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arxiv: gr-qc/0601136 · v1 · submitted 2006-01-30 · 🌀 gr-qc

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Black hole and cosmological space-times in Born-Infeld-Einstein theory

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classification 🌀 gr-qc
keywords space-timesblackborn-infeldcosmologicalsingularitysphericallysymmetrictheory
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In this paper I examine black hole and cosmological space-times in Born-Infeld-Einstein theory with electric and magnetic charges. The field equations are derived and written in the form $G_{\mu\nu}=-\kappa T_{\mu\nu}$ for spherically symmetric space-times. The energy-momentum tensor is not the Born-Infeld energy-momentum tensor, but can be obtained from Born-Infeld theory by letting $a\to ia$, where $a$ is the Born-Infeld parameter. It is shown that there is a curvature singularity in spherically symmetric space-times at a nonzero radial coordinate and that, as in Reissner-Nordstrom space-times, there are zero, one or two horizons. Charged black holes have either two horizons and a timelike singularity or one horizon with a spacelike, timelike, or null singularity. Anisotropic cosmological solutions with electric and magnetic fields are obtained from the spherically symmetric solutions.

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Cited by 1 Pith paper

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  1. Bouncing cosmologies from Born-Infeld-type gravity

    gr-qc 2026-04 unverdicted novelty 7.0

    A new ghost-free Born-Infeld-type f(R, G) gravity is built that admits a large family of bouncing cosmologies with varied asymptotic behaviors.