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  • Open Access

Exact black holes and black branes with bumpy horizons supported by superfluid pions

Fabrizio Canfora*

Andrés Gomberoff†

Carla Henríquez-Baez‡

Aldo Vera§

  • Facultad de Ciencias, Ingeniería y Tecnología, Universidad Mayor, Avenida Manuel Montt 367, Santiago, Chile and Centro Multidisciplinario de Física, Vicerrectoría de Investigación, Universidad Mayor, Camino La Pirámide 5750, Santiago, Chile

  • Centro Multidisciplinario de Física, Vicerrectoría de Investigación, Universidad Mayor, Camino La Pirámide 5750, Santiago, Chile

  • Núcleo de Matemática, Física y Estadística, Universidad Mayor, Avenida Manuel Montt 367, Santiago, Chile and Centro Multidisciplinario de Física, Vicerrectoría de Investigación, Universidad Mayor, Camino La Pirámide 5750, Santiago, Chile

  • *Contact author: fabrizio.canfora@uss.cl
  • †Contact author: andres.gomberoff@umayor.cl
  • ‡Contact author: carla.henriquez@umayor.cl
  • §Contact author: aldo.vera@umayor.cl

Phys. Rev. D 113, 084068 – Published 30 April, 2026

DOI: https://doi.org/10.1103/9shw-n7rs

Abstract

We present exact solutions of the Einstein–SU(2) nonlinear sigma model in 3+1 spacetime dimensions, describing bumpy black holes and black branes. Using an Ansatz for superfluid pion multivortices, the matter sector reduces to a first-order Bogomol’nyi–Prasad–Sommerfield system, while the Einstein equations reduce to a Liouville equation with a smooth source governing the horizon deformation. These solutions describe horizons of different constant curvatures, with nontrivial bumpy geometries protected by an integer topological invariant, namely the vorticity, which also controls the number of bumps and the black hole thermodynamics. Remarkably, such horizons arise in a minimal and physically motivated matter model, without invoking exotic fields or modified gravity. The physical implications of these results in holography and astrophysics are briefly described.

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References (52)

