Binary Black Holes at the Extremes in the Era of Gravitational Wave Astronomy

引力波天文学时代极端的双黑洞

• 批准号: 1912578
• 负责人: Aaron Zimmerman
• 金额: $ 15万
• 依托单位: University of Texas at Austin
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-06-15 至 2022-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1912578&HistoricalAwards=false
• 关键词: Binary; Black; Holes; Extremes; Era

This award supports research in gravitational wave detector data analysis and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. This research project is devoted to the analysis and modeling of gravitational waves. These ripples in the very fabric of space and time are produced when the densest objects in the Universe -- such as black holes and neutron stars -- orbit and collide. The detection of gravitational waves by the NSF-funded LIGO and European Virgo collaborations has opened up a new window on the Universe, revealing previously invisible events like pairs of black holes merging. Members of the Austin Relativity group will participate in the analysis of gravitational waves as members of the LIGO collaboration, helping to infer the properties of the sources of these ripples. To ensure the maximum scientific benefit from the detection of gravitational waves, models for how these waves are produced require continuing refinement. Members of the research group will perform numerical simulations on supercomputers in order to explore the orbit and collision of pairs of black holes. The focus will be on extreme configurations -- such as systems with very unequal masses and complicated orbits -- with the goal of making new connections to pen and paper approximations for how gravitational waves are produced in these cases. These research activities will provide training for graduate students in high-performance computing and data analysis, skillsets which are in great demand and of great benefit to society. In addition, members of the group will engage in outreach activities in order to educate and inspire the public about this new field of physics and astronomy. Finally, members of the group will participate in outreach to high school women, in order to promote diversity within STEM fields.This project focuses on the study of binary black holes with significantly different masses, whose gravitational waves are challenging to model. This project will connect numerical simulations of these binaries with analytical approximations which are capable of modeling binaries with very unequal masses, in particular the self-force approximation. Targeted simulations will test the self-force and other approximations, provide independent verification of their predictions, reveal their limitations, and point to refined approaches for use in GW science. The key tool for making comparisons will be invariant quantities, such as the redshift factor and orbital frequency shifts of the black holes. Advances in modeling these binaries will have immediate benefits for the current era of GW detectors, and will be crucial for the success of future, space-based missions. In addition, the PI and other members of the research group will directly participate in the analysis of gravitational waves. Members of the group measure the properties of these binaries which produce these waves using Bayesian parameter estimation. These inferences are a crucial first step in the use of gravitational wave detections for understanding the population of binary black holes, inferring the nuclear equation of state from observations of binary neutron stars, testing the theory of relativity, and using gravitational waves to measure cosmic expansion.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.

该奖项支持引力波探测器数据分析的研究，并解决了NSF“宇宙之窗”大创意的优先领域。该研究项目致力于引力波的分析和建模。当宇宙中的致密物体--如黑洞和中子星--绕轨道运行并碰撞时，空间和时间结构中的这些涟漪就会产生。由NSF资助的LIGO和欧洲Virgo合作项目对引力波的探测为宇宙打开了一扇新的窗口，揭示了以前看不见的事件，如成对的黑洞合并。奥斯汀相对论小组的成员将作为LIGO合作的成员参与引力波的分析，帮助推断这些涟漪来源的性质。为了确保从引力波的探测中获得最大的科学效益，这些波是如何产生的模型需要不断完善。研究小组的成员将在超级计算机上进行数值模拟，以探索黑洞对的轨道和碰撞。重点将放在极端配置上-例如具有非常不相等的质量和复杂轨道的系统-目标是与笔和纸近似建立新的联系，以了解引力波在这些情况下是如何产生的。这些研究活动将为研究生提供高性能计算和数据分析方面的培训，这些技能对社会有很大的需求和很大的好处。此外，该小组的成员将参与外联活动，以教育和激励公众了解物理学和天文学的这一新领域。最后，为了促进STEM领域的多样性，小组成员还将参与对高中女生的宣传活动。该项目的重点是研究质量显著不同的双黑洞，其引力波具有挑战性。该项目将把这些双星的数值模拟与能够模拟质量非常不相等的双星的分析近似，特别是自作用力近似联系起来。有针对性的模拟将测试自我力量和其他近似，提供独立的验证他们的预测，揭示他们的局限性，并指出在GW科学中使用的改进方法。进行比较的关键工具将是不变量，例如红移因子和黑洞的轨道频率偏移。在模拟这些双星方面的进展将对当前的GW探测器时代产生直接的好处，并将对未来的太空任务的成功至关重要。此外，PI和研究小组的其他成员将直接参与引力波的分析。该小组的成员使用贝叶斯参数估计来测量产生这些波的这些二进制文件的属性。这些推论是利用引力波探测来理解双黑洞种群的关键第一步，从双中子星的观测中推断核状态方程，检验相对论，该奖项反映了NSF的法定使命，并通过使用基金会的智力价值进行评估，更广泛的影响审查标准。

