thermodynamic properties of asymptotically anti-de sitter black holes in d=4 einstein–yang–mills theory

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ID: 256265
2015
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Abstract
We investigate the thermodynamics of spherically symmetric black hole solutions in a four-dimensional Einstein–Yang–Mills-SU(2) theory with a negative cosmological constant. Special attention is paid to configurations with a unit magnetic charge. We find that a set of Reissner–Nordström–Anti-de Sitter black holes can become unstable to forming non-Abelian hair. However, the hairy black holes are never thermodynamically favoured over the full set of abelian monopole solutions. The thermodynamics of the generic configurations possessing a noninteger magnetic charge is also discussed.
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kichakova2015physicsthermodynamic Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;Olga Kichakova;Jutta Kunz;Eugen Radu;Yasha Shnir
Journal ACS chemical biology
Year 2015
DOI
10.1016/j.physletb.2015.05.052
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