Conformal Tightness of Holographic Scaling in Black Hole Thermodynamics
arXiv:0903.1960 · doi:10.1088/0264-9381/30/17/175007
Abstract
The near-horizon conformal symmetry of nonextremal black holes is shown to be a mandatory ingredient for the holographic scaling of the scalar-field contribution to the black hole entropy. This conformal tightness is revealed by semiclassical first-principle scaling arguments through an analysis of the multiplicative factors in the entropy due to the radial and angular degrees of freedom associated with a scalar field. Specifically, the conformal SO(2,1) invariance of the radial degree of freedom conspires with the area proportionality of the angular momentum sums to yield a robust holographic outcome.
23 pages, 1 figure. v2 & v3: expanded explanations and proofs, references added, typos corrected; v3: published version
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