Collaborative Research: Imaging the Beginning of Time from the South Pole: Completing the BICEP Array Survey

合作研究：从南极想象时间的开始：完成 BICEP 阵列调查

• 批准号: 2220448
• 负责人: Chao-Lin Kuo
• 金额: $ 160.87万
• 依托单位: Stanford University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-09-01 至 2027-08-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2220448&HistoricalAwards=false
• 关键词: Collaborative; Research; Imaging; Beginning; Time

The theory of the "Big Bang" provides an established cosmological model for the origin of our Universe from its earliest known periods through its subsequent large-scale evolution. However, this theory leaves open the question of explaining the initial conditions. Current thoughts are consistent with the entire observable Universe being spawned in a dramatic, exponential "Inflation" of a sub-nuclear volume that lasted about one trillionth of a trillionth of a trillionth of a second. Following this short inflationary period, the Universe continues to expand, but at a less rapid rate. While this basic "Inflationary paradigm" is accepted by most cosmologists, the detailed physics mechanism responsible for inflation is still not known, but there is a testable prediction that this violent space-time expansion would have produced primordial gravitational waves now propagating through the expanding Universe and forming a cosmic gravitational-wave background (CGB). The CGB amplitude defines the energy scale of Inflation that imprints a faint signature in the polarization of the Cosmic Microwave Background (CMB) radiation. Therefore, detecting this polarization signature is arguably the most important goal in cosmology today. This award will continue addressing the oldest question ever posed by mankind "How did the Universe begin?", and it does so via observations made at one of the harshest places on Earth – the Amundsen-Scott South Pole Station in Antarctica. The most recent, community driven Decadal Survey Astro2020 report “Pathways to Discovery in Astronomy and Astrophysics for the 2020s” reaffirmed the importance of search for B-modes polarization signatures of primordial gravitational waves and Inflation, and specifically endorsed the CMB Stage-4 science to be pursued by systematically supported CMB experiments in Antarctica and Chile. The recently released BICEP results place stringent limits on Inflationary models which, for the first time, go well beyond what can be done with temperature data alone, and which rule out two entire classes of previously popular single-field models—natural Inflation and simple monomial potentials. This award aims to complete deployment of all four BICEP Array receivers and then operate them as the Stage-3+ generation observing system. BICEP Array will measure the polarized sky in six frequency bands to reach an ultimate sensitivity to the amplitude of PGW of σ(r) ≲ 0.003, extrapolating from achieved performance, and after conservatively accounting for the Galactic dust, Galactic synchrotron and CMB lensing foregrounds. These measurements will be a definitive test of slow-roll models of Inflation, which generally predict a gravitational-wave signal above approximately r=0.01. BICEP Array will therefore realize the goal set by the NASA/DOE/NSF Task Force for CMB Research in 2005 to achieve sensitivity at this level, and confirmed as “the most exciting quest of all” by the Astro2010, and advance the B-mode search strongly endorsed by the Astro2020 Decadal Survey. The project will continue to provide excellent training for undergraduate and graduate students and postdoctoral fellows including those from underrepresented groups in laboratories that have exceptional track records in this regard. Cosmology and research in Antarctica both capture the public imagination, making this combination a remarkably effective vehicle for stimulating interest in science. This project advances the goals of the NSF Windows on the Universe Big Idea.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

