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dc.contributor.authorBabich, Daniel
dc.contributor.authorLoeb, Abraham
dc.date.accessioned2019-09-24T12:04:57Z
dc.date.issued2005
dc.identifier.citationBabich, Daniel, and Abraham Loeb. 2005. “Polarization of 21 Cm Radiation from the Epoch of Reionization.” The Astrophysical Journal 635 (1): 1–10. https://doi.org/10.1086/497297.
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41393441*
dc.description.abstractWe consider the polarization of 21 cm line radiation from the epoch of reionization due to both intrinsically polarized emission and secondary mechanisms. We argue that Thomson scattering of the 21 cm quadrupole by the reionized universe is likely to produce the largest effect. The 21 cm quadrupole is sourced by baryonic density fluctuations and the fluctuations in the ionization fraction due to discrete H II regions. Since Thomson scattering produces only E-type polarization and is achromatic, its unique fingerprint could in principle be separated from foregrounds associated with polarized synchrotron emission, which should not be correlated with the cosmic signal. We estimate that Poisson fluctuations of H II regions at the end of reionization (z(R) similar to 6-20) produce a brightness temperature-polarization cross-correlation signal of similar to 0.1-0.3 mK on angular scales of tens of arcminutes. This cross-correlation signal is within the instrument sensitivities of the future Square Kilometre Array (SKA) and close to the sensitivities of the forthcoming Mileura Widefield Array (MWA) and Low Frequency Array (LOFAR).
dc.language.isoen_US
dc.publisherAmerican Astronomical Society
dash.licenseLAA
dc.titlePolarization of 21 cm Radiation from the Epoch of Reionization
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalThe Astrophysical Journal
dash.depositing.authorLoeb, Abraham::9975df1f269ab49c1ad5a328a1ec1476::600
dc.date.available2019-09-24T12:04:57Z
dash.workflow.comments1Science Serial ID 97076
dc.identifier.doi10.1086/497297
dash.source.volume635;1
dash.source.page1-10


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