抄録
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 μK-arcmin with a typical angular resolution of 0.5° 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.
| 本文言語 | English |
|---|---|
| ホスト出版物のタイトル | Space Telescopes and Instrumentation 2020 |
| ホスト出版物のサブタイトル | Optical, Infrared, and Millimeter Wave |
| 編集者 | Makenzie Lystrup, Marshall D. Perrin |
| 出版社 | SPIE |
| ISBN（電子版） | 9781510636736 |
| DOI | |
| 出版ステータス | Published - 2020 |
| イベント | Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave - Virtual, Online, United States 継続期間: 2020 12月 14 → 2020 12月 22 |
出版物シリーズ
| 名前 | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| 巻 | 11443 |
| ISSN（印刷版） | 0277-786X |
| ISSN（電子版） | 1996-756X |
Conference
| Conference | Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave |
|---|---|
| 国/地域 | United States |
| City | Virtual, Online |
| Period | 20/12/14 → 20/12/22 |
ASJC Scopus subject areas
- 電子材料、光学材料、および磁性材料
- 凝縮系物理学
- コンピュータ サイエンスの応用
- 応用数学
- 電子工学および電気工学
フィンガープリント
「LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。引用スタイル
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS
LiteBIRD satellite : JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. / Hazumi, M.; Ade, P. A.R.; Adler, A. その他.
Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave. ed. / Makenzie Lystrup; Marshall D. Perrin. SPIE, 2020. 114432F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11443).研究成果: Conference contribution
}
TY - GEN
T1 - LiteBIRD satellite
T2 - Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
AU - Hazumi, M.
AU - Ade, P. A.R.
AU - Adler, A.
AU - Allys, E.
AU - Arnold, K.
AU - Auguste, D.
AU - Aumont, J.
AU - Aurlien, R.
AU - Austermann, J.
AU - Baccigalupi, C.
AU - Banday, A. J.
AU - Banjeri, R.
AU - Barreiro, R. B.
AU - Basak, S.
AU - Beall, J.
AU - Beck, D.
AU - Beckman, S.
AU - Bermejo, J.
AU - De Bernardis, P.
AU - Bersanelli, M.
AU - Bonis, J.
AU - Borrill, J.
AU - Boulanger, F.
AU - Bounissou, S.
AU - Brilenkov, M.
AU - Brown, M.
AU - Bucher, M.
AU - Calabrese, E.
AU - Campeti, P.
AU - Carones, A.
AU - Casas, F. J.
AU - Challinor, A.
AU - Chan, V.
AU - Cheung, K.
AU - Chinone, Y.
AU - Cliche, J. F.
AU - Colombo, L.
AU - Columbro, F.
AU - Cubas, J.
AU - Cukierman, A.
AU - Curtis, D.
AU - D'alessandro, G.
AU - Dachlythra, N.
AU - De Petris, M.
AU - Dickinson, C.
AU - Diego-Palazuelos, P.
AU - Dobbs, M.
AU - Dotani, T.
AU - Duband, L.
AU - Duff, S.
AU - Duval, J. M.
AU - Ebisawa, K.
AU - Elleflot, T.
AU - Eriksen, H. K.
AU - Errard, J.
AU - Essinger-Hileman, T.
AU - Finelli, F.
AU - Flauger, R.
AU - Franceschet, C.
AU - Fuskeland, U.
AU - Galloway, M.
AU - Ganga, K.
AU - Gao, J. R.
AU - Genova-Santos, R.
AU - Gerbino, M.
AU - Gervasi, M.
AU - Ghigna, T.
AU - Gjerløw, E.
AU - Gradziel, M. L.
AU - Grain, J.
AU - Grupp, F.
AU - Gruppuso, A.
AU - Gudmundsson, J. E.
AU - De Haan, T.
AU - Halverson, N. W.
AU - Hargrave, P.
AU - Hasebe, T.
AU - Hasegawa, M.
AU - Hattori, M.
AU - Henrot-Versillé, S.
AU - Herman, D.
AU - Herranz, D.
AU - Hill, C. A.
AU - Hilton, G.
AU - Hirota, Y.
AU - Hivon, E.
AU - Hlozek, R. A.
AU - Hoshino, Y.
AU - De La Hoz, E.
AU - Hubmayr, J.
AU - Ichiki, K.
AU - Iida, T.
AU - Imada, H.
AU - Ishimura, K.
AU - Ishino, H.
AU - Jaehnig, G.
AU - Kaga, T.
AU - Kashima, S.
AU - Katayama, N.
AU - Kato, A.
AU - Kawasaki, T.
AU - Keskitalo, R.
AU - Kisner, T.
AU - Kobayashi, Y.
AU - Kogiso, N.
AU - Kogut, A.
AU - Kohri, K.
AU - Komatsu, E.
AU - Komatsu, K.
AU - Konishi, K.
AU - Krachmalnicoff, N.
AU - Kreykenbohm, I.
AU - Kuo, C. L.
AU - Kushino, A.
AU - Lamagna, L.
AU - Lanen, J. V.
AU - Lattanzi, M.
AU - Lee, A. T.
AU - Leloup, C.
AU - Levrier, F.
AU - Linder, E.
AU - Louis, T.
AU - Luzzi, G.
AU - Maciaszek, T.
AU - Maffei, B.
AU - Maino, D.
AU - Maki, M.
AU - Mandelli, S.
AU - Martinez-Gonzalez, E.
AU - Masi, S.
AU - Matsumura, T.
AU - Mennella, A.
AU - Migliaccio, M.
AU - Minami, Y.
AU - Mitsuda, K.
