Kesden, Michael and Cooray, Asantha and Kamionkowski, Marc (2003) Lensing reconstruction with CMB temperature and polarization. Physical Review D, 67 (12). Art. No. 123507. ISSN 0556-2821 http://resolver.caltech.edu/CaltechAUTHORS:KESprd03
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:KESprd03
Weak gravitational lensing by an intervening large-scale structure induces a distinct signature in the cosmic microwave background (CMB) that can be used to reconstruct the weak-lensing displacement map. Estimators for individual Fourier modes of this map can be combined to produce an estimator for the lensing-potential power spectrum. The naive estimator for this quantity will be biased upwards by the uncertainty associated with reconstructing individual modes; we present an iterative scheme for removing this bias. The variance and covariance of the lensing-potential power spectrum estimator are calculated and evaluated numerically in a LambdaCDM universe for Planck and future polarization-sensitive CMB experiments.
|Additional Information:||©2003 The American Physical Society. Received 25 February 2003; published 11 June 2003. We thank Wayne Hu for useful discussions. This work was supported in part by NASA NAG5-11985 and DOE DEFG03-92-ER40701. M.K. acknowledges the support of the NSF Graduate program and A.C. acknowledges support from the Sherman Fairchild Foundation.|
|Subject Keywords:||radiofrequency cosmic radiation; electromagnetic wave polarisation; iterative methods; gravitational lenses; cosmology; Fourier analysis|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Lindsay Cleary|
|Deposited On:||19 Sep 2006|
|Last Modified:||26 Dec 2012 09:03|
Repository Staff Only: item control page