Hide metadata

Cosmic magnetization in three-form inflation

dc.date.accessioned2017-08-15T13:11:37Z
dc.date.available2017-08-15T13:11:37Z
dc.date.created2012-06-05T14:01:46Z
dc.date.issued2012
dc.identifier.citationKoivisto, Tomi Sebastian Urban, Federico . Cosmic magnetization in three-form inflation. Physical Review D. Particles and fields. 2012, 85(8)
dc.identifier.urihttp://hdl.handle.net/10852/57051
dc.description.abstractA completely new mechanism to generate the observed amount of large-scale cosmological magnetic fields is introduced in the context of three-form inflation. The amplification of the fields occurs via fourth order dynamics of the vector perturbations and avoids the backreaction problem that plagues most previously introduced mechanisms. © 2012 American Physical Societyen_US
dc.languageEN
dc.publisherAmerican Physical Society
dc.titleCosmic magnetization in three-form inflationen_US
dc.typeJournal articleen_US
dc.creator.authorKoivisto, Tomi Sebastian
dc.creator.authorUrban, Federico
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin927973
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review D. Particles and fields&rft.volume=85&rft.spage=&rft.date=2012
dc.identifier.jtitlePhysical Review D. Particles and fields
dc.identifier.volume85
dc.identifier.issue8
dc.identifier.pagecount6
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevD.85.083508
dc.identifier.urnURN:NBN:no-59790
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2821
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/57051/2/PhysRevD.85.083508.pdf
dc.type.versionPublishedVersion


Files in this item

Name:
PhysRevD.85.083508.pdf
Size:
238.8Kb
Format:
application/
View/Open

Appears in the following Collection

Hide metadata