Technologies for Future Gravitational-Wave Observatories: Lasers, Optics, Materials, Cryogenics, and Simulations

未来引力波天文台技术：激光、光学、材料、低温和模拟

• 批准号: 2012021
• 负责人: David Tanner
• 金额: $ 90万
• 依托单位: University of Florida
• 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: 2020-07-01 至 2024-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2012021&HistoricalAwards=false
• 关键词: Technologies; Future; Gravitational; Wave; Observatories

This award supports research in relativity and relativistic astrophysics and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. Beginning in September 2015, the two Advanced LIGO observatories, in conjunction with Virgo, have carried out observational campaigns for gravitational waves, with more than 10 inspirals of compact objects reported from observing runs O1 and O2. The just-ended O3 run detected more than 50 additional signals, most of which appear likely to be inspirals of black holes and/or neutron stars. One report of a novel source has been published, with other very interesting announcements expected. Improvements in sensitivity and performance are continuing, and Florida’s research aims at contributing to these improvements as well as to designs of third-generation gravitational-wave detectors. This work will develop national and international scientific infrastructure through the direct participation of the University of Florida LIGO group in research and operations at the LIGO Observatories. The research will go beyond gravitational-wave science. High-power optical isolators developed in this project have commercial applications to the laser and optics industries. A single-frequency 2.1 μm laser, tunable over GHz of frequency, can affect many areas of precision science. The Florida group also gives students and postdoctoral scientists the opportunity to develop scientific skills from a diverse set of disciplines spanning lasers and optics, electronics and feedback control systems, vacuum and cryogenics, and large-scale detector commissioning and operation. In addition, the group places high value on the education of undergraduate students and each year has involved undergraduates in research.Advanced LIGO was designed for a 10x sensitivity improvement and much better low-frequency response than initial LIGO. With the introduction of squeezing and the A+ upgrade, the sensitivity will be increased further. These gains require improved performance in all aspects of the detector, including the Input Optics, a responsibility of the Florida LIGO group for many years. Work will address high-power optical isolation, RF modulation, adaptive elements for mode matching, shadow sensors for sensing and control of suspended mirrors and platforms, and improved simulations of the input optics and power/signal recycling cavities. It also addresses basic research needed for next generation detectors to increase the science reach of the observatories. This longer-ranged research includes studies of impurities in silicon, a nearly ideal material for the test masses of cryogenic detectors, cryogenic shadow sensors, and the development of a single-frequency non-planar ring oscillator laser operating at 2.1 μm wavelength.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”大构想的优先领域。从 2015 年 9 月开始，两个高级 LIGO 观测站与 Virgo 联合开展了引力波观测活动。 ，观测运行 O1 和 O2 报告了 10 多个致密天体的螺旋，刚刚结束的 O3 运行检测到了 50 多个附加信号，其中大部分是。看起来很可能是黑洞和/或中子星的灵感，一份关于新来源的报告已经发表，预计灵敏度和性能的其他改进正在继续，佛罗里达州的研究旨在为这些改进做出贡献。这项工作将通过佛罗里达大学 LIGO 小组直接参与 LIGO 天文台的研究和运营来开发国家和国际科学基础设施。该项目开发的高功率光学隔离器在激光和光学行业具有商业应用，频率可调谐超过 GHz，佛罗里达小组也能影响精密科学的许多领域。为学生和博士后科学家提供了发展激光和光学、电子和反馈控制系统、真空和低温以及大规模探测器调试和操作等多种学科的科学技能的机会。高度重视本科生的教育，每年都有本科生参与研究。高级 LIGO 的灵敏度比初始 LIGO 提高了 10 倍，低频响应也更好。随着压缩的引入和 A+ 升级，灵敏度将提高。这些增益需要提高探测器各个方面的性能，包括输入光学，这是佛罗里达 LIGO 小组多年来的职责，将解决高功率光学隔离、射频调制、模式匹配的自适应元件、阴影传感器用于悬浮镜子和平台的传感和控制，以及改进输入光学和功率/信号回收腔的模拟，它还解决了下一代探测器所需的基础研究，以扩大天文台的科学范围。硅中的杂质，这是一种近乎理想的材料，用于低温探测器反射、低温阴影传感器的测试质量，以及开发工作在 2.1 μm 波长的单频非平面环形振荡器激光器。该奖项通过使用基金会的智力价值和更广泛的影响审查标准进行评估，NSF 的法定使命被认为值得支持。

