4.6 Article

QUBIC VI: Cryogenic half wave plate rotator, design and performance

出版社

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2022/04/039

关键词

CMBR detectors; CMBR experiments; CMBR polarisation; gravitational waves and CMBR polarization

资金

  1. France: ANR (Agence Nationale de la Recherche)
  2. France: DIM-ACAV (Domaine d'Interet Majeur-Astronomie et Conditions d'Apparition de la Vie)
  3. France: CNRS/IN2P3 (Centre national de la recherche scientifique/Institut national de physique nucleaire et de physique des particules)
  4. France: CNRS/INSU (Centre national de la recherche scientifique/Institut national 8 Battistelli et al. de sciences de l'univers)
  5. Italy: CNR/PNRA (Consiglio Nazionale delle Ricerche/Programma Nazionale Ricerche in Antartide)
  6. Italy: INFN (Istituto Nazionale di Fisica Nucleare)
  7. Argentina: MINCyT (Ministerio de Ciencia, Tecnologia e Innovacion)
  8. Argentina: CNEA (Comision Nacional de Energia Atomica)
  9. Argentina: CONICET (Consejo Nacional de Investigaciones Cientificas y Tecnicas)
  10. Irish Research Council under the Government of Ireland Postgraduate Scholarship Scheme
  11. National University of Ireland, Maynooth
  12. Science Foundation Ireland

向作者/读者索取更多资源

This paper presents the design and testing results of a crucial optical element, half-wave plate (HWP), for the QUBIC experiment. The rotating precision of the QUBIC HWP reaches 0.15 degrees using a stepper motor and custom-made optical encoder, without causing any thermal issues during measurements. Finite element thermal simulations estimate a maximum temperature gradient within the HWP of <= 10 mK. Polarization modulation measurements at 150 GHz demonstrate a polarization efficiency of over 99%.
Setting an upper limit or detection of B-mode polarization imprinted by gravitational waves from Inflation is one goal of modern large angular scale cosmic microwave background (CMB) experiments around the world. A great effort is being made in the deployment of many ground-based, balloon-borne and satellite experiments, using different methods to separate this faint polarized component from the incoming radiation. QUBIC exploits one of the most widely-used techniques to extract the input Stokes parameters, consisting in a rotating half-wave plate (HWP) and a linear polarizer to separate and modulate polarization components. QUBIC uses a step-by-step rotating HWP, with 15 degrees steps, combined with a 0.4 degrees s(-1) azimuth sky scan speed. The rotation is driven by a stepper motor mounted on the cryostat outer shell to avoid heat load at internal cryogenic stages. The design of this optical element is an engineering challenge due to its large 370 mm diameter and the 8K operation temperature that are unique features of the QUBIC experiment. We present the design for a modulator mechanism for up to 370 mm, and the first optical tests by using the prototype of QUBIC HWP (180 mm diameter). The tests and results presented in this work show that the QUBIC HWP rotator can achieve a precision of 0.15 degrees in position by using the stepper motor and custom-made optical encoder. The rotation induces < 5.0 mW (95% C.L) of power load on the 4K stage, resulting in no thermal issues on this stage during measurements. We measure a temperature settle-down characteristic time of 28 s after a rotation through a 15 degrees step, compatible with the scanning strategy, and we estimate a maximum temperature gradient within the HWP of <= 10 mK. This was calculated by setting up finite element thermal simulations that include the temperature profiles measured during the rotator operations. We report polarization modulation measurements performed at 150 GHz, showing a polarization efficiency > 99% (68% C.L.) and a median cross-polarization chi(Pol) of 0.12%, with 71% of detectors showinga chi(Pol )+ 2 sigma upper limit < 1%, measured using selected detectors that had the best signal-to-noise ratio.

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