Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD

Yuki Sakurai; Tomotake Matsumura; Nobuhiko Katayama; Hiroaki Imada; Kunimoto Komatsu; Hiroaki Kanai; Ryota Takaku; Shinya Sugiyama; Tommaso Ghigna; Teruhito Iida; Hajime Sugai; Hiroyuki Ohsaki; Yutaka Terao; Toshiki Shimomura; Kuniaki Konishi; Haruyuki Sakurai; Junji Yumoyo; Muneyoshi Maki; Junichi Suzuki; Hirokazu Ishino; Shogo Nakamura; Akito Kusaka; Charles Hill; Masashi Hazumi; Hirokazu Kataza; Shin Utsunomiya; Ryo Yamamoto; Makoto Tashiro; Yukikatsu Terada

doi:10.1117/12.2312391

Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD

Yuki Sakurai, Tomotake Matsumura, Nobuhiko Katayama, Hiroaki Imada, Kunimoto Komatsu, Hiroaki Kanai, Ryota Takaku, Shinya Sugiyama, Tommaso Ghigna, Teruhito Iida, Hajime Sugai, Hiroyuki Ohsaki, Yutaka Terao, Toshiki Shimomura, Kuniaki Konishi, Haruyuki Sakurai, Junji Yumoyo, Muneyoshi Maki, Junichi Suzuki, Hirokazu IshinoShogo Nakamura, Akito Kusaka, Charles Hill, Masashi Hazumi, Hirokazu Kataza, Shin Utsunomiya, Ryo Yamamoto, Makoto Tashiro, Yukikatsu Terada

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Citations (Scopus)

Abstract

We present our design and development of a polarization modulator unit (PMU) for LiteBIRD space mission. LiteBIRD is a next generation cosmic microwave background (CMB) polarization satellite to measure the primordial B-mode. The science goal of LiteBIRD is to measure the tensor-to-scalar ratio with the sensitivity of δr < 10^-3. The baseline design of LiteBIRD is to employ the PMU based on a continuous rotating half-wave plate (HWP) at a telescope aperture with a diameter of 400 mm. It is an essential for LiteBIRD to achieve the science goal because it significantly reduces detector noise and systematic uncertainties. The LiteBIRD PMU consists of a multi-layered sapphire as a broadband achromatic HWP and a mechanism to continuously rotate it at 88 rpm. The whole system is maintained at below 10K to minimize the thermal emission from the HWP. In this paper, we discuss the current development status of the broadband achromatic HWP and the cryogenic rotation mechanism.

Original language	English
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Print)	9781510619692
DOIs	https://doi.org/10.1117/12.2312391
Publication status	Published - 2018
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 - Austin, United States Duration: Jun 12 2018 → Jun 15 2018

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10708
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018
Country/Territory	United States
City	Austin
Period	6/12/18 → 6/15/18

Keywords

Cosmic microwave background
LiteBIRD
broadband achromatic half-wave plate
cryogenic rotation mechanism
inflation
millimeter-wave polarization
polarization modulator
space program

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2312391

Cite this

Sakurai, Y., Matsumura, T., Katayama, N., Imada, H., Komatsu, K., Kanai, H., Takaku, R., Sugiyama, S., Ghigna, T., Iida, T., Sugai, H., Ohsaki, H., Terao, Y., Shimomura, T., Konishi, K., Sakurai, H., Yumoyo, J., Maki, M., Suzuki, J., ... Terada, Y. (2018). Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD. In J. Zmuidzinas, & J-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX [107080E] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708). SPIE. https://doi.org/10.1117/12.2312391

Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD. / Sakurai, Yuki; Matsumura, Tomotake; Katayama, Nobuhiko; Imada, Hiroaki; Komatsu, Kunimoto; Kanai, Hiroaki; Takaku, Ryota; Sugiyama, Shinya; Ghigna, Tommaso; Iida, Teruhito; Sugai, Hajime; Ohsaki, Hiroyuki; Terao, Yutaka; Shimomura, Toshiki; Konishi, Kuniaki; Sakurai, Haruyuki; Yumoyo, Junji; Maki, Muneyoshi; Suzuki, Junichi; Ishino, Hirokazu; Nakamura, Shogo; Kusaka, Akito; Hill, Charles; Hazumi, Masashi; Kataza, Hirokazu; Utsunomiya, Shin; Yamamoto, Ryo; Tashiro, Makoto; Terada, Yukikatsu.

Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2018. 107080E (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10708).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Sakurai, Y, Matsumura, T, Katayama, N, Imada, H, Komatsu, K, Kanai, H, Takaku, R, Sugiyama, S, Ghigna, T, Iida, T, Sugai, H, Ohsaki, H, Terao, Y, Shimomura, T, Konishi, K, Sakurai, H, Yumoyo, J, Maki, M, Suzuki, J, Ishino, H, Nakamura, S, Kusaka, A, Hill, C, Hazumi, M, Kataza, H, Utsunomiya, S, Yamamoto, R, Tashiro, M & Terada, Y 2018, Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX., 107080E, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10708, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018, Austin, United States, 6/12/18. https://doi.org/10.1117/12.2312391

Sakurai Y, Matsumura T, Katayama N, Imada H, Komatsu K, Kanai H et al. Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD. In Zmuidzinas J, Gao J-R, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. SPIE. 2018. 107080E. (Proceedings of SPIE - The International Society for Optical Engineering). https://doi.org/10.1117/12.2312391

Sakurai, Yuki ; Matsumura, Tomotake ; Katayama, Nobuhiko ; Imada, Hiroaki ; Komatsu, Kunimoto ; Kanai, Hiroaki ; Takaku, Ryota ; Sugiyama, Shinya ; Ghigna, Tommaso ; Iida, Teruhito ; Sugai, Hajime ; Ohsaki, Hiroyuki ; Terao, Yutaka ; Shimomura, Toshiki ; Konishi, Kuniaki ; Sakurai, Haruyuki ; Yumoyo, Junji ; Maki, Muneyoshi ; Suzuki, Junichi ; Ishino, Hirokazu ; Nakamura, Shogo ; Kusaka, Akito ; Hill, Charles ; Hazumi, Masashi ; Kataza, Hirokazu ; Utsunomiya, Shin ; Yamamoto, Ryo ; Tashiro, Makoto ; Terada, Yukikatsu. / Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD. Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX. editor / Jonas Zmuidzinas ; Jian-Rong Gao. SPIE, 2018. (Proceedings of SPIE - The International Society for Optical Engineering).

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title = "Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD",

abstract = "We present our design and development of a polarization modulator unit (PMU) for LiteBIRD space mission. LiteBIRD is a next generation cosmic microwave background (CMB) polarization satellite to measure the primordial B-mode. The science goal of LiteBIRD is to measure the tensor-to-scalar ratio with the sensitivity of δr < 10-3. The baseline design of LiteBIRD is to employ the PMU based on a continuous rotating half-wave plate (HWP) at a telescope aperture with a diameter of 400 mm. It is an essential for LiteBIRD to achieve the science goal because it significantly reduces detector noise and systematic uncertainties. The LiteBIRD PMU consists of a multi-layered sapphire as a broadband achromatic HWP and a mechanism to continuously rotate it at 88 rpm. The whole system is maintained at below 10K to minimize the thermal emission from the HWP. In this paper, we discuss the current development status of the broadband achromatic HWP and the cryogenic rotation mechanism.",

keywords = "Cosmic microwave background, LiteBIRD, broadband achromatic half-wave plate, cryogenic rotation mechanism, inflation, millimeter-wave polarization, polarization modulator, space program",

author = "Yuki Sakurai and Tomotake Matsumura and Nobuhiko Katayama and Hiroaki Imada and Kunimoto Komatsu and Hiroaki Kanai and Ryota Takaku and Shinya Sugiyama and Tommaso Ghigna and Teruhito Iida and Hajime Sugai and Hiroyuki Ohsaki and Yutaka Terao and Toshiki Shimomura and Kuniaki Konishi and Haruyuki Sakurai and Junji Yumoyo and Muneyoshi Maki and Junichi Suzuki and Hirokazu Ishino and Shogo Nakamura and Akito Kusaka and Charles Hill and Masashi Hazumi and Hirokazu Kataza and Shin Utsunomiya and Ryo Yamamoto and Makoto Tashiro and Yukikatsu Terada",