  1. W. Israel, Event horizons in static vacuum space-times, Phys. Rev. 164, 1776 (1967).
  2. B. Carter, Axisymmetric black hole has only two degrees of freedom, Phys. Rev. Lett. 26, 331 (1971).
  3. S. W. Hawking, Black holes in general relativity, Commun. Math. Phys. 25, 152 (1972).
  4. D. C. Robinson, Uniqueness of the Kerr black hole, Phys. Rev. Lett. 34, 905 (1975).
  5. J. L. Friedman, K. Schleich, and D. M. Witt, Topological censorship, Phys. Rev. Lett. 71, 1486 (1993); 75, 1872(E) (1995).
  6. G. W. Gibbons and S. W. Hawking, Cosmological event horizons, thermodynamics, and particle creation, Phys. Rev. D 15, 2738 (1977).
  7. B. Linet, The static, cylindrically symmetric strings in general relativity with cosmological constant, J. Math. Phys. (N.Y.) 27, 1817 (1986).
  8. J. P. S. Lemos, Cylindrical black hole in general relativity, Phys. Lett. B 353, 46 (1995).
  9. D. Birmingham, Topological black holes in Anti-de Sitter space, Classical Quantum Gravity 16, 1197 (1999).
  10. R.-G. Cai and Y.-Z. Zhang, Black plane solutions in four-dimensional space-times, Phys. Rev. D 54, 4891 (1996).
  11. L. Vanzo, Black holes with unusual topology, Phys. Rev. D 56, 6475 (1997).
  12. D. Klemm, Four-dimensional black holes with unusual horizons, Phys. Rev. D 89, 084007 (2014).
  13. R. Emparan and H. S. Reall, A Rotating black ring solution in five-dimensions, Phys. Rev. Lett. 88, 101101 (2002).
  14. H. Elvang and P. Figueras, Black saturn, J. High Energy Phys. 05 (2007) 050.
  15. S. S. Gubser, On nonuniform black branes, Classical Quantum Gravity 19, 4825 (2002).
  16. D. Licht, R. Luna, and R. Suzuki, Black ripples, flowers and dumbbells at large D, J. High Energy Phys. 04 (2020) 108.
  17. H. Iguchi and T. Mishima, Black di-ring and infinite nonuniqueness, Phys. Rev. D 75, 064018 (2007); 78, 069903(E) (2008).
  18. R. Gregory and R. Laflamme, Black strings and p-branes are unstable, Phys. Rev. Lett. 70, 2837 (1993).
  19. L. Lehner and F. Pretorius, Black strings, low viscosity fluids, and violation of cosmic censorship, Phys. Rev. Lett. 105, 101102 (2010).
  20. P. Figueras, M. Kunesch, and S. Tunyasuvunakool, End point of black ring instabilities and the weak cosmic censorship conjecture, Phys. Rev. Lett. 116, 071102 (2016).
  21. N. A. Collins and S. A. Hughes, Towards a formalism for mapping the space-times of massive compact objects: Bumpy black holes and their orbits, Phys. Rev. D 69, 124022 (2004).
  22. C. A. R. Herdeiro and E. Radu, Kerr black holes with scalar hair, Phys. Rev. Lett. 112, 221101 (2014).
  23. C. Herdeiro, E. Radu, and H. Rúnarsson, Kerr black holes with Proca hair, Classical Quantum Gravity 33, 154001 (2016).
  24. D. D. Doneva and S. S. Yazadjiev, New Gauss-Bonnet black holes with curvature-induced scalarization in extended scalar-tensor theories, Phys. Rev. Lett. 120, 131103 (2018).
  25. H. O. Silva, J. Sakstein, L. Gualtieri, T. P. Sotiriou, and E. Berti, Spontaneous scalarization of black holes and compact stars from a Gauss-Bonnet coupling, Phys. Rev. Lett. 120, 131104 (2018).
  26. D. D. Doneva, F. M. Ramazanoğlu, H. O. Silva, T. P. Sotiriou, and S. S. Yazadjiev, Spontaneous scalarization, Rev. Mod. Phys. 96, 015004 (2024).
  27. Y. Chen and E. Teo, Black holes with bottle-shaped horizons, Phys. Rev. D 93, 124028 (2016).
  28. P. Ferrero, J. P. Gauntlett, J. M. P. Ipiña, D. Martelli, and J. Sparks, Accelerating black holes and spinning spindles, Phys. Rev. D 104, 046007 (2021).
  29. P. Ferrero, J. P. Gauntlett, J. M. Pérez Ipiña, D. Martelli, and J. Sparks, D3-Branes wrapped on a spindle, Phys. Rev. Lett. 126, 111601 (2021).
  30. S. Giri, Black holes with spindles at the horizon, J. High Energy Phys. 06 (2022) 145.
  31. A. Boido, J. P. Gauntlett, D. Martelli, and J. Sparks, Gravitational blocks, spindles and GK geometry, Commun. Math. Phys. 403, 917 (2023).
  32. I. D. Novikov and V. S. Manko, Generalizations of the Kerr and Kerr-Newman metrics possessing an arbitrary set of mass-multipole moments, Classical Quantum Gravity 9, 2477 (1992).
  33. T. Johannsen and D. Psaltis, A metric for rapidly spinning black holes suitable for strong-field tests of the No-Hair Theorem, Phys. Rev. D 83, 124015 (2011).
  34. S. Vigeland, N. Yunes, and L. Stein, Bumpy black holes in alternate theories of gravity, Phys. Rev. D 83, 104027 (2011).
  35. R. Emparan, P. Figueras, and M. Martinez, Bumpy black holes, J. High Energy Phys. 12 (2014) 072.
  36. S. Dubovsky, P. Tinyakov, and M. Zaldarriaga, Bumpy black holes from spontaneous Lorentz violation, J. High Energy Phys. 11 (2007) 083.
  37. K. Hristov and M. Suh, Spindle black holes in AdS4×SE7, J. High Energy Phys. 10 (2023) 141.
  38. M. Suh, Baryonic spindles from conifolds, J. High Energy Phys. 02 (2025) 181.
  39. N. Farhangkhah and M. H. Dehghani, Lovelock black holes with nonmaximally symmetric horizons, Phys. Rev. D 90, 044014 (2014).
  40. F. Canfora, M. Lagos, and A. Vera, Superconducting multivortices and a novel BPS bound in chiral perturbation theory, J. High Energy Phys. 10 (2024) 224.
  41. L. Onsager, Statistical hydrodynamics, Il Nuovo Cimento 6, 279 (1949).
  42. R. P. Feynman, Application of quantum mechanics to liquid helium, in Progress in Low Temperature Physics, Vol. 1 (Elsevier, New York, 1955), pp. 17–53.
  43. S. A. Hartnoll, D. M. Ramirez, and J. E. Santos, Entropy production, viscosity bounds and bumpy black holes, J. High Energy Phys. 03 (2016) 170.
  44. P. Kovtun, D. T. Son, and A. O. Starinets, Viscosity in strongly interacting quantum field theories from black hole physics, Phys. Rev. Lett. 94, 111601 (2005).
  45. The pion mass can be safely neglected in the present context as it is orders of magnitude smaller than the solitons of the theory.

  46. R. J. Donnelly, Quantized Vortices in Helium II, Cambridge Studies in Low Temperature Physics, Vol. 3 (Cambridge University Press, Cambridge, England, 1991).
  47. A. L. Fetter, Rotating trapped Bose-Einstein condensates, Rev. Mod. Phys. 81, 647 (2009).
  48. D. R. Brill, J. Louko, and P. Peldán, Thermodynamics of (3+1)-dimensional black holes with toroidal or higher genus horizons, Phys. Rev. D 56, 3600 (1997).
  49. R. L. Arnowitt, S. Deser, and C. W. Misner, The dynamics of general relativity, Gen. Relativ. Gravit. 40, 1997 (2008).
  50. R. M. Wald, Black hole entropy is the Noether charge, Phys. Rev. D 48, R3427 (1993).
  51. M. Barriola and A. Vilenkin, Gravitational field of a global monopole, Phys. Rev. Lett. 63, 341 (1989).
  52. E. Poli, T. Bland, S. J. M. White, M. J. Mark, F. Ferlaino, S. Trabucco, and M. Mannarelli, Glitches in rotating supersolids, Phys. Rev. Lett. 131, 223401 (2023).

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