Lensing on Cosmic Microwave Background and its Correlation with Large-Scale Structure Surveys

Details Lensing on Cosmic Microwave Background and its Correlation with Large-Scale Structure Surveys Lensing on Cosmic Microwave Background and its Correlation with Large-Scale Structure Surveys

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iaus..225...87b&link_type=abstract

Gravitational Lensing Impact on Cosmology, IAU Symposium, vol. 225. Edited by Yannick Mellier and Georges Meylan, ISBN 052185196

Computer Science

Scientific paper

Lenses acting on the Cosmic Microwave Background can potentially be a very efficient and robust probe of the large-scale matter distribution in the Universe. Their most immediate signature is the way they affect the statistical properties of both the temperature and the polarization fields, in particular they both induce non-Gaussian properties that can be explicitly computed.

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