Searches for continuous gravitational waves from nine young supernova remnants
Searches for continuous gravitational waves from nine young supernova remnants
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DOI：
10.1088/0004-637x/813/1/39
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发表时间：
2014-12
期刊：
影响因子：
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通讯作者：
J. Aasi;B. Abbott;R. Abbott;T. Abbott;M. Abernathy;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;V. Adya;C. Affeldt;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;A. Ain;P. Ajith;A. Alemic;B. Allen;A. Allocca;D. Amariutei;S. Anderson;W. Anderson;K. Arai;M. Araya;C. Arceneaux;J. Areeda;S. Ast;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;B. Aylott;S. Babak;P. Baker;F. Baldaccini;G. Ballardin;S. Ballmer;J. Barayoga;M. Barbet;S. Barclay;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;J. Bartlett;M. Barton;I. Bartos;R. Bassiri;A. Basti;J. Batch;T. Bauer;C. Baune;V. Bavigadda;B. Behnke;M. Bejger;C. Belczynski;A. Bell;C. Bell;M. Benacquista;J. Bergman;G. Bergmann;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;S. Bhagwat;R. Bhandare;I. Bilenko;G. Billingsley;J. Birch;S. Biscans;M. Bitossi;C. Biwer;M. Bizouard;J. Blackburn;L. Blackburn;C. Blair;D. Blair;S. Bloemen;O. Bock;T. Bodiya;M. Boer;G. Bogaert;P. Bojtos;C. Bond;F. Bondu;L. Bonelli;R. Bonnand;R. Bork;M. Born;V. Boschi;S. Bose;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;N. Brown;S. Buchman;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;D. Buskulic;C. Buy;L. Cadonati;G. Cagnoli;J. C. Bustillo;E. Calloni;J. Camp;K. Cannon;J. Cao;C. Capano;F. Carbognani;S. Caride;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;C. Cepeda;E. Cesarini;R. Chakraborty;T. Chalermsongsak;S. Chamberlin;S. Chao;P. Charlton;É. Chassande-Mottin;Y. Chen;A. Chincarini;A. Chiummo;H. Cho;M. 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;N. Cornish;A. Corsi;C. Costa;M. Coughlin;J. Coulon;S. Countryman;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;K. Craig;J. Creighton;T. Creighton;J. Cripe;S. Crowder;A. Cumming;L. Cunningham;E. Cuoco;C. Cutler;K. Dahl;T. D. Canton;M. Damjanic;S. Danilishin;S. D’Antonio;K. Danzmann;L. Dartez;V. Dattilo;I. Dave;H. Daveloza;M. Davier;G. Davies;E. Daw;R. Day;D. DeBra;G. Debreczeni;J. Degallaix;M. D. Laurentis;S. Deléglise;W. D. Pozzo;T. Denker;T. Dent;H. Dereli;V. Dergachev;R. Rosa;R. Derosa;R. DeSalvo;S. Dhurandhar;M. Díaz;L. Fiore;A. Lieto;I. Palma;A. Virgilio;G. Dojcinoski;V. Dolique;E. Dominguez;F. Donovan;K. Dooley;S. Doravari;R. Douglas;T. Downes;M. Drago;J. Driggers;Z. Du;M. Ducrot;S. Dwyer;T. Eberle;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;R. Essick;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;S. Fairhurst;X. Fan;Q. Fang;S. Farinon;B. Farr;W. Farr;Marc