Scaling symmetry and scalar hairy rotating AdS₃ black holes
classification
✦ hep-th
gr-qc
keywords
blackhairyholesrotatingrelationscalingsmarrsymmetry
read the original 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.
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