Fate of three-dimensional black holes coupled to a scalar field and the Bekenstein-Hawking entropy.
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Publication:2462908
DOI10.1016/j.physletb.2004.07.023zbMath1123.83304arXivhep-th/0403089OpenAlexW1851630024MaRDI QIDQ2462908
Publication date: 5 December 2007
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/0403089
Related Items (8)
Bootstrapping gravity solutions ⋮ Gravity coupled to a scalar field from a Chern-Simons action: describing rotating hairy black holes and solitons with gauge fields ⋮ Exploring accelerating hairy black holes in 2+1 dimensions: the asymptotically locally anti-de Sitter class and its holography ⋮ The CFT-interpolating black hole in three dimensions ⋮ Scalar solitons and the microscopic entropy of hairy black holes in three dimensions ⋮ Thermodynamics of exotic black holes, negative temperature, and Bekenstein-Hawking entropy ⋮ THOUGHTS ON THE AREA THEOREM ⋮ Hairy black hole entropy and the role of solitons in three dimensions
Cites Work
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- Entropy from conformal field theory at Killing horizons
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