LiteBIRD, Lite satellite for the study of B-mode polarization and Inflation from cosmic microwave background Radiation Detection

被引：29

作者：

Ishino, H. ^{[1
]}

Akiba, Y. ^{[2
]}

Arnold, K. ^{[3
]}

Barron, D. ^{[4
]}

Borrill, J. ^{[4
,5
]}

Chendra, R. ^{[6
]}

Chinone, Y. ^{[4
]}

Cho, S. ^{[7
]}

Cukierman, A. ^{[4
]}

de Haan, T. ^{[4
]}

Dobbs, M. ^{[8
]}

Dominjon, A. ^{[9
]}

Dotani, T. ^{[10
]}

Elleflot, T. ^{[11
]}

Errard, J. ^{[12
]}

Fujino, T. ^{[13
]}

Fuke, H. ^{[10
]}

Funaki, T. ^{[1
]}

Goeckner-Wald, N. ^{[4
]}

Halverson, N. ^{[14
]}

Harvey, P. ^{[4
]}

Hasebe, T. ^{[9
]}

Hasegawa, M. ^{[15
]}

Hattori, K. ^{[16
]}

Hattori, M. ^{[17
]}

Hazumi, M. ^{[15
]}

Hidehira, N. ^{[1
]}

Hill, C. ^{[4
]}

Hilton, G. ^{[18
]}

Holzapfel, W. ^{[4
]}

Hori, Y. ^{[4
]}

Hubmayr, J. ^{[18
]}

Ichiki, K. ^{[19
]}

Imada, H. ^{[10
]}

Inatani, J. ^{[9
]}

Inoue, M. ^{[20
]}

Inoue, Y. ^{[2
]}

Trie, F. ^{[13
]}

Irwin, K. ^{[7
]}

Ishitsuka, H. ^{[2
]}

Jeong, O. ^{[4
]}

Kanai, H. ^{[13
]}

Karatsu, K. ^{[9
]}

Kashima, S. ^{[9
]}

Katayama, N. ^{[16
]}

Kawano, I. ^{[10
]}

Kawasaki, T. ^{[21
]}

Keating, B. ^{[11
]}

Kernasovskiy, S. ^{[7
]}

Keskitalo, R. ^{[4
]}

机构：

[1] Okayama Univ, Okayama, Japan

[2] Grad Univ Adv Studies SOKENDAI, Hayama, Japan

[3] Univ Wisconsin, Madison, WI 53706 USA

[4] Univ Calif Berkeley, Berkeley, CA 94720 USA

[5] Lawrence Berkeley Natl Lab, Berkeley, CA USA

[6] Tokyo Inst Technol, Tokyo, Japan

[7] Stanford Univ, Stanford, CA 94305 USA

[8] McGill Univ, Montreal, PQ, Canada

[9] Natl Astron Observ Japan, Mitaka, Tokyo, Japan

[10] Japan Aerosp Explorat Agcy JAXA, Tokyo, Japan

[11] Univ Calif San Diego, San Diego, CA 92103 USA

[12] ILP, Paris, France

[13] Yokohama Natl Univ, Yokohama, Kanagawa, Japan

[14] Univ Colorado, Boulder, CO 80309 USA

[15] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki, Japan

[16] Kavli Inst Phys & Math Universe IPMU, Kashiwa, Chiba, Japan

[17] Tohoku Univ, Sendai, Miyagi, Japan

[18] NIST, Boulder, CO USA

[19] Nagoya Univ, Nagoya, Aichi, Japan

[20] Osaka Prefecture Univ, Sakai, Osaka, Japan

[21] Kitasato Univ, Tokyo, Japan

[22] Max Planck Inst Astrophys, Garching, Germany

[23] Osaka Univ, Suita, Osaka, Japan

[24] Kansei Gakuin Univ, Nishinomiya, Hyogo, Japan

[25] RIKEN, Wako, Saitama, Japan

[26] Univ Tsukuba, Tsukuba, Ibaraki, Japan

[27] Saitama Univ, Saitama, Japan

[28] Konan Univ, Kobe, Hyogo, Japan

[29] Cardiff Univ, Cardiff, S Glam, Wales

[30] Univ Tokyo, Tokyo, Japan

[31] Astroparticle & Cosmol APC Lab, Paris, France

[32] NIFS, Tokyo, Japan

[33] Natl Inst Informat & Commun Technol NICT, Tokyo, Japan

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2016: OPTICAL, INFRARED, AND MILLIMETER WAVE | 2016年 / 9904卷

关键词：

Cosmic Microwave Background; LiteBIRD; B-mode polarization; NEXT-GENERATION; POLARIMETERS;

D O I：

10.1117/12.2231995

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

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.

引用

页数：8

共 48 条

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