AccelNet-Implementation: The International Pulsar Timing Array

AccelNet-Implementation：国际脉冲星计时阵列

• 批准号: 2114721
• 负责人: Maura McLaughlin
• 金额: $ 199.81万
• 依托单位: West Virginia University Research Corporation
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-01-01 至 2026-12-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2114721&HistoricalAwards=false
• 关键词: AccelNet; Implementation; International; Pulsar; Timing

Gravitational waves are ripples in spacetime, predicted to exist by Einstein's theory of general relativity. They are emitted by accelerating, massive objects and travel at the speed of light, unimpeded by matter such as galaxies, stars, and gas. Gravitational waves from the merger of two black holes were detected by the LIGO collaboration in 2015, allowing astronomers to "see" previously invisible objects and probe the most energetic processes in the universe. The International Pulsar Timing Array (IPTA) is a world-wide network of researchers and students working to directly detect gravitational at frequencies 11 orders of magnitude smaller than LIGO through observations of precise celestial clocks called radio pulsars using the world's largest radio telescopes. This AccelNet-Implementation project will broaden the reach of the IPTA beyond researchers and students from North America, Europe, and Australia to include China, India, and South Africa. In addition to enhancing observations of pulsars distributed across the sky, the expanded IPTA network will provide sophisticated cyber-infrastructure and training for students and postdoctoral researchers in astrophysics, radio instrumentation, signal processing, and data science. The IPTA expects to detect gravitational waves from supermassive binary black holes at the cores of merging galaxies. These detections will provide new insights into galaxy growth and evolution through cosmic time, transforming our understanding of the Universe. By the end of the award period, the IPTA will detect and characterize the stochastic background of gravitational waves produced by all the supermassive binary black holes in the Universe. It is also likely to detect the first individual supermassive black hole binary that stands out above the background. This international coordination of research will also result in very high impact synergistic science such as neutron star mass measurements, characterization of the interstellar medium, tests of general relativity, and the discovery of exotic pulsar systems and radio transients such as Fast Radio Bursts. Coordination will be facilitated through annual workshops, meetings, and shared data and analysis portal. Students and postdoctoral researchers in the IPTA will be involved in an international mentoring network and will learn valuable outreach skills, while at the same time bringing the excitement of this work to K-12 students worldwide.The Accelerating Research through International Network-to-Network Collaborations (AccelNet) program is designed to accelerate the process of scientific discovery and prepare the next generation of U.S. researchers for multiteam international collaborations. The AccelNet program supports strategic linkages among U.S. research networks and complementary networks abroad that will leverage research and educational resources to tackle grand scientific challenges that require significant coordinated international efforts.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.

引力波是时空中的涟漪，爱因斯坦的广义相对论预言了它的存在。它们是由加速的大质量物体发射的，以光速传播，不受星系，恒星和气体等物质的阻碍。2015年，LIGO合作探测到了两个黑洞合并产生的引力波，使天文学家能够“看到”以前不可见的物体，并探测宇宙中最具能量的过程。国际脉冲星定时阵列（IPTA）是一个由研究人员和学生组成的全球网络，致力于通过使用世界上最大的射电望远镜观测称为射电天文钟的精确天体时钟，以比LIGO小11个数量级的频率直接探测引力。这一网络实施项目将扩大IPTA的影响范围，使其超越北美、欧洲和澳大利亚的研究人员和学生，包括中国、印度和南非。除了加强对分布在天空中的卫星的观测外，扩展后的IPTA网络还将为天体物理学、无线电仪器、信号处理和数据科学领域的学生和博士后研究人员提供先进的网络基础设施和培训。IPTA希望探测到来自合并星系核心的超大质量双黑洞的引力波。这些探测将为星系在宇宙时间中的生长和演化提供新的见解，改变我们对宇宙的理解。到奖励期结束时，IPTA将探测和表征宇宙中所有超大质量双黑洞产生的引力波的随机背景。它也有可能探测到第一个在背景之上脱颖而出的超大质量黑洞双星。这种研究的国际协调也将导致非常高的影响协同科学，如中子星星质量测量，星际介质的表征，广义相对论的测试，以及发现奇异的脉冲星系统和无线电瞬变，如快速无线电爆发。 将通过年度讲习班、会议以及共享数据和分析门户促进协调。 IPTA的学生和博士后研究人员将参与国际指导网络，并将学习宝贵的推广技能，与此同时，我们也将这项工作带给全世界的K-12学生。通过国际网络对网络合作加速研究（中网）该计划旨在加速科学发现的进程，并为下一代美国研究人员参加国际多团队合作做好准备合作。该奖项反映了NSF的法定使命，并通过使用基金会的知识价值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

The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave Background

• DOI: 10.3847/2041-8213/acf4fd
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal Letters
• 作者: G. Agazie;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;B. Bécsy;L. Blecha;A. Brazier;P. Brook;S. Burke-Spolaor;J. A. Casey-Clyde;M. Charisi;S. Chatterjee;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;M. DeCesar;P. Demorest;T. Dolch;B. Drachler;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;E. Gardiner;N. Garver-Daniels;P. Gentile;J. Glaser;D. Good;K. Gültekin;J. Hazboun;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;N. Laal;M. Lam;W. Lamb;T. Joseph W. Lazio;N. Lewandowska;Tingting Liu;D. Lorimer;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;C. Mingarelli;A. Mitridate;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;A. Susobhanan;J. Swiggum;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;S. Vigeland;H. Wahl;C. Witt;O. Young

