A Method for Calculating Lensing Quantities for CMBR Intensity

Mathematics – Probability

Scientific paper

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Scientific paper

A method is presented for calculating modifications of CMBR intensity characteristics (probability distribution functions and power spectra) caused by gravitational lensing of matter inhomogeneities. In the flat-sky approximation, the method allows to encode the density power spectra into a linear filter expressing the lensing contribution to CMBR signal. Applications to Dark Energy research are discussed.

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