Unmasking the Remnants of Gamma-Ray Bursts in the Era of Gravitational Wave Astronomy

揭开引力波天文学时代伽马射线暴残余的面纱

• 批准号: 2011608
• 负责人: Alessandra Corsi
• 金额: $ 26.25万
• 依托单位: Texas Tech University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-08-01 至 2025-07-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2011608&HistoricalAwards=false
• 关键词: Unmasking; Remnants; Gamma; Ray; Bursts

This award supports research in relativity and relativistic astrophysics and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. The era of gravitational-wave multi-messenger astronomy started on 2017 August 17, when LIGO (the Laser Interferometer Gravitational Wave Observatory) discovered an event dubbed GW170817. This was the very first direct observation of gravitational waves from a binary neutron star in-spiral, which was accompanied by the detection of light at all wavelengths. The multi-messenger observations of GW170817 have crucially informed a large variety of fields including gravitational physics, nuclear physics, cosmology, and relativistic astrophysics. In spite of the spectacular progress, several questions remain open. A key one is whether the stellar object leftover from the merger is a short-lived neutron star, a long-lived neutron star, or a promptly formed black hole. This award supports searches of LIGO data for signatures aimed at uncovering the nature of the merger remnant. Studying how the nature of the remnant depends on the properties of the merging objects can unlock the fundamental physics of matter at densities much larger than those that can be probed in Earth-based laboratories and clarify the physics of some of the most exotic objects in the stellar graveyard. This project also supports the training of graduate and undergraduate students who will constitute the next generation of scientists, and several outreach activities aimed at presenting LIGO results to the general public and K12 students. Specific intellectual goals are: (i) Unmasking the remnants of compact object mergers accompanied by gamma-ray bursts by carrying out searches for gravitational waves from newly formed neutron stars; (ii) Assessing the efficiency of the newly-developed Cross-Correlation Algorithm (CoCoA) in detecting the full zoo of possible gravitational wave signals from merger remnants, and its efficacy in post-detection parameter estimation; (iii) Quantifying the potential for discovery of gravitational waves from neutron stars formed in long gamma-ray bursts by future upgraded gravitational wave detectors. Broader impact goals are: (i) Bringing age-appropriate presentations and LIGO-related outreach activities to under-represented groups by leveraging the TTU Honors College-Bayless Elementary School mentoring program; (ii) Presenting a LIGO prize to the South Plains Regional Science Fair; (iii) Presenting LIGO results to the general public during the Astronight at TTU.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.

该奖项支持相对论和相对论天体物理学的研究，并解决了NSF“宇宙之窗”大理念的优先领域。引力波多信使天文学的时代始于2017年8月17日，当时LIGO（激光干涉引力波天文台）发现了一个名为GW 170817的事件。这是第一次直接观测到来自螺旋状双中子星星的引力波，同时还探测到了所有波长的光。对GW 170817的多信使观测为包括引力物理、核物理、宇宙学和相对论天体物理在内的众多领域提供了重要信息。尽管取得了令人瞩目的进展，但仍有几个问题有待解决。一个关键的问题是，合并后的恒星物体是一颗寿命短的中子星星星，还是一颗寿命长的中子星星星，还是一个迅速形成的黑洞。该奖项支持对LIGO数据的签名搜索，旨在揭示合并残余物的性质。研究残骸的性质如何取决于合并物体的性质，可以解开物质的基本物理学，其密度远远大于地球实验室可以探测的密度，并澄清恒星墓地中一些最奇特物体的物理学。该项目还支持培养将成为下一代科学家的研究生和本科生，以及旨在向公众和K12学生展示LIGO结果的几项推广活动。具体的智力目标是：通过搜寻新形成的中子星产生的引力波，揭开伴随伽马射线爆发的致密物体合并的残余物;评估新开发的互相关算法（可可CoCoA）在探测合并残余物可能产生的全部引力波信号方面的效率，及其在探测后参数估计方面的功效; ㈢用今后升级的引力波探测器对发现中子星引力波的潜力进行量化，中子星引力波是在长伽马射线爆发中形成的。更广泛的影响目标是：（i）通过利用TTU荣誉学院-贝利斯小学辅导方案，向代表性不足的群体提供适合年龄的演讲和与LIGO有关的外联活动;（ii）向南平原地区科学博览会颁发LIGO奖;（三）在TTU的Astronight期间向公众展示LIGO结果。该奖项反映了NSF的法定使命，并通过使用基金会的学术价值和更广泛的影响审查标准。

项目成果

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3b

• DOI: 10.3847/1538-4357/ac532b
• 发表时间: 2021-11
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;N. Adhikari;R. Adhikari;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;S. Albanesi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;T. Andrade;N. Andrés;T. Andri'c;S. Angelova;S. Ansoldi;J. Antelis;S. Antier;S. Appert;K. Arai;K. Arai;Y. Arai;S. Araki;A. Araya;M. Araya;J. Areeda;M. Arène;N. Aritomi;N. Arnaud;S. Aronson;K. Arun;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. Aston;P. Astone;F. Aubin;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;M. Barton;I. Bartos;R. Bassiri;A. Basti;M. Bawaj;J. Bayley;A. Baylor;M. Bazzan;B. B'ecsy;V. Bedakihale;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;U. Bhardwaj;D. Bhattacharjee;S. Bhaumik;I. Bilenko;G. Billingsley;S. Bini;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;C. Blair;D. Blair;R. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;L. D. Bonavena;F. Bondu;E. Bonilla;R. Bonnand;P. Booker;B. A. Boom;R. Bork;V. Boschi;N. Bose;S. Bose;V. Bossilkov;V. Boudart;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;A. Bramley;A. Branch;M. Branchesi;J. Brau;M. Breschi;T. Briant;J. Briggs;A. Brillet;M. Brinkmann;P. Brockill;A. Brooks;J. Brooks;D. Brown;S. Brunett;G. Bruno;R. Bruntz;J. Bryant;T. Bulik;H. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;C. Buy;R. Byer;L. Cadonati;G. Cagnoli;C. Cahillane;J. C. Bustillo;J. Callaghan;T. Callister;E. 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Strunk;R. Sturani;A. Stuver;S. Sudhagar;V. Sudhir;R. Sugimoto;H. Suh;T. Summerscales;H. Sun;L. Sun;S. Sunil;A. Sur;J. Suresh;P. Sutton;Takamasa Suzuki;Toshikazu Suzuki;B. Swinkels;M. J. Szczepa'nczyk;P. Szewczyk;M. Tacca;H. Tagoshi;S. Tait;H. Takahashi;R. Takahashi;A. Takamori;S. Takano;H. Takeda;M. Takeda;C. Talbot;C. Talbot;H. Tanaka;Kazuyuki D. Tanaka;Kenta Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;L. Tao;E. Mart'in;C. Taranto;J. Tasson;S. Telada;R. Tenorio;J. Terhune;L. Terkowski;M. Thirugnanasambandam;M. Thomas;P. Thomas;E. E. Thompson-E.;J. E. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;A. Toivonen;K. Toland;A. Tolley;T. Tomaru;Y. Tomigami;T. Tomura;M. Tonelli;A. Torres-Forn'e;C. Torrie;I. T. E. Melo;D. Toyra;A. Trapananti;F. Travasso;G. Traylor;M. Trevor;M. Tringali;A. Tripathee;L. Troiano;A. Trovato;L. Trozzo;R. Trudeau;D. Tsai;D. Tsai;K. W. Tsang;T. Tsang;J. Tsao;M. Tse;R. Tso;K. Tsubono;S. Tsuchida;L. 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