Systematic effect induced by misalignment in a Reflective Polarization Modulator for CMB, and application to the LiteBIRD case
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866912874187718656 |
|---|---|
| author | Stellati, S. Piacentini, F. Micheli, S. Novelli, A. Columbro, F. Coppolecchia, A. de Bernardis, P. Masi, S. Najafi, M. Occhiuzzi, A. Pagano, L. Paiella, A. Collaboration, LiteBIRD |
| author_facet | Stellati, S. Piacentini, F. Micheli, S. Novelli, A. Columbro, F. Coppolecchia, A. de Bernardis, P. Masi, S. Najafi, M. Occhiuzzi, A. Pagano, L. Paiella, A. Collaboration, LiteBIRD |
| contents | [Abridged] The LiteBIRD mission aims to measure the Cosmic Microwave Background (CMB) polarization with unprecedented precision, targeting the detection of primordial B modes and a precise determination of the tensor-to-scalar ratio r. A central component of LiteBIRD are the polarization modulators based on Half-Wave Plates (HWP). In this work, we investigate systematic effects caused by a small, constant misalignment between the reflective HWP's rotation axis and optical axis, which mimics a wedge-like effect. This effect can introduce HWP-synchronous pointing errors, biasing polarization measurements and generating spurious B modes. Using the LiteBIRD simulation framework, we implement this wedge-like misalignment in time-ordered data and evaluate its impact on reconstructed maps and angular power spectra. Our results show that the contamination predominantly mimics lensing B modes rather than primordial tensor modes, and its impact is reduced when increasing the number of detectors. By estimating the resulting error on the tensor-to-scalar ratio, we set constraints on the maximum allowable wedge angle to ensure systematic effects remain below mission requirements. This study emphasizes the critical importance of precise optical alignment in CMB polarization experiments. Future work will address the additional effects of time-dependent HWP wobbling and more realistic scenarios with non-ideal detector pairs. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_03564 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Systematic effect induced by misalignment in a Reflective Polarization Modulator for CMB, and application to the LiteBIRD case Stellati, S. Piacentini, F. Micheli, S. Novelli, A. Columbro, F. Coppolecchia, A. de Bernardis, P. Masi, S. Najafi, M. Occhiuzzi, A. Pagano, L. Paiella, A. Collaboration, LiteBIRD Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics [Abridged] The LiteBIRD mission aims to measure the Cosmic Microwave Background (CMB) polarization with unprecedented precision, targeting the detection of primordial B modes and a precise determination of the tensor-to-scalar ratio r. A central component of LiteBIRD are the polarization modulators based on Half-Wave Plates (HWP). In this work, we investigate systematic effects caused by a small, constant misalignment between the reflective HWP's rotation axis and optical axis, which mimics a wedge-like effect. This effect can introduce HWP-synchronous pointing errors, biasing polarization measurements and generating spurious B modes. Using the LiteBIRD simulation framework, we implement this wedge-like misalignment in time-ordered data and evaluate its impact on reconstructed maps and angular power spectra. Our results show that the contamination predominantly mimics lensing B modes rather than primordial tensor modes, and its impact is reduced when increasing the number of detectors. By estimating the resulting error on the tensor-to-scalar ratio, we set constraints on the maximum allowable wedge angle to ensure systematic effects remain below mission requirements. This study emphasizes the critical importance of precise optical alignment in CMB polarization experiments. Future work will address the additional effects of time-dependent HWP wobbling and more realistic scenarios with non-ideal detector pairs. |
| title | Systematic effect induced by misalignment in a Reflective Polarization Modulator for CMB, and application to the LiteBIRD case |
| topic | Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2509.03564 |