Surveying black holes and neutron stars with gravitational waves

用引力波测量黑洞和中子星

• 批准号: ST/K005014/1
• 负责人: John Veitch
• 金额: $ 55.89万
• 依托单位: University of Birmingham
• 依托单位国家: 英国
• 项目类别: Fellowship
• 财政年份: 2014
• 资助国家: 英国
• 起止时间: 2014 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FK005014%2F1
• 关键词: Surveying; black; holes; neutron; stars

Black holes and neutron stars are some of the strangest objects in our universe, formed in the supernova explosions at the end of the lives of the most massive stars. Neutron stars contain the mass of the Sun compressed into a sphere only a few tens of kilometres across; so dense that atoms can no longer exist, so the entire star consists of neutrons packed together by gravity. Black holes are thought to be more massive still, and so dense that not even light can escape from beyond their event horizons. These fascinating objects are a physicist's dream laboratory: a place where all our theories are pushed to their limits and beyond. Understanding how they are formed can also shed light on the evolution of the stars that they came from.When two of these objects are found in a binary system, their small size allow them to orbit each other in a few hours or less.According to Einstein's general theory of relativity these systems have so much matter in such a small space that they distort the space-time around them, whipping up gravitational waves that extract energy from the orbit and change the dimensions of everything they pass through. Luckily, by the time they reach us at Earth, these gravitational waves are so weak that the changes in length are equivalent to changing the distance between the Sun and Saturn by one hair's width, far too small to notice. Eventually so much energy is extracted that the objects orbit each other hundreds of times a second before they finally collide, releasing a huge amount of energy that can produce the brightest explosions in the universe if a neutron star is involved, but are completely invisible if only black holes are. Invisible that is, except to gravitational wave observatories, which are designed to measure the distortion of space-time produced by these events throughout the universe. The second generation of these observatories, called Advanced LIGO and Advanced Virgo, will come online in 2015 and start to make detections of binary collisions soon afterwards. By precisely measuring the distortions produced as a gravitational wave passes by, it will be possible to measure the nature of the binary system that produced it, even when no electromagnetic signal can be seen. Gravitational waves form in effect an entirely new spectrum with which we can observe the universe, opening up new avenues for discovery.The hunt for these gravitational waves is an incredibly exciting field of science. It pushes the limits of what is technologically possible in every part of its design. Knowing that we will soon be observing black holes and neutron stars fuels the curiosity that drives this global effort forward. We are about to open up a new tool that will allow us to observe space-time itself, and will eventually lead to a better understanding of the nature and evolution of the universe.

黑洞和中子星是我们宇宙中最奇怪的物体之一，它们是在最大质量恒星生命结束时的超新星爆炸中形成的。中子星含有太阳的质量，被压缩成一个直径只有几十公里的球体;密度如此之大，以至于原子不再存在，所以整个星星都是由引力聚集在一起的中子组成的。黑洞被认为质量更大，密度如此之大，以至于连光都无法从它们的视界之外逃逸出来。这些迷人的物体是物理学家的梦想实验室：一个将我们所有的理论推向极限和超越的地方。了解它们是如何形成的，也可以揭示它们所来自的恒星的演化。当在一个双星系统中发现两个这样的物体时，它们的小尺寸使它们能够在几个小时或更短的时间内绕对方运行。根据爱因斯坦的广义相对论，这些系统在如此小的空间中有如此多的物质，以至于它们扭曲了周围的时空，掀起引力波，从轨道中提取能量，改变它们所经过的一切物体的尺寸。幸运的是，当它们到达地球时，这些引力波是如此微弱，以至于长度的变化相当于太阳和土星之间的距离改变了一根头发的宽度，太小了以至于注意不到。最终，大量的能量被提取出来，以至于在它们最终碰撞之前，这些物体每秒会相互绕轨道运行数百次，释放出巨大的能量，如果涉及中子星星，这些能量可以产生宇宙中最明亮的爆炸，但如果只有黑洞，则完全看不见。看不见，也就是说，除了引力波观测站，引力波观测站被设计用来测量这些事件在整个宇宙中产生的时空扭曲。第二代天文台，名为Advanced LIGO和Advanced Virgo，将于2015年上线，并在不久之后开始探测双星碰撞。通过精确测量引力波经过时产生的扭曲，即使在看不到电磁信号的情况下，也有可能测量产生引力波的双星系统的性质。引力波实际上形成了一个全新的光谱，我们可以用它来观察宇宙，为发现开辟了新的途径。寻找这些引力波是一个令人难以置信的令人兴奋的科学领域。它在设计的每一个部分都突破了技术上的极限。知道我们很快就会观测到黑洞和中子星，激发了推动这一全球努力的好奇心。我们即将开发一种新的工具，它将使我们能够观察时空本身，并最终导致更好地理解宇宙的性质和演化。

