Перейти к основному содержанию
AkademIndex

Продукты

Для разработчиков

AkademBaseОткрытый API экосистемы
Статья

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

Masashi HazumiHigh Energy Accelerator Research Organization (Japan)Peter A. AdeCardiff Univ. (United Kingdom)Alexandre AdlerStockholm Univ. (Sweden)Erwan AllysLab. de Physique de l'Ecole Normale Superieure, ENS, Univ. PSL, CNRS, Sorbonne Univ., Univ. de Paris (France)Kam ArnoldUniv. of California, San Diego (United States)Didier AugusteUniv. Paris-Saclay, CNRS/IN2P3, IJCLab (France)Jonathan AumontIRAP, Univ. de Toulouse, CNRS, CNES, UPS (France)Ragnhild AurlienHigh Energy Accelerator Research Organization (Japan)Jason AustermannHigh Energy Accelerator Research Organization (Japan)Carlo BaccigalupiHigh Energy Accelerator Research Organization (Japan)Anthony J. BandayIRAP, Univ. de Toulouse, CNRS, CNES, UPS (France)R. BanjeriHigh Energy Accelerator Research Organization (Japan)Rita B. BarreiroHigh Energy Accelerator Research Organization (Japan)Soumen BasakCardiff Univ. (United Kingdom)Jim BeallHigh Energy Accelerator Research Organization (Japan)Dominic BeckHigh Energy Accelerator Research Organization (Japan)Shawn BeckmanHigh Energy Accelerator Research Organization (Japan)Juan BermejoHigh Energy Accelerator Research Organization (Japan)Paolo de BernardisHigh Energy Accelerator Research Organization (Japan)Marco BersanelliJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Julien BonisUniv. Paris-Saclay, CNRS/IN2P3, IJCLab (France)Julian BorrillHigh Energy Accelerator Research Organization (Japan)Francois BoulangerLab. de Physique de l'Ecole Normale Superieure, ENS, Univ. PSL, CNRS, Sorbonne Univ., Univ. de Paris (France)Sophie BounissouJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Maksym BrilenkovHigh Energy Accelerator Research Organization (Japan)Michael BrownCardiff Univ. (United Kingdom)Martin BucherJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Erminia CalabreseCardiff Univ. (United Kingdom)Paolo CampetiHigh Energy Accelerator Research Organization (Japan)Alessandro CaronesJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Francisco J. CasasHigh Energy Accelerator Research Organization (Japan)Anthony ChallinorVictor ChanKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Kolen CheungHigh Energy Accelerator Research Organization (Japan)Yuji ChinoneHigh Energy Accelerator Research Organization (Japan)Jean F. ClicheJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Loris ColomboKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Fabio ColumbroHigh Energy Accelerator Research Organization (Japan)Javier CubasCardiff Univ. (United Kingdom)Ari CukiermanHigh Energy Accelerator Research Organization (Japan)David CurtisJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Giuseppe D'AlessandroKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Nadia DachlythraStockholm Univ. (Sweden)Marco De PetrisKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Clive DickinsonCardiff Univ. (United Kingdom)Patricia Diego-PalazuelosHigh Energy Accelerator Research Organization (Japan)Matt DobbsJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Tadayasu DotaniKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Lionel DubandKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Shannon DuffHigh Energy Accelerator Research Organization (Japan)Jean M. DuvalKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Ken EbisawaKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Tucker ElleflotKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Hans K. EriksenHigh Energy Accelerator Research Organization (Japan)Josquin ErrardJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Thomas Essinger-HilemanIRAP, Univ. de Toulouse, CNRS, CNES, UPS (France)Fabio FinelliCardiff Univ. (United Kingdom)Raphael FlaugerUniv. of California, San Diego (United States)Cristian FranceschetKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Unni FuskelandHigh Energy Accelerator Research Organization (Japan)Mathew GallowayHigh Energy Accelerator Research Organization (Japan)Ken GangaJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Jian R. GaoCardiff Univ. (United Kingdom)Ricardo Genova-SantosCardiff Univ. (United Kingdom)Martina GerbinoCardiff Univ. (United Kingdom)Massimo GervasiCardiff Univ. (United Kingdom)Tommaso GhignaCardiff Univ. (United Kingdom)Eirik GjerløwHigh Energy Accelerator Research Organization (Japan)Marcin L. GradzielCardiff Univ. (United Kingdom)Julien GrainJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Frank GruppCardiff Univ. (United Kingdom)Alessandro GruppusoCardiff Univ. (United Kingdom)Jon E. GudmundssonStockholm Univ. (Sweden)Tijmen de HaanHigh Energy Accelerator Research Organization (Japan)Nils W. HalversonCardiff Univ. (United Kingdom)Peter HargraveCardiff Univ. (United Kingdom)Takashi HasebeStockholm Univ. (Sweden)Masaya HasegawaHigh Energy Accelerator Research Organization (Japan)Makoto HattoriHigh Energy Accelerator Research Organization (Japan)Sophie Henrot-VersilléUniv. Paris-Saclay, CNRS/IN2P3, IJCLab (France)Daniel HermanHigh Energy Accelerator Research Organization (Japan)Diego HerranzHigh Energy Accelerator Research Organization (Japan)Charles A. HillHigh Energy Accelerator Research Organization (Japan)Gene HiltonHigh Energy Accelerator Research Organization (Japan)Yukimasa HirotaJapan Aerospace Exploration Agency, Institute of Space and Astronautical Science (Japan)Eric HivonKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Renee A. HlozekKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Yurika HoshinoCardiff Univ. (United Kingdom)Elena de la HozHigh Energy Accelerator Research Organization (Japan)Johannes HubmayrHigh Energy Accelerator Research Organization (Japan)Kiyotomo IchikiStockholm Univ. (Sweden)Teruhito IidaLab. de Physique de l'Ecole Normale Superieure, ENS, Univ. PSL, CNRS, Sorbonne Univ., Univ. de Paris (France)Hiroaki ImadaStockholm Univ. (Sweden)Kosei IshimuraStockholm Univ. (Sweden)Hirokazu IshinoIRAP, Univ. de Toulouse, CNRS, CNES, UPS (France)Greg JaehnigCardiff Univ. (United Kingdom)Tooru KagaKavli Institute for the Physics and Mathematics of the Universe/Graduate Univ. for Advanced Studies (Japan)Shingo KashimaStockholm Univ. (Sweden)Nobuhiko KatayamaCardiff Univ. (United Kingdom)Akihiro KatoHigh Energy Accelerator Research Organization (Japan)
2020en
ABI

Аннотация

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.

Перевод пока недоступен

Идентификаторы

Цитирования и источники

Цитирований: 2Использованных источников: 0