Explorations of Extreme and Eccentric Binary Black Hole Mergers

极端和偏心双黑洞合并的探索

• 批准号: 2207920
• 负责人: Carlos Lousto
• 金额: $ 45万
• 依托单位: Rochester Institute of Tech
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2022
• 资助国家: 美国
• 起止时间: 2022-09-01 至 2025-08-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2207920&HistoricalAwards=false
• 关键词: Explorations; Extreme; Eccentric; Binary; Black

Gravitational Wave Astronomy provides a revolutionary new view of the universe that can probe previously unexplorable regions, including the interiors of neutron stars, collisions of black holes, which emit energy at luminosities exceeding the entire visible universe, and even remnants of the big bang. To gain new insight into the dynamics of the universe, gravitational wave astronomers need to be able to infer the nature of the sources from the observed signals. The physical parameters of these sources can be extracted from the observed signals if the dependence of the waveform on source parameters is known to sufficiently high-accuracy. This project aims at modeling merging black-hole binaries using numerical simulations of the fully nonlinear Einstein equations on supercomputers. This project will keep RIT group at the forefront of black holes Supercomputer simulations, contributing to the development of students and postdoctoral fellows careers in STEM disciplines.This award principal goals are to produce waveforms for LIGO/Virgo/KAGRA (LVK) source parametrization efforts, and to model the remnant mass, spin, and gravitational recoil from highly-precessing spinning eccentric binary black holes in order to elucidate the distributions of these quantities and how they affect the distribution and growth of black holes. This work will produce and publicly release gravitational waveforms in previously not sampled regions of parameter space for LVK data analysis, to directly use these waveforms for studies and modeling of binary black holes dynamics, and will improve the accuracy and efficiency of the numerical simulations.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.

引力波天文学提供了一种革命性的宇宙新观点，可以探测以前无法探索的区域，包括中子星的内部、黑洞的碰撞（其发出的能量超过整个可见宇宙的光度），甚至是大爆炸的残余物。为了获得对宇宙动力学的新见解，引力波天文学家需要能够从观测到的信号推断源的性质。如果已知波形对源参数的依赖性足够高精度，则可以从观测到的信号中提取这些源的物理参数。该项目旨在利用超级计算机上的完全非线性爱因斯坦方程的数值模拟来对合并黑洞双星进行建模。 该项目将使 RIT 小组保持在黑洞超级计算机模拟的最前沿，为 STEM 学科的学生和博士后职业发展做出贡献。该奖项的主要目标是为 LIGO/Virgo/KAGRA (LVK) 源参数化工作生成波形，并对来自高进动旋转偏心双黑洞的残余质量、自旋和引力反冲进行建模，以阐明这些量的分布以及它们如何产生影响黑洞的分布和生长。这项工作将产生并公开发布之前未采样的参数空间区域的引力波形，用于LVK数据分析，直接使用这些波形进行双黑洞动力学的研究和建模，并将提高数值模拟的准确性和效率。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

