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Black holes in asymptotically Lifshitz spacetime
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy.
2009 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, no 3, 070- p.Article in journal (Refereed) Published
Abstract [en]

A model of 3 + 1 dimensional gravity with negative cosmological constant coupled to abelian gauge fields has been proposed as a gravity dual for Lifshitz like critical phenomena in 2 + 1 dimensions. The finite temperature behavior is described by black holes that are asymptotic to the Lifshitz fixed point geometry. There is a one-parameter family of charged black holes, where the magnitude of the charge is uniquely determined by the black hole area. These black holes are thermodynamically stable and become extremal in the limit of vanishing size. The theory also has a discrete spectrum of localized objects described by non-singular spacetime geometries. The finite temperature behavior of Wilson loops is reminiscent of strongly coupled gauge theories in 3 + 1 dimensions, including screening at large distances.

Place, publisher, year, edition, pages
2009. no 3, 070- p.
Keyword [en]
Field Theories in Lower Dimensions, Gauge-gravity correspondence, Black Holes
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:uu:diva-129089DOI: 10.1088/1126-6708/2009/03/070ISI: 000265600800070OAI: oai:DiVA.org:uu-129089DiVA: diva2:337563
Available from: 2010-08-06 Created: 2010-08-05 Last updated: 2017-12-12Bibliographically approved

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