2010
DOI: 10.1007/jhep03(2010)100
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Phase transitions between Reissner-Nordstrom and dilatonic black holes in 4D AdS spacetime

Abstract: We study Einstein-Maxwell-dilaton gravity models in four-dimensional antide\ud Sitter (AdS) spacetime which admit the Reissner-Nordstrom (RN) black hole solution.\ud We show that below a critical temperature the AdS-RN solution becomes unstable against\ud scalar perturbations and the gravitational system undergoes a phase transition. We show\ud using numerical calculations that the new phase is a charged dilatonic black hole. Using\ud the AdS/CFT correspondence we discuss the phase transition in the dual field… Show more

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Cited by 117 publications
(181 citation statements)
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References 44 publications
(62 reference statements)
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“…The gauge field is dual to a conserved global current in the QFT, while the scalar drives the low energy dynamics and is dual to the most important scalar operator of the theory, [58,[61][62][63][64][65]. An important ingredient in the analysis of Einstein Maxwell Dilaton theories is the analytical study of asymptotics of physical observables, by a convenient parametrization of the two-derivative effective action, motivated by string-related supergravities, [58]:…”
Section: Jhep09(2012)011mentioning
confidence: 99%
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“…The gauge field is dual to a conserved global current in the QFT, while the scalar drives the low energy dynamics and is dual to the most important scalar operator of the theory, [58,[61][62][63][64][65]. An important ingredient in the analysis of Einstein Maxwell Dilaton theories is the analytical study of asymptotics of physical observables, by a convenient parametrization of the two-derivative effective action, motivated by string-related supergravities, [58]:…”
Section: Jhep09(2012)011mentioning
confidence: 99%
“…The fact that it has finite entropy at extremality argues against this. This issue can be resolved in the generic Einstein Maxwell Dilaton setup, [58,[61][62][63][64][65]. Then, the low energy fixed point displays hyperscaling violation, [54,66,67].…”
Section: Jhep09(2012)011mentioning
confidence: 99%
“…The corresponding finite-temperature solution can be easily generalized, 12) with the other fields and parameters remaining invariant.…”
Section: The Solutionmentioning
confidence: 99%
“…we can take the following coordinate transformation: 12) to convert the black hole metric into the form of (5.5) with…”
Section: Gauss-bonnet Corrections To η/S At Finite Temperaturementioning
confidence: 99%
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