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dc.contributor.authorAudretsch, Jürgende
dc.contributor.authorGähler, Franzde
dc.contributor.authorStraumann, Norbertde
dc.date.accessioned2009-04-30de
dc.date.accessioned2016-03-31T11:41:28Z-
dc.date.available2009-04-30de
dc.date.available2016-03-31T11:41:28Z-
dc.date.issued1984de
dc.identifier.other314262547de
dc.identifier.urihttp://nbn-resolving.de/urn:nbn:de:bsz:93-opus-39881de
dc.identifier.urihttp://elib.uni-stuttgart.de/handle/11682/6948-
dc.identifier.urihttp://dx.doi.org/10.18419/opus-6931-
dc.description.abstractFollowing an axiomatic formulation for general relativity, an equivalent class of pseudo-Riemannian manifolds is derived from the Lorentz conformal structure given by the sets of all possible light rays and all possible free falling objects, the latter set defining the affine geodesics. In particular the set of null geodesics defined by the Lorentz conformal structure characterize a Weyl space-time structure. \par It has been shown by one of the authors that when the classical trajectories of matter fields defined over the Weyl space-time are assumed to coincide with the geodesics of that space, then a set of Lorentzian space-times arise naturally. In the present paper the authors improve this result by use of fiber bundles and the WKB limit to derive the short wave limits to Dirac and Klein-Gordon fields.en
dc.language.isoende
dc.rightsinfo:eu-repo/semantics/openAccessde
dc.subject.classificationRaum-Zeit , Riemannsche Geometriede
dc.subject.ddc530de
dc.titleWave fields in Weyl spaces and conditions for the existence of a preferred pseudo-Riemannian structureen
dc.typearticlede
dc.date.updated2014-10-16de
ubs.fakultaetFakultätsübergreifend / Sonstige Einrichtungde
ubs.institutSonstige Einrichtungde
ubs.opusid3988de
ubs.publikation.sourceCommunications in mathematical physics 95 (1984), S. 41-51. URL http://projecteuclid.org/euclid.cmp/1103941452de
ubs.publikation.typZeitschriftenartikelde
Enthalten in den Sammlungen:15 Fakultätsübergreifend / Sonstige Einrichtung

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