Black holes and black branes in Lifshitz spacetimes

J. Tarrio; S.J.G. Vandoren

doi:10.1007/JHEP09(2011)017

Black holes and black branes in Lifshitz spacetimes

J. Tarrio, S.J.G. Vandoren

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Abstract

We construct analytic solutions describing black holes and black branes in asymptotically Lifshitz spacetimes with arbitrary dynamical exponent z and for arbitrary number of dimensions. The model considered consists of Einstein gravity with negative cosmological constant, a scalar, and N U(1) gauge fields with dilatonic-like couplings. We study the phase diagrams and thermodynamic instabilities of the solution, and find qualitative differences between the cases with 1 ≤ z 2.

Original language	English
Article number	17
Pages (from-to)	017
Number of pages	28
Journal	Journal of High Energy Physics
Volume	2011
Issue number	09
DOIs	https://doi.org/10.1007/JHEP09(2011)017
Publication status	Published - 2011

Keywords

Gauge-gravity correspondence
Black Holes
Holography and condensed matter physics (AdS/CMT)

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10.1007/JHEP09(2011)017Licence: CC BY-NC

JHEP09(2011)017Final published version, 546 KBLicence: CC BY-NC

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title = "Black holes and black branes in Lifshitz spacetimes",

abstract = "We construct analytic solutions describing black holes and black branes in asymptotically Lifshitz spacetimes with arbitrary dynamical exponent z and for arbitrary number of dimensions. The model considered consists of Einstein gravity with negative cosmological constant, a scalar, and N U(1) gauge fields with dilatonic-like couplings. We study the phase diagrams and thermodynamic instabilities of the solution, and find qualitative differences between the cases with 1 ≤ z 2.",

keywords = "Gauge-gravity correspondence, Black Holes, Holography and condensed matter physics (AdS/CMT)",

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AU - Vandoren, S.J.G.

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AB - We construct analytic solutions describing black holes and black branes in asymptotically Lifshitz spacetimes with arbitrary dynamical exponent z and for arbitrary number of dimensions. The model considered consists of Einstein gravity with negative cosmological constant, a scalar, and N U(1) gauge fields with dilatonic-like couplings. We study the phase diagrams and thermodynamic instabilities of the solution, and find qualitative differences between the cases with 1 ≤ z 2.

KW - Gauge-gravity correspondence

KW - Black Holes

KW - Holography and condensed matter physics (AdS/CMT)

U2 - 10.1007/JHEP09(2011)017

DO - 10.1007/JHEP09(2011)017

M3 - Article

SN - 1126-6708

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SP - 017

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

IS - 09

M1 - 17

ER -

Black holes and black branes in Lifshitz spacetimes

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