T Maki and K Shiraishi 1993 Class. Quantum Grav. 10 2171 doi:10.1088/0264-9381/10/10/024
T Maki and K Shiraishi
Show affiliationsAdopting a simple ansatz, we find exact solutions to the Einstein-Maxwell-dilaton equations, which stand for the multi-black hole configuration with maximal charge in a cosmological metric and dilaton field background driven by a cosmological term.
04.70.-s Physics of black holes
04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields
85A40 Cosmology (For relativistic cosmology, see 83F05)
Issue 10 (October 1993)
T Maki and K Shiraishi 1993 Class. Quantum Grav. 10 2171
Takuya Maki and Kiyoshi Shiraishi 1994 Class. Quantum Grav. 11 2781
Kiyoshi Shiraishi 1996 Class. Quantum Grav. 13 1655
Kiyoshi Shiraishi and Takuya Maki 1994 Class. Quantum Grav. 11 695
Takuya Maki and Kiyoshi Shiraishi 1995 Class. Quantum Grav. 12 159
K Shiraishi and S Hirenzaki 1992 Class. Quantum Grav. 9 2277
K Shiraishi 1989 Class. Quantum Grav. 6 2029
Takuya Maki and Kiyoshi Shiraishi 1994 Class. Quantum Grav. 11 227
K Shiraishi 1990 Class. Quantum Grav. 7 135
A N F Aleixo and A B Balantekin 2005 J. Phys. A: Math. Gen. 38 8603