Thermodynamically stable asymptotically flat hairy black holes with a dilaton potential
arXiv:1901.01269 · doi:10.1007/JHEP03(2019)205
Abstract
We present a detailed analysis of the thermodynamics of exact asymptotically flat hairy black holes in Einstein-Maxwell-dilaton theory. We compute the regularized action, quasilocal stress tensor, and conserved charges by using a `counterterm method' similar to the one extensively used in the AdS-CFT duality. In the presence of a non-trivial dilaton potential that vanishes at the boundary we prove that, for some range of parameters, there exist thermodynamically stable black holes in the grand canonical and canonical ensembles. To the best of our knowledge, this is the first example of a thermodynamically stable asymptotically flat black hole, without imposing artificial conditions corresponding to embedding in a finite box.
arXiv comment47 pages, 27 figures; v2: typos fixed, refs. added; v3: comments added, typos fixed, matches the published version
References in corpus (24)
- The Large N Limit of Superconformal Field Theories and Supergravity
- The World as a Hologram
- The Dynamics of General Relativity
- A Stress Tensor for Anti-de Sitter Gravity
- Holographic Reconstruction of Spacetime and Renormalization in the AdS/CFT Correspondence
- N=2 Extremal Black Holes
- Kerr black holes with scalar hair
- Supersymmetry and Attractors
- Black Hole Entropy Function and the Attractor Mechanism in Higher Derivative Gravity
- The evolution of unstable black holes in anti-de Sitter space
- Moduli, Scalar Charges, and the First Law of Black Hole Thermodynamics
- Misner String Entropy
- Rotating Circular Strings, and Infinite Non-Uniqueness of Black Rings
- Holographic Renormalization of Asymptotically Flat Spacetimes
- An instability of higher-dimensional rotating black holes
- Gauged Supergravities
- Exact asymptotically flat charged hairy black holes with a dilaton potential
- Trace Anomaly and Counterterms in Designer Gravity
- Moduli and (un)attractor black hole thermodynamics
- Quasilocal formalism and thermodynamics of asymptotically flat black objects
- Thermodynamic instability of doubly spinning black objects
- On Asymptotic Flatness and Lorentz Charges
- Quasilocal equilibrium condition for black ring
- Hairy Black Hole Stability in AdS, Quantum Mechanics on the Half-Line and Holography
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- Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities
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