High precision simulations of weak lensing effect on Cosmic Microwave Background polarization
arXiv:1303.6550 · doi:10.1051/0004-6361/201321575
Abstract
We study accuracy, robustness and self-consistency of pixel-domain simulations of the gravitational lensing effect on the primordial CMB anisotropies due to the large-scale structure of the Universe. In particular, we investigate dependence of the results precision on some crucial parameters of such techniques and propose a semi-analytic framework to determine their values so the required precision is a priori assured and the numerical workload simultaneously optimized. Our focus is on the B-mode signal but we discuss also other CMB observables, such as total intensity, T, and E-mode polarization, emphasizing differences and similarities between all these cases. Our semi-analytic considerations are backed up by extensive numerical results. Those are obtained using a code, nicknamed lenS2HAT -- for Lensing using Scalable Spherical Harmonic Transforms (S2HAT) -- which we have developed in the course of this work. The code implements a version of the pixel-domain approach of Lewis (2005) and permits performing the simulations at very high resolutions and data volumes, thanks to its efficient parallelization provided by the S2HAT library -- a parallel library for a calculation of the spherical harmonic transforms. The code is made publicly available.
20 pages, 14 figures, submitted to A&A, matches version accepted for publication in A&A
References in corpus (11)
- Detection of Gravitational Lensing in the Cosmic Microwave Background
- Correlation of CMB with large-scale structure: II. Weak lensing
- Libsharp - spherical harmonic transforms revisited
- CMB Lensing Constraints on Neutrinos and Dark Energy
- Non-Gaussian structure of the lensed CMB power spectra covariance matrix
- A Large Sky Simulation of the Gravitational Lensing of the Cosmic Microwave Background
- Probing the neutrino mass hierarchy with CMB weak lensing
- Full-sky maps for gravitational lensing of the CMB
- Astrophysical foregrounds and primordial tensor-to-scalar ratio constraints from CMB B-mode polarization observations
- Fast CMB lensing using statistical interpolation on the sphere
- By Dawn's Early Light: CMB Polarization Impact on Cosmological Constraints
Cited by in corpus (18)
- Full covariance of CMB and lensing reconstruction power spectra
- CMB weak-lensing beyond the Born approximation: a numerical approach
- CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
- Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
- The Accuracy of Weak Lensing Simulations
- Internal delensing of Cosmic Microwave Background polarization B-modes with the POLARBEAR experiment
- Impact of Polarized Galactic Foreground Emission on CMB Lensing Reconstruction and Delensing of B-Modes
- Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
- Multiple Lensing of the Cosmic Microwave Background anisotropies
- MillimeterDL: Deep Learning Simulations of the Microwave Sky
- Comparison of delensing methodologies and assessment of the delensing capabilities of future experiments
- CMB lensing reconstruction biases from masking extragalactic sources
- Probing the statistical properties of CMB -mode polarization through Minkowski Functionals
- Planck intermediate results. XLI. A map of lensing-induced B-modes
- Lensing simulations by Taylor expansion -- not so inefficient after all
- Detecting chiral gravity with the pure pseudospectrum reconstruction of the cosmic microwave background polarized anisotropies
- An algorithm for the numerical evaluation of the associated Legendre functions that runs in time independent of degree and order
- Cross-correlation of POLARBEAR CMB Polarization Lensing with High- Sub-mm Herschel-ATLAS galaxies