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  • Open Access
  • Access by Xinjiang University

Black hole singularity is a surface not a point

Andrew J. S. Hamilton*

Tyler McMaken

  • Department of Mathematics and Physics, University of Mary, 7500 University Drive, Bismarck, North Dakota 58504, USA

Phys. Rev. D 114, 024088 – Published 30 July, 2026

DOI: https://doi.org/10.1103/1pvt-3pn5

Abstract

It is widely repeated in the popular literature and elsewhere that the singularity at the center of a black hole is a point. It is not true. Two observers who free fall into a spherical black hole along two different angular trajectories at the same time t do not encounter each other at the central singularity; rather, they lose causal contact with each other already well away from the singularity. Counterintuitively, in general relativity two points can be spatially close yet causally distant. The singularity is a surface not a point. The story for rotating black holes is more complicated, but the same conclusion holds. For a rotating black hole, the singular surface almost certainly resides at its inner horizon, where even the tiniest classical or quantum perturbations ignite the exponential mass inflation instability, precipitating collapse to a spacelike singular surface. There are implications for quantum gravity. We argue that, whatever the ultimate theory of quantum gravity may be, the quantum states of a black hole probably reside at its effectively two-dimensional singular surface, which coevolves unitarily with, and in thermodynamic equilibrium with, the hot atmosphere of trapped Hawking radiation that the black hole generates within its event horizon.

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References (44)

