Abstract
We study electrically charged, dilaton black holes, which possess infinitesimal angular momentum in the presence of one or two Liouville type potentials. These solutions are neither asymptotically flat nor (anti)-de Sitter. Some properties of the solutions are discussed.
Similar content being viewed by others
References
Belinsky, V. and Ruffini, R. (1980). Physics Letters B89, 195.
Brown, J. and York, J. (1993). Physical Review D47, 1407.
Cai, R. and Wang, A. (2004). Physical Review D70, 084042.
Chan, K., Horne, J., and Mann, R. (1995). Nuclear Physics B447, 441.
Casadio, R., Harms, B., Leblanc, Y., and Cox, P. H. (1997). Physical Review D55, 814.
Dehghani, M. H. (2005). Physical Review D71, 064010.
Dehghani, M. H. and Farhangkhah, N. (2005). Physical Review D71, 044008.
Ghosh, T. and Mitra, P. (2003). Classical Quantum Gravity 20, 1403.
Horne, J. and Horowitz, G. (1992). Physical Review D46, 1340.
Kleihaus, B., Kunz, J., and Navarro-Lerida, F. (2004). Physical Review D69, 064028.
Mignemi, S. and Wiltshire, D. (1989). Classical Quantum Gravity 6, 987.
Mignemi, S. and Wiltshire, D. (1992). Physical Review D46, 1475.
Poletti, S. and Wiltshire, D. (1995) Physical Review D50, 7260
Poletti, S. and Wiltshire, D. (1994) Physical Review D52, 3753(E).
Shiraishi, K. (1992). Physics Letters A166, 298
Wiltshire, D. (1991). Physical Review D44, 1100.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Sheykhi, A., Riazi, N. Rotating Solutions of Einstein-Maxwell-Dilaton Gravity with Unusual Asymptotics. Int J Theor Phys 45, 2453–2463 (2006). https://doi.org/10.1007/s10773-006-9213-1
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-006-9213-1