Black holes in two spacetime dimensions

J. D. Brown, Marc Henneaux, and Claudio Teitelboim
Phys. Rev. D 33, 319 – Published 15 January 1986
PDFExport Citation

Abstract

It is shown that the analog of the black hole exists in two-dimensional gravity. It is given by a metric which solves the vacuum field equation (constant curvature) everywhere except on a singular line. This geometry possesses an event horizon. There is as well an analog of Hawking radiation with temperature proportional to the strength (mass) of the singularity.

  • Received 29 November 1984

DOI:https://doi.org/10.1103/PhysRevD.33.319

©1986 American Physical Society

Authors & Affiliations

J. D. Brown and Marc Henneaux

  • Center for Theoretical Physics, University of Texas at Austin, Austin, Texas 78712

Claudio Teitelboim

  • Center for Theoretical Physics, University of Texas at Austin, Austin, Texas 78712 and Centro de Estudios Científicos de Santiago, Casilla 16443, Santiago 9, Chile

References (Subscription Required)

Click to Expand
Issue

Vol. 33, Iss. 2 — 15 January 1986

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 D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×