Asymptotic properties of black hole solutions in dimensionally reduced Einstein-Gauss-Bonnet gravity

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dc.creatorMignemi, S.
dc.date2007-03-08
dc.date.accessioned2026-07-07T11:01:47Z
dc.date.available2026-07-07T11:01:47Z
dc.descriptionWe study the asymptotic behavior of the spherically symmetric solutions of the system obtained from the dimensional reduction of the six-dimensional Einstein- Gauss-Bonnet action. We show that in general the scalar field that parametrizes the size of the internal space is not trivial, but nevertheless the solutions depend on a single parameter. In analogy with other models containing Gauss-Bonnet terms, naked singularities are avoided if a minimal radius for the horizon is assumed.
dc.description9 pages, plain TeX
dc.identifierhttps://arxiv.org/abs/gr-qc/0703059
dc.identifierhttp://arxiv.org/abs/gr-qc/0703059
dc.identifierGen.Rel.Grav.39:815-824,2007
dc.identifierdoi:10.1007/s10714-007-0423-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188056
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymptotic properties of black hole solutions in dimensionally reduced Einstein-Gauss-Bonnet gravity
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