2005/12/31 by Christophe Galfard, Cristiano Germani, Akihiro Ishibashi · 35 citations
Physics and Astronomy · #AdS black hole #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black brane #Black hole (networking) #Brane #Charged black hole #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Extremal black hole #Horizon #Nonsingular black hole models #Physics #Quantum mechanics #Randall–Sundrum model #Spacetime #Theoretical physics #astro-ph #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.73.064014
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 73(6) (American Physical Society) · 21 pages, 6 figures, RevTex; v2: clarifications added, figures updated, eq.31 corrected, comment on small four dimensional cosmological constant limit added, character size increased, results unchanged. v3: reference added, version accepted in Phys. Rev. D (2006)
arxiv created 2006/02/25 · openalex publication_date 2006/03/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the possibility of having a static, asymptotically AdS black hole localized on a braneworld with matter fields, within the framework of the Randall and Sundrum scenario. We attempt to look for such a brane black hole configuration by slicing a given bulk spacetime and taking ℤ2 symmetry about the slices. We find that such configurations are possible, and as an explicit example, we provide a family of asymptotically AdS brane black hole solutions for which both the bulk and brane metrics are regular on and outside the black hole horizon and brane matter fields are realistic in the sense that the dominant energy condition is satisfied. We also find that our braneworld models exhibit signature change inside the black hole horizon.