项目成果

All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

在第三次 Advanced LIGO 和 Advanced Virgo 运行中对短引力波爆发进行全天搜索

• DOI: 10.1103/physrevd.104.122004
• 发表时间: 2021
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Abbott, R.;Abbott, T. D.;Acernese, F.;Ackley, K.;Adams, C.;Adhikari, N.;Adhikari, R. X.;Adya, V. B.;Affeldt, C.;Agarwal, D.
• 通讯作者: Agarwal, D.

A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers from the First and Second Gravitational-wave Observing Runs

• DOI: 10.3847/1538-4357/ab7d3e
• 发表时间: 2020-01
• 期刊: The Astrophysical Journal
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Sanders;K. Santiago;E. Santos;N. Sarin;B. Sassolas;B. Sathyaprakash;O. Sauter;R. Savage;V. Savant;D. Sawant;S. Sayah;D. Schaetzl;P. Schale;M. Scheel;J. Scheuer;P. Schmidt;R. Schnabel;R. Schofield;A. Schönbeck;E. Schreiber;B. Schulte;B. Schutz;O. Schwarm;E. Schwartz;J. Scott;S. Scott;E. Seidel;D. Sellers;A. Sengupta;N. Sennett;D. Sentenac;V. Sequino;A. Sergeev;Y. Setyawati;D. Shaddock;T. Shaffer;M. Shahriar;A. Sharma;P. Sharma;P. Shawhan;H. Shen;M. Shikauchi;R. Shink;D. Shoemaker;D. Shoemaker;K. Shukla;S. ShyamSundar;K. Siellez;M. Sieniawska;D. Sigg;L. Singer;Devesh Singh;N. Singh;A. Singha;A. Singhal;A. Sintes;V. Sipala;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. Smetana;J. R. Smith;Rory Smith;S. Somala;E. Son;S. Soni;B. Sorazu;V. Sordini;F. Sorrentino;T. Souradeep;E. Sowell;A. Spencer;M. Spera;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;M. Standke;D. Steer;M. Steinke;J. Steinlechner;S. Steinlechner;D. Steinmeyer;D. Stocks;D. Stops;M. Stover;K. Strain;G. Stratta;A. Strunk;R. Sturani;A. Stuver;S. Sudhagar;V. Sudhir;T. Summerscales;L. Sun;S. Sunil;A. Sur;J. Suresh;P. Sutton;B. Swinkels;M. Szczepańczyk;M. Tacca;S. Tait;C. Talbot;A. Tanasijczuk;D. Tanner;D. Tao;M. Tápai;A. Tapia;E. Martín;J. Tasson;R. Taylor;R. Tenorio;L. Terkowski;M. Thirugnanasambandam;M. Thomas;P. Thomas;J. E. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;C. Tinsman;T. R. Saravanan;S. Tiwari;S. Tiwari;V. Tiwari;K. Toland;M. Tonelli;Z. Tornasi;A. Torres-Forné;C. Torrie;I. T. E. Melo;D. Töyrä;E. Trail;F. Travasso;G. Traylor;M. Tringali;A. Tripathee;A. Trovato;R. Trudeau;K. W. Tsang;M. Tse;R. Tso;L. Tsukada;D. Tsuna;T. Tsutsui;M. Turconi;A. Ubhi;K. Ueno;D. Ugolini;C. Unnikrishnan;A. Urban;S. Usman;A. Utina;H. Vahlbruch;G. Vajente;G. Valdes;M. Valentini;N. Bakel;M. Beuzekom;J. V. D. Brand;C. Broeck;D. Vander-Hyde;L. V. D. Schaaf;J. V. Heijningen;A. V. Veggel;M. Vardaro;V. Varma;S. Vass;M. Vasúth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;Gautam Venugopalan;D. Verkindt;D. Veske;F. Vetrano;A. Viceré;A. Viets;S. Vinciguerra;D. Vine;J. Vinet;S. Vitale;F. Vivanco;T. Vo;H. Vocca;C. Vorvick;S. Vyatchanin;A. Wade;L. Wade;M. Wade;R. Walet;M. Walker;G. Wallace;L. Wallace;S. Walsh;Junfeng Wang;S. Wang;Wenwen Wang;R. Ward;Z. A. Warden;J. Warner;M. Was;J. Watchi;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;F. Wellmann;L. Wen;P. Wessels;J. Westhouse;K. Wette;J. Whelan;B. Whiting;C. Whittle;D. Wilken;D. Williams;J. Willis;B. Willke;W. Winkler;C. Wipf;H. Wittel;G. Woan;J. Woehler;J. Wofford;C. Wong;J. Wright;D. Wu;D. Wysocki;L. Xiao;H. Yamamoto;Le Yang;Y. Yang;Z. Yang;M. Yap;M. Yazback;D. Yeeles;Hang Yu;Haocun Yu;S. Yuen;A. Zadrożny;A. Zadrożny;M. Zanolin;T. Zelenova;J. Zendri;M. Zevin;J. Zhang;L. Zhang;T. Zhang;Chunnong Zhao;G. Zhao;Minchuan Zhou;Zifan Zhou;Xingjiang Zhu;A. B. Zimmerman;M. Zucker;J. Zweizig

