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dc.creatorMortonson, Michael J.
dc.creatorHu, Wayne
dc.date.accessioned2011-02-24T16:30:11Z
dc.date.available2011-02-24T16:30:11Z
dc.date.issued2010-03-26
dc.identifier.citationMichael J. Mortonson, Wayne Hu, "Observational limits on patchy reionization: Implications for B modes," Physical Review D 81, no. 6 (2010), doi:10.1103/PhysRevD.81.067302en_US
dc.identifier.issn1550-2368
dc.identifier.urihttp://hdl.handle.net/1811/48057
dc.description.abstractThe recent detection of secondary CMB anisotropy by the South Pole Telescope limits temperature fluctuations from the optical depth-modulated Doppler effect to T_3000 < √13μK at multipoles ℓ ∼ 3000. This bound is the first empirical constraint on optical depth fluctuations at arcminute scales, τ_3000=0.001T_3000/μK, implying that these fluctuations are no more than a few percent of the mean. Modulation of the quadrupole source to polarization generates B modes that are bounded as B_3000 = 0.003T_3000. The maximal extrapolation to the ℓ ∼ 100 gravitational wave regime yields B_100 = 0.1T_3000 and remains in excess of gravitational lensing if the comoving size of ionized regions is R ≳ 80 Mpc. If patchy reionization produces much of the observed arcminute scale temperature fluctuations, current bounds on B_100 already require R ≲ 200 Mpc, and limits on both T_3000 and B_100 can be expected to improve rapidly.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Physical Societyen_US
dc.rights©2010 The American Physical Societyen_US
dc.titleObservational limits on patchy reionization: Implications for B modesen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.81.067302
dc.identifier.osuauthormortonson.1


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