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Warped black holes in 3D general massive gravity
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We study regular spacelike warped black holes in the three dimensional general massive gravity model, which contains both the gravitational Chern-Simons term and the linear combination of curvature squared terms characterizing the new massive gravity besides the Einstein-Hilbert term. The parameters of the metric are found by solving a quartic equation constrained by an inequality that imposes the absence of closed timelike curves. Explicit expressions for the central charges are suggested by exploiting the fact that these black holes are discrete quotients of spacelike warped AdS(3) and a known formula for the entropy. Previous results obtained separately in topological massive gravity and in new massive gravity are recovered as special cases.
Forward citations
Cited by 3 Pith papers
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Optimal Control Theory of the (2+1)-Dimensional BTZ Black Hole
Geodesics of the Weinhold and Ruppeiner thermodynamic metrics are computed for the BTZ black hole and interpreted as optimal evaporation/accretion protocols.
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Thermodynamic Stability and Fluctuations of the (2+1)-dimensional GMG Warped Black Hole
Thermodynamic instability and fluctuation analysis of the GMG warped black hole, including exact on-shell angular momentum trajectories and thermodynamic lengths for isentropic/isoenergetic processes.
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Note on WAdS$_3$ black holes in extended BHT gravity
Using Wald's formalism and the thermodynamics method, the paper computes conserved charges and dual CFT central charges for WAdS3 black holes in NMG and ENMG, finding results consistent with earlier work.
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