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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2786
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dc.contributor.authorSivaram, C-
dc.contributor.authorde Andrade, L. C. G-
dc.date.accessioned2008-07-22T05:01:18Z-
dc.date.available2008-07-22T05:01:18Z-
dc.date.issued1993-02-
dc.identifier.citationAstrophysics and Space Science, Vol. 201, No. 1, pp. 121 - 123en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2786-
dc.description.abstractGeneral relativistic electrodynamics in a torsion background can give rise to a situation where the photons can have a non-zero rest mass and magnetic moment. Astrophysical limits are used to constrain these parameters.en
dc.format.extent216966 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993Ap%26SS.201..121Sen
dc.subjectElectrodynamicsen
dc.subjectElementary particle interactionsen
dc.subjectGauge invarianceen
dc.subjectRelativityen
dc.subjectStellar magnetospheresen
dc.subjectPhoton densityen
dc.subjectTorsionen
dc.titleAstrophysical limits on gauge invariance breaking in electrodynamics with torsionen
dc.typeArticleen
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