corner
corner

Phys. Rev. D 33, 319–323 (1986)

Black holes in two spacetime dimensions

Download: PDF (444 kB) Buy this article Export: BibTeX or EndNote (RIS)

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

Received 29 November 1984; published in the issue dated 15 January 1986

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.

© 1986 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.33.319
DOI:
10.1103/PhysRevD.33.319
PACS:
04.20.Jb, 02.40.+m