Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1925
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dc.contributor.authorSethi, S.K.-
dc.date.accessioned2007-02-02T11:23:16Z-
dc.date.available2007-02-02T11:23:16Z-
dc.date.issued2003-07-
dc.identifier.citationMonthly Notice of the Royal Astronomical Society, 2003, Vol.342, p962-970.en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/1925-
dc.descriptionRestricted Access. An open access version is available at NASA ADS (alternative location).en
dc.description.abstractWe study the effect of large-scale tangled magnetic fields on the galaxy two-point correlation function in the redshift space. We show that (i) the magnetic field effects can be comparable to the gravity-induced clustering for present magnetic field strength B0~= 5 × 10-8 G, (ii) the absence of this signal from the present data gives an upper bound B0<~ 3 × 10-8 G and (iii) the future data can probe the magnetic fields of ~=10-8 G. A comparison with other constraints on the present magnetic field shows that they are marginally compatible. However, if the magnetic fields corresponding to B0~= 10-8 G existed at the last scattering surface, they will cause unacceptably large cosmic microwave background radiation anisotropies.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2003MNRAS.342..962Sen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003MNRAS.342..962S&link_type=ARTICLE&db_key=ASTen
dc.rights(2003) Royal Astronomical Societyen
dc.subjectmagnetic fieldsen
dc.subjectMHDen
dc.subjectcosmology: theoryen
dc.subjectlarge-scale structure of Universeen
dc.titleLarge-scale magnetic fields: galaxy two-point correlation functionen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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