Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3627
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSethi, S.K.-
dc.contributor.authorNath, Biman B.-
dc.contributor.authorSubramanian, Kandaswamy-
dc.date.accessioned2008-08-04T10:31:47Z-
dc.date.available2008-08-04T10:31:47Z-
dc.date.issued2008-06-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2008, Vol.387, p1589en
dc.identifier.issnE-ISSN: 1365-2966-
dc.identifier.issnP-ISSN: 0035-8711-
dc.identifier.urihttp://hdl.handle.net/2289/3627-
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractWe study the implications of primordial magnetic fields for the thermal and ionization history of the post-recombination era. In particular, we compute the effects of dissipation of primordial magnetic fields owing to ambipolar diffusion and decaying turbulence in the intergalactic medium (IGM) and the collapsing haloes, and compute the effects of the altered thermal and ionization history on the formation of molecular hydrogen. We show that, for magnetic field strengths in the range 2 × 10-10 <~ B0 <~ 2 × 10-9G, the molecular hydrogen fraction in IGM and collapsing halo can increase by a factor of 5 to 1000 over the case with no magnetic fields. We discuss the implication of the increased molecular hydrogen fraction on the radiative transfer of ultraviolet photons and the formation of first structures in the universe.en
dc.format.extent1160926 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the RASen
dc.relation.urihttp://adsabs.harvard.edu/abs/2008MNRAS.387.1589Sen
dc.relation.urihttp://arxiv.org/abs/0804.3473en
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2008.13302.xen
dc.rights2008 Royal Astronomical Societyen
dc.subjectmagnetic fieldsen
dc.subjectMHDen
dc.subjectmolecular processesen
dc.subjectcosmology: miscellaneousen
dc.titlePrimordial magnetic fields and formation of molecular hydrogenen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2008 MNRAS V387 p1589.pdf
  Restricted Access
Restricted Access1.13 MBAdobe PDFView/Open Request a copy


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