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

dc.creatorVollick, Dan N.
dc.date2006-01-30
dc.date.accessioned2026-07-07T06:58:06Z
dc.date.available2026-07-07T06:58:06Z
dc.descriptionIn 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 $G_{μν}=-κT_{μν}$ 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.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0601136
dc.identifierhttp://arxiv.org/abs/gr-qc/0601136
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/107229
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack hole and cosmological space-times in Born-Infeld-Einstein theory
dc.typetext

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