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Scalar-tensor black holes coupled to Born-Infeld nonlinear electrodynamics

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arxiv 0704.3784 v1 pith:V6EOPHKR submitted 2007-04-28 gr-qc

Scalar-tensor black holes coupled to Born-Infeld nonlinear electrodynamics

classification gr-qc
keywords blackholeselectrodynamicssolutionscausalfieldscalarscalar-tensor
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The non-existence of asymptotically flat, neutral black holes and asymptotically flat, charged black holes in the Maxwell electrodynamics, with non-trivial scalar field has been proved for a large class of scalar-tensor theories. The no-scalar-hair theorems, however, do not apply in the case of non-linear electrodynamics. In the present work numerical solutions describing charged black holes coupled to Born-Infeld type non-linear electrodynamics in scalar-tensor theories of gravity with massless scalar field are found. The causal structure and properties of the solutions are studied, and a comparison between these solutions and the corresponding solutions in the General Relativity is made. The presence of the scalar field leads to a much more simple causal structure. The present class of black holes has a single, non-degenerate horizon, i.e., its causal structure resembles that of the Schwarzschild black hole.

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  1. Nonlinear electrodynamics and stability of spherically symmetric space-times in scalar-tensor gravity

    gr-qc 2026-07 accept novelty 5.0

    For NED with Maxwell weak-field limit, monopole stability of STT solutions with F=0 is identical to Maxwell-STT, and the zero-charge limit of V_eff erases all NED traces.