1998/05/31 by Yoshitaka Degura, Kenji Sakamoto, Kiyoshi Shiraishi
Physics and Astronomy · #gr-qc
published as Grav.Cosmol. 7 (2001) 153-158 · 17 pages, 11 figures, RevTeX 3.0, fixed figures
arxiv created 1998/06/11 · arxiv updated 2009/11/30
Nonrotating and rotating black hole soltuions in (2+1) dimensions are studied in a model including a real scalar field with a simple potential coupled to gravity.