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作者单位:T. Matsumura (1) Y. Akiba (2) J. Borrill (3) Y. Chinone (1) M. Dobbs (4) H. Fuke (5) A. Ghribi (6) M. Hasegawa (1) K. Hattori (1) M. Hattori (7) M. Hazumi (1) W. Holzapfel (6) Y. Inoue (2) K. Ishidoshiro (7) H. Ishino (8) H. Ishitsuka (2) K. Karatsu (9) N. Katayama (10) I. Kawano (5) A. Kibayashi (8) Y. Kibe (8) K. Kimura (1) N. Kimura (1) K. Koga (11) M. Kozu (16) E. Komatsu (12) A. Lee (6) H. Matsuhara (5) S. Mima (11) K. Mitsuda (5) K. Mizukami (13) H. Morii (1) T. Morishima (7) S. Murayama (13) M. Nagai (14) R. Nagata (1) S. Nakamura (13) M. Naruse (15) K. Natsume (13) T. Nishibori (5) H. Nishino (10) A. Noda (5) T. Noguchi (9) H. Ogawa (16) S. Oguri (1) I. Ohta (17) C. Otani (11) P. Richards (6) S. Sakai (5) N. Sato (1) Y. Sato (5) Y. Sekimoto (9) A. Shimizu (2) K. Shinozaki (5) H. Sugita (5) T. Suzuki (1) A. Suzuki (6) O. Tajima (1) S. Takada (14) S. Takakura (18) Y. Takei (5) T. Tomaru (1) Y. Uzawa (9) T. Wada (5) H. Watanabe (2) M. Yoshida (1) N. Yamasaki (5) T. Yoshida (5) K. Yotsumoto (5)
1. High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan 2. The Graduate University for Advanced Studies (SOKENDAI), Hayama, Kanagawa, Japan 3. Lawrence Berkeley National Laboratory, Berkeley, CA, ?94720, USA 4. McGill University, Montreal, QC, Canada 5. Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, Japan 6. Physics, University of California, Berkeley, Berkeley, CA, ?94720, USA 7. Tohoku University, Sendai, Miyagi, Japan 8. Okayama University, Okayama, Okayama, Japan 9. National Astronomical Observatory of Japan (NAOJ), Mitaka, Tokyo, Japan 10. Kavli Institute for The Physics and Mathematics of The Universe (IPMU), The University of Tokyo, Kashiwa, Chiba, Japan 11. Terahertz-wave Research Group, RIKEN, Sendai, Miyagi, Japan 16. Osaka Prefecture University, Osaka, Japan 12. Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild Str. 1, 85741?, Garching, Germany 13. Yokohama National University, Yokohama, Kanagawa, Japan 14. University of Tsukuba, Tsukuba, Ibaraki, Japan 15. Saitama University, Saitama, Japan 17. Kinki University, Higashiosaka, Osaka, Japan 18. University of Osaka, Osaka, Japan
ISSN:1573-7357
文摘
LiteBIRD is a next-generation satellite mission to measure the polarization of the cosmic microwave background (CMB) radiation. On large angular scales the B-mode polarization of the CMB carries the imprint of primordial gravitational waves, and its precise measurement would provide a powerful probe of the epoch of inflation. The goal of LiteBIRD is to achieve a measurement of the characterizing tensor to scalar ratio \(r\) to an uncertainty of \(\delta r=0.001\) . In order to achieve this goal we will employ a kilo-pixel superconducting detector array on a cryogenically cooled sub-Kelvin focal plane with an optical system at a temperature of 4?K. We are currently considering two detector array options; transition edge sensor (TES) bolometers and microwave kinetic inductance detectors. In this paper we give an overview of LiteBIRD and describe a TES-based polarimeter designed to achieve the target sensitivity of 2? \(\upmu \) K?arcmin over the frequency range 50-20?GHz.