项目成果

Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910

• DOI: 10.3847/2041-8213/abffcd
• 发表时间: 2020-12
• 期刊: The Astrophysical Journal Letters
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;T. Abbott;S. Abraham;F. Acernese;K. Ackley;A. Adams;C. Adams;R. Adhikari;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;K. M. Aleman;G. Allen;A. Allocca;P. Altin;A. Amato;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;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;S. Aston;P. Astone;F. Aubin;P. Aufmuth;K. AultONeal;C. Austin;S. Babak;F. Badaracco;M. Bader;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. Ballmer;M. Bals;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;R. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;S. Barnum;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;M. Benjamin;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;D. Bersanetti;A. Bertolini;J. Betzwieser;R. Bhandare;A. Bhandari;D. Bhattacharjee;S. Bhaumik;J. Bidler;I. Bilenko;G. Billingsley;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;J. Blackman;C. Blair;D. Blair;R. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;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;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;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;L. Cadonati;M. Caesar;G. Cagnoli;C. Cahillane;H. Cain;J. C. Bustillo;J. Callaghan;T. Callister;E. 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Merzougui;S. Meshkov;C. Messenger;C. Messick;P. Meyers;F. Meylahn;A. Mhaske;A. Miani;H. Miao;I. Michaloliakos;C. Michel;Y. Michimura;H. Middleton;L. Milano;A. Miller;M. Millhouse;J. Mills;E. Milotti;M. Milovich-Goff;O. Minazzoli;Y. Minenkov;N. Mio;L. Mir;A. Mishkin;C. Mishra;T. Mishra;T. Mistry;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;O. Miyakawa;A. Miyamoto;Y. Miyazaki;K. Miyo;S. Miyoki;G. Mo;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;D. Moraru;F. Morawski;A. More;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;W. Ni;S. Nichols;A. Nishizawa;S. Nissanke;F. Nocera;M. Noh;M. Norman;C. North;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. Oh;M. Ohashi;N. Ohishi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;K. Okutomi;C. Olivetto;K. Oohara;C. Ooi;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;L. F. Ortega;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;M. Page;G. Pagliaroli;A. Pai;S. Pai;J. R. Palamos;O. Palashov;C. Palomba;K. Pan;P. K. Panda;H. Pang;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;B. Patricelli;E. Payne;T. Pechsiri;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;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;F. Pilo;L. Pinard;I. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;M. Pitkin;E. Placidi;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;P. Popolizio;E. Porter;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;T. Prestegard;M. Principe;G. Prodi;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;V. Quetschke;P. J. Quinonez;R. Quitzow-James;F. Raab;G. Raaijmakers;H. Radkins;N. Radulesco;P. Raffai;S. X. Rail;S. Raja;C. Rajan;K. Ramirez;T. Ramirez;A. Ramos-Buades;J. Rana;P. Rapagnani;U. Rapol;B. Ratto;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;D. Reitze;P. Relton;P. Rettegno;F. Ricci;C. J. Richardson;J. Richardson;L. Richardson;P. Ricker;G. Riemenschneider;K. Riles;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;J. Rocha;S. Rodriguez;R. D. Rodriguez-Soto;L. Rolland;J. Rollins;V. Roma;M. Romanelli;R. Romano;C. Romel;A. Romero;I. Romero-Shaw;J. Romie;C. Rose;D. Rosi'nska;S. Rosofsky;M. Ross;S. Rowan;S. Rowlinson;S. Roy;S. Roy;D. Rozza;P. Ruggi;K. Ryan;S. Sachdev;T. Sadecki;J. Sadiq;N. Sago;S. Saito;Y. Saito;K. Sakai;Y. Sakai;M. Sakellariadou;Y. Sakuno;O. Salafia;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;E. Sanchez;J. H. Sánchez;L. Sanchez;N. Sanchis-Gual;J. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;S. Sato;T. Sato;O. Sauter;R. Savage;V. Savant;T. Sawada;D. Sawant;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;A. Schindler-Tyka;P. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;E. Seidel;T. Sekiguchi;Y. Sekiguchi;D. Sellers;A. Sengupta;N. Sennett;D. Sentenac;E. Seo;V. Sequino;Y. Setyawati;T. Shaffer;M. Shahriar;B. Shams;L. Shao;S. Sharifi;A. Sharma;P. Sharma;P. Shawhan;N. Shcheblanov;H. Shen;S. Shibagaki;M. Shikauchi;R. Shimizu;T. Shimoda;K. Shimode;R. Shink;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;K. Shukla;S. Shyamsundar;M. Sieniawska;D. Sigg;L. Singer;D. Singh;N. Singh;A. Singha;A. Sintes;V. Sipala;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. Smetana;J. R. Smith;R. Smith;S. Somala;K. Somiya;E. Son;K. Soni;S. Soni;B. Sorazu;V. Sordini;F. Sorrentino;N. Sorrentino;H. Sotani;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. Spencer;M. Spera;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;D. Steer;J. Steinlechner;S. Steinlechner;D. Stops;M. Stover;K. Strain;L. Strang;G. Stratta;A. Strunk;R. Sturani;A. Stuver;J. Sudbeck;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;H. Tanaka;Kazuyuki Tanaka;Kenta Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;A. Tapia;E. Martín;J. Tasson;S. Telada;R. Tenorio;L. Terkowski;M. Test;M. Thirugnanasambandam;M. Thomas;P. Thomas;J. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;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. 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. Tsukada;D. Tsuna;T. Tsutsui;T. Tsuzuki;M. Turconi;D. Tuyenbayev;A. Ubhi;N. Uchikata;T. Uchiyama;R. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;D. Ugolini;C. Unnikrishnan;F. Uraguchi;A. Urban;T. Ushiba;S. A. Usman;A. Utina;H. Vahlbruch;G. Vajente;A. Vajpeyi;G. Valdes;M. Valentini;V. Valsan;N. Bakel;M. Beuzekom;J. Brand;C. Broeck;D. Vander-Hyde;L. V. D. Schaaf;J. V. Heijningen;M. Putten;M. Vardaro;A. Vargas;V. Varma;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;J. Venneberg;Gautam Venugopalan;D. Verkindt;Y. Verma;D. Veske;F. Vetrano;A. Vicer'e;A. Viets;V. Villa-Ortega;J. Vinet;S. Vitale;T. Vo;H. Vocca;E. V. Reis;C. Vorvick;S. Vyatchanin;L. Wade;M. Wade;K. Wagner;R. Walet;M. Walker;G. Wallace;L. Wallace;S. Walsh;J. Wang;J. Wang;W. H. Wang;R. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;L. Wei;M. Weinert;A. Weinstein;R. Weiss;C. Weller;F. Wellmann;L. Wen;P. Wessels;J. Westhouse;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. J. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;W. Winkler;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;I. C. Wong;J. Wrangel;C. Wu;D. Wu;H. Wu;S. Wu;D. Wysocki;L. Xiao;W-R. Xu;T. Yamada;H. Yamamoto;Kazuhiro Yamamoto;Kohei Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;F. Yang;L. Yang;Yang Yang-Yang;Yi Yang;Z. Yang;M. Yap;D. Yeeles;Anjali B. Yelikar;M. Ying;K. Yokogawa;J. Yokoyama;T. Yokozawa;A. Yoon;T. Yoshioka;Hang Yu;Haocun Yu;H. Yuzurihara;A. Zadro.zny;M. Zanolin;S. Zeidler;T. Zelenova;J. Zendri;M. Zevin;M. Zhan;H. Zhang;J. Zhang;L. Zhang;R. Zhang;T. Zhang;C. Zhao;G. Zhao;Yue Zhao;Yuhang Zhao;Z. Zhou;X. Zhu;Z. Zhu;M. Zucker;J. Zweizig;D. Antonopoulou;Z. Arzoumanian;T. Enoto;C. Espinoza;S. Guillot

