Investigations in Gravitational Radiation

引力辐射研究

• 批准号: ST/N005716/1
• 负责人: Edward Daw
• 金额: $ 37.36万
• 依托单位: University of Sheffield
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2016
• 资助国家: 英国
• 起止时间: 2016 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FN005716%2F1
• 关键词: Investigations; Gravitational; Radiation

Einstein's General Relativity predicts that dynamical systems in strong gravitational fields will emit vast amounts of energy in the form of gravitational waves (GW). These are ripples in the very fabric of spacetime that travel from their sources at the speed of light, carrying information about physical processes responsible for their emission. They are among the most elusive signals from the deepest reaches in the Universe. Experiments aimed at detecting them have been in development for several decades, and are now reaching sensitivities where detection is expected within a few years.The worldwide network of interferometric detectors includes the American advanced Laser Interferometer Gravitational-Wave Observatory (aLIGO), the French-Italian-Dutch-Polish advanced Virgo and the German-UK GEO600 that are being enhanced with a new detector (KAGRA) under construction in Japan. The former detectors have all reached sensitivities close to their design goals and have taken the most sensitive data to date. Cooperation amongst different projects has enabled continuous data acquisition, with sensitivity to a wide range of sources and phenomena, over most of the sky. Modelling GW sources has allowed deeper searches and data from LIGO, Virgo, and GEO have increased our understanding of astronomical phenomena. For example, we have built accurate models to describe the dynamics of spinning black hole binaries for improving efficiency of detection and accuracy of parameter estimation, initiated studies on distinguishing models of the formation and evolution of compact binaries and supernovae, ruled out merging neutron star binary as progenitor of the gamma ray burst (GRB) GRB070201, and shown that less than 1% of the Crab pulsar's radiated power is in GW.We are now entering a new era as advanced detectors begin their first phase of operation and within a few years will, we expect, routinely observe GW. The aLIGO detectors are based on the quasi-monolithic silica suspension concept developed in the UK for GEO600 and on the high power lasers developed by our German colleagues in GEO600. The AdV detector also uses a variant of the silica suspension technology. Further, KAGRA is being built with input on cryogenic bonding technology from the UK groups.The consortium groups have initiated and led searches for astronomical sources, thanks to funding support received since first data taking runs began 12 years ago. Key ingredients of several searches (accurate waveforms models, geometric formulation of data analysis to optimise searches, algorithms to search for generic bursts, Bayesian search and inference techniques) were developed at Cardiff and Glasgow.We propose a programme that leads to full exploitation of data from aLIGO and AdV, building on the analysis of data from the most recent LIGO/Virgo science runs and from GEO600 while the advanced detectors were under construction. In particular, we will refine waveform models and carry out deep and wide parameter space searches for coalescing binaries, GW emitted in coincidence with GRBs and supernovae, and continuous signals from rotating neutron stars.In parallel, we propose essential detector R&D. Detector sensitivity is mainly limited by thermal noise associated with the substrates of the mirrors, their reflective coatings, and their suspension elements, as well as by noise resulting from the quantum nature of the light used in sensing. Our research is targeted towards making innovative improvements in these areas, essential to maximize the astrophysical potential of GW observatories. We have major responsibilities for the silica suspensions in aLIGO, both in the US and for a possible 3rd aLIGO detector in India, and in the development of enhancements and upgrades to the aLIGO detectors in the areas of mirror coatings for low thermal noise, silicon substrates, room temperature and cryogenic suspensions and improved interferometer topologies to combat quantum noise.

爱因斯坦的一般相对论预测，强力引力场中的动力系统将以引力波（GW）的形式发出大量能量。这些是时空的涟漪，它以光速从源头传播，携带有关负责发射的物理过程的信息。它们是宇宙中最深处的最难以捉摸的信号之一。旨在检测它们的实验已经开发了几十年了，现在已经达到了预期在几年内进行检测的敏感性。全球干涉探测器网络包括美国先进的激光干涉仪重力仪重力波动台（Aligo）（Aligo）（Aligo），French-Dutchian-Italian-Italian-Italian-Dutch-Polish先进的Virgo和German-uk Geo600（Kag）在kag中加强了一名新的探测器（KAG）（KAG）是一名新的（KAG）。前探测器都达到了接近其设计目标的敏感性，并采用了迄今为止最敏感的数据。在不同项目之间的合作使数据获取能够连续获取，对大多数天空的敏感性，对广泛的来源和现象的敏感性。建模GW来源允许Ligo，处女座和GEO的更深入的搜索和数据增加了我们对天文现象的理解。 For example, we have built accurate models to describe the dynamics of spinning black hole binaries for improving efficiency of detection and accuracy of parameter estimation, initiated studies on distinguishing models of the formation and evolution of compact binaries and supernovae, ruled out merging neutron star binary as progenitor of the gamma ray burst (GRB) GRB070201, and shown that less than 1% of the Crab pulsar's radiated power在GW中。我们现在正在进入一个新时代，因为高级探测器开始了他们的第一阶段的运营，并且在几年之内将在几年内常规观察GW。 Aligo探测器基于在英国为GEO600开发的准空石二氧化硅悬架概念以及我们德国同事在Geo600中开发的高功率激光器。 ADV检测器还使用二氧化硅悬浮技术的变体。此外，Kagra是基于英国集团的低温粘合技术的投入而建立的。财团团体已经启动并领导了对天文来源的搜索，这要归功于自12年前首次数据运行以来获得的资金支持。在卡迪夫（Cardiff）和格拉斯哥（Glasgow）开发了多种搜索的关键成分（准确的波形模型，数据分析以优化搜索以优化搜索，搜索通用爆发的算法，贝叶斯搜索和推理技术）的算法。我们提出了一个程序，该程序可导致一项从Aligo和Advo from Aligo的全面剥削和Advection 3的unigo conciention和Advection of Alago conciention ofical/virgo ligo的分析的程序。正在建设中。特别是，我们将完善波形模型，并进行深层和广泛的参数空间搜索以合并的二进制文件，GW与GRBS和Supernovae的巧合发出，以及来自旋转中子星的连续信号。检测器灵敏度主要受热噪声，与镜子的底物，反射涂层以及它们的悬浮元素以及噪声相关的热噪声限制，以及由传感中使用的光的量子性质产生的噪声。我们的研究旨在在这些领域进行创新的改进，这对于最大程度地提高了GW观测值的天体物理潜力至关重要。在美国和印度可能的第三架阿里戈探测器以及在低热噪声，硅温度，室温和高温悬架和硬化量化量的镜像中，我们对阿里戈的二氧化硅悬浮液以及印度可能的第三架阿里戈探测器以及对阿里格探测器的增强和升级的升级和升级，均负有主要责任。

项目成果

Erratum: "First Search for Gravitational Waves from Known Pulsars with Advanced LIGO" (2017, ApJ, 839, 12)

勘误表：“首次利用先进的 LIGO 搜索已知脉冲星的引力波”(2017, ApJ, 839, 12)

• DOI: 10.3847/1538-4357/aa9aee
• 发表时间: 2017
• 期刊: The Astrophysical Journal
• 作者: Abbott B

THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914

• DOI: 10.3847/2041-8205/833/1/l1
• 发表时间: 2016-02
• 期刊: The Astrophysical Journal Letters
• 作者: The Ligo Scientific Collaboration;T. Abbott;R. Abbott;T. Abbott;M. Abernathy;F. Acernese;K. Ackley

Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence

• DOI: 10.1103/physrevd.94.064035
• 发表时间: 2016-09-14
• 期刊: PHYSICAL REVIEW D
• 影响因子: 5
• 作者: Abbott, B. P.;Abbott, R.;Zlochower, Y.
• 通讯作者: Zlochower, Y.

Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-Based Cross-Correlation Search in Advanced LIGO Data

• DOI: 10.3847/1538-4357/aa86f0
• 发表时间: 2017-06
• 作者: The Ligo Scientific Collaboration;T. Abbott;R. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;V. Adya;C. Affeldt;M. Afrough;B. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;B. Allen;G. Allen;A. Allocca;P. Altin;A. Amato;A. Ananyeva;S. Anderson;W. Anderson;S. Antier;S. Appert;K. Arai;M. Araya;J. Areeda;N. Arnaud;K. Arun;S. Ascenzi;G. Ashton;M. Ast;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;K. AultONeal;A. Ávila-Álvarez;S. Babak;P. Bacon;M. Bader;S. Bae;P. Baker;F. Baldaccini;G. Ballardin;S. Ballmer;S. Banagiri;J. Barayoga;S. Barclay;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;I. Bartos;R. Bassiri;A. Basti;J. Batch;C. Baune;M. Bawaj;M. Bazzan;B. B'ecsy;C. Beer;M. Bejger;I. Belahcene;A. Bell;B. Berger;G. Bergmann;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;S. Bhagwat;R. Bhandare;I. Bilenko;G. Billingsley;C. Billman;J. Birch;R. Birney;O. Birnholtz;S. Biscans;A. Bisht;M. Bitossi;C. Biwer;M. Bizouard;J. K. Blackburn;J. Blackman;C. Blair;D. Blair;R. Blair;S. Bloemen;O. Bock;N. Bode;M. Boer;G. Bogaert;A. Bohe;F. Bondu;R. Bonnand;B. A. Boom;R. Bork;V. Boschi;S. Bose;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;V. Braginsky;M. Branchesi;J. Brau;T. Briant;A. Brillet;M. Brinkmann;V. Brisson;P. Brockill;J. Broida;A. Brooks;D. Brown;D. Brown;N. Brown;S. Brunett;C. Buchanan;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;D. Buskulic;C. Buy;R. Byer;M. Cabero;L. Cadonati;G. Cagnoli;C. Cahillane;J. C. Bustillo;T. Callister;E. Calloni;J. Camp;M. Canepa;P. Canizares;K. Cannon;H. Cao;J. Cao;C. Capano;E. Capocasa;F. Carbognani;S. Caride;M. Carney;J. C. Diaz;C. Casentini;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;C. Cepeda;L. Baiardi;G. Cerretani;E. Cesarini;S. Chamberlin;M. Chan;S. Chao;P. Charlton;E. Chassande-Mottin;D. Chatterjee;K. Chatziioannou;B. Cheeseboro;H. Chen;Y. Chen;H.-P. Cheng;A. Chincarini;A. Chiummo;T. Chmiel;H. Cho;M. Cho;J. Chow;N. Christensen;Q. Chu;A. J. Chua;S. Chua;A. K. Chung;S. Chung;G. Ciani;R. Ciolfi;C. Cirelli;A. Cirone;F. Clara;J. Clark;F. Cleva;C. Cocchieri;E. Coccia;P. Cohadon;A. Colla;C. Collette;L. Cominsky;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;K. Corley;N. Cornish;A. Corsi;S. Cortese;C. Costa;M. Coughlin;S. Coughlin;J. Coulon;S. Countryman;P. Couvares;P. Covas;E. Cowan;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;J. Cripe;S. Crowder;T. Cullen;A. Cumming;L. Cunningham;E. Cuoco;T. D. Canton;S. Danilishin;S. D’Antonio;K. Danzmann;A. Dasgupta;C. F. S. Costa;V. Dattilo;I. Dave;M. Davier;D. Davis;E. Daw;B. Day;S. De;D. DeBra;E. Deelman;J. Degallaix;M. D. Laurentis;S. Del'eglise;W. D. Pozzo;T. Denker;T. Dent;V. Dergachev;R. Rosa;R. Derosa;R. DeSalvo;J. Devenson;R. Devine;S. Dhurandhar;M. D'iaz;L. Fiore;M. Giovanni;T. D. Girolamo;A. D. Lieto;S. D. Pace;I. Palma;F. Renzo;Zoheyr