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Scaling symmetry and scalar hairy rotatingAdS3black holes

Byoungjoon Ahn, Seungjoon Hyun, Sang-A Park, Sang-Heon Yi
2016 Physical Review D  

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2015 pre-print arXiv:1508.06484v2 fatcat:rt6jbcz62fbv5c6vxcahjszcfy

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2015 accepted
arXiv:1508.06484v3 fatcat:bmiasprlnjaeho6thmt6p2lfqu
2015 pre-print
arXiv:1508.06484v1 fatcat:46irrolsxndvrgjpyef6gwaqrm
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.
doi:10.1103/physrevd.93.024041 fatcat:5gulvg5x5nfmzabkwku6objcxa
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Byoungjoon Ahn, Seungjoon Hyun, Sang-A Park, Sang-Heon Yi. "Scaling symmetry and scalar hairy rotatingAdS3black holes." Physical Review D 93.2 (2016)