AU - Montgomery, J.
AU - Montier, L.
AU - Morgante, G.
AU - Mot, B.
AU - Murata, Y.
AU - Murphy, J. A.
AU - Nagai, M.
AU - Nagano, Y.
AU - Nagasaki, T.
AU - Nagata, R.
AU - Nakamura, S.
AU - Namikawa, T.
AU - Natoli, P.
AU - Nerval, S.
AU - Nishibori, T.
AU - Nishino, H.
AU - Noviello, F.
AU - O'sullivan, C.
AU - Ogawa, H.
AU - Ogawa, H.
AU - Oguri, S.
AU - Ohsaki, H.
AU - Ohta, I. S.
AU - Okada, N.
AU - Okada, N.
AU - Pagano, L.
AU - Paiella, A.
AU - Paoletti, D.
AU - Patanchon, G.
AU - Peloton, J.
AU - Piacentini, F.
AU - Pisano, G.
AU - Polenta, G.
AU - Poletti, D.
AU - Prouvé, T.
AU - Puglisi, G.
AU - Rambaud, D.
AU - Raum, C.
AU - Realini, S.
AU - Reinecke, M.
AU - Remazeilles, M.
AU - Ritacco, A.
AU - Roudil, G.
AU - Rubino-Martin, J. A.
AU - Russell, M.
AU - Sakurai, H.
AU - Sakurai, Y.
AU - Sandri, M.
AU - Sasaki, M.
AU - Savini, G.
AU - Scott, D.
AU - Seibert, J.
AU - Sekimoto, Y.
AU - Sherwin, B.
AU - Shinozaki, K.
AU - Shiraishi, M.
AU - Shirron, P.
AU - Signorelli, G.
AU - Smecher, G.
AU - Stever, S.
AU - Stompor, R.
AU - Sugai, H.
AU - Sugiyama, S.
AU - Suzuki, A.
AU - Suzuki, J.
AU - Svalheim, T. L.
AU - Switzer, E.
AU - Takaku, R.
AU - Takakura, H.
AU - Takakura, S.
AU - Takase, Y.
AU - Takeda, Y.
AU - Tartari, A.
AU - Taylor, E.
AU - Terao, Y.
AU - Thommesen, H.
AU - Thompson, K. L.
AU - Thorne, B.
AU - Toda, T.
AU - Tomasi, M.
AU - Tominaga, M.
AU - Trappe, N.
AU - Tristram, M.
AU - Tsuji, M.
AU - Tsujimoto, M.
AU - Tucker, C.
AU - Ullom, J.
AU - Vermeulen, G.
AU - Vielva, P.
AU - Villa, F.
AU - Vissers, M.
AU - Vittorio, N.
AU - Wehus, I.
AU - Weller, J.
AU - Westbrook, B.
AU - Wilms, J.
AU - Winter, B.
AU - Wollack, E. J.
AU - Yamasaki, N. Y.
AU - Yoshida, T.
AU - Yumoto, J.
AU - Zannoni, M.
AU - Zonca, A.
N1 - Funding Information: This work is supported in Japan by ISAS/JAXA for Pre-Phase A2 studies, by the acceleration program of JAXA research and development directorate, by the World Premier International Research Center Initiative (WPI) of MEXT, by the JSPS Core-to-Core Program of A. Advanced Research Networks, and by JSPS KAKENHI Grant Numbers JP15H05891, JP17H01115, and JP17H01125. The Italian LiteBIRD phase A contribution is supported by the Italian Space Agency (ASI Grants No. 2020-9-HH.0 and 2016-24-H.1-2018), the National Institute for Nuclear Physics (INFN) and the National Institute for Astrophysics (INAF). The French LiteBIRD phase A contribution is supported by the Centre National d’Etudes Spatiale (CNES), by the Centre National de la Recherche Scientifique (CNRS), and by the Commissariat à l’Energie Atomique (CEA). The Canadian contribution is supported by the Canadian Space Agency. The US contribution is supported by NASA grant no. 80NSSC18K0132. Norwegian participation in LiteBIRD is supported by the Research Council of Norway (Grant No. 263011). The Spanish LiteBIRD phase A contribution is supported by the Spanish Agencia Estatal de Investigación (AEI), project refs. PID2019-110610RB-C21 and AYA2017-84185-P. Funds that support the Swedish contributions come from the Swedish National Space Agency (SNSA/Rymdstyrelsen) and the Swedish Research Council (Reg. no. 2019-03959). The German participation in LiteBIRD is supported in part by the Excellence Cluster ORIGINS, which is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy (Grant No. EXC-2094 - 390783311). This research used resources of the Central Computing System owned and operated by the Computing Research Center at KEK, as well as resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy. Publisher Copyright: © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.
PY - 2020
Y1 - 2020
N2 - 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 μK-arcmin with a typical angular resolution of 0.5° 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.
AB - 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 μK-arcmin with a typical angular resolution of 0.5° 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.
KW - B-mode polarization
KW - Cosmic in ation
KW - Cosmic microwave background
KW - LiteBIRD
KW - Primordial gravi- tational waves
KW - Quantum gravity
KW - Space telescope
UR - http://www.scopus.com/inward/record.url?scp=85099878190&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85099878190&partnerID=8YFLogxK
U2 - 10.1117/12.2563050
DO - 10.1117/12.2563050
M3 - Conference contribution
AN - SCOPUS:85099878190
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2020
A2 - Lystrup, Makenzie
A2 - Perrin, Marshall D.
PB - SPIE
Y2 - 14 December 2020 through 22 December 2020
ER -