LiteBIRD: lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection

H. Ishino, Y. Akiba,K. Arnold,D. Barron, J. Borrill, R. Chendra,Y. Chinone,Seongjae Cho,A. Cukierman,T. de Haan,M. Dobbs,A. Dominjon,Tadayasu Dotani,T. Elleflot,J. Errard,T. Fujino, H. Fuke,T. Funaki,Neil Goeckner-Wald,N. W. Halverson,P. Harvey, T. Hasebe,M. Hasegawa,K. Hattori,Makoto Hattori,M. Hazumi, N. Hidehira,Charles Hill, G. C. Hilton,W. L. Holzapfel,Y. Hori,J. Hubmayr,K. Ichiki,Hiroaki Imada, J. Inatani,M. Inoue,Y. Inoue, F. Irie,K. D. Irwin,H. Ishitsuka,O. Jeong,H. Kanai, K. Karatsu, S. Kashima,N. Katayama,Isao Kawano, T. Kawasaki,Brian Keating,S. A. Kernasovskiy, R. Keskitalo,A. Kibayashi,Y. Kida,N. Kimura, Kimihiro Kimura,T. S. Kisner,Kazunori Kohri,Eiichiro Komatsu,K. Komatsu,C. L. Kuo, S. Kuromiya,Akito Kusaka,A. T. Lee,D. Li,Eric V. Linder,M. Maki,Hideo Matsuhara,Tomotake Matsumura, S. Matsuoka,Shuji Matsuura,S. Mima,Y. Minami,K. Mitsuda,Makoto Nagai,T. Nagasaki,R. Nagata,Makoto Nakajima,Shogo Nakamura,T. Namikawa,Masato Naruse,Toshiyuki Nishibori, K. Nishijo,H. Nishino,Atsushi Noda,T. Noguchi,Hideo Ogawa, W. Ogburn,S. Oguri,I. S. Ohta,N. Okada,Atsushi Okamoto,Takahiro Okamura,Chiko Otani,Giampaolo Pisano,Gabriel M. Rebeiz, P. L. Richards,Shin-ichiro Sakai,Yuki Sakurai,Y. Sato,Nobuaki Sato, Y. Segawa,Shigeyuki Sekiguchi,Yutaro Sekimoto, M. Sekine,U. Seljak,Blake D. Sherwin, T. Shimizu,Keisuke Shinozaki,Shibo Shu, R. Stompor,Hajime Sugai,Hiroyuki Sugita,J. Suzuki,T. Suzuki,A. Suzuki,O. Tajima,S. Takada,S. Takakura,Kazufumi Takano,S. Takatori,Yoh Takei, D. Tanabe,Takayuki Tomaru,N. Tomita,Paul Turin, S. Uozumi,Shin Utsunomiya,Y. Uzawa,Takehiko Wada,Hiroki Watanabe, B. Westbrook,Y. Yamada,R. Yamamoto,Noriko Y. Yamasaki,T. Yamashita,T. Yoshida,Mitsuhiro Yoshida,K. Yotsumoto

Proceedings of SPIE(2016)

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摘要
LiteBIRD is a next generation satellite aiming for the detection of the Cosmic Microwave Background (CMB) B-mode polarization imprinted by the primordial gravitational waves generated in the era of the inflationary universe. The science goal of LiteBIRD is to measure the tensor-to-scaler ratio r with a precision of delta r < 10(-3), offering us a crucial test of the major large-single-field slow-roll inflation models. LiteBIRD is planned to conduct an all sky survey at the sun-earth second Lagrange point (L2) with an angular resolution of about 0.5 degrees to cover the multipole moment range of 2 <= l <= 200. We use focal plane detector arrays consisting of 2622 superconducting detectors to measure the frequency range from 40 to 400 GHz with the sensitivity of 2.5 mu K.arcmin. We report an overview and the status of the project, including the ongoing studies.
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关键词
Cosmic Microwave Background,LiteBIRD,B-mode polarization
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