Doctor;V. Dolique;F. Donovan;K. Dooley;S. Doravari;I. Dorrington;R. Douglas;M. D. Álvarez;T. Downes;M. Drago;R. Drever;J. Driggers;Z. Du;M. Ducrot;J. Duncan;S. Dwyer;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;R. Eisenstein;R. Essick;Z. Etienne;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;H. Fair;S. Fairhurst;X. Fan;S. Farinon;B. Farr;W. Farr;E. Fauchon-Jones;Marc Favata;M. Fays;H. Fehrmann;J. Feicht;M. Fejer;Á. Fernández-Galiana;I. Ferrante;E. Ferreira;F. Ferrini;F. Fidecaro;I. Fiori;D. Fiorucci;R. Fisher;R. Flaminio;M. Fletcher;H. Fong;P. Forsyth;S. Forsyth;J. Fournier;S. Frasca;F. Frasconi;Z. Frei;A. Freise;R. Frey;V. Frey;E. Fries;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;H. Gabbard;M. Gabel;B. Gadre;S. Gaebel;J. Gair;D. Galloway;L. Gammaitoni;M. Ganija;S. Gaonkar;F. Garufi;S. Gaudio;G. Gaur;V. Gayathri;N. Gehrels;G. Gemme;Eric Genin;A. Gennai;D. George;J. George;L. Gergely;V. Germain;S. Ghonge;A. Ghosh;A. Ghosh;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;K. Gill;L. Glover;E. Goetz;R. Goetz;S. Gomes;G. Gonz'alez;J. M. Castro;A. Gopakumar;M. Gorodetsky;S. Gossan;M. Gosselin;R. Gouaty;A. Grado;C. Graef;M. Granata;A. Grant;S. Gras;C. Gray;G. Greco;A. Green;P. Groot;H. Grote;S. Grunewald;P. Gruning;G. Guidi;X. Guo;A. Gupta;M. Gupta;K. Gushwa;E. Gustafson;R. Gustafson;B. Hall;E. Hall;G. Hammond;M. Haney;M. Hanke;J. Hanks;C. Hanna;O. Hannuksela;J. Hanson;T. Hardwick;J. Harms;G. Harry;I. Harry;M. Hart;C. Haster;K. Haughian;J. Healy;A. Heidmann;M. Heintze;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;J. Hennig;J. Henry;A. Heptonstall;M. Heurs;S. Hild;D. Hoak;D. Hofman;K. Holt;D. Holz;P. Hopkins;C. Horst;J. Hough;E. Houston;E. Howell;Y. Hu;E. Huerta;D. Huet;B. Hughey;S. Husa;S. Huttner;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;N. Indik;D. Ingram;R. Inta;G. Intini;H. N. Isa;J. Isac;M. Isi;B. Iyer;K. Izumi;T. Jacqmin;K. Jani;P. Jaranowski;S. Jawahar;F. Jim'enez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;J. Junker;C. Kalaghatgi;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;S. Karki;K. Karvinen;M. Kasprzack;M. Katolik;E. Katsavounidis;W. Katzman;S. Kaufer;K. Kawabe;F. K'ef'elian;D. Keitel;A. Kemball;R. Kennedy;C. Kent;J. Key;F. Khalili;I. Khan;S. Khan;Z. Khan;E. Khazanov;N. Kijbunchoo;Chunglee