Four-Dimensional Entropy from Three-Dimensional Gravity

Carlip, S.

doi:10.1103/PhysRevLett.115.071302

Title: Four-Dimensional Entropy from Three-Dimensional Gravity

Full Record
Other Related Research

Authors:: Carlip, S.

Publication Date:: Thu Aug 13 00:00:00 EDT 2015

Sponsoring Org.:: USDOE

OSTI Identifier:: 1210097

Grant/Contract Number:: FG02-91ER40674

Resource Type:: Publisher's Accepted Manuscript

Journal Name:: Physical Review Letters

Additional Journal Information:: Journal Volume: 115; Journal Issue: 7; Journal ID: ISSN 0031-9007

Publisher:: American Physical Society

Country of Publication:: United States

Language:: English

Citation Formats


                    Carlip, S. Four-Dimensional Entropy from Three-Dimensional Gravity.  United States: N. p., 2015. 
Web.  doi:10.1103/PhysRevLett.115.071302.

Copy to clipboard


                    Carlip, S. Four-Dimensional Entropy from Three-Dimensional Gravity.  United States.  https://doi.org/10.1103/PhysRevLett.115.071302

Copy to clipboard


                    Carlip, S. Thu .  
"Four-Dimensional Entropy from Three-Dimensional Gravity".  United States.  https://doi.org/10.1103/PhysRevLett.115.071302.

Copy to clipboard


                    
@article{osti_1210097,

  title        = {Four-Dimensional Entropy from Three-Dimensional Gravity},

  author       = {Carlip, S.},

  abstractNote = {},

  doi          = {10.1103/PhysRevLett.115.071302},

  journal      = {Physical Review Letters},

  number       = 7,

  volume       = 115,

  place        = {United States},

  year         = {Thu Aug 13 00:00:00 EDT 2015},

  month        = {Thu Aug 13 00:00:00 EDT 2015}

}

Copy to clipboard

Journal Article:

Free Publicly Available Full Text

Accepted Manuscript (Publisher)

Publisher's Version of Record
https://doi.org/10.1103/PhysRevLett.115.071302

Other availability

Search WorldCat to find libraries that may hold this journal

Citation Metrics:

Cited by: 5 works

Citation information provided by
Web of Science

Save / Share:

Export Metadata

Save to My Library

Similar Records in DOE PAGES and OSTI.GOV collections:

Three-dimensional gravity and string ghosts

Journal Article Carlip, S ; Kogan, I I - Physical Review Letters; (United States)

It is known that much of the structure of string theory can be derived from three-dimensional topological field theory and gravity. We show here that, at least for simple topologies, the string diffeomorphism ghosts can also be explained in terms of three-dimensional physics.
https://doi.org/10.1103/PhysRevLett.67.3647
Black holes in three-dimensional topological gravity

Journal Article Carlip, S ; Gegenberg, J ; Mann, R B ; ... - Physical Review, D

We investigate the black hole solution to (2+1)-dimensional gravity coupled to topological matter, with a vanishing cosmological constant. We calculate the total energy, angular momentum, and entropy of the black hole in this model and compare with results obtained in Einstein gravity. We find that the theory with topological matter reverses the identification of energy and angular momentum with the parameters in the metric, compared with general relativity, and that the entropy is determined by the circumference of the inner rather than the outer horizon. We speculate that this results from the contribution of the topological matter fields to themore »« less
https://doi.org/10.1103/PhysRevD.51.6854
A note on black hole entropy in loop quantum gravity

Journal Article Carlip, S. - Classical and Quantum Gravity
Cited by 10
https://doi.org/10.1088/0264-9381/32/15/155009
Microscopic entropy of the three-dimensional rotating black hole of Bergshoeff-Hohm-Townsend massive gravity

Journal Article Giribet, Gaston ; Oliva, Julio ; Instituto de Fisica, Facultad de Ciencias, Universidad Austral de Chile, Casilla 567, Valdivia ; ... - Physical Review. D, Particles Fields

Asymptotically anti-de Sitter rotating black holes for the Bergshoeff-Hohm-Townsend massive gravity theory in three dimensions are considered. In the special case when the theory admits a unique maximally symmetric solution, apart from the mass and the angular momentum, the black hole is described by an independent 'gravitational hair' parameter, which provides a negative lower bound for the mass. This bound is saturated at the extremal case, and since the temperature and the semiclassical entropy vanish, it is naturally regarded as the ground state. The absence of a global charge associated with the gravitational hair parameter reflects itself through the firstmore »« less
https://doi.org/10.1103/PHYSREVD.80.124046
Statistical Entropy of Four-Dimensional Rotating Black Holes from Near-Horizon Geometry

Journal Article Cvetic, M ; Larsen, F ; Cvetic, M - Physical Review Letters

We show that a class of four-dimensional rotating black holes allow five-dimensional embeddings as black rotating strings. Their near-horizon geometry factorizes locally as a product of the three-dimensional anti{endash}de Sitter space-time and a two-dimensional sphere (AdS{sub 3}{times}S{sup 2} ), with angular momentum encoded in the global space-time structure. Following the observation that the isometries on the AdS{sub 3} space induce a two-dimensional (super)conformal field theory on the boundary, we reproduce the microscopic entropy with the correct dependence on the black hole angular momentum. {copyright} {ital 1999} {ital The American Physical Society }
https://doi.org/10.1103/PhysRevLett.82.484

Similar Records