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，并介绍了NSF“宇宙上的Windows”的优先领域。从2015年9月开始，两个先进的Ligo观察与处女座结合进行了引力波的观察运动，其中有10多种来自O1和O2奔跑的紧凑型物体的灵感。恰好的O3运行检测到了50多个信号，其中大多数可能是黑洞和/或中子星的灵感。一份新闻来源的报告已发表，预计还有其他非常有趣的公告。灵敏度和性能的改善仍在继续，佛罗里达的研究旨在为这些改进以及第三代重力波探测器的设计做出贡献。这项工作将通过佛罗里达大学Ligo集团直接参与Ligo天文台的研究和运营来发展国家和国际科学基础设施。这项研究将超越重力波科学。该项目开发的高功率光学隔离器在激光和光学行业中具有商业应用。单频2.1μm激光器，可在频率的GHz上进行调节，可能会影响精确科学的许多领域。佛罗里达小组还为学生和博士后科学家提供了从涉及激光和光学，电子和反馈控制系统，真空和低温的一系列学科的科学技能的机会，以及大规模的探测器调试和操作。此外，该小组对本科生的教育具有很高的价值，并且每年都涉及研究本科生。高级LIGO设计用于10倍的敏感性提高，低频反应比初始LIGO更好。随着挤压和A+升级的引入，灵敏度将进一步提高。这些收益需要提高探测器的各个方面的性能，包括输入光学，这是佛罗里达州LIGO集团多年来的责任。工作将解决高功率光学隔离，RF调制，用于模式匹配的自适应元素，用于敏感性和控制悬浮镜和平台的阴影传感器，以及对输入光学和电源/信号回收空腔的改进模拟。它还解决了下一代探测器增加观察者科学范围所需的基础研究。这项较长的研究包括对硅杂质的研究，这是低温探测器测试量的几乎理想的材料，低温阴影传感器以及单频非平面环振荡器激光在2.1μm波长下运行的单次非平面环振荡器激光。这些奖项通过NSF的法定宣传和构成的构成良好的构成良好的影响，并构成了诚实的构成，并构成了构成的构成型构成的支持。 标准。

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