Detailed study of HWP non-idealities and their impact on future measurements of CMB polarization anisotropies from space
Serena Giardiello, Martina Gerbino, Luca Pagano, Josquin Errard,, Alessandro Gruppuso, Hirokazu Ishino, Massimiliano Lattanzi, Paolo Natoli,, Guillaume Patanchon, Francesco Piacentini, Giampaolo Pisano

TL;DR
This paper investigates how non-idealities in the half-wave plate of future CMB space missions affect the measurement of B-mode polarization, providing simulation-based analysis and accuracy requirements to mitigate biases in tensor-to-scalar ratio estimates.
Contribution
It introduces a comprehensive simulation pipeline to quantify HWP non-idealities' impact on CMB B-mode measurements and establishes precision requirements for HWP property measurements.
Findings
Quantified systematic bias on r due to HWP non-idealities.
Derived accuracy requirements for HWP properties to keep bias below 10^{-5}.
Analyzed effects of frequency-dependent HWP properties and foregrounds.
Abstract
We study the propagation of a specific class of instrumental systematics to the reconstruction of the B-mode power spectrum of the cosmic microwave background (CMB). We focus on the non-idealities of the half-wave plate (HWP), a polarization modulator that is to be deployed by future CMB experiments, such as the phase-A satellite mission LiteBIRD. We study the effects of non-ideal HWP properties, such as transmittance, phase shift, and cross-polarization. To this end, we developed a simple, yet stand-alone end-to-end simulation pipeline adapted to LiteBIRD. We analyzed the effects of a possible mismatch between the measured frequency profiles of HWP properties (used in the mapmaking stage of the pipeline) and the actual profiles (used in the sky-scanning step). We simulated single-frequency, CMB-only observations to emphasize the effects of non-idealities on the BB power spectrum. We…
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Taxonomy
TopicsCosmology and Gravitation Theories · Radio Astronomy Observations and Technology · Electrical and Electromagnetic Research