Favata;M. Fays;H. Fehrmann;M. Fejer;D. Feldbaum;I. Ferrante;E. Ferreira;F. Ferrini;F. Fidecaro;I. Fiori;R. Fisher;R. Flaminio;J. Fournier;S. Franco;S. Frasca;F. Frasconi;Z. Frei;A. Freise;R. Frey;T. Fricke;P. Fritschel;V. Frolov;S. Fuentes-Tapia;P. Fulda;M. Fyffe;J. Gair;L. Gammaitoni;S. Gaonkar;F. Garufi;A. Gatto;N. Gehrels;G. Gemme;B. Gendre;E. Génin;A. Gennai;L. Gergely;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;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;S. Grunewald;G. Guidi;C. Guido;X. Guo;K. Gushwa;E. Gustafson;R. Gustafson;J. Hacker;E. Hall;G. Hammond;M. Hanke;J. Hanks;C. Hanna;M. Hannam;J. Hanson;T. Hardwick;J. Harms;G. Harry;I. Harry;M. Hart;M. Hartman;C. Haster;K. Haughian;S. Hee;A. Heidmann;M. Heintze;G. Heinzel;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;A. Heptonstall;M. Heurs;M. Hewitson;S. Hild;D. Hoak;K. Hodge;D. Hofman;S. Hollitt;K. Holt;P. Hopkins;D. Hosken;J. Hough;E. Houston;E. Howell;Y. Hu;E. Huerta;B. Hughey;S. Husa;S. Huttner;M. Huynh;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;A. Idrisy;N. Indik;D. Ingram;R. Inta;G. Islas;J. Isler;T. Isogai;B. Iyer;K. Izumi;M. Jacobson;H. Jang;P. Jaranowski;S. Jawahar;Y. Ji;F. Jiménez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;M. Kasprzack;E. Katsavounidis;W. Katzman;H. Kaufer;S. Kaufer;T. Kaur;K. Kawabe;F. Kawazoe;F. Kéfélian;G. M. Keiser;D. Keitel;D. Kelley;W. Kells;D. Keppel;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;M. Korobko;W. Korth;I. Kowalska;D. Kozak;V. Kringel;B. Krishnan;A. Królak;C. Krueger;G. Kuehn;A. Kumar;P. Kumar;L. Kuo;A. Kutynia;M. Landry;B. Lantz;S. Larson;P. Lasky;A. Lazzarini;C. Lazzaro;J. Le;P. Leaci;S. Leavey;E. Lebigot;E. Lebigot;C. Lee;H. Lee;H. Lee;M. Leonardi;J. Leong;N. Leroy;N. Letendre;Y. Levin;B. Levine;J. Lewis;T. G. F. Li;K. Libbrecht;A. Libson;A. Lin;T. Littenberg;N. Lockerbie;V. Lockett;J. Logue;A. Lombardi;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo
中科院分区：
文献类型：
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作者：
J. Aasi;B. Abbott;R. Abbott;T. Abbott;M. Abernathy;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;V. Adya;C. Affeldt;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;A. Ain;P. Ajith;A. Alemic;B. Allen;A. Allocca;D. Amariutei;S. Anderson;W. Anderson;K. Arai;M. Araya;C. Arceneaux;J. Areeda;S. Ast;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;B. Aylott;S. Babak;P. Baker;F. Baldaccini;G. Ballardin;S. Ballmer;J. Barayoga;M. Barbet;S. Barclay;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;J. Bartlett;M. Barton;I. Bartos;R. Bassiri;A. Basti;J. Batch;T. Bauer;C. Baune;V. Bavigadda;B. Behnke;M. Bejger;C. Belczynski;A. Bell;C. Bell;M. Benacquista;J. Bergman;G. Bergmann;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;S. Bhagwat;R. Bhandare;I. Bilenko;G. Billingsley;J. Birch;S. Biscans;M. Bitossi;C. Biwer;M. Bizouard;J. Blackburn;L. Blackburn;C. Blair;D. Blair;S. Bloemen;O. Bock;T. Bodiya;M. Boer;G. Bogaert;P. Bojtos;C. Bond;F. Bondu;L. Bonelli;R. Bonnand;R. Bork;M. Born;V. Boschi;S. Bose;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;N. Brown;S. Buchman;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;D. Buskulic;C. Buy;L. Cadonati;G. Cagnoli;J. C. Bustillo;E. Calloni;J. Camp;K. Cannon;J. Cao;C. Capano;F. Carbognani;S. Caride;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;C. Cepeda;E. Cesarini;R. Chakraborty;T. Chalermsongsak;S. Chamberlin;