The effect of reionization on the CMB-density correlation

dc.creatorGiannantonio, Tommaso
dc.creatorCrittenden, Robert
dc.date2007-06-02
dc.date.accessioned2026-07-07T11:41:14Z
dc.date.available2026-07-07T11:41:14Z
dc.descriptionIn this paper we show how the rescattering of CMB photons after cosmic reionization can give a significant linear contribution to the temperature-matter cross-correlation measurements. These anisotropies, which arise via a late time Doppler effect, are on scales much larger than the typical scale of non-linear effects at reionization; they can contribute to degree scale cross-correlations and could affect the interpretation of similar correlations resulting from the integrated Sachs-Wolfe effect. While expected to be small at low redshifts, these correlations can be large given a probe of the density at high redshift, and so could be a useful probe of the cosmic reionization history.
dc.description8 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/0706.0274
dc.identifierhttp://arxiv.org/abs/0706.0274
dc.identifierMon.Not.Roy.Astron.Soc.381:819,2007
dc.identifierdoi:10.1111/j.1365-2966.2007.12282.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200465
dc.subjectAstrophysics
dc.titleThe effect of reionization on the CMB-density correlation
dc.typetext

Files

Collections