中文

利用 LiteBIRD 宇宙微波背景偏振巡天探测宇宙暴胀

天体物理仪器与方法 2023-03-28 v3 宇宙学与河外天体物理

摘要

LiteBIRD,即用于通过宇宙背景辐射探测研究 B 模偏振与暴胀的轻量(Lite)卫星,是一项针对原初宇宙学与基础物理的空间任务。日本宇宙航空研究开发机构(JAXA)于 2019 年 5 月将 LiteBIRD 选为战略大型(L 级)任务,预计在 2020 年代后期使用 JAXA 的 H3 火箭发射。LiteBIRD 计划绕日地拉格朗日点 L2 运行,在那里它将用三年时间、以 34 至 448 GHz 之间 15 个频带的三个望远镜,绘制全天宇宙微波背景(CMB)偏振图,以实现前所未有的 2.2μ\muK-arcmin 总灵敏度,在 100 GHz 处典型角分辨率为 0.5^\circ。LiteBIRD 的主要科学目标是搜寻宇宙暴胀的信号, either making a discovery or ruling out well-motivated inflationary models。LiteBIRD 的观测还将为我们提供关于引力的量子性质以及超出粒子物理与宇宙学标准模型的其他新物理的见解。我们概述了 LiteBIRD 项目,包括科学目标、任务与系统需求、运行概念、航天器与载荷舱设计、预期科学成果、潜在设计扩展以及与其他项目的协同。

关键词

引用

@article{arxiv.2202.02773,
  title  = {Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey},
  author = {LiteBIRD Collaboration and E. Allys and K. Arnold and J. Aumont and R. Aurlien and S. Azzoni and C. Baccigalupi and A. J. Banday and R. Banerji and R. B. Barreiro and N. Bartolo and L. Bautista and D. Beck and S. Beckman and M. Bersanelli and F. Boulanger and M. Brilenkov and M. Bucher and E. Calabrese and P. Campeti and A. Carones and F. J. Casas and A. Catalano and V. Chan and K. Cheung and Y. Chinone and S. E. Clark and F. Columbro and G. D'Alessandro and P. de Bernardis and T. de Haan and E. de la Hoz and M. De Petris and S. Della Torre and P. Diego-Palazuelos and M. Dobbs and T. Dotani and J. M. Duval and T. Elleflot and H. K. Eriksen and J. Errard and T. Essinger-Hileman and F. Finelli and R. Flauger and C. Franceschet and U. Fuskeland and M. Galloway and K. Ganga and M. Gerbino and M. Gervasi and R. T. Génova-Santos and T. Ghigna and S. Giardiello and E. Gjerløw and J. Grain and F. Grupp and A. Gruppuso and J. E. Gudmundsson and N. W. Halverson and P. Hargrave and T. Hasebe and M. Hasegawa and M. Hazumi and S. Henrot-Versillé and B. Hensley and L. T. Hergt and D. Herman and E. Hivon and R. A. Hlozek and A. L. Hornsby and Y. Hoshino and J. Hubmayr and K. Ichiki and T. Iida and H. Imada and H. Ishino and G. Jaehnig and N. Katayama and A. Kato and R. Keskitalo and T. Kisner and Y. Kobayashi and A. Kogut and K. Kohri and E. Komatsu and K. Komatsu and K. Konishi and N. Krachmalnicoff and C. L. Kuo and L. Lamagna and M. Lattanzi and A. T. Lee and C. Leloup and F. Levrier and E. Linder and G. Luzzi and J. Macias-Perez and T. Maciaszek and B. Maffei and D. Maino and S. Mandelli and E. Martínez-González and S. Masi and M. Massa and S. Matarrese and F. T. Matsuda and T. Matsumura and L. Mele and M. Migliaccio and Y. Minami and A. Moggi and J. Montgomery and L. Montier and G. Morgante and B. Mot and Y. Nagano and T. Nagasaki and R. Nagata and R. Nakano and T. Namikawa and F. Nati and P. Natoli and S. Nerval and F. Noviello and K. Odagiri and S. Oguri and H. Ohsaki and L. Pagano and A. Paiella and D. Paoletti and A. Passerini and G. Patanchon and F. Piacentini and M. Piat and G. Pisano and G. Polenta and D. Poletti and T. Prouvé and G. Puglisi and D. Rambaud and C. Raum and S. Realini and M. Reinecke and M. Remazeilles and A. Ritacco and G. Roudil and J. A. Rubino-Martin and M. Russell and H. Sakurai and Y. Sakurai and M. Sasaki and D. Scott and Y. Sekimoto and K. Shinozaki and M. Shiraishi and P. Shirron and G. Signorelli and F. Spinella and S. Stever and R. Stompor and S. Sugiyama and R. M. Sullivan and A. Suzuki and T. L. Svalheim and E. Switzer and R. Takaku and H. Takakura and Y. Takase and A. Tartari and Y. Terao and J. Thermeau and H. Thommesen and K. L. Thompson and M. Tomasi and M. Tominaga and M. Tristram and M. Tsuji and M. Tsujimoto and L. Vacher and P. Vielva and N. Vittorio and W. Wang and K. Watanuki and I. K. Wehus and J. Weller and B. Westbrook and J. Wilms and B. Winter and E. J. Wollack and J. Yumoto and M. Zannoni},
  journal= {arXiv preprint arXiv:2202.02773},
  year   = {2023}
}

备注

155 pages, accepted for publication in PTEP