The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget

NANOGrav 15 年数据集：探测器特征和噪声预算

• DOI: 10.3847/2041-8213/acda88
• 发表时间: 2023
• 期刊: The Astrophysical Journal Letters
• 作者: Agazie, Gabriella;Anumarlapudi, Akash;Archibald, Anne M.;Arzoumanian, Zaven;Baker, Paul T.;Bécsy, Bence;Blecha, Laura;Brazier, Adam;Brook, Paul R.;Burke-Spolaor, Sarah
• 通讯作者: Burke-Spolaor, Sarah

The NANOGrav 15 yr Data Set: Search for Signals from New Physics

• DOI: 10.3847/2041-8213/acdc91
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal Letters
• 作者: A. Afzal;G. Agazie;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;B. B'ecsy;J. Blanco-Pillado;L. Blecha;K. Boddy;A. Brazier;P. Brook;S. Burke-Spolaor;R. Burnette;R. Case;M. Charisi;S. Chatterjee;K. Chatziioannou;B. Cheeseboro;Siyuan Chen;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;C. Cutler;M. DeCesar;D. DeGan;P. Demorest;Heling Deng;T. Dolch;B. Drachler;R. V. Eckardstein;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;N. Garver-Daniels;P. Gentile;K. A. Gersbach;J. Glaser;D. Good;Lydia Guertin;K. Gultekin;J. Hazboun;S. Hourihane;K. Islo;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;N. Laal;M. Lam;W. Lamb;T. Lazio;Vincent S. H. Lee;N. Lewandowska;Rafael R. Lino dos Santos;T. Littenberg;Tianyu Liu;D. Lorimer;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;J. Nay;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;T. Schroder;L. Schult;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;Peter Stratmann;Jerry P. Sun;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;T. Trickle;J. E. Turner;C. Unal;M. Vallisneri;Sonali Verma;S. Vigeland;H. Wahl;Qiaohong Wang;C. Witt;Davis Wright;O. Young;K. Zurek

The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

• DOI: 10.3847/2041-8213/ace18a
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal Letters
• 作者: G. Agazie;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;B. B'ecsy;L. Blecha;A. Brazier;P. Brook;S. Burke-Spolaor;R. Case;J. A. Casey-Clyde;M. Charisi;S. Chatterjee;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;M. DeCesar;P. Demorest;Matthew C. Digman;T. Dolch;B. Drachler;E. Ferrara;W. Fiore;E. Fonseca;Gabriel Freedman;N. Garver-Daniels;P. Gentile;J. Glaser;D. Good;K. Gultekin;J. Hazboun;S. Hourihane;R. Jennings;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;Tingting Liu;D. Lorimer;Jingshu Luo;R. Lynch;Chung-Pei Ma;D. Madison;A. McEwen;J. McKee;M. Mclaughlin;N. McMann;B. W. Meyers;P. Meyers;C. Mingarelli;A. Mitridate;P. Natarajan;C. Ng;D. Nice;S. Ocker;K. Olum;T. Pennucci;B. Perera;P. Petrov;N. Pol;H. Radovan;S. Ransom;P. Ray;Jo√£o Romano;S. C. Sardesai;A. Schmiedekamp;C. Schmiedekamp;K. Schmitz;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;A. Susobhanan;J. Swiggum;Jacob M. Taylor;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;R. V. Haasteren;S. Vigeland;H. Wahl;C. Witt;O. Young

The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars

• DOI: 10.3847/2041-8213/acda9a
• 发表时间: 2023-06
• 期刊: The Astrophysical Journal Letters
• 作者: G. Agazie;Md F. Alam;A. Anumarlapudi;A. Archibald;Z. Arzoumanian;P. Baker;L. Blecha;Victoria Bonidie;A. Brazier;P. Brook;S. Burke-Spolaor;B. B'ecsy;Christopher Chapman;M. Charisi;S. Chatterjee;T. Cohen;J. Cordes;N. Cornish;F. Crawford;H. Cromartie;K. Crowter;M. DeCesar;P. Demorest;T. Dolch;B. Drachler;E. Ferrara;W. Fiore;E. Fonseca;G. Freedman;N. Garver-Daniels;P. Gentile;J. Glaser;D. Good;K. Gultekin;J. Hazboun;R. Jennings;Cody Jessup;A. Johnson;Megan L. Jones;A. Kaiser;D. Kaplan;L. Kelley;M. Kerr;J. Key;A. Kuske;N. Laal;M. Lam;W. Lamb;T. Lazio;N. Lewandowska;Ye Lin;Tianyu Liu;D. Lorimer;Jing Luo;R. Lynch;Chung-Pei Ma;D. Madison;Kaleb Maraccini;A. McEwen;J. McKee;Maura A. McLaughlin;N. McMann;B. W. Meyers;C. Mingarelli;A. Mitridate;C. Ng;D. Nice;S. Ocker;K. Olum;Elisa Panciu;T. Pennucci;B. Perera;N. Pol;H. Radovan;S. Ransom;P. Ray;J. Romano;Laura Salo;S. C. Sardesai;C. Schmiedekamp;A. Schmiedekamp;K. Schmitz;B. Shapiro-Albert;X. Siemens;J. Simon;M. Siwek;I. Stairs;D. Stinebring;K. Stovall;A. Susobhanan;J. Swiggum;S. Taylor;J. E. Turner;C. Unal;M. Vallisneri;S. Vigeland;H. Wahl;Qiaohong Wang;C. Witt;O. Young