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

• DOI: 10.1103/physrevd.106.102008
• 发表时间: 2022-01
• 期刊: Physical Review D
• 影响因子: 5
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;H. Abe;F. Acernese;K. Ackley;N. Adhikari;R. Adhikari;V. K. Adkins;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;S. Albanesi;R. Alfaidi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;T. Andrade;N. Andrés;M. Andr'es-Carcasona;T. Andri'c;S. Angelova;S. Ansoldi;J. Antelis;S. Antier;T. Apostolatos;E. Z. Appavuravther;S. Appert;S. Apple;K. Arai;A. Araya;M. Araya;J. Areeda;M. Arène;N. Aritomi;N. Arnaud;M. Arogeti;S. Aronson;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. D. Melo;S. Aston;P. Astone;F. Aubin;K. AultONeal;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;J. Baird;R. Bajpai;T. Baka;M. Ball;G. Ballardin;S. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;B. Banerjee;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;S. Basak;R. Bassiri;A. Basti;M. Bawaj;J. Bayley;M. Bazzan;B. Becher;B. B'ecsy;V. Bedakihale;F. Beirnaert;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;M. Benjamin;T. Bennett;J. Bentley;M. BenYaala;S. Bera;M. Berbel;F. Bergamin;B. Berger;S. Bernuzzi;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;A. Bhandari;U. Bhardwaj;R. Bhatt;D. Bhattacharjee;S. Bhaumik;A. Bianchi;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;G. N. Bolingbroke;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. 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Miyoki;G. Mo;L. M. Modafferi;E. Moguel;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;J. Moragues;D. Moraru;F. Morawski;A. More;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;N. Morisue;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;H. Narola;L. Naticchioni;B. Nayak;R. Nayak;B. Neil;J. Neilson;A. Nelson;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;J. Ni;W. Ni;S. Nichols;T. Nishimoto;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;M. Norman;C. North;S. Nozaki;G. Nurbek;L. Nuttall;Y. Obayashi;J. Oberling;B. O'Brien;J. O'Dell;E. Oelker;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. Oh;M. Ohashi;T. Ohashi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;C. Olivetto;K. Oohara;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;R. Pagano;M. Page;G. Pagliaroli;A. Pai;S. Pai;S. Pal;J. R. Palamos;O. Palashov;C. Palomba;H. Pan;K. Pan;P. Panda;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Panther;F. Paoletti;A. Paoli;A. Paolone;George Pappas;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;R. Pedurand;M. Pegoraro;A. Pele;F. Arellano;S. Penano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;C. Perkins;A. Perreca;S. Perriès;D. Pesios;J. Petermann;D. Petterson;H. Pfeiffer;H. Pham;K. A. Pham;K. S. Phukon;H. Phurailatpam;O. Piccinni;M. Pichot;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;C. Pineda-Bosque;I. Pinto;M. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;A. Pisarski;M. Pitkin;A. Placidi;E. Placidi;M. L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;E. Porter;R. Poulton;A. Poverman;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;N. Quartey;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;A. Ray;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;B. Revenu;A. Reza;M. Rezac;F. Ricci;D. Richards;J. Richardson;L. Richardson;G. Riemenschneider;K. Riles;S. Rinaldi;K. Rink;N. Robertson;R. Robie;F. Robinet;A. Rocchi;S. Rodriguez;L. Rolland;J. Rollins;M. Romanelli;R. Romano;C. Romel;A. Romero;I. Romero-Shaw;J. Romie;S. Ronchini;L. Rosa;C. Rose;D. Rosi'nska;M. Ross;S. Rowan;S. Rowlinson;S. Roy;S. Roy;S. Roy;D. Rozza;P. Ruggi;K. Ruiz-Rocha;K. Ryan;S. Sachdev;T. Sadecki;J. Sadiq;S. Saha;Y. Saito;K. Sakai;M. Sakellariadou;S. Sakon;O. Salafia;F. Salces-Carcoba;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;O. Sauter;R. Savage;V. Savant;T. Sawada;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;M. Schiworski;P. Schmidt;S. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;Y. Sekiguchi;D. Sellers;A. Sengupta;D. Sentenac;E. Seo;V. Sequino;A. Sergeev;Y. Setyawati;T. Shaffer;M. Shahriar;M. Shaikh;B. Shams;L. Shao;A. Sharma;P. Sharma;P. Shawhan;N. Shcheblanov;A. Sheela;Y. Shikano;M. Shikauchi;H. Shimizu;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;S. Shyamsundar;M. Sieniawska;D. Sigg;L. Silenzi;L. Singer;D. Singh;M. Singh;N. Singh;A. Singha;A. Sintes;V. Sipala;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. Smetana;J. R. Smith;L. Smith;R. Smith;J. Soldateschi;S. Somala;K. Somiya;I. Song;K. Soni;V. Sordini;F. Sorrentino;N. Sorrentino;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. Spencer;M. Spera;P. Spinicelli;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;F. Stachurski;D. Steer;J. Steinlechner;S. Steinlechner;N. Stergioulas;D. Stops;M. Stover;K. Strain;L. Strang;G. Stratta;M. D. Strong;A. Strunk;R. Sturani;A. Stuver;M. Suchenek;S. Sudhagar;V. Sudhir;R. Sugimoto;H. Suh;A. G. Sullivan;T. Summerscales;L. Sun;S. Sunil;A. Sur;J. Suresh;P. Sutton;Takamasa Suzuki;Takanori Suzuki;Toshikazu Suzuki;B. Swinkels;M. J. Szczepa'nczyk;P. Szewczyk;M. Tacca;H. Tagoshi;S. Tait;H. Takahashi;R. Takahashi;S. Takano;H. Takeda;M. Takeda;C. Talbot;C. Talbot;K. Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;L. Tao;R. D. Tapia;E. Mart'in;C. Taranto;A. Taruya;J. Tasson;R. Tenorio;J. Terhune;L. Terkowski;M. Thirugnanasambandam;M. Thomas;P. Thomas;E. E. Thompson-E.;J. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;A. Toivonen;A. Tolley;T. Tomaru;T. Tomura;M. Tonelli;Z. Tornasi;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;K. W. Tsang;T. Tsang;J. Tsao;M. Tse;R. Tso;S. Tsuchida;L. Tsukada;D. Tsuna;T. Tsutsui;K. Turbang;M. Turconi;D. Tuyenbayev;A. Ubhi;N. Uchikata;T. Uchiyama;R. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;C. Unnikrishnan;A. Urban;T. Ushiba;A. Utina;G. Vajente;A. Vajpeyi;G. Valdes;M. Valentini;V. Valsan;N. Bakel;M. Beuzekom;M. Dael;J. Brand;C. Broeck;D. Vander-Hyde;H. Haevermaet;J. V. Heijningen;M. Putten;N. Remortel;M. Vardaro;A. Vargas;V. Varma;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;J. Venneberg;G. Venugopalan;D. Verkindt;P. Verma;Y. Verma;Sander M. Vermeulen;D. Veske;F. Vetrano;A. Vicer'e;S. Vidyant;A. Viets;A. Vijaykumar;V. Villa-Ortega;J. Vinet;A. Virtuoso;S. Vitale;H. Vocca;E. V. Reis;J. Wrangel;C. Vorvick;S. Vyatchanin;L. Wade;M. Wade;K. Wagner;R. Walet;M. Walker;G. Wallace;L. Wallace;J. Wang;J. Wang;W. H. Wang;R. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;C. Weaving;S. Webster;M. Weinert;A. Weinstein;R. Weiss;C. Weller;R. Weller;F. Wellmann;L. Wen;P. Wessels;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;D. Wong;I. C. Wong;M. Wright;C. Wu;D. Wu;H. Wu;D. Wysocki;L. Xiao;T. Yamada;H. Yamamoto;K. Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;F. Yang;K. Z. Yang;L. Yang;Y. Yang;Y. Yang;Yang Yang-Yang;M. Yap;D. Yeeles;S. Yeh;A. Yelikar;M. Ying;J. Yokoyama;T. Yokozawa;J. Yoo;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;Y. Zhang;C. Zhao;G. Zhao;Y. Zhao;Yue Zhao;R. Zhou;Z. Zhou;X. Zhu;Z. Zhu;M. Zucker;J. Zweizig

