Hairy black hole entropy and the role of solitons in three dimensions

DOI10.1007/JHEP02(2012)136zbMath1309.81182arXiv1112.6198MaRDI QIDQ2340548

Ricardo Troncoso, Cristián Martínez, Francisco Julio Sobreira de Araujo Correa

Publication date: 20 April 2015

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1112.6198

zbMATH Keywords

AdS-CFT correspondenceblack holesclassical theories of gravity

Mathematics Subject Classification ID

Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Exact solutions to problems in general relativity and gravitational theory (83C15) Measures of information, entropy (94A17) Soliton solutions (35C08)

Related Items (7)

Bootstrapping gravity solutions ⋮ Boundary conditions for general relativity on \(\mathrm{AdS}_{3}\) and the KdV hierarchy ⋮ Gravity coupled to a scalar field from a Chern-Simons action: describing rotating hairy black holes and solitons with gauge fields ⋮ A Cardy-like formula for rotating black holes with planar horizon ⋮ Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of \(\mathrm{ADS}_3\) boundary conditions ⋮ Exact black-hole formation with a conformally coupled scalar field in three dimensions ⋮ Higher spin gravity in 3D: black holes, global charges and thermodynamics

Cites Work

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