A new proof of Birkhoff's theorem

dc.creatorSchmidt, H. -J.
dc.date1997-09-26
dc.date.accessioned2026-07-07T06:32:26Z
dc.date.available2026-07-07T06:32:26Z
dc.descriptionAssuming SO(3)-spherical symmetry, the 4-dimensional Einstein equation reduces to an equation conformally related to the field equation for 2-dimensional gravity following from the Lagrangian L = R^(1/3). Solutions for 2-dimensional gravity always possess a local isometry because the traceless part of its Ricci tensor identically vanishes. Combining both facts, we get a new proof of Birkhoff's theorem; contrary to other proofs, no coordinates must be introduced. The SO(m)-spherically symmetric solutions of the (m+1)-dimensional Einstein equation can be found by considering L = R^(1/m) in two dimensions. This yields several generalizations of Birkhoff's theorem in an arbitrary number of dimensions, and to an arbitrary signature of the metric.
dc.description17 pages, LaTeX, no figures, Grav. and Cosm. in print
dc.identifierhttps://arxiv.org/abs/gr-qc/9709071
dc.identifierhttp://arxiv.org/abs/gr-qc/9709071
dc.identifierGrav.Cosmol. 3 (1997) 185-190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98900
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA new proof of Birkhoff's theorem
dc.typetext

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