2015
DOI: 10.1007/jhep02(2015)070
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Van Der Waals black holes in d dimensions

Abstract: We generalize the recent solution proposed by Rajagopal et al. to arbitrary number of dimensions and horizon topologies. We comment on the regime of validity of these solution. Among our main results, we argue that the Van Der Waals (VdW) black hole (BH) metric is to be interpreted as a near horizon metric. This is supported by inspecting the energy conditions. We analyze the limiting cases of a perfect fluid, interacting points and non interacting balls gas equation of state and map them to known black holes.… Show more

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Cited by 41 publications
(40 citation statements)
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References 20 publications
(53 reference statements)
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“…As shown in Eqs. (15) and (19), it is obvious that the heat capacity is divergent in this case. Therefore, the corresponding phase transition is second order.…”
Section: Van Der Waals Behaviour Of Thermodynamics Entropymentioning
confidence: 94%
“…As shown in Eqs. (15) and (19), it is obvious that the heat capacity is divergent in this case. Therefore, the corresponding phase transition is second order.…”
Section: Van Der Waals Behaviour Of Thermodynamics Entropymentioning
confidence: 94%
“…A similar situation occurs for black hole solutions in the presence of rotation, higher dimensions, or higher curvature corrections. Asymptotically AdS black holes whose thermodynamics match exactly that of the Van der Waals fluid were constructed in [162,163] in the context of Einstein gravity. Surprisingly, the solution is supported by 'exotic matter' that does not obey any of the energy conditions everywhere outside of the horizon.…”
Section: Charged Ads Black Holes and Van Der Waals Fluidsmentioning
confidence: 99%
“…and for the 2+1 dimensional space-time, P = −Λ 8π [27]. Furthermore, using the Einstein field equation and the energy momentum tensor definition will yield the energy conditions as follows:…”
Section: Anyon Van Der Waals Black Holementioning
confidence: 99%