, Effective one-body approach to general relativistic two-body dynamics, Phys. Rev. D 59, 084006 (1999).
  34. G. Kälin and R. A. Porto, From boundary data to bound states, J. High Energy Phys. 01 (2020) 072.
  35. H.-P. Nollert, About the significance of quasinormal modes of black holes, Phys. Rev. D 53, 4397 (1996).
  36. H.-P. Nollert and R. H. Price, Quantifying excitations of quasinormal mode systems, J. Math. Phys. (N.Y.) 40, 980 (1999).
  37. E. Barausse, V. Cardoso, and P. Pani, Can environmental effects spoil precision gravitational-wave astrophysics?, Phys. Rev. D 89, 104059 (2014).
  38. J. L. Jaramillo, R. Panosso Macedo, and L. Al Sheikh, Pseudospectrum and black hole quasinormal mode instability, Phys. Rev. X 11, 031003 (2021).
  39. M. H.-Y. Cheung, K. Destounis, R. P. Macedo, E. Berti, and V. Cardoso, Destabilizing the fundamental mode of black holes: The elephant and the flea, Phys. Rev. Lett. 128, 111103 (2022).
  40. E. Berti, V. Cardoso, M. H.-Y. Cheung, F. Di Filippo, F. Duque, P. Martens, and S. Mukohyama, Stability of the fundamental quasinormal mode in time-domain observations against small perturbations, Phys. Rev. D 106, 084011 (2022).
  41. V. Cardoso, S. Kastha, and R. Panosso Macedo, Physical significance of the black hole quasinormal mode spectra instability, Phys. Rev. D 110, 024016 (2024).
  42. A. Ianniccari, A. J. Iovino, A. Kehagias, P. Pani, G. Perna, D. Perrone, and A. Riotto, Deciphering the instability of the black hole ringdown quasinormal spectrum, Phys. Rev. Lett. 133, 211401 (2024).
  43. P. H. C. Siqueira, L. T. de Paula, R. Panosso Macedo, and M. Richartz, Probing the unstable spectrum of Schwarzschild-like black holes, Phys. Rev. D 111, 104039 (2025).
  44. M. S. Churilova, R. A. Konoplya, and A. Zhidenko, Analytic formula for quasinormal modes in the near-extreme Kerr-Newman–de Sitter spacetime governed by a non-Pöschl-Teller potential, Phys. Rev. D 105, 084003 (2022).
  45. A. Zimmerman, H. Yang, Z. Mark, Y. Chen, and L. Lehner, Quasinormal modes beyond Kerr, Astrophys. Space Sci. Proc. 40, 217 (2015).
  46. Z. Mark, H. Yang, A. Zimmerman, and Y. Chen, Quasinormal modes of weakly charged Kerr-Newman spacetimes, Phys. Rev. D 91, 044025 (2015).
  47. A. Hussain and A. Zimmerman, Approach to computing spectral shifts for black holes beyond Kerr, Phys. Rev. D 106, 104018 (2022).
  48. D. Li, A. Hussain, P. Wagle, Y. Chen, N. Yunes, and A. Zimmerman, Isospectrality breaking in the Teukolsky formalism, Phys. Rev. D 109, 104026 (2024).
  49. P. Wagle, D. Li, Y. Chen, and N. Yunes, Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation equations, Phys. Rev. D 109, 104029 (2024).
  50. S. Ma and H. Yang, Excitation of quadratic quasinormal modes for Kerr black holes, Phys. Rev. D 109, 104070 (2024).
  51. C. Weller, D. Li, and Y. Chen, Spectroscopy of bumpy BHs: The nonrotating case, Phys. Rev. D 111, 024064 (2025).
  52. D. Li, P. Wagle, Y. Chen, and N. Yunes, Perturbations of spinning black holes in dynamical Chern-Simons gravity: Slow rotation quasinormal modes, arXiv:2503.15606.
  53. B. F. Schutz and C. M. Will, Black hole normal modes: A semianalytic approach, Astrophys. J. Lett. 291, L33 (1985).
  54. C. Bender, S. Orszag, and S. Orszag, Advanced Mathematical Methods for Scientists and Engineers I: Asymptotic Methods and Perturbation Theory, Advanced Mathematical Methods for Scientists and Engineers (Springer, New York, 1999).
  55. H. E. Camblong, L. N. Epele, H. Fanchiotti, and C. A. Garcia Canal, Renormalization of the inverse square potential, Phys. Rev. Lett. 85, 1590 (2000).
  56. S. A. Coon and B. R. Holstein, Anomalies in quantum mechanics: The 1/r2 Potential, Am. J. Phys. 70, 513 (2002).
  57. R. H. Price, Nonspherical perturbations of relativistic gravitational collapse. II. Integer-spin, zero-rest-mass fields, Phys. Rev. D 5, 2439 (1972).
  58. J. Steinhauer, The continuous spectrum of quasinormal modes in a Schwarzschild black hole, arXiv:2503.01029.
  59. R. A. Konoplya and A. Zhidenko, First few overtones probe the event horizon geometry, J. High Energy Astrophys. 44, 419 (2024).
  60. H. O. Silva, G. Tambalo, K. Glampedakis, K. Yagi, and J. Steinhoff, Quasinormal modes and their excitation beyond general relativity, Phys. Rev. D 110, 024042 (2024).
  61. V. Baibhav, M. H.-Y. Cheung, E. Berti, V. Cardoso, G. Carullo, R. Cotesta, W. Del Pozzo, and F. Duque, Agnostic black hole spectroscopy: Quasinormal mode content of numerical relativity waveforms and limits of validity of linear perturbation theory, Phys. Rev. D 108, 104020 (2023).
  62. P. J. Nee, S. H. Völkel, and H. P. Pfeiffer, Role of black hole quasinormal mode overtones for ringdown analysis, Phys. Rev. D 108, 044032 (2023).
  63. M. Giesler et al., Overtones and nonlinearities in binary black hole ringdowns, Phys. Rev. D 111, 084041 (2025).
  64. S. Thomopoulos, S. H. Völkel, and H. P. Pfeiffer, Ringdown spectroscopy of phenomenologically modified black holes, arXiv:2504.17848.
  65. S. Völkel, Tabulated data for bound states and eigenfunctions (2025), 10.5281/zenodo.15577458.

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