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Primordial torsion fields as an explanation of the anisotropy in cosmological electromagnetic propagation

dc.contributor.authorDobado González, Antonio
dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-20T18:50:03Z
dc.date.available2023-06-20T18:50:03Z
dc.date.issued1997-12-14
dc.description© World Scientic Publishing Company. We are grateful to B. Nodland for his comments to the preliminary version of this letter and also to J. P. Ralston for his suggestions. This work has been supported in part by the Ministerio de Educaci_on y Ciencia (Spain) (CICYT AEN96-1634).
dc.description.abstractIn this letter we provide a simple explanation of the recent finding of anisotropy in electromagnetic (EM) propagation claimed by Nodland and Ralston. We consider, as a possible origin of such effect, the effective coupling between EM fields and some tiny background torsion field. The coupling is obtained after integrating out charged fermions, it is gauge-invariant and does not require the introduction of any new physics.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Educación y Ciencia (Spain)
dc.description.sponsorshipCICYT
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22737
dc.identifier.doi10.1142/S0217732397003125
dc.identifier.issn0217-7323
dc.identifier.officialurlhttp://link.springer.com/article/10.1007%2Fs100529800993?LI=true
dc.identifier.relatedurlhttp://link.springer.com
dc.identifier.relatedurlhttp://arxiv.org/abs/hep-ph/9710313
dc.identifier.urihttps://hdl.handle.net/20.500.14352/58728
dc.issue.number38
dc.journal.titleModern Physics Letters A
dc.language.isoeng
dc.page.final3007
dc.page.initial3003
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.projectIDAEN96-1634
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordSpace-Time
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titlePrimordial torsion fields as an explanation of the anisotropy in cosmological electromagnetic propagation
dc.typejournal article
dc.volume.number12
dcterms.references1. B. Nodland and J. P. Ralston, Phys. Rev. Lett. 78, 3043 (1997). 2. D. J. Eisenstein and E. F. Bunn, astro-ph/9704247; S. M. Carroll and G. B. Field, Phys. Rev. Lett. 79, 2394 (1997); J. P. Leahy, astro-ph/9704285; J. F. C. Wardle, R. A. Perley and M. H. Cohen, Phys. Rev. Lett. 79, 1801 (1997); T. J. Loredo, E. E. Flanagan and I. M. Wasserman, astro-ph/9706258. 3. B. Nodland and J. P. Ralston, Phys. Rev. Lett. 79, 1958 (1997); astro-ph/9706126; astro-ph/9708114. 4. D. V. Ahluwalia and T. Goldman, Mod. Phys. Lett. A8, 2623 (1993); R. W. Kuhne, ibid. A12, 2473 (1997). 5. F. W. Hehl, P. von der Heyde, G. D. Kerlick and J. M. Nester, Rev. Mod. Phys. 48, 393 (1976). 6. A. Dobado and A. L. Maroto, Phys. Rev. D54, 5185 (1996). 7. V. De Sabbata and M. Gasperini, Phys. Lett. A83, 115 (1981). 8. S. M. Carroll and G. B. Field, Phys. Rev. D50, 3867 (1994); R. T. Hammond, ibid. D52, 6918 (1995).
dspace.entity.typePublication
relation.isAuthorOfPublication16523fad-99a9-422c-9a8e-c949ccffadec
relation.isAuthorOfPublicatione14691a1-d3b0-47b7-96d5-24d645534471
relation.isAuthorOfPublication.latestForDiscovery16523fad-99a9-422c-9a8e-c949ccffadec

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