Scaling symmetry and scalar hairy rotating AdS_3 black holes
arXiv:1508.06484 · doi:10.1103/PhysRevD.93.024041
Abstract
By using the scaling symmetry in the reduced action formalism, we derive the novel Smarr relation which holds even for the hairy rotating AdS_3 black holes. And then, by using the Smarr relation we argue that the hairy rotating AdS_3 black holes are stable thermodynamically, compared to the non-hairy ones.
1+18 pages, plain LaTeX; v2 typos fixed, references added; v3 accepted for publication in PRD
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