  1. V. A. Belinskii, I. M. Khalatnikov, and E. M. Lifshitz, Oscillatory approach to a singular point in the relativistic cosmology, Adv. Phys. 19, 525 (1970).
  2. V. A. Belinskii, I. M. Khalatnikov, and E. M. Lifshitz, A general solution of the Einstein equations with a time singularity, Adv. Phys. 31, 639 (1982).
  3. L. Andersson, H. van Elst, W. C. Lim, and C. Uggla, Asymptotic silence of generic cosmological singularities, Phys. Rev. Lett. 94, 051101 (2005).
  4. R. Geroch, E. H. Kronheimer, and R. Penrose, Ideal points in space-time, Proc. R. Soc. A 327, 545 (1972).
  5. A. García-Parrado and J. M. M. Senovilla, Causal structures and causal boundaries, Classical Quantum Gravity 22, R1 (2005).
  6. W. Rindler, Essential Relativity: Special, General, and Cosmological (Springer-Verlag, New York, Heidelberg, Berlin, 1977).
  7. M. D. Kruskal, Maximal extension of Schwarzschild metric, Phys. Rev. 119, 1743 (1960).
  8. G. Szekeres, On the singularities of a Riemann manifold, Publ. Math. Debrecen 7, 285 (1960).
  9. R. Penrose, Conformal treatment of infinity, Gen. Relativ. Gravit. 43, 901 (2011).
  10. S. Chandrasekhar, The Mathematical Theory of Black Holes (Clarendon Press, Oxford, England, 1983).
  11. B. Greene, The Fabric of the Cosmos (Alfred A. Knopf, New York, 2004).
  12. N. d. Tyson, Death by Black Hole (W. W. Norton & Company, New York, 2007).
  13. M. Bartusiak, Black Hole: How an Idea Abandoned by Newtonians, Hated by Einstein, and Gambled On by Hawking Became Loved (Yale University Press, New Haven, CT, 2016).
  14. K. Schwarzschild, Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie, Sitzungsber. Preuss. Akad. Wiss. Berlin Klasse Math. Phys. Tech. 1916, 189 (1916).
  15. C. S. Reynolds, Observational constraints on black hole spin, Annu. Rev. Astron. Astrophys. 59, 117 (2021).
  16. J. A. Orosz, J. E. McClintock, J. P. Aufdenberg, R. A. Remillard, M. J. Reid, R. Narayan, and L. Gou, The mass of the black hole in Cygnus X-1, Astrophys. J. 742, 84 (2011).
  17. L. Gou, J. E. McClintock, M. J. Reid, J. A. Orosz, J. F. Steiner, R. Narayan, J. Xiang, R. A. Remillard, K. A. Arnaud, and S. W. Davis, The extreme spin of the black hole in Cygnus X-1, Astrophys. J. 742, 85 (2011).
  18. R. P. Kerr, Gravitational field of a spinning mass as an example of algebraically special metrics, Phys. Rev. Lett. 11, 237 (1963).
  19. R. P. Kerr, Discovering the Kerr and Kerr-Schild metrics, in The Kerr Spacetime: Rotating Black Holes in General Relativity, edited by D. L. Wiltshire, M. Visser, and S. Scott (Cambridge University Press, Cambridge, England, 2009), pp. 38–72,
  20. A. J. S. Hamilton and J. P. Lisle, The river model of black holes, Am. J. Phys. 76, 519 (2008).
  21. B. Carter, Global structure of the Kerr family of gravitational fields, Phys. Rev. 174, 1559 (1968).
  22. R. H. Boyer and R. W. Lindquist, Maximal analytic extension of the Kerr metric, J. Math. Phys. (N.Y.) 8, 265 (1967).
  23. E. Poisson and W. Israel, Internal structure of black holes, Phys. Rev. D 41, 1796 (1990).
  24. A. J. S. Hamilton and G. Polhemus, Stereoscopic visualization in curved spacetime: Seeing deep inside a black hole, New J. Phys. 12, 123027 (2010).
  25. The color of the sky from Gaia’s early data release 3 (2020).
  26. S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, England, 1973).
  27. R. Penrose, Structure of space-time, in Battelle Rencontres: 1967 Lectures in Mathematics and Physics, edited by C. de Witt-Morette and J. A. Wheeler (W. A. Benjamin, New York, 1968), pp. 121–235.
  28. B. Carter, Hamilton-Jacobi and Schrödinger separable solutions of Einstein’s equations, Commun. Math. Phys. 10, 280 (1968).
  29. C. Barrabès, W. Israel, and E. Poisson, Collision of light-like shells and mass inflation in rotating black holes, Classical Quantum Gravity 7, L273 (1990).
  30. T. McMaken and A. J. S. Hamilton, Geometry near the inner horizon of a rotating, accreting black hole, Phys. Rev. D 103, 084014 (2021).
  31. R. H. Price, Nonspherical perturbations of relativistic gravitational collapse. I. Scalar and gravitational perturbations, Phys. Rev. 5, 2419 (1972).
  32. M. Dafermos and J. Luk, The interior of dynamical vacuum black holes I: The C0-stability of the Kerr Cauchy horizon, Ann. Math. 202, 309 (2025).
  33. A. J. S. Hamilton and P. P. Avelino, The physics of the relativistic counter-streaming instability that drives mass inflation inside black holes, Phys. Rep. 495, 1 (2010).
  34. A. J. S. Hamilton, Mass inflation followed by Belinskii-Khalatnikov-Lifshitz collapse inside accreting, rotating black holes, Phys. Rev. D 96, 084041 (2017).
  35. N. Zilberman, M. Casals, A. Ori, and A. C. Ottewill, Two-point function of a quantum scalar field in the interior region of a Kerr black hole, Phys. Rev. D 106, 125011 (2022).
  36. N. Zilberman, M. Casals, A. Ori, and A. C. Ottewill, Quantum fluxes at the inner horizon of a spinning black hole, Phys. Rev. Lett. 129, 261102 (2022).
  37. T. McMaken and A. J. S. Hamilton, Hawking radiation inside a rotating black hole, Phys. Rev. D 109, 065023 (2024).
  38. S. W. Hawking, Particle creation by black holes, Commun. Math. Phys. 43, 199 (1975).
  39. A. Strominger and C. Vafa, Microscopic origin of the Bekenstein-Hawking entropy, Phys. Lett. B 379, 99 (1996).
  40. A. Ashtekar, J. Baez, A. Corichi, and K. Krasnov, Quantum geometry and black hole entropy, Phys. Rev. Lett. 80, 904 (1998).
  41. S. Carlip, Black hole entropy from conformal field theory in any dimension, Phys. Rev. Lett. 82, 2828 (1999).
  42. J. Maldacena, The large N limit of superconformal field theories and supergravity, Adv. Theor. Math. Phys. 2, 231 (1998).
  43. E. T. Newman, E. Couch, K. Chinnapared, A. Exton, A. Prakash, and R. Torrence, Metric of a rotating, charged mass, J. Math. Phys. (N.Y.) 6, 918 (1965).
  44. A. J. S. Hamilton, The interior structure of rotating black holes II. Uncharged black holes, Phys. Rev. D 84, 124056 (2011).

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