LIGO’s quantum response to squeezed states

• DOI: 10.1103/physrevd.104.062006
• 发表时间: 2021-05
• 期刊: Physical Review D
• 影响因子: 5
• 作者: L. McCuller;S. Dwyer;A. Green;Haocun Yu;L. Barsotti;C. Blair;D. Brown;A. Effler;M. Evans;Á. Fernández-Galiana;P. Fritschel;V. Frolov;N. Kijbunchoo;G. Mansell;F. Matichard;N. Mavalvala;D. McClelland;T. McRae;A. Mullavey;D. Sigg;B. Slagmolen;M. Tse;T. Vo;R. Ward;C. Whittle;R. Abbott;C. Adams;R. Adhikari;A. Ananyeva;S. Appert;K. Arai;J. Areeda;Y. Asali;0. S. M. Aston;C. Austin;A. Baer;M. Ball;S. Ballmer;S. Banagiri;D. Barker;J. Bartlett;B. Berger;J. Betzwieser;D. Bhattacharjee;G. Billingsley;S. Biscans;R. Blair;N. Bode;P. Booker;R. Bork;A. Bramley;A. Brooks;A. Buikema;C. Cahillane;K. Cannon;X. Chen;0. A. A. Ciobanu-0.-A.-A.-Ciobanu-2105164804;F. Clara;C. Compton;S. Cooper;K. Corley;0. S. T. Countryman;0. P. B. Covas;D. Coyne;L. Datrier;D. Davis;C. D. Fronzo;K. Dooley;J. Driggers;T. Etzel;T. Evans;J. Feicht;P. Fulda;M. Fyffe;J. Giaime;K. Giardina;P. Godwin;E. Goetz;S. Gras;C. Gray;R. Gray;E. Gustafson;R. Gustafson;J. Hanks;J. Hanson;T. Hardwick;R. Hasskew;M. Heintze;A. Helmling-Cornell;N. Holland;J. Jones;S. Kandhasamy;S. Karki;M. Kasprzack;K. Kawabe;P. King;J. Kissel;Rahul Kumar;M. Landry;B. Lane;B. Lantz;M. Laxen;Y. Lecoeuche;J. Leviton;J. Liu;M. Lormand;A. Lundgren;0. R. Macas;M. Macinnis;D. Macleod;S. Márka;0. Z. Marka;0. D. V. Martynov;K. Mason;T. Massinger;R. McCarthy;S. Mccormick;J. McIver;G. Mendell;K. Merfeld;E. Merilh;F. Meylahn;T. Mistry;R. Mittleman;G. Moreno;C. Mow-Lowry;S. Mozzon;0. T. J. N. Nelson;P. Nguyen;L. Nuttall;0. J. Oberling;R. Oram;C. Osthelder;D. Ottaway;H. Overmier;J. R. Palamos;W. Parker;E. Payne;A. Pele;R. Penhorwood;C. Perez;M. Pirello;H. Radkins;K. Ramirez;J. Richardson;K. Riles;N. Robertson;J. Rollins;C. Romel;J. Romie;M. Ross;K. Ryan;T. Sadecki;E. Sanchez;L. Sanchez;T. R. Saravanan;R. Savage;D. Schaetzl;R. Schnabel;R. Schofield;E. Schwartz;D. Sellers;T. Shaffer;J. R. Smith;S. Soni;B. Sorazu;A. Spencer;K. Strain;L. Sun;M. Szczepańczyk;M. Thomas;P. Thomas;K. Thorne;K. Toland;C. Torrie;G. Traylor;A. Urban;G. Vajente;G. Valdes;D. Vander-Hyde;P. Veitch;K. Venkateswara;Gautam Venugopalan;A. Viets;C. Vorvick;M. Wade;J. Warner;B. Weaver;R. Weiss;B. Willke;C. Wipf;L. Xiao;H. Yamamoto;Hang Yu;L. Zhang;M. Zucker;J. V. R. I. O. Technology;Ligo Hanford Observatory;U. Florida;Ligo Livingston Observatory;OzGrav;U. Adelaide;A. N. University;Ligo;C. I. O. Technology.;S. University;C. Fullerton;C. University;Louisiana State University;Christopher Newport University;U. Oregon;U. Minnesota;S. University;Missouri University of Science;Technology;M. F. Physics;L. Hannover;Resceu;U. Tokyo;U. O. S. Australia;U. Birmingham;Universitat de les Illes Balears;Supa;U. Glasgow;Cardiff University;The University of Mississippi;T. O. S. University;U. Columbia;U. Michigan;Inter-University Centre for Astronomy;Astrophysics;U. Portsmouth;The University of Sheffield;S. University;A. College;S. O. PhysicsAstronomy;The Valley;U. Washington;U. Hamburg;Concordia University Wisconsin;Kenyon College

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run

• DOI: 10.1103/physrevx.11.021053
• 发表时间: 2021-06-09
• 期刊: PHYSICAL REVIEW X
• 影响因子: 12.5
• 作者: Abbott, R.;Abbott, T. D.;Zweizig, J.
• 通讯作者: Zweizig, J.

