Ehlers-Harrison transformations and black holes in Dilaton-Axion Gravity with multiple vector fields

Details Ehlers-Harrison transformations and black holes in Dilaton-Axion Gravity with multiple vector fields Ehlers-Harrison transformations and black holes in Dilaton-Axion Gravity with multiple vector fields

1996-12-02

arxiv.org/abs/gr-qc/9612007v1

Phys.Rev. D55 (1997) 3580-3592

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

37 pages, Latex

Scientific paper

10.1103/PhysRevD.55.3580

Dilaton-axion gravity with $p U(1)$ vector fields is studied on space-times admitting a timelike Killing vector field. Three-dimensional sigma-model is derived in terms of K\"ahler geometry, and holomorphic representation of the SO(2,2+p) global symmetry is constructed. A general static black hole solution depending on $2p+5$ parameters is obtained via SO(2,2+p) covariantization of the Schwarzschild solution. The metric in the curvature coordinates looks as the variable mass Reissner-Nordstr\"om one and generically possesses two horizons. The inner horizon is pushed to the singularity if electric and magnetic SO(p) charge vectors are parallel. For non-parallel charges the inner horizon has a finite area except for an extremal limit when this property is preserved only for orthogonal charges. Extremal dyon configurations with orthogonal charges have finite horizon radii continuously varying from zero to the ADM mass. New general solution is endowed with a NUT parameter, asymptotic values of dilaton and axion, and a gauge parameter which can be used to ascribe any given value to one of scalar charges.

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