Generation of magnetic field in the pre-recombination era

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2222

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DC Field	Value	Language
dc.contributor.author	Gopal, Rajesh	-
dc.contributor.author	Sethi, S.K.	-
dc.date.accessioned	2007-04-03T09:41:10Z	-
dc.date.available	2007-04-03T09:41:10Z	-
dc.date.issued	2005-10	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, 2005, Vol.363, Issue 2, p521-528.	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2289/2222	-
dc.description	Restricted Access. An open access version is available at arXiv.org.(one of the alternative locations)	en
dc.description.abstract	We study the possibility of generating magnetic fields during the evolution of electron, proton and photon plasma in the pre-recombination era. We show that a small magnetic field can be generated in the second order of perturbation theory for scalar modes with adiabatic initial conditions. The amplitude of the field is <~10-30G at the present epoch for scales from sub-kiloparsec to 〉~100Mpc.	en
dc.format.extent	8338 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Blackwell Publishing for the Royal Astronomical Society	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0411170	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005MNRAS.363..521G	en
dc.relation.uri	http://dx.doi.org/10.1111/j.1365-2966.2005.09442.x	en
dc.rights	(2005) Blackwell Publishing for the Royal Astronomical Society	en
dc.title	Generation of magnetic field in the pre-recombination era	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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