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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2589
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dc.contributor.authorde Andrade, L. C. G-
dc.contributor.authorSivaram, C-
dc.date.accessioned2008-07-09T07:47:33Z-
dc.date.available2008-07-09T07:47:33Z-
dc.date.issued1993-
dc.identifier.citationAstrophysics and Space Science , Vol. 209, No. 1, pp. 109 - 111en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2589-
dc.description.abstractA recent model of torsion-modified electrodynamics which breaks the electromagnetic conformal invariance is shown to lead to the generation of magnetic fields in the Early Universe.en
dc.format.extent208908 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1993Ap%26SS.209..109Den
dc.subjectAstronomical modelsen
dc.subjectElectrodynamicsen
dc.subjectInterstellar magnetic fieldsen
dc.subjectTorsionen
dc.subjectUniverseen
dc.subjectCosmologyen
dc.subjectElectric currenten
dc.subjectElectromagnetic fieldsen
dc.subjectInvarianceen
dc.subjectMathematical modelsen
dc.subjectPhotonsen
dc.subjectProtonsen
dc.titleTorsion, massive electrodynamics and primordial magnetic fields in the Early Universeen
dc.typeArticleen
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