Static Einstein-Maxwell Black Holes with No Spatial Isometries in AdS Space

Carlos A. R. Herdeiro and Eugen Radu
Phys. Rev. Lett. 117, 221102 – Published 22 November 2016
PDFHTMLExport Citation

Abstract

We explicitly construct static black hole solutions to the fully nonlinear, D=4, Einstein-Maxwell–anti-de Sitter (AdS) equations that have no continuous spatial symmetries. These black holes have a smooth, topologically spherical horizon (section), but without isometries, and approach, asymptotically, global AdS spacetime. They are interpreted as bound states of a horizon with the Einstein-Maxwell–AdS solitons recently discovered, for appropriate boundary data. In sharp contrast to the uniqueness results for a Minkowski electrovacuum, the existence of these black holes shows that single, equilibrium, black hole solutions in an AdS electrovacuum admit an arbitrary multipole structure.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 9 June 2016

DOI:https://doi.org/10.1103/PhysRevLett.117.221102

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Carlos A. R. Herdeiro and Eugen Radu

  • Departamento de Física da Universidade de Aveiro and CIDMA, Campus de Santiago, 3810-183 Aveiro, Portugal

Article Text (Subscription Required)

Click to Expand

Supplemental Material (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 117, Iss. 22 — 25 November 2016

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×