LiteBIRD: A Satellite for the Studies of B-Mode Polarization and Inflation from Cosmic Background Radiation Detection

被引：221

作者：

Hazumi, M. ^{[19
,22
,29
,49
]}

Ade, P. A. R. ^{[47
]}

Akiba, Y. ^{[19
,49
]}

Alonso, D. ^{[41
]}

Arnold, K. ^{[16
]}

Aumont, J. ^{[20
]}

Baccigalupi, C. ^{[25
]}

Barron, D. ^{[48
]}

Basak, S. ^{[11
,25
]}

Beckman, S. ^{[15
]}

Borrill, J. ^{[6
,48
]}

Boulanger, F. ^{[20
]}

Bucher, M. ^{[3
]}

Calabrese, E. ^{[47
]}

Chinone, Y. ^{[15
,29
]}

Cho, S. ^{[13
]}

Cukierman, A. ^{[15
]}

Curtis, D. W. ^{[48
]}

de Haan, T. ^{[43
]}

Dobbs, M. ^{[42
]}

Dominjon, A. ^{[34
]}

Dotani, T. ^{[22
]}

Duband, L. ^{[18
]}

Ducout, A. ^{[29
]}

Dunkley, J. ^{[10
,41
]}

Duval, J. M. ^{[18
]}

Elleflot, T. ^{[16
]}

Eriksen, H. K. ^{[24
]}

Errard, J. ^{[3
]}

Fischer, J. ^{[48
]}

Fujino, T. ^{[53
]}

Funaki, T. ^{[12
]}

Fuskeland, U. ^{[24
]}

Ganga, K. ^{[3
]}

Goeckner-Wald, N. ^{[15
]}

Grain, J. ^{[20
]}

Halverson, N. W. ^{[4
,9
,17
]}

Hamada, T. ^{[2
,19
]}

Hasebe, T. ^{[22
]}

Hasegawa, M. ^{[19
,49
]}

Hattori, K. ^{[36
]}

Hattori, M. ^{[2
]}

Hayes, L. ^{[48
]}

Hidehira, N. ^{[12
]}

Hill, C. A. ^{[15
,43
]}

Hilton, G. ^{[38
]}

Hubmayr, J. ^{[38
]}

Ichiki, K. ^{[31
]}

Iida, T. ^{[29
]}

Imada, H. ^{[22
]}

机构：

[1] Aoyama Gakuin Univ, Sagamihara, Kanagawa 2525258, Japan

[2] Tohoku Univ, Astron Inst, Grad Sch Sci, Sendai, Miyagi 9808578, Japan

[3] Univ Paris Diderot, AstroParticule & Cosmol APC, CNRS IN2P3, Sorbonne Paris Cite,CEA Irfu,Obs Paris, Paris, France

[4] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA

[5] CNRS, IRAP, F-31028 Toulouse 4, France

[6] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA

[7] Univ Cambridge, DAMTP, Cambridge CB3 0WA, England

[8] Univ Tokyo, Dept Astron, Tokyo 1130033, Japan

[9] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA

[10] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[11] Indian Inst Sci Educ & Res Thiruvananthapuram, Sch Phys, Maruthamala PO, Thiruvananthapuram 695551, Kerala, India

[12] Okayama Univ, Dept Phys, Okayama, Okayama 7008530, Japan

[13] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[14] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan

[15] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[16] Univ Calif San Diego, Dept Phys, San Diego, CA 92093 USA

[17] Univ Colorado, Dept Phys, Boulder, CO 80309 USA

[18] French Alternat Energies & Atom Energy Commiss CE, Grenoble, France

[19] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan

[20] Univ Paris Sud 11, IAS, CNRS, UMR 8617, Batiment 121, F-91405 Orsay, France

[21] Acad Sinica, Inst Phys, 128,Sect 2,Acad Rd, Nankang, Taiwan

[22] Japan Aerosp Explorat Agcy JAXA, ISAS, Sagamihara, Kanagawa 2525210, Japan

[23] Japan Aerosp Explorat Agcy JAXA, Res & Dev Directorate, Tsukuba, Ibaraki 3058505, Japan

[24] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway

[25] Int Sch Adv Studies SISSA, Via Bonomea 265, I-34136 Trieste, Italy

[26] Kansei Gakuin Univ, Nishinomiya, Hyogo 6628501, Japan

[27] Kavli Inst Cosmol, Cambridge CB3 0HA, England

[28] KIPAC, SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[29] Univ Tokyo, Kavli Inst Phys & Math Universe Kavli IPMU, WPI, UTIAS, Kashiwa, Chiba 2778583, Japan

[30] Kitazato Univ, Sagamihara, Kanagawa 2520373, Japan

[31] Nagoya Univ, Kobayashi Maskawa Inst Origin Particle & Universe, Nagoya, Aichi 4648602, Japan

[32] Univ Paris Saclay, Univ Paris Sud, CNRS IN2P3, LAL, Orsay, France

[33] Max Planck Inst Astrophys, D-85741 Garching, Germany

[34] NAOJ, Mitaka, Tokyo 1818588, Japan

[35] NIFS, Toki, Gifu 5095202, Japan

[36] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058563, Japan

[37] Natl Inst Informat & Commun Technol NICT, Kobe, Hyogo 6512492, Japan

[38] NIST, Boulder, CO 80305 USA

[39] Osaka Prefecture Univ, Sakai, Osaka 5998531, Japan

[40] Osaka Univ, Toyonaka, Osaka 5600043, Japan

[41] Oxford Astrophys, Oxford OX1 3RH, England

[42] McGill Univ, Phys Dept, Montreal, PQ H3A 0G4, Canada

[43] Lawrence Berkeley Natl Lab, Phys Div, Berkeley, CA 94720 USA

[44] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA

[45] RIKEN, Wako, Saitama 3510198, Japan

[46] Saitama Univ, Saitama, Saitama 3388570, Japan

[47] Cardiff Univ, Sch Phys & Astron, Cardiff CF10 3XQ, S Glam, Wales

[48] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[49] Grad Univ Adv Studies SOKENDAI, Hayama, Kanagawa 2400115, Japan

[50] Univ Manchester, Manchester M13 9PL, Lancs, England

来源：

JOURNAL OF LOW TEMPERATURE PHYSICS | 2019年 / 194卷 / 5-6期

关键词：

Cosmic inflation; Cosmic microwave background; B-mode polarization; Primordial gravitational wave; Quantum gravity; Satellite; GRAVITY-WAVES;

D O I：

10.1007/s10909-019-02150-5

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

LiteBIRD is a candidate satellite for a strategic large mission of JAXA. With its expected launch in the middle of the 2020s with a H3 rocket, LiteBIRD plans to map the polarization of the cosmic microwave background radiation over the full sky with unprecedented precision. The full success of LiteBIRD is to achieve delta r < 0.001, where r is the total error on the tensor-to-scalar ratio r. The required angular coverage corresponds to 2 <= l <= 200, where l is the multipole moment. This allows us to test well-motivated cosmic inflation models. Full-sky surveys for 3years at a Lagrangian point L2 will be carried out for 15 frequency bands between 34 and 448 GHz with two telescopes to achieve the total sensitivity of 2.5 mu K arcmin with a typical angular resolution of 0.5 degrees at 150 GHz. Each telescope is equipped with a half-wave plate system for polarization signal modulation and a focal plane filled with polarization-sensitive TES bolometers. A cryogenic system provides a 100 mK base temperature for the focal planes and 2 K and 5 K stages for optical components.

引用

页码：443 / 452

页数：10

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