The LiteBIRD mission is a JAXA strategic L-class mission for all sky CMB surveys which will be launched in the 2020s. The main target of the mission is the detection of primordial gravitational waves with a sensitivity of the tensor-to-scalar ratio δr<0.001. The polarization modulator unit (PMU) represents a critical and powerful component to suppress 1/f noise contribution and mitigate systematic uncertainties induced by detector gain drift, both for the high-frequency telescope (HFT) and for the mid-frequency telescope (MFT). Each PMU is based on a continuously-rotating transmissive half-wave plate (HWP) held by a superconducting magnetic bearing in a 5K environment. In this contribution we will present the design and expected performance of the LiteBIRD PMUs and testing performed on every PMU subsystem with a room-temperature rotating disk used as a stand-in for the cryogenic HWP rotor.
A polarization modulator unit for the mid- and high-frequency telescopes of the LiteBIRD mission / Columbro, Fabio; de Bernardis, Paolo; Lamagna, Luca; Masi, Silvia; Paiella, Alessandro; Piacentini, Francesco; Pisano, Giampaolo. - 11443:(2020), pp. 114436Z-1-114436Z-16. (Intervento presentato al convegno SPIE Conference Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave tenutosi a Online Only) [10.1117/12.2577818].
A polarization modulator unit for the mid- and high-frequency telescopes of the LiteBIRD mission
Columbro, Fabio
Primo
;de Bernardis, Paolo;Lamagna, Luca;Masi, Silvia;Paiella, Alessandro;Piacentini, Francesco;Pisano, Giampaolo
2020
Abstract
The LiteBIRD mission is a JAXA strategic L-class mission for all sky CMB surveys which will be launched in the 2020s. The main target of the mission is the detection of primordial gravitational waves with a sensitivity of the tensor-to-scalar ratio δr<0.001. The polarization modulator unit (PMU) represents a critical and powerful component to suppress 1/f noise contribution and mitigate systematic uncertainties induced by detector gain drift, both for the high-frequency telescope (HFT) and for the mid-frequency telescope (MFT). Each PMU is based on a continuously-rotating transmissive half-wave plate (HWP) held by a superconducting magnetic bearing in a 5K environment. In this contribution we will present the design and expected performance of the LiteBIRD PMUs and testing performed on every PMU subsystem with a room-temperature rotating disk used as a stand-in for the cryogenic HWP rotor.File | Dimensione | Formato | |
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