Solitons and black holes in Einstein-Born-Infeld-dilaton theory -: art. no. 124013
被引:43
作者:
Clément, G
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机构:CNRS, Lab Annecy Le Vieux Phys Theor, F-74941 Annecy Le Vieux, France
Clément, G
Gal'tsov, D
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机构:CNRS, Lab Annecy Le Vieux Phys Theor, F-74941 Annecy Le Vieux, France
Gal'tsov, D
机构:
[1] CNRS, Lab Annecy Le Vieux Phys Theor, F-74941 Annecy Le Vieux, France
[2] Moscow MV Lomonosov State Univ, Dept Theoret Phys, Moscow 119899, Russia
来源:
PHYSICAL REVIEW D
|
2000年
/
62卷
/
12期
关键词:
D O I:
10.1103/PhysRevD.62.124013
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Static spherically symmetric asymptotically flat solutions to the U(1) Born-Infeld theory coupled to gravity and to a dilaton are investigated. The dilaton enters in such a way that the theory is SL(2,R) symmetric for a unit value of the dilaton coupling constant. We find globally regular solutions for any value of the effective coupling which is the ratio of the gravitational and dilaton couplings; they form a continuous sequence labeled by the sole free parameter of the local solution near the origin. The allowed values of this parameter are bounded from below, and, as the limiting value is approached, the mass and the dilaton charge rise indefinitely and tend to a strict equality tin suitable units). Together with the electric charge they saturate the BPS bound of the corresponding linear U(1) theory. Beyond this boundary the solutions become compact (singular), while the limiting solution at the exact boundary value is noncompact and nonasymptotically flat. The black holes in this theory exist for any value of the event horizon radius and also form a sequence labeled by a continuously varying parameter restricted to a finite interval. The singularity inside the black hole exhibits a power-law mass inflation.