1991/08/14 by James H. Horne, Gary T. Horowitz · 2 voices · 8 citations
Physics and Astronomy · Social Sciences · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #International Science and Diplomacy #hep-th
paper · pdf · doi:10.1016/0550-3213(92)90536-k
published as Nucl.Phys. B368 (1992) 444-462 · 17 pages
arxiv created 1991/08/14 · arxiv published 1991/08/14 · arxiv updated 1991/08/14 · openalex publication_date 1992/01/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
A family of exact conformal field theories is constructed which describe charged black strings in three dimensions. Unlike previous charged black hole or extended black hole solutions in string theory, the low energy spacetime metric has a regular inner horizon (in addition to the event horizon) and a timelike singularity. As the charge to mass ratio approaches unity, the event horizon remains but the singularity disappears.