Constraints on the Cosmic Expansion History from GWTC–3

• DOI: 10.3847/1538-4357/ac74bb
• 发表时间: 2021-11
• 期刊: The Astrophysical Journal
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;H. Abe;F. Acernese;K. Ackley

Search for continuous gravitational waves from 20 accreting millisecond X-ray pulsars in O3 LIGO data

• DOI: 10.1103/physrevd.105.022002
• 发表时间: 2021-09
• 作者: R. 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;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. Andric;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. Bécsy;V. Bedakihale;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;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. Calloni;J. Cameron;J. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. Cannon;H. Cao;Z. Cao;E. Capocasa;E. Capote;G. Carapella;F. Carbognani;J. Carlin;M. Carney;M. Carpinelli;G. Carrillo;Gregorio Carullo;T. Carver;J. C. Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;M. Ceasar;G. Cella;P. Cerdá-Durán;E. Cesarini;W. Chaibi;K. Chakravarti;S. Subrahmanya;E. Champion;C. Chan;C. Chan;C. Chan;K. Chan;M. Chan;K. Chandra;P. Chanial;S. Chao;P. Charlton;E. Chase;É. Chassande-Mottin;C. Chatterjee;D. Chatterjee;D. Chatterjee;M. Chaturvedi;S. Chaty;C. Chen;H. Chen;J. Chen;K. Chen;X. Chen;Y. Chen;Y.-R. Chen;Z. Chen;H. Cheng;C. Cheong;H. Cheung;H. Chia;F. Chiadini;C. Chiang;G. Chiarini;R. Chierici;A. Chincarini;M. Chiofalo;A. Chiummo;G. Cho;H. Cho;Rupesh Kumar Choudhary;S. Choudhary;N. Christensen;H. Chu;Q. Chu;Y. Chu;S. Chua;K. Chung;G. Ciani;P. Ciecieląg;M. Cieślar;M. Cifaldi;A. Ciobanu;R. Ciolfi;F. Cipriano;A. Cirone;F. Clara;E. Clark;J. Clark;L. Clarke;P. Clearwater;S. Clesse;F. Cleva;E. Coccia;E. Codazzo;D. Cohen;L. Cohen;M. Colleoni;C. Collette;A. Colombo;M. Colpi;C. Compton;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carrión;S. Corezzi;K. Corley;N. Cornish;D. Corre;A. Corsi;S. Cortese;C. Costa;R. Cotesta;M. Coughlin;J. Coulon;S. Countryman;B. Cousins;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;A. Criswell;M. Croquette;S. Crowder;J. Cudell;T. Cullen;A. Cumming;R. Cummings;L. Cunningham;E. Cuoco;P. Dabadie;T. D. Canton;S. Dall’Osso;G. Dálya;A. Dana;L. M. DaneshgaranBajastani;Beatrice D'Angelo;S. Danilishin;S. D’Antonio;K. Danzmann;C. Darsow-Fromm;A. Dasgupta;L. Datrier;S. Datta;V. Dattilo;I. Dave;M. Davier;G. Davies;D. Davis;M. Davis;E. Daw;R. Dean;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Deléglise;V. D. Favero;F. D. Lillo;N. D. Lillo;W. D. Pozzo;L. DeMarchi;F. Matteis

