Weak Lensing of the Primary CMB Bispectrum
Asantha Cooray (1), Devdeep Sarkar (1), Paolo Serra (1) ((1) UC, Irvine)

TL;DR
Weak gravitational lensing modifies the CMB bispectrum by smoothing and reducing its amplitude, significantly impacting the estimation of primordial non-Gaussianity parameters like f_NL in current and future experiments.
Contribution
This paper quantifies the lensing effect on the CMB bispectrum and highlights its importance for accurate non-Gaussianity measurements, which was not fully accounted for previously.
Findings
Lensing decreases the bispectrum amplitude by smoothing between multipoles 100 and 2000.
Neglecting lensing biases the f_NL estimate low by about 6% for WMAP.
For Planck, lensing increases the minimum detectable f_NL from 5 to 7.
Abstract
The cosmic microwave background (CMB) bispectrum is a well-known probe of the non-Gaussianity of primordial perturbations. Just as the intervening large-scale structure modifies the CMB angular power spectrum through weak gravitational lensing, the CMB primary bispectrum generated at the last scattering surface is also modified by lensing. We discuss the lensing modification to the CMB bispectrum and show that lensing leads to an overall decrease in the amplitude of the primary bispectrum at multipoles of interest between 100 and 2000 through additional smoothing introduced by lensing. Since weak lensing is not accounted for in current estimators of the primordial non-Gaussianity parameter, the existing measurements of of the local model with WMAP out to is biased low by about 6%. For a high resolution experiment such as Planck, the lensing…
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