Input optics systems of the KAGRA detector during O3GK

• DOI: 10.1093/ptep/ptac166
• 发表时间: 2022-10
• 期刊: Progress of Theoretical and Experimental Physics
• 影响因子: 3.5
• 作者: T. Akutsu;M. Ando;K. Arai;Y. Arai;S. Araki;A. Araya;N. Aritomi;H. Asada;Y. Aso;S. Bae;Y. Bae;L. Baiotti;R. Bajpai;M. Barton;K. Cannon;Z. Cao;E. Capocasa;M. Chan;C. Chen;K. Chen;Y. Chen;C. Chiang;H. Chu;Y. Chu;S. Eguchi;Y. Enomoto;R. Flaminio;Y. Fujii;Y. Fujikawa;M. Fukunaga;M. Fukushima;T. Furuhata;D. Gao;G. Ge;S. Ha;A. Hagiwara;S. Haino;W. Han;K. Hasegawa;K. Hattori;H. Hayakawa;K. Hayama;Y. Himemoto;Y. Hiranuma;N. Hirata;E. Hirose;Z. Hong;B. Hsieh;G-Z. Huang;H. Huang;P. Huang;Y. Huang;Y. Huang;D. Hui;S. Ide;B. Ikenoue;S. Imam;K. Inayoshi;Y. Inoue;K. Ioka;K. Ito;Y. Itoh;K. Izumi;C. Jeon;H. Jin;K. Jung;P. Jung;K. Kaihotsu;T. Kajita;M. Kakizaki;M. Kamiizumi;S. Kanbara;N. Kanda;G. Kang;Y. Kataoka;K. Kawaguchi;N. Kawai;T. Kawasaki;C. Kim;J. Kim;J. Kim;W. Kim;Y. Kim;N. Kimura;N. Kita;H. Kitazawa;Y. Kojima;K. Kokeyama;K. Komori;A. Kong;K. Kotake;C. Kozakai;R. Kozu;R. Kumar;J. Kume;C. Kuo;H. Kuo;Y. Kuromiya;S. Kuroyanagi;K. Kusayanagi;K. Kwak;H. Lee;H. W. Lee;Ray-Kuang Lee;M. Leonardi;K. L. Li;L. Lin;C.Y. Lin;F. Lin;F. Lin;H. Lin;G. Liu;L. Luo;E. Majorana;M. Marchiò;Y. Michimura;N. Mio;O. Miyakawa;A. Miyamoto;Y. Miyazaki;K. Miyo;S. Miyoki;Y. Mori;S. Morisaki;Y. Moriwaki;K. Nagano;S. Nagano;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;T. Narikawa;L. Naticchioni;R. Negishi;L. Quynh;W. Ni;A. Nishizawa;S. Nozaki;Y. Obuchi;W. Ogaki;J. Oh;K. Oh;S. -. Oh;M. Ohashi;N. Ohishi;M. Ohkawa;H. Ohta;Y. Okutani;K. Okutomi;K. Oohara;C. Ooi;S. Oshino;S. Otabe;K. Pan;H. Pang;A. Parisi;J. Park;F. Arellano;I. Pinto;N. Sago;S. Saito;Y. Saito;K. Sakai;Y. Sakai;Y. Sakuno;S. Sato;T. Sato;T. Sawada;T. Sekiguchi;Y. Sekiguchi;L. Shao;S. Shibagaki;R. Shimizu;T. Shimoda;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;K. Somiya;E. Son;H. Sotani;R. Sugimoto;J. Suresh;T. Suzuki;H. Tagoshi;H. Takahashi;R. Takahashi;A. Takamori;S. Takano;H. Takeda;M. Takeda;H. Tanaka;K. Tanaka;T. Tanaka;S. Tanioka;E. Mart'in;S. Telada;T. Tomaru;Y. Tomigami;T. Tomura;F. Travasso;L. Trozzo;T. Tsang;J. Tsao;K. Tsubono;S. Tsuchida;T. Tsutsui;T. Tsuzuki;D. Tuyenbayev;N. Uchikata;T. Uchiyama;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;F. Uraguchi;T. Ushiba;M. Putten;H. Vocca;J. Wang;T. Washimi;C. Wu;H. Wu;S. Wu;W-R. Xu;T. Yamada;K. Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;Y. Yang;K. Yano;K. Yokogawa;J. Yokoyama;T. Yokozawa;T. Yoshioka;H. Yuzurihara;S. Zeidler;M. Zhan;H. Zhang;Y. Zhao;Z. Zhu;R. Goetz;M. Heintze;J. Liu;C. Muller;R. Savage;D. Tanner

Pykat: Python package for modelling precision optical interferometers

Pykat：用于精密光学干涉仪建模的 Python 包

• DOI: 10.1016/j.softx.2020.100613
• 发表时间: 2020
• 期刊: SoftwareX
• 影响因子: 3.4
• 作者: Brown, Daniel D.;Jones, Philip;Rowlinson, Samuel;Leavey, Sean;Green, Anna C.;Töyrä, Daniel;Freise, Andreas
• 通讯作者: Freise, Andreas