项目成果

Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010

• DOI: 10.1103/physrevd.89.102006
• 发表时间: 2014-03
• 作者: The Ligo Scientific Collaboration;T. V. C. J. Aasi;B. Abbott;R. Abbott;T. Abbott;M. Abernathy;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;C. Affeldt;M. Agathos;N. Aggarwal;O. Aguiar;A. Ain;P. Ajith;A. Alemic;B. Allen;A. Allocca;D. Amariutei;M. Andersen;R. Anderson;S. Anderson;W. Anderson;K. Arai;M. Araya;C. Arceneaux;J. Areeda;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;L. Austin;B. Aylott;S. Babak;P. Baker;G. Ballardin;S. Ballmer;J. Barayoga;M. Barbet;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;M. Barton;I. Bartos;R. Bassiri;A. Basti;J. Batch;J. Bauchrowitz;T. Bauer;V. Bavigadda;B. Behnke;M. Bejger;M. Beker;C. Belczynski;A. Bell;C. Bell;M. Benacquista;G. Bergmann;D. Bersanetti;A. Bertolini;J. Betzwieser;P. Beyersdorf;I. Bilenko;G. Billingsley;J. Birch;S. Biscans;M. Bitossi;M. Bizouard;E. Black;J. K. Blackburn;L. Blackburn;D. Blair;S. Bloemen;O. Bock;T. Bodiya;M. Boer;G. Bogaert;C. Bogan;C. Bond;F. Bondu;L. Bonelli;R. Bonnand;R. Bork;M. Born;V. Boschi;S. Bose;L. Bosi;C. Bradaschia;P. Brady;V. Braginsky;M. Branchesi;J. Brau;T. Briant;D. Bridges;A. Brillet;M. Brinkmann;V. Brisson;A. Brooks;D. Brown;D. Brown;F. Bruckner;S. Buchman;T. Bulik;H. Bulten;A. Buonanno;R. Burman;D. Buskulic;C. Buy;L. Cadonati;G. Cagnoli;J. C. Bustillo;E. Calloni;J. Camp;P. Campsie;K. Cannon;B. Canuel;J. Cao;C. Capano;F. Carbognani;L. Carbone;S. Caride;A. Castiglia;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;C. Celerier;G. Cella;C. Cepeda;E. Cesarini;R. Chakraborty;T. Chalermsongsak;S. Chamberlin;S. Chao;P. Charlton;É. Chassande-Mottin;X. Chen;Y. Chen;A. Chincarini;A. Chiummo;H. Cho;J. Chow;N. Christensen;Q. Chu;S. Chua;S. Chung;G. Ciani;F. Clara;J. Clark;F. Cleva;E. Coccia;P. Cohadon;A. Colla;C. Collette;M. Colombini;L. Cominsky;M. Constancio;A. Conte;D. Cook;T. Corbitt;M. Cordier;N. Cornish;A. Corpuz;A. Corsi;C. Costa;M. Coughlin;S. Coughlin;J. Coulon;S. Countryman;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;K. Craig;J. Creighton;S. Crowder;A. Cumming;L. Cunningham;E. Cuoco;K. Dahl;T. D. Canton;M. Damjanic;S. Danilishin;S. D’Antonio;K. Danzmann;V. Dattilo;H. Daveloza;M. Davier;G. Davies;E. Daw;R. Day;T. Dayanga;G. Debreczeni;J. Degallaix;S. Del'eglise;W. D. Pozzo;T. Denker;T. Dent;H. Dereli;V. Dergachev;R. Rosa;R. Derosa;R. DeSalvo;S. Dhurandhar;M. D'iaz;L. Fiore;A. Lieto;I. Palma;A. Virgilio;V. Dolique;A. Donath;F. Donovan;K. Dooley;S. Doravari;S. Dossa;R. Douglas;T. Downes;M. Drago;R. Drever;J. Driggers;Z. Du;M. Ducrot;S. Dwyer;T. Eberle;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;G. EndrHoczi;R. Essick;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;S. Fairhurst;Q. Fang;S. Farinon;B. Farr;W. Farr;Marc Favata;H. Fehrmann;M. Fejer;D. Feldbaum;F. Feroz;I. Ferrante;F. Ferrini;F. Fidecaro;L. Finn;I. Fiori;R. Fisher;R. Flaminio;J. Fournier;S. Franco;S. Frasca;F. Frasconi;M. Frede;Z. Frei;A. Freise;R. Frey;T. Fricke;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;J. Gair;L. Gammaitoni;S. Gaonkar;F. Garufi;N. Gehrels;G. Gemme;B. Gendre;E. Génin;A. Gennai;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;C. Gill;J. Gleason;E. Goetz;R. Goetz;L. Goggin;L. Gondán;G. Gonz'alez;N. Gordon;M. Gorodetsky;S. Gossan;S. Gossler;R. Gouaty;C. Graf;P. Graff;M. Granata;A. Grant;S. Gras;C. Gray;R. Greenhalgh;A. Gretarsson;P. Groot;H. Grote;K. Grover;S. Grunewald;G. Guidi;C. Guido;K. Gushwa;E. Gustafson;R. Gustafson;D. Hammer;G. Hammond;M. Hanke;J. Hanks;C. Hanna;J. Hanson;J. Harms;G. Harry;I. Harry;E. Harstad;M. Hart;M. Hartman;C. Haster;K. Haughian;A. Heidmann;M. Heintze;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;A. Heptonstall;M. Heurs;M. Hewitson;S. Hild;D. Hoak;K. Hodge;K. Holt;S. Hooper;P. Hopkins;D. Hosken;J. Hough;E. Howell;Y. Hu;B. Hughey;S. Husa;S. Huttner;M. Huynh;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;D. Ingram;R. Inta;T. Isogai;A. Ivanov;B. Iyer;K. Izumi;M. Jacobson;E. James;H. Jang;P. Jaranowski;Y. Ji;F. Jim'enez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;K. Haris;P. Kalmus;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;J. Karlén;M. Kasprzack;E. Katsavounidis;W. Katzman;H. Kaufer;K. Kawabe;F. Kawazoe;F. K'ef'elian;G. M. Keiser;D. Keitel;D. Kelley;W. Kells;A. Khalaidovski;F. Khalili;E. Khazanov;C. Kim;K. Kim;N. Kim;N. Kim;Y. Kim;E. King;P. King;D. Kinzel;J. Kissel;S. Klimenko;J. Kline;S. Koehlenbeck;K. Kokeyama;V. Kondrashov;S. Koranda;W. Korth;I. Kowalska;D. Kozak;A. Kremin;V. Kringel;B. Krishnan;A. Kr'olak;G. Kuehn;A. Kumar;D. Kumar;P. Kumar;R. Kumar;L. Kuo;A. Kutynia;P. Kwee;M. Landry;B. Lantz;S. Larson;P. Lasky;C. Lawrie;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;E. Lebigot;C. Lee;H. Lee;H. Lee;J. Lee;M. Leonardi;J. Leong;A. L. Roux;N. Leroy;N. Letendre;Y. Levin;B. Levine;J. Lewis;T. G. F. Li;K. Libbrecht;A. Libson;A. Lin;T. Littenberg;V. Litvine;N. Lockerbie;V. Lockett;D. Lodhia;K. Loew;J. Logue;A. Lombardi;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;M. Lubinski;H. Luck;Erik Luijten;A. Lundgren;R. Lynch;Y. Ma;J. Macarthur;E. Macdonald;T. Macdonald;B. Machenschalk;M. Macinnis;D. Macleod;F. Magaña-Sandoval;M. Mageswaran;C. Maglione;K. Mailand;E. Majorana;I. Maksimovic;V. Malvezzi;N. Man;G. Manca;I. Mandel;V. Mandic;V. Mangano;N. Mangini;M. Mantovani;F. Marchesoni;F. Marion;S. M'arka;Z. M'arka;A. Markosyan;E. Maros;J. Marque;F. Martelli;I. Martin;R. Martin;L. Martinelli;D. Martynov;J. Marx;K. Mason;A. Masserot;T. Massinger;F. Matichard;L. Matone;R. Matzner;N. Mavalvala;N. Mazumder;G. Mazzolo;R. McCarthy-;D. McClelland;S. Mcguire;G. Mcintyre;J. McIver;K. McLin;D. Meacher;G. Meadors;M. Mehmet;J. Meidam;M. Meinders;A. Melatos;G. Mendell;R. Mercer;S. Meshkov;C. Messenger;P. Meyers;H. Miao;C. Michel;E. Mikhailov;L. Milano;S. Milde;J. Miller;Y. Minenkov;C. Mingarelli;C. Mishra;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;B. Moe;P. Moesta;A. Moggi;M. Mohan;S. Mohapatra;D. Moraru;G. Moreno;N. Morgado;S. Morriss;K. Mossavi;B. Mours;C. Mow-Lowry;C. Mueller;G. Mueller;S. Mukherjee;A. Mullavey;J. Munch;D. Murphy;P. Murray;A. Mytidis;M. Nagy;I. Nardecchia;L. Naticchioni;R. Nayak;V. Necula;G. Nelemans;I. Neri;M. Neri;G. Newton;T. Nguyen;A. Nitz;F. Nocera;D. Nolting;M. Normandin;L. Nuttall;E. Ochsner;J. O'Dell;E. Oelker;J. Oh;S. Oh;F. Ohme;P. Oppermann;B. O'reilly;R. O’Shaughnessy;C. Osthelder;D. Ottaway;R. Ottens;H. Overmier;B. Owen;C. Padilla;A. Pai;O. Palashov;C. Palomba;H. Pan;Y. Pan;C. Pankow;F. Paoletti;M. Papa;H. Paris;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Pedraza;S. Penn;A. Perreca;M. Phelps;M. Pichot;M. Pickenpack;F. Piergiovanni;V. Pierro;L. Pinard;I. Pinto;M. Pitkin;J. Poeld;R. Poggiani;A. Poteomkin;J. Powell;J. Prasad;S. Premachandra;T. Prestegard;L. Price;M. Prijatelj;S. Privitera;G. Prodi;L. Prokhorov;O. Puncken;M. Punturo;P. Puppo;J. Qin;V. Quetschke;E. Quintero;G. Quiroga;R. Quitzow-James;F. Raab;D. Rabeling;I. R'acz;H. Radkins;P. Raffai;S. Raja;G. Rajalakshmi;M. Rakhmanov;C. Ramet;K. Ramirez;P. Rapagnani;V. Raymond;M. Razzano;V. Re;J. Read;S. Recchia;C. Reed;T. Regimbau;S. Reid;D. Reitze;E. Rhoades;F. Ricci;K. Riles;N. Robertson;F. Robinet;A. Rocchi;M. Rodruck;L. Rolland;J. Rollins;R. Romano;G. Romanov;J. Romie;D. Rosi'nska;S. Rowan;A. Rudiger;P. Ruggi;K. Ryan;F. Salemi;L. Sammut;V. Sandberg;J. Sanders;V. Sannibale;I. Santiago-Prieto;E. Saracco;B. Sassolas;B. Sathyaprakash;P. Saulson;R. Savage;J. Scheuer;R. Schilling;R. Schnabel;R. Schofield;E. Schreiber;D. Schuette;B. Schutz;J. Scott;S. Scott;D. Sellers;A. Sengupta;D. Sentenac;V. Sequino;A. Sergeev;D. Shaddock;S. Shah;M. Shahriar;M. Shaltev;B. Shapiro;P. Shawhan;D. Shoemaker;T. Sidery;K. Siellez;X. Siemens;D. Sigg;D. Simakov;A. Singer;L. Singer;R. Singh;A. Sintes;B. Slagmolen;J. Slutsky;J. R. Smith;M. Smith;R. Smith;N. Smith-Lefebvre;E. Son;B. Sorazu;T. Souradeep;A. Staley;J. Stebbins;J. Steinlechner;S. Steinlechner;B. Stephens;S. Steplewski;S. Stevenson;R. Stone;D. Stops;K. Strain;N. Straniero;S. Strigin;R. Sturani;A. Stuver;T. Summerscales;S. Susmithan;P. Sutton;B. Swinkels;M. Tacca;D. Talukder;D. Tanner;S. Tarabrin;R. Taylor;M. Thirugnanasambandam;M. Thomas;P. Thomas;K. Thorne;K. Thorne;E. Thrane;V. Tiwari;K. Tokmakov;C. Tomlinson;M. Tonelli;C. Torres;C. Torrie;F. Travasso;G. Traylor;M. Tse;D. Ugolini;C. Unnikrishnan;A. Urban;K. Urbanek;H. Vahlbruch;G. Vajente;G. Valdes;M. Vallisneri;M. Beuzekom;J. Brand;C. Broeck;M. V. D. Sluys;J. V. Heijningen;A. V. Veggel;S. Vass;M. Vas'uth;R. Vaulin;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;D. Verkindt;S. Verma;F. Vetrano;A. Vicer'e;R. Vincent-Finley;J. Vinet;S. Vitale;T. Vo;H. Vocca;C. Vorvick;W. Vousden;S. Vyachanin;A. Wade;L. Wade;M. Wade;M. Walker;L. Wallace;M. Wang;X. Wang;R. Ward;M. Was;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;T. Welborn;L. Wen;P. Wessels;M. West;T. Westphal;K. Wette;J. Whelan;S. Whitcomb;D. White;B. Whiting;K. Wiesner;C. Wilkinson;K. Williams;L. Williams;R. Williams;T. Williams;A. Williamson;J. Willis;B. Willke;M. Wimmer;W. Winkler;C. Wipf;A. Wiseman;H. Wittel;G. Woan;J. Worden;J. Yablon;I. Yakushin;H. Yamamoto;C. Yancey;H. Yang;Z. Yang;S. Yoshida;M. Yvert;A. Zadro.zny;M. Zanolin;J. Zendri;Fan Zhang;L. Zhang;C. Zhao;X. Zhu;M. Zucker;S. Zuraw;J. Zweizig

Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data.

• DOI: 10.1103/physrevlett.113.231101
• 发表时间: 2014-06
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: J. Aasi;B. Abbott;R. Abbott;T. Abbott;M. Abernathy;T. Accadia;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;C. Affeldt;M. Agathos;N. Aggarwal;O. Aguiar;A. Ain;P. Ajith;A. Alemic;B. Allen;A. Allocca;D. Amariutei;M. Andersen;R. Anderson;S. Anderson;W. Anderson;K. Arai;M. Araya;C. Arceneaux;J. Areeda;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;L. Austin;B. Aylott;S. Babak;P. Baker;G. Ballardin;S. Ballmer;J. Barayoga;M. Barbet;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;M. Barton;I. Bartos;R. Bassiri;A. Basti;J. Batch;J. Bauchrowitz;T. Bauer;B. Behnke;M. Bejger;M. Beker;C. Belczynski;A. Bell;C. Bell;G. Bergmann;D. Bersanetti;A. Bertolini;J. Betzwieser;P. Beyersdorf;I. Bilenko;G. Billingsley;J. Birch;S. Biscans;M. Bitossi;M. Bizouard;E. Black;J. Blackburn;L. Blackburn;D. Blair;S. Bloemen;M. Blom;O. Bock;T. Bodiya;M. Boer;G. Bogaert;C. Bogan;C. Bond;F. Bondu;L. Bonelli;R. Bonnand;R. Bork;M. Born;V. Boschi;S. Bose;L. Bosi;C. Bradaschia;P. Brady;V. Braginsky;M. Branchesi;J. Brau;T. Briant;D. Bridges;A. Brillet;M. Brinkmann;V. Brisson;A. Brooks;D. Brown;D. Brown;F. Brückner;S. Buchman;T. Bulik;H. Bulten;A. Buonanno;R. Burman;D. Buskulic;C. Buy;L. Cadonati;G. Cagnoli;J. C. Bustillo;E. Calloni;J. Camp;P. Campsie;K. Cannon;B. Canuel;J. Cao;C. Capano;F. Carbognani;L. Carbone;S. Caride;A. Castiglia;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;C. Celerier;G. Cella;C. Cepeda;E. Cesarini;R. Chakraborty;T. Chalermsongsak;S. Chamberlin;S. Chao;P. Charlton;É. Chassande-Mottin;X. Chen;Y. Chen;A. Chincarini;A. Chiummo;H. Cho;J. Chow;N. Christensen;Q. Chu;S. Chua;S. Chung;G. Ciani;F. Clara;J. Clark;F. Cleva;E. Coccia;P. Cohadon;A. Colla;C. Collette;M. Colombini;L. Cominsky;M. Constancio;A. Conte;D. Cook;T. Corbitt;M. Cordier;N. Cornish;A. Corpuz;A. Corsi;C. Costa;M. Coughlin;S. Coughlin;J. Coulon;S. Countryman;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;K. Craig;J. Creighton;S. Crowder;A. Cumming;L. Cunningham;E. Cuoco;K. Dahl;T. D. Canton;M. Damjanic;S. Danilishin;S. D’Antonio;K. Danzmann;V. Dattilo;H. Daveloza;M. Davier;G. Davies;E. Daw;R. Day;T. Dayanga;G. Debreczeni;J. Degallaix;S. Deléglise;W. Del Pozzo;T. Denker;T. Dent;H. Dereli;V. Dergachev;R. De Rosa;R. Derosa;R. DeSalvo;S. Dhurandhar;M. Díaz;L. Di Fiore;A. Di Lieto;I. Di Palma;A. D. Di Virgilio;A. Donath;F. Donovan;K. Dooley;S. Doravari;S. Dossa;R. Douglas;T. Downes;M. Drago;R. Drever;J. Driggers;Z. Du;S. Dwyer;T. Eberle;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;G. Endrőczi;R. Essick;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;S. Fairhurst;Q. Fang;S. Farinon;B. Farr;W. Farr;Marc