Higher spin gravity in 3D: Black holes, global charges and thermodynamics
By A. Pérez, D. Tempo, Ricardo Troncoso. 2012
146 citations recorded by the source corpus.
Abstract Global charges and thermodynamic properties of three-dimensional higher spin black holes that have been recently found in the literature are revisited. Since these solutions possess a relaxed asymptotically AdS behavior, following the canonical approach, it is shown that the global charges, and in particular the energy, acquire explicit nontrivial contributions given by nonlinear terms in the deviations with respect to the reference background. It is also found that there are cases for which the first law of thermodynamics can be readily worked out in the canonical ensemble, i.e., without work terms associated to the presence of higher spin fields, and remarkably, the semiclassical higher spin black hole entropy is exactly reproduced from Cardy formula.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/60ec0555509c21adc86205478156e6e3e4ba48fa
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
In Statistical and Nonlinear Physics
Citations in the corpus
- Thermodynamics of higher spin black holes in AdS3 (2013, methodology): “13) Similar μ-dependent terms appear in the black hole energy (mass) computed via canonical methods [22].”
- Towards metric-like higher spin gauge theories in three dimensions (2012, methodology): “13 A modification of the relation M = MBTZ was also proposed in [44] via a direct construction of the corresponding conserved charge in the CS formulation.”
- Black holes in three dimensional higher spin gravity: a review (2012, methodology): “The alternative approach [73] (see also [86]) based on evaluating the Euclidean Chern-Simons action with appropriate boundary terms leads to the same final result.”
- Thermodynamics of higher spin black holes in 3D (2012, methodology): “The answer to this question was recently provided in [43] (see also [44] ) and we apply their proposal to compute explicitly the grand potential for the system.”