1998
DOI: 10.1088/1126-6708/1998/02/009
|View full text |Cite
|
Sign up to set email alerts
|

Black hole entropy from near-horizon microstates

Abstract: Black holes whose near-horizon geometries are locally, but not necessarily globally, AdS 3 (three-dimensional anti-de Sitter space) are considered. Using the fact that quantum gravity on AdS 3 is a conformal field theory, we microscopically compute the black hole entropy from the asymptotic growth of states. Precise numerical agreement with the Bekenstein-Hawking area formula for the entropy is found. The result pertains to any consistent quantum theory of gravity, and does not use string theory or supersymmet… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

60
1,583
2
2

Year Published

2000
2000
2024
2024

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 1,058 publications
(1,647 citation statements)
references
References 25 publications
60
1,583
2
2
Order By: Relevance
“…Since the BH entropy is the exponent of the partition functions at the "leading order", this result implies the relation (1.1) holds at the leading order. However, this is in contrast to Strominger's computation on the BTZ black hole entropy from a conformal field theory at spatial infinity [18] that implies a holography (1.1) at spatial infinity at the same (leading) order. So, at least for the leading order, both the holography at spatial infinity and that of the horizon give an identical result, and one can not distinguish between these very different approaches.…”
Section: Introductioncontrasting
confidence: 69%
See 2 more Smart Citations
“…Since the BH entropy is the exponent of the partition functions at the "leading order", this result implies the relation (1.1) holds at the leading order. However, this is in contrast to Strominger's computation on the BTZ black hole entropy from a conformal field theory at spatial infinity [18] that implies a holography (1.1) at spatial infinity at the same (leading) order. So, at least for the leading order, both the holography at spatial infinity and that of the horizon give an identical result, and one can not distinguish between these very different approaches.…”
Section: Introductioncontrasting
confidence: 69%
“…[12] or Ref. [18], where the classical effect was dominant; but, one can not distinguish between them at the leading order. However, quite interestingly, it is known [40] that this WZW approaches gives the correct '− 3 2 lnS BH ' term already, as is consistent with the (horizon) holographic principle, though this approach has some undesirable features of the non-unitary Hilbert space and infinite degeneracy of the vacuum [8].…”
Section: Comparison With Other Approaches a Wess-zumino-witten(wzw) Mmentioning
confidence: 99%
See 1 more Smart Citation
“…The combined Virasoro/current algebras admit the following spectral flow automorphisms: 6) in the SU (2) case, and…”
Section: Review: Partition Functions In Cftmentioning
confidence: 99%
“…For these we take 6) with N ∈ Z. The angular coordinate φ has the standard 2π periodicity, and fermions are taken to be periodic in φ.…”
Section: Conical Defectsmentioning
confidence: 99%