note = "Funding Information: This work was supported by MEXT KAKENHI Grant Numbers JP17H01125, JP17K14272, JP15H05441. This work was also supported by JSPS Core-to-Core Program, A. Advanced Research Networks and World Premier International Research Center Initiative (WPI), MEXT, Japan. Publisher Copyright: {\textcopyright} 2018 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018 ; Conference date: 12-06-2018 Through 15-06-2018",

year = "2018",

doi = "10.1117/12.2312391",

language = "English",

isbn = "9781510619692",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao",

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AU - Sakurai, Yuki

AU - Matsumura, Tomotake

AU - Katayama, Nobuhiko

AU - Imada, Hiroaki

AU - Komatsu, Kunimoto

AU - Kanai, Hiroaki

AU - Takaku, Ryota

AU - Sugiyama, Shinya

AU - Ghigna, Tommaso

AU - Iida, Teruhito

AU - Sugai, Hajime

AU - Ohsaki, Hiroyuki

AU - Terao, Yutaka

AU - Shimomura, Toshiki

AU - Konishi, Kuniaki

AU - Sakurai, Haruyuki

AU - Yumoyo, Junji

AU - Maki, Muneyoshi

AU - Suzuki, Junichi

AU - Ishino, Hirokazu

AU - Nakamura, Shogo

AU - Kusaka, Akito

AU - Hill, Charles

AU - Hazumi, Masashi

AU - Kataza, Hirokazu

AU - Utsunomiya, Shin

AU - Yamamoto, Ryo

AU - Tashiro, Makoto

AU - Terada, Yukikatsu

N1 - Funding Information: This work was supported by MEXT KAKENHI Grant Numbers JP17H01125, JP17K14272, JP15H05441. This work was also supported by JSPS Core-to-Core Program, A. Advanced Research Networks and World Premier International Research Center Initiative (WPI), MEXT, Japan. Publisher Copyright: © 2018 SPIE.

PY - 2018

Y1 - 2018

N2 - We present our design and development of a polarization modulator unit (PMU) for LiteBIRD space mission. LiteBIRD is a next generation cosmic microwave background (CMB) polarization satellite to measure the primordial B-mode. The science goal of LiteBIRD is to measure the tensor-to-scalar ratio with the sensitivity of δr < 10-3. The baseline design of LiteBIRD is to employ the PMU based on a continuous rotating half-wave plate (HWP) at a telescope aperture with a diameter of 400 mm. It is an essential for LiteBIRD to achieve the science goal because it significantly reduces detector noise and systematic uncertainties. The LiteBIRD PMU consists of a multi-layered sapphire as a broadband achromatic HWP and a mechanism to continuously rotate it at 88 rpm. The whole system is maintained at below 10K to minimize the thermal emission from the HWP. In this paper, we discuss the current development status of the broadband achromatic HWP and the cryogenic rotation mechanism.

AB - We present our design and development of a polarization modulator unit (PMU) for LiteBIRD space mission. LiteBIRD is a next generation cosmic microwave background (CMB) polarization satellite to measure the primordial B-mode. The science goal of LiteBIRD is to measure the tensor-to-scalar ratio with the sensitivity of δr < 10-3. The baseline design of LiteBIRD is to employ the PMU based on a continuous rotating half-wave plate (HWP) at a telescope aperture with a diameter of 400 mm. It is an essential for LiteBIRD to achieve the science goal because it significantly reduces detector noise and systematic uncertainties. The LiteBIRD PMU consists of a multi-layered sapphire as a broadband achromatic HWP and a mechanism to continuously rotate it at 88 rpm. The whole system is maintained at below 10K to minimize the thermal emission from the HWP. In this paper, we discuss the current development status of the broadband achromatic HWP and the cryogenic rotation mechanism.

KW - Cosmic microwave background

KW - LiteBIRD

KW - broadband achromatic half-wave plate

KW - cryogenic rotation mechanism

KW - inflation

KW - millimeter-wave polarization

KW - polarization modulator

KW - space program

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DO - 10.1117/12.2312391

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AN - SCOPUS:85052001485

SN - 9781510619692

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX 2018

Y2 - 12 June 2018 through 15 June 2018

ER -

Design and development of a polarization modulator unit based on a continuous rotating half-wave plate for LiteBIRD

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