Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4024
Full metadata record
DC FieldValueLanguage
dc.contributor.authorKahniashvili, Tina-
dc.contributor.authorTevzadze, Alexander G.-
dc.contributor.authorSethi, S.K.-
dc.contributor.authorPandey, Kanhaiya L.-
dc.contributor.authorRatra, Bharat-
dc.date.accessioned2011-04-08T07:49:57Z-
dc.date.available2011-04-08T07:49:57Z-
dc.date.issued2010-10-15-
dc.identifier.citationPhysical Review D, 2010, Vol.82, p83005en
dc.identifier.issn1550-2368 (Online)-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2289/4024-
dc.descriptionOpen Accessen
dc.description.abstractWe study limits on a primordial magnetic field arising from cosmological data, including that from big bang nucleosynthesis, cosmic microwave background polarization plane Faraday rotation limits, and large-scale structure formation. We show that the physically relevant quantity is the value of the effective magnetic field, and limits on it are independent of how the magnetic field was generated.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/2010PhRvD..82h3005Ken
dc.relation.urihttp://arxiv.org/abs/1009.2094en
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.82.083005en
dc.rights2010 The American Physical Societyen
dc.titlePrimordial magnetic field limits from cosmological dataen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2010_PRD_82_083005.pdfOpen Access.384.02 kBAdobe PDFView/Open


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.