1994/09/26 by S. Carlip, Steven Carlip · 11 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Charged black hole #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Entropy (arrow of time) #Extremal black hole #General relativity #Horizon #Logarithm #Mathematical analysis #Mathematics #Noncommutative and Quantum Gravity Theories #Nonsingular black hole models #Physics #Quantum mechanics #Statistical mechanics #Statistical physics #Theoretical physics #Theory of relativity #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.51.632
published as Phys.Rev.D51:632-637,1995 · 12 pages, UCD-94-32 and NI-94011
arxiv created 1994/09/26 · openalex publication_date 1995/01/15 · arxiv updated 2010/04/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The presence of a horizon breaks the gauge invariance of (2+1)-dimensional general relativity, leading to the appearance of new physical states at the horizon. I show that the entropy of the (2+1)-dimensional black hole can be obtained as the logarithm of the number of these microscopic states.