大爆炸理论为我们的宇宙的起源提供了一个既定的宇宙学模型，从它已知的最早时期到后来的大规模演化。然而，这一理论留下了解释初始条件的问题。目前的想法与整个可见宇宙在持续约一万亿分之一秒的亚核体积的戏剧性、指数性“膨胀”中产生的情况是一致的。在这一短暂的通货膨胀期之后，宇宙继续膨胀，但速度较慢。虽然这一基本的“膨胀范式”被大多数宇宙学家接受，但导致膨胀的详细物理机制仍不清楚，但有一个可测试的预测表明，这种剧烈的时空膨胀将产生原始引力波，现在正在膨胀的宇宙中传播，并形成宇宙引力波背景(CGB)。CGB幅度定义了宇宙微波背景(CMB)辐射的偏振中留下微弱信号的膨胀的能量标度。因此，探测这种偏振信号可以说是当今宇宙学最重要的目标。该奖项将继续探讨人类提出的最古老的问题：宇宙是如何开始的？它将通过在地球上最严酷的地方之一-南极洲的阿蒙森-斯科特南极站-进行的观测来实现这一目标。最近由社区推动的《2020年十年天体观测报告》《2020年代天文学和天体物理学的发现之路》重申了寻找原始引力波和暴胀的B模偏振特征的重要性，并特别核准了由南极和智利系统支持的CMB实验进行的CMB第四阶段科学。BICEP最近发布的结果对通货膨胀模型施加了严格的限制，这是第一次远远超出了仅使用温度数据可以完成的范围，并排除了两类以前很受欢迎的单场模型-自然膨胀和简单单项式势。该合同旨在完成所有四个BICEP阵列接收器的部署，然后将其作为Stage-3+代观测系统运行。二头肌阵列将在六个频段测量极化天空，以达到对σ(R)≲0.003的PGW幅度的最终敏感性，根据取得的性能进行推断，并在保守地考虑了银河系尘埃、银河同步加速器和CMB透镜前景后。这些测量将是对慢滚膨胀模型的决定性测试，这些模型通常预测引力波信号在大约r=0.01以上。因此，二头肌阵列将实现NASA/DOE/NSF CMB研究特别工作组在2005年设定的目标，即达到这一水平的灵敏度，并在2010年Astro2010被确认为“最令人兴奋的探索”，并推进得到Astro2020十年调查强烈支持的B模式搜索。该项目将继续为本科生和研究生以及博士后研究员提供出色的培训，包括那些在这方面有出色记录的实验室中任职人数不足的群体。宇宙学和南极洲的研究都吸引了公众的想象力，使这种结合成为激发人们对科学感兴趣的非常有效的工具。这个项目推进了NSF宇宙大理想之窗的目标。这一奖项反映了NSF的法定使命，并通过使用基金会的智力优势和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

BICEP/Keck. XVI. Characterizing Dust Polarization through Correlations with Neutral Hydrogen

• DOI: 10.3847/1538-4357/acb64c
• 发表时间: 2022-10
• 期刊: The Astrophysical Journal
• 作者: B. C. P. Ade;Z. Ahmed;M. Amiri;D. Barkats;R. Thakur;D. Beck;C. Bischoff;J. Bock;H. Boenish;E. Bullock;V. Buza;IV J.R.Cheshire;S. Clark;J. Connors;J. Cornelison;M. Crumrine;A. Cukierman;E. Denison;M. Dierickx;L. Duband;M. Eiben;S. Fatigoni;J. Filippini;S. Fliescher;C. Giannakopoulos;N. Goeckner-wald;D. Goldfinger;J. Grayson;P. Grimes;G. Halal;G. Hall;M. Halpern;E. Hand;S. Harrison;S. Henderson;S. Hildebrandt;J. Hubmayr;H. Hui;K. Irwin;J. Kang;K. Karkare;E. Karpel;S. Kefeli;S. A. Kernasovskiy;J. Kovac;C. Kuo;K. Lau;E. Leitch;A. Lennox;K. Megerian;L. Minutolo;L. Moncelsi;Y. Nakato;T. Namikawa;H. T. Nguyen;R. O’Brient;IV R.W.Ogburn;S. Palladino;M. Petroff;T. Prouvé;C. Pryke;B. Racine;C. Reintsema;S. Richter;A. Schillaci;B. Schmitt;R. Schwarz;C. Sheehy;B. Singari;A. Soliman;T. S. Germaine;B. Steinbach;R. Sudiwala;G. Teply;K. Thompson;J. Tolan;C. Tucker;A. Turner;C. Umilta;C. Vergés;A. Vieregg;A. Wandui;A. Weber;D. Wiebe;J. Willmert;C. Wong;W.L.K. Wu;H. Yang;K. Yoon;E. Young;C. Yu;L. Zeng;C. Zhang;S. University;Kipacslac;U. Columbia;HarvardCfA;Caltech;U. Cincinnati;S. University;Nasa Jpl;M. I. O. Astrophysics;U. Chicago;U. Minnesota;Nist;Sbt Grenoble;U. I. Urbana-Champaign;H. University;T. U. O. Tokyo;Aix-Marseille Université;Brookhaven National Laboratory

BICEP/Keck. XVII. Line-of-sight Distortion Analysis: Estimates of Gravitational Lensing, Anisotropic Cosmic Birefringence, Patchy Reionization, and Systematic Errors

二头肌/凯克。

• DOI: 10.3847/1538-4357/acc85c
• 发表时间: 2023
• 期刊: The Astrophysical Journal
• 作者: Ade, P. A. R.;Ahmed, Z.;Amiri, M.;Barkats, D.;Thakur, R. Basu;Bischoff, C. A.;Beck, D.;Bock, J. J.;Boenish, H.;Bullock, E.
• 通讯作者: Bullock, E.