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AdS and Lifshitz Black Holes in Conformal and Einstein-Weyl Gravities

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arxiv 1204.1062 v2 pith:YLTZTJQ6 submitted 2012-04-04 hep-th

AdS and Lifshitz Black Holes in Conformal and Einstein-Weyl Gravities

classification hep-th
keywords blackholeslifshitzconformaleinstein-weylgravitygravitiesadditional
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study black hole solutions in extended gravities with higher-order curvature terms, including conformal and Einstein-Weyl gravities. In addition to the usual AdS vacuum, the theories admit Lifshitz and Schr\"odinger vacua. The AdS black hole in conformal gravity contains an additional parameter over and above the mass, which may be interpreted as a massive spin-2 hair. By considering the first law of thermodynamics, we find that it is necessary to introduce an associated additional intensive/extensive pair of thermodynamic quantities. We also obtain new Liftshitz black holes in conformal gravity and study their thermodynamics. We use a numerical approach to demonstrate that AdS black holes beyond the Schwarzschild-AdS solution exist in Einstein-Weyl gravity. We also demonstrate the existence of asymptotically Lifshitz black holes in Einstein-Weyl gravity. The Lifshitz black holes arise at the boundary of the parameter ranges for the AdS black holes. Outside the range, the solutions develop naked singularities. The asymptotically AdS and Lifshitz black holes provide an interesting phase transition, in the corresponding boundary field theory, from a relativistic Lorentzian system to a non-relativistic Lifshitz system.

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Cited by 3 Pith papers

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  1. The Role of the Volume in Black Hole Thermodynamics

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    Conserved charges built from a Kerr-Schild background show the first law requires the Killing vector and AdS background to be held fixed, explaining why the rotating-frame energy F fails while E works, and why the geo...

  2. The Role of the Volume in Black Hole Thermodynamics

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    Adapting Barnich-Compère conserved charges, the first law requires unvarying components for both the Killing vector and AdS background (true for E's ξ but not F's β), while V_C enters the β-Smarr relation due to simpl...

  3. Aspects of the Black Hole Interior Volume and Entropy

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    A doctoral thesis compiles and reproduces prior semiclassical results claiming the interior scalar-mode entropy of black holes is proportional to horizon entropy with a coefficient less than one.