Redshift factor and the small mass-ratio limit in binary black hole simulations

• DOI: 10.1103/physrevd.106.044006
• 发表时间: 2022-03
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Sergi Navarro Albalat;A. Zimmerman;M. Giesler;M. Scheel

Success of the small mass-ratio approximation during the final orbits of binary black hole simulations

• DOI: 10.1103/physrevd.107.084021
• 发表时间: 2022-07
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Sergi Navarro Albalat;A. Zimmerman;M. Giesler;M. Scheel

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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Grunewald;P. Gruning;D. Guerra;G. Guidi;A. R. Guimaraes;G. Guix'e;H. Gulati;H.-K. Guo;Y. Guo;Anchal Gupta;Anchal Gupta;P. Gupta;E. Gustafson;R. Gustafson;F. Guzmán;S. Ha;L. Haegel;A. Hagiwara;S. Haino;O. Halim;E. Hall;E. Hamilton;G. Hammond;W. Han;M. Haney;J. Hanks;C. Hanna;M. Hannam;O. Hannuksela;H. Hansen;T. Hansen;J. Hanson;T. Harder;T. Hardwick;K. Haris;J. Harms;G. Harry;I. Harry;D. Hartwig;K. Hasegawa;B. Haskell;R. Hasskew;C. Haster;K. Hattori;K. Haughian;H. Hayakawa;K. Hayama;F. Hayes;J. Healy;A. Heidmann;A. Heidt;M. Heintze;J. Heinze;J. Heinzel;H. Heitmann;F. Hellman;P. Hello;A. Helmling-Cornell;G. Hemming;M. Hendry;I. Heng;E. Hennes;J. Hennig;M. Hennig;A. Hernandez;F. Vivanco;M. Heurs;S. Hild;P. Hill;Y. Himemoto;A. Hines;Y. Hiranuma;N. Hirata;E. Hirose;S. Hochheim;D. Hofman;J. Hohmann;D. Holcomb;N. Holland;I. J. Hollows;Z. J. Holmes;K. Holt;D. Holz;Z. Hong;P. Hopkins;J. Hough;S. Hourihane;E. Howell;C. Hoy;D. Hoyland;A. Hreibi;B. Hsieh;Y. Hsu;G-Z. Huang;H. Huang;P. Huang;Y. Huang;Y. Huang;Y. Huang;M. Hubner;A. Huddart;B. Hughey;D. Hui;V. Hui;S. Husa;S. Huttner;R. Huxford;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;S. Ide;B. Idzkowski;A. Iess;B. Ikenoue;S. Imam;K. Inayoshi;C. Ingram;Y. Inoue;K. Ioka;M. Isi;K. Isleif;K. Ito;Y. Itoh;B. Iyer;K. Izumi;V. JaberianHamedan;T. Jacqmin;S. Jadhav;S. Jadhav;A. James;A. Jan;K. Jani;J. Janquart;K. Janssens;N. Janthalur;P. Jaranowski;D. Jariwala;R. Jaume;A. Jenkins;K. Jenner;C. Jeon;M. Jeunon;W. Jia;H. Jin;G. Johns;A. Jones;D. Jones;J. Jones;P. Jones;R. Jones;R. Jonker;L. Ju;P. Jung;K. Jung;J. Junker;V. Juste;K. Kaihotsu;T. Kajita;M. Kakizaki;C. Kalaghatgi;V. Kalogera;B. Kamai;M. Kamiizumi;N. Kanda;S. Kandhasamy;G. Kang;J. Kanner;Y. Kao;S. Kapadia;D. Kapasi;S. Karat;C. Karathanasis;S. Karki;R. Kashyap;M. Kasprzack;W. Kastaun;S. Katsanevas;E. Katsavounidis;W. Katzman;T. Kaur;K. Kawabe;K. Kawaguchi;N. Kawai;T. Kawasaki;F. K'ef'elian;D. Keitel;J. Key;S. Khadka;F. Khalili;S. Khan;E. Khazanov;N. Khetan;M. Khursheed;N. Kijbunchoo;C. Kim;J. Kim;J. Kim;K. Kim;W. Kim;Y. Kim;C. Kimball;N. Kimura;M. Kinley-Hanlon;R. Kirchhoff;J. Kissel;N. Kita;H. Kitazawa;L. Kleybolte;S. Klimenko;A. Knee;T. Knowles;E. Knyazev;P. Koch;G. Koekoek;Y. Kojima;K. Kokeyama;S. Koley;P. Kolitsidou;M. Kolstein;K. Komori;V. Kondrashov;A. Kong;A. Kontos;N. Koper;M. Korobko;K. Kotake;M. Kovalam;D. Kozak;C. Kozakai;R. Kozu;V. Kringel;N. Krishnendu;A. Kr'olak;G. Kuehn;F. Kuei;P. Kuijer;A. Kumar;P. Kumar;Rahul Kumar;Rakesh Kumar;J. Kume;K. Kuns;C. Kuo;H. Kuo;Y. Kuromiya;S. Kuroyanagi;K. Kusayanagi;S. Kuwahara;K. Kwak;P. Lagabbe;D. Laghi;É. Lalande;T. Lam;A. Lamberts;M. Landry;B. Lane;R. Lang;J. Lange;B. Lantz;I. L. Rosa;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;Y. Lecoeuche;H. Lee;H. Lee;H. W. Lee;J. Lee;K. Lee;Ray-Kuang Lee;J. Lehmann;A. Lemaitre;M. Leonardi;N. Leroy;N. Letendre;C. Lévesque;Y. Levin;J. Leviton;K. Leyde;A. Li;B. Li;J. Li;K. Li;T. G. F. Li;X. Li;C.Y. Lin;F. Lin;F. Lin;H. Lin;L. Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;M. Llorens-Monteagudo;R. K. Lo;A. Lockwood;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Luck;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;R. Macas;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;C. Makarem;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;J. Mango;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;M. Marchiò;F. Marion;Z. Mark;S. M'arka;Z. M'arka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. 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Pannarale;B. Pant;F. Panther;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Paul;E. Payne;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;C. Perkins;A. Perreca;S. Perriès;J. Petermann;D. Petterson;H. Pfeiffer;K. A. Pham;K. S. Phukon;O. Piccinni;M. Pichot;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;I. Pinto;M. Pinto;K. Piotrzkowski;M. Pirello;M. Pitkin;E. Placidi;L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;P. Popolizio;E. Porter;R. Poulton;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;M. Principe;G. Prodi;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;V. Quetschke;R. Quitzow-James;F. Raab;G. Raaijmakers;H. Radkins;N. Radulesco;P. Raffai;S. X. 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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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