Numerical-relativity validation of effective-one-body waveforms in the intermediate-mass-ratio regime

中间质量比状态下有效单体波形的数值相对论验证

• DOI: 10.1103/physrevd.105.124061
• 发表时间: 2022
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Nagar, Alessandro;Healy, James;Lousto, Carlos O.;Bernuzzi, Sebastiano;Albertini, Angelica
• 通讯作者: Albertini, Angelica

Search of the Early O3 LIGO Data for Continuous Gravitational Waves from the Cassiopeia A and Vela Jr. Supernova Remnants

• DOI: 10.1103/physrevd.105.082005
• 发表时间: 2021-11
• 作者: The Ligo Scientific 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;S. Albanesi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;T. Andrade;N. Andrés;T. Andri'c;S. Angelova;S. Ansoldi;J. Antelis;S. Antier;S. Appert;K. Arai;M. Araya;J. Areeda;M. Arène;N. Arnaud;S. Aronson;K. Arun;Y. Asali;G. Ashton;M. Assiduo;S. Aston;P. Astone;F. Aubin;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;A. Baer;S. Bagnasco;Y. Bai;J. Baird;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;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. Calloni;J. Cameron;J. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. Cannon;H. Cao;E. Capote;G. Carapella;F. Carbognani;J. Carlin;M. Carney;M. Carpinelli;G. Carrillo;Gregorio Carullo;T. Carver;J. C. Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;M. Ceasar;G. Cella;P. Cerd'a-Dur'an;E. Cesarini;W. Chaibi;K. Chakravarti;S. Subrahmanya;E. Champion;C. Chan;C. Chan;C. Chan;K. Chan;K. Chandra;P. Chanial;S. Chao;P. Charlton;E. Chase;É. Chassande-Mottin;C. Chatterjee;D. Chatterjee;D. Chatterjee;M. Chaturvedi;S. Chaty;H. Chen;J. Chen;X. Chen;Y. Chen;Z. Chen;H. Cheng;C. Cheong;H. Cheung;H. Chia;F. Chiadini;G. Chiarini;R. Chierici;A. Chincarini;M. Chiofalo;A. Chiummo;G. Cho;H. Cho;Rupesh Kumar Choudhary;S. Choudhary;N. Christensen;Q. Chu;S. Chua;K. Chung;G. Ciani;P. Ciecieląg;M. Cie'slar;M. Cifaldi;A. Ciobanu;R. Ciolfi;F. Cipriano;A. Cirone;F. Clara;E. Clark;J. Clark;L. Clarke;P. Clearwater;S. Clesse;F. Cleva;E. Coccia;E. Codazzo;P. Cohadon;D. Cohen;L. Cohen;M. Colleoni;C. Collette;A. Colombo;M. Colpi;C. Compton;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carri'on;S. Corezzi;K. Corley;N. Cornish;D. Corre;A. Corsi;S. Cortese;C. Costa;R. Cotesta;M. Coughlin;J. Coulon;S. Countryman;B. Cousins;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;A. Criswell;M. Croquette;S. Crowder;J. Cudell;T. Cullen;A. Cumming;R. Cummings;L. Cunningham;E. Cuoco;M. Curyło;P. Dabadie;T. D. Canton;S. Dall’Osso;G. D'alya;A. Dana;L. M. DaneshgaranBajastani;B. D'Angelo;S. Danilishin;S. D’Antonio;K. Danzmann;C. Darsow-Fromm;A. Dasgupta;L. Datrier;S. Datta;V. Dattilo;I. Dave;M. Davier;G. Davies;D. Davis;M. Davis;E. Daw;R. Dean;D. DeBra;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Del'eglise;V. D. Favero;F. D. Lillo;N. D. Lillo;W. D. Pozzo;L. DeMarchi;F. Matteis;V. D'Emilio;N. Demos;T. Dent;A. Depasse;R. Pietri;R. Rosa;C. D. Rossi;R. DeSalvo;R. D. Simone;S. Dhurandhar;M. D'iaz;M. Diaz-Ortiz;N. Didio;T. Dietrich;L. Fiore;C. D. Fronzo;C. Giorgio;F. D. Giovanni;M. Giovanni;T. D. Girolamo;A. Lieto;B. Ding;S. D. Pace;I. Palma;F. Renzo;A. K. Divakarla;A. 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