LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

被引：49

作者：

Hazumi, Masashi ^{[1
,2
,3
,4
]}

Ade, Peter A. ^{[5
]}

Adler, Alexandre ^{[6
]}

Allys, Erwan ^{[7
]}

Arnold, Kam ^{[8
]}

Auguste, Didier ^{[9
]}

Aumont, Jonathan ^{[10
]}

Aurlien, Ragnhild ^{[11
]}

Austermann, Jason ^{[12
]}

Baccigalupi, Carlo ^{[13
]}

Banday, Anthony J. ^{[10
]}

Banjeri, R. ^{[11
]}

Barreiro, Rita B. ^{[14
]}

Basak, Soumen ^{[15
]}

Beall, Jim ^{[12
]}

Beck, Dominic ^{[16
]}

Beckman, Shawn ^{[17
]}

Bermejo, Juan ^{[18
]}

de Bernardis, Paolo ^{[19
,20
]}

Bersanelli, Marco ^{[21
,22
]}

Bonis, Julien ^{[9
]}

Borrill, Julian ^{[23
,24
]}

Boulanger, Francois ^{[7
]}

Bounissou, Sophie ^{[25
]}

Brilenkov, Maksym ^{[11
]}

Brown, Michael ^{[26
]}

Bucher, Martin ^{[27
]}

Calabrese, Erminia ^{[5
]}

Campeti, Paolo ^{[13
]}

Carones, Alessandro ^{[28
,29
]}

Casas, Francisco J. ^{[14
]}

Challinor, Anthony ^{[30
,31
,32
]}

Chan, Victor ^{[33
]}

Cheung, Kolen ^{[17
]}

Chinone, Yuji ^{[34
]}

Cliche, Jean F. ^{[35
]}

Colombo, Loris ^{[21
,22
]}

Columbro, Fabio ^{[19
,20
]}

Cubas, Javier ^{[36
]}

Cukierman, Ari ^{[16
,17
]}

Curtis, David ^{[24
]}

D'Alessandro, Giuseppe ^{[19
,20
]}

Dachlythra, Nadia ^{[6
]}

De Petris, Marco ^{[19
,20
]}

Dickinson, Clive ^{[26
]}

Diego-Palazuelos, Patricia ^{[14
]}

Dobbs, Matt ^{[35
]}

Dotani, Tadayasu ^{[2
]}

Duband, Lionel ^{[37
]}

Duff, Shannon ^{[12
]}

机构：

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

[2] Japan Aerosp Explorat Agcy JAXA, Inst Space & Astronaut Sci ISAS, Sagamihara, Kanagawa 2525210, Japan

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

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

[5] Cardiff Univ, Sch Phys & Astron, Cardiff CF10 3XQ, Wales

[6] Stockholm Univ, Stockholm, Sweden

[7] Univ Paris, Sorbonne Univ, Univ PSL, CNRS,Lab Phys Ecole Normale Super,ENS, F-75005 Paris, France

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

[9] Univ Paris Saclay, IJCLab, CNRS, IN2P3, F-91405 Orsay, France

[10] Univ Toulouse, CNES, CNRS, IRAP,UPS, Toulouse, France

[11] Univ Oslo, Inst Theoret Astrophys, NO-0315 Oslo, Norway

[12] Natl Inst Stand & Technol NIST, Boulder, CO 80305 USA

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

[14] Inst Fis Cantabria IFCA, CSIC UC, Ave Castros SN, Santander 39005, Spain

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

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

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

[18] Inst Univ Microgravedad Ignacio Riva IDR UPM, Plaza Cardenal Cisneros 3, Madrid 28040, Spain

[19] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, Rome, Italy

[20] Ist Nazl Fis Nucl, Rome, Italy

[21] Univ Milan, Dipartimento Fis, INAF IASF, Milan, Italy

[22] Sezione Ist Nazl Fis Nucl, Milan, Italy

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

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

[25] Univ Paris Sud 11, CNRS, Inst Astrophys Spatiale IAS, UMR 8617, Batiment 121, F-91405 Orsay, France

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

[27] Univ Paris, CNRS, Astroparticule & Cosmol, F-75013 Paris, France

[28] Univ Roma Tor Vergata, Dipartimento Fis, I-2 Rome, Italy

[29] Ist Nazl Fis Nucl, I-2 Rome, Italy

[30] Ctr Math Sci, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England

[31] Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[32] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England

[33] Univ Toronto, Toronto, ON, Canada

[34] Univ Tokyo, Res Ctr Early Universe, Sch Sci, RESCEU, Tokyo, Japan

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

[36] Univ Politecn Madrid, Madrid, Spain

[37] Univ Grenoble Alpes, IRIG DSBT, CEA, F-38000 Grenoble, France

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

[39] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA

[40] OAS Bologna, INAF, Via Piero Gobetti,93-3, I-40129 Bologna, Italy

[41] SRON Netherlands Inst Space Res, Utrecht, Netherlands

[42] Inst Astrofis Canarias IAC, Madrid, Spain

[43] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy

[44] Sez INFN Ferrara, Via Saragat 1, I-44122 Ferrara, Italy

[45] Univ Milano Bicocca, Phys Dept, Pzza Sci 3, I-20126 Milan, Italy

[46] Univ Oxford, Oxford, England

[47] Natl Univ Ireland Maynooth, Maynooth, Kildare, Ireland

[48] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany

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

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

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2020: OPTICAL, INFRARED, AND MILLIMETER WAVE | 2021年 / 11443卷

基金：

瑞典研究理事会;

关键词：

LiteBIRD; cosmic inflation; cosmic microwave background; B-mode polarization; primordial gravitational waves; quantum gravity; space telescope; MODE POLARIZATION; SUBDEGREE SCALES; POWER SPECTRUM; SQUARE DEGREES; GRAVITY-WAVES; PROBE; CMB;

D O I：

10.1117/12.2563050

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. JAXA selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with its expected launch in the late 2020s using JAXA's H3 rocket. LiteBIRD plans to map the cosmic microwave background (CMB) polarization over the full sky with unprecedented precision. Its main scientific objective is to carry out a definitive search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with an insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. To this end, LiteBIRD will perform full-sky surveys for three years at the Sun-Earth Lagrangian point L2 for 15 frequency bands between 34 and 448 GHz with three telescopes, to achieve a total sensitivity of 2.16 mu K-arcmin with a typical angular resolution of 0.5 degrees at 100 GHz. We provide an overview of the LiteBIRD project, including scientific objectives, mission requirements, top-level system requirements, operation concept, and expected scientific outcomes.

引用

页数：20

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