1999/12/15 by Roberto Emparan, Gary T. Horowitz, Gary T Horowitz +2 · 8 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #BTZ black hole #Black Holes and Theoretical Physics #Black brane #Black hole (networking) #Black hole thermodynamics #Black string #Brane cosmology #Extremal black hole #Micro black hole #Noncommutative and Quantum Gravity Theories #String theory #gr-qc #hep-th
paper · pdf · doi:10.1088/1126-6708/2000/01/021
published as JHEP 0001 (2000) 021 · 30 pages
arxiv created 1999/12/15 · openalex publication_date 2000/01/18 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We extend our recent discussion of four-dimensional black holes bound to a two-brane to include a negative cosmological constant on the brane. We find that for large masses, the solutions are precisely BTZ black holes on the brane, and BTZ `black strings' in the bulk. For smaller masses, there are localized black holes which look like BTZ with corrections that fall off exponentially. We compute when the maximum entropy configuration changes from the black string to the black hole. We also present exact solutions describing rotating black holes on two-branes which are either asymptotically flat or asymptotically AdS3. The mass and angular momentum on the brane agree with that in the bulk.