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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1925

Title: Large-scale magnetic fields: galaxy two-point correlation function
Authors: Sethi, S.K.
Keywords: magnetic fields
MHD
cosmology: theory
large-scale structure of Universe
Issue Date: Jul-2003
Publisher: Blackwell Publishing for the Royal Astronomical Society
Citation: Monthly Notice of the Royal Astronomical Society, 2003, Vol.342, p962-970.
Abstract: We 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.
Description: Restricted Access. An open access version is available at NASA ADS (alternative location).
URI: http://hdl.handle.net/2289/1925
ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?2003MNRAS.342..962S
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003MNRAS.342..962S&link_type=ARTICLE&db_key=AST
Copyright: (2003) Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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