期刊
CLASSICAL AND QUANTUM GRAVITY
卷 30, 期 17, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/30/17/175007
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资金
- National Science Foundation [0602340, 0602301, PHY05-51164]
- University of San Francisco Faculty Development Fund
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.
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