Kim;J. Kim;W. Kim;W. Kim;Y. Kim;S. Kimbrell;E. King;P. King;R. Kirchhoff;J. S. Kissel;L. Kleybolte;S. Klimenko;P. Koch;S. Koehlenbeck;S. Koley;V. Kondrashov;A. Kontos;M. Korobko;W. Korth;I. Kowalska;D. Kozak;C. Kramer;V. Kringel;B. Krishnan;A. Kr'olak;G. Kuehn;P. Kumar;R. Kumar;S. Kumar;L. Kuo;A. Kutynia;S. Kwang;B. Lackey;K. Lai;M. Landry;R. Lang;J. Lange;B. Lantz;R. Lanza;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;C. Lee;H. Lee;H. Lee;H. W. Lee;K. Lee;J. Lehmann;A. Lenon;M. Leonardi;N. Leroy;N. Letendre;Y. Levin;T. G. F. Li;A. Libson;T. Littenberg;J. Liu;R. K. Lo;N. Lockerbie;L. London;J. Lord;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;C. Lousto;G. Lovelace;H. Luck;D. Lumaca;A. Lundgren;R. Lynch;Y. Ma;S. Macfoy;B. Machenschalk;M. Macinnis;D. Macleod;I. M. Hernandez;F. Magaña-Sandoval;L. M. Zertuche;R. Magee;E. Majorana;I. Maksimovic;N. Man;V. Mandic;V. Mangano;G. Mansell;M. Manske;M. Mantovani;F. Marchesoni;F. Marion;S. M'arka;Z. M'arka;C. Markakis;A. Markosyan;E. Maros;F. Martelli;L. Martellini;I. Martin;D. Martynov;K. Mason;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;F. Matichard;L. Matone;N. Mavalvala;R. Mayani;N. Mazumder;R. Mccarthy;D. McClelland;S. Mccormick;L. McCuller;S. Mcguire;G. Mcintyre;J. McIver;D. McManus;T. McRae;S. McWilliams;D. Meacher;G. Meadors;J. Meidam;E. Mejuto-Villa;A. Melatos;G. Mendell;R. Mercer;E. Merilh;M. Merzougui;S. Meshkov;C. Messenger;C. Messick;R. Metzdorff;P. Meyers;F. Mezzani;H. Miao;C. Michel;H. Middleton;E. Mikhailov;L. Milano;A. Miller;A. Miller;B. Miller;J. Miller;M. Millhouse;O. Minazzoli;Y. Minenkov;J. Ming;C. Mishra;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;A. Moggi;M. Mohan;S. Mohapatra;M. Montani;B. Moore;C. Moore;D. Moraru;G. Moreno;S. Morriss;B. Mours;C. Mow-Lowry;G. Mueller;A. Muir;A. Mukherjee;D. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;K. Napier;I. Nardecchia;L. Naticchioni;R. Nayak;G. Nelemans;T. Nelson;M. Neri;M. Nery;A. Neunzert;J. Newport;G. Newton;K. Ng;T. Nguyen;D. Nichols;A. B. Nielsen;S. Nissanke;A. Nitz;A. Noack;F. Nocera;D. Nolting;M. Normandin;L. Nuttall;J. Oberling;E. Ochsner;E. Oelker;G. Ogin;J. Oh;S. -. Oh;F. Ohme;M. Oliver;P. Oppermann;R. Oram;B. O'reilly;R. Ormiston;L. F. Ortega;R. O’Shaughnessy;D. Ottaway;H. Overmier;B. Owen;A. Pace;J. Page;M. Page;A. Pai;S. Pai;J. R. Palamos;O. Palashov;C. Palomba;A. Pal-Singh;H. Pan;B. Pang;P. T. Pang;C. Pankow;F. Pannarale;B. C. Pant;F. Paoletti;A. Paoli;M. Papa;H. Paris;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;B. Patricelli;B. Pearlstone;M. Pedraza;R. Pedurand;L. Pekowsky;A. Pele;S. Penn;C. Perez;A. Perreca;L. Perri;H. Pfeiffer;M. Phelps;O. Piccinni;M. Pichot;F. Piergiovanni;V. Pierro;G. Pillant;L. Pinard;I. Pinto;M. Pitkin;R. Poggiani;P. Popolizio;E. Porter;A. Post;J. Powell;J. Prasad;J. Pratt;V. Predoi;T. Prestegard;M. Prijatelj;M. Principe;S. Privitera;R. Prix;G. Prodi;L. Prokhorov;O. Puncken;M. Punturo;P. Puppo;M. Purrer;H. Qi;J. Qin;S. Qiu;V. Quetschke;E. Quintero;R. Quitzow-James;F. Raab;D. Rabeling;H. Radkins;P. Raffai;S. Raja;C. Rajan;M. Rakhmanov;K. Ramirez;P. Rapagnani;V. Raymond;M. Razzano;J. Read;T. Regimbau;L. Rei;S. Reid;D. Reitze;H. Rew;S. Reyes;F. Ricci;P. Ricker;S. Rieger;K. Riles;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;L. Rolland;J. Rollins;V. Roma;R. Romano;C. Romel;J. Romie;D. Rosi'nska;M. Ross;S. Rowan;A. Rudiger;P. Ruggi;K. Ryan;M. Rynge;S. Sachdev;T. Sadecki;L. Sadeghian;M. Sakellariadou;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;L. Sammut;L. Sampson;E. Sanchez;V. Sandberg;B. Sandeen;J. Sanders;B. Sassolas;B. Sathyaprakash;P. Saulson;O. Sauter;R. Savage;A. Sawadsky;P. Schale;J. Scheuer;E. Schmidt;J. Schmidt;P. Schmidt;R. Schnabel;R. Schofield;A. Schonbeck;E. Schreiber;D. Schuette;B. Schulte;B. Schutz;S. Schwalbe;J. Scott;S. Scott;E. Seidel;D. Sellers;A. Sengupta;D. Sentenac;V. Sequino;A. Sergeev;D. Shaddock;T. Shaffer;A. A. Shah-A.;M. Shahriar;L. Shao;B. Shapiro;P. Shawhan;A. Sheperd;D. Shoemaker;D. Shoemaker;K. Siellez;X. Siemens;M. Sieniawska;D. Sigg;A. D. Silva;A. Singer;L. Singer;A. Singh;R. Singh;A. Singhal;A. Sintes;B. Slagmolen;B. Smith;J. R. Smith;R. Smith;E. Son;J. Sonnenberg;B. Sorazu;F. Sorrentino;T. Souradeep;A. Spencer;A. Srivastava;A. Staley;M. Steinke;J. Steinlechner;S. Steinlechner;D. Steinmeyer;B. Stephens;R. Stone;K. Strain;G. Stratta;S. Strigin;R. Sturani;A. Stuver;T. Summerscales;L. Sun;S. Sunil;P. Sutton;B. Swinkels;M. J. Szczepa'nczyk;M. Tacca;D. Talukder;D. Tanner;M. T'apai;A. Taracchini;J. A. Taylor;R. Taylor;T. Theeg;E. Thomas;M. Thomas;P. Thomas;K. Thorne;K. Thorne;E. Thrane;S. Tiwari;V. Tiwari;K. Tokmakov;K. Toland;M. Tonelli;Z. Tornasi;C. Torrie;D. Toyra;F. Travasso;G. Traylor;D. Trifirò;J. Trinastic;M. Tringali;L. Trozzo;K. W. Tsang;M. Tse;R. Tso;D. Tuyenbayev;K. Ueno;D. Ugolini;C. Unnikrishnan;A. Urban;S. Usman;K. Vahi;H. Vahlbruch;G. Vajente;G. Valdes;M. Vallisneri;N. Bakel;M. Beuzekom;J. Brand;C. Broeck;D. Vander-Hyde;L. V. D. Schaaf;J. V. Heijningen;A. V. Veggel;M. Vardaro;V. Varma;S. Vass;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;Gautam Venugopalan;D. Verkindt;F. Vetrano;A. Vicer'e;A. Viets;S. Vinciguerra;D. Vine;J. Vinet;S. Vitale;T. Vo;H. Vocca;C. Vorvick;D. Voss;W. Vousden;S. Vyatchanin;A. Wade;L. Wade;M. Wade;R. Walet;M. Walker;L. Wallace;S. Walsh;G. Wang;H. Wang;J. Wang;M. Wang;Y.-F. Wang;Y. Wang;R. Ward;J. Warner;M. Was;J. Watchi;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;L. Wen;E. Wessel;P. Wessels;T. Westphal;K. Wette;J. Whelan;B. Whiting;C. Whittle;D. Williams;R. Williams;A. Williamson;J. Willis;B. Willke;M. Wimmer;W. Winkler;C. Wipf;H. Wittel;G. Woan;J. Woehler;J. Wofford;K. Wong;J. Worden;J. Wright;D. Wu;G. Wu;W. Yam;H. Yamamoto;C. Yancey;M. Yap;Hang Yu;Haocun Yu;M. Yvert;A. Zadro.zny;M. Zanolin;T. Zelenova;J. Zendri;M. Zevin;L. Zhang;M. Zhang;T. Zhang;Y.H. Zhang;C. Zhao;M. Zhou;Z. Zhou;X. Zhu;M. Zucker;J. Zweizig;D. Steeghs;L. Wang

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