Combining Systematic Effects in CMB Polarization Experiments through map-based simulations: application to LiteBIRD's HWP non-idealities and detectors non-linearity

arXiv:2609.00841 · astro-ph.CO, astro-ph.IM · Submitted 2026-09-01 · Read on arXiv

astro-ph.CO, astro-ph.IM

Submitted: 2026-09-01

Updated: 2026-09-01

Comments: 27 pages, 12 figures

Code: https://github.com/litebird/litebird_sim

License: http://creativecommons.org/licenses/by/4.0/

The gist: We quantify the impact of coupled instrumental systematics on next-generation CMB polarization experiments targeting primordial B-mode polarization, with a focus on the forthcoming LiteBIRD satellite

Terminology

Abstract

We quantify the impact of coupled instrumental systematics on next-generation CMB polarization experiments targeting primordial B-mode polarization, with a focus on the forthcoming LiteBIRD satellite mission. We study the interplay between the non-linear response of Transition-Edge Sensor (TES) bolometers and Half-Wave Plate (HWP) non-idealities, in particular synchronous signals arising from differential emissivity. We develop a map-based formalism that captures the resulting intensity-to-polarization leakage by explicitly solving the binning map-making equations, avoiding the need for computationally expensive time-ordered data simulations. We apply this framework to LiteBIRD, adopting its baseline scanning strategy and frequency configuration, and perform analyses at both single- and multi-frequency levels, including Galactic foregrounds and blind component separation. We find that while detector non-linearity and HWP non-idealities individually induce negligible bias on the tensor-to-scalar ratio r, their coupling can generate non-trivial contamination, driven by large signals such as the solar dipole and amplified in high-frequency channels by foreground leakage. From these results, we derive joint requirements on detector non-linearity and HWP differential emission, and discuss their implications for the instrument design and calibration strategy of LiteBIRD and future CMB polarization missions targeting r 10-3.

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