Favata;H. Fehrmann;M. Fejer;D. Feldbaum;F. Feroz;I. Ferrante;F. Ferrini;F. Fidecaro;L. Finn;I. Fiori;R. Fisher;R. Flaminio;J. Fournier;S. Franco;S. Frasca;F. Frasconi;M. Frede;Z. Frei;A. Freise;R. Frey;T. Fricke;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;J. Gair;L. Gammaitoni;S. Gaonkar;F. Garufi;N. Gehrels;G. Gemme;E. Génin;A. Gennai;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;C. Gill;J. Gleason;E. Goetz;R. Goetz;L. Gondán;G. González;N. Gordon;M. Gorodetsky;S. Gossan;S. Gossler;R. Gouaty;C. Gräf;P. Graff;M. Granata;A. Grant;S. Gras;C. Gray;R. Greenhalgh;A. Gretarsson;P. Groot;H. Grote;K. Grover;S. Grunewald;G. Guidi;C. Guido;K. Gushwa;E. Gustafson;R. Gustafson;D. Hammer;G. Hammond;M. Hanke;J. Hanks;C. Hanna;J. Hanson;J. Harms;G. Harry;I. Harry;E. Harstad;M. Hart;M. Hartman;C. Haster;K. Haughian;A. Heidmann;M. Heintze;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;A. Heptonstall;M. Heurs;M. Hewitson;S. Hild;D. Hoak;K. Hodge;K. Holt;S. Hooper;P. Hopkins;D. Hosken;J. Hough;E. Howell;Yi-ming Hu;E. Huerta;B. Hughey;S. Husa;S. Huttner;M. Huynh;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;D. Ingram;R. Inta;T. Isogai;A. Ivanov;B. Iyer;K. Izumi;M. Jacobson;E. James;H. Jang;P. Jaranowski;Y. Ji;F. Jiménez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;H. K;P. Kalmus;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;J. Karlén;M. Kasprzack;E. Katsavounidis;W. Katzman;H. Kaufer;K. Kawabe;F. Kawazoe;F. Kéfélian;G. M. Keiser;D. Keitel;D. Kelley;W. Kells;A. Khalaidovski;F. Khalili;E. Khazanov;C. Kim;K. Kim;N. Kim;N. Kim;Y. Kim;E. King;P. King;D. Kinzel;J. Kissel;S. Klimenko;J. Kline;S. Koehlenbeck;K. Kokeyama;V. Kondrashov;S. Koranda;W. Korth;I. Kowalska;D. Kozak;A. Kremin;V. Kringel;A. Królak;G. Kuehn;A. Kumar;P. Kumar;R. Kumar;L. Kuo;A. Kutynia;P. Kwee;M. Landry;B. Lantz;S. Larson;P. Lasky;C. Lawrie;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;E. Lebigot;C. Lee;H. Lee;H. Lee;J. Lee;M. Leonardi;J. Leong;A. Le Roux;N. Leroy;N. Letendre;Y. Levin;B. Levine;J. Lewis;T. G. F. Li;K. Libbrecht;A. Libson;A. Lin;T. Littenberg;V. Litvine;N. Lockerbie;V. Lockett;D. Lodhia;K. Loew;J. Logue;A. Lombardi;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;M. Lubinski;H. Lück;Erik Luijten;A. Lundgren;R. Lynch;Y. Ma;J. Macarthur;E. Macdonald;T. Macdonald;B. Machenschalk;M. Macinnis;D. Macleod;F. Magaña-Sandoval;M. Mageswaran;C. Maglione;K. Mailand;E. Majorana;I. Maksimovic;V. Malvezzi;N. Man;G. Manca;I. Mandel;V. Mandic;V. Mangano;N. Mangini;M. Mantovani;F. Marchesoni;F. Marion;S. Márka;Z. Márka;A. Markosyan;E. Maros;J. Marque;F. Martelli;I. Martin;R. Martin;L. Martinelli;D. Martynov;J. Marx;K. Mason;A. Masserot;T. Massinger;F. Matichard

Implementation of an $\mathcal{F}$-statistic all-sky search for continuous gravitational waves in Virgo VSR1 data

在 Virgo VSR1 数据中实现连续引力波的 $mathcal{F}$ 统计全天搜索

• DOI: 10.1088/0264-9381/31/16/165014
• 发表时间: 2014
• 期刊: Classical and Quantum Gravity
• 影响因子: 3.5
• 作者: Aasi J

Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers

使用松散相干算法对来自 LIGO 干涉仪的数据搜索猎户座支线的连续引力波

• DOI: 10.1103/physrevd.93.042006
• 发表时间: 2016
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Aasi J

Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run

• DOI: 10.1103/physrevd.89.122003
• 发表时间: 2014-06-12
• 期刊: PHYSICAL REVIEW D
• 影响因子: 5
• 作者: Aasi, J.;Abbott, B. P.;Zweizig, J.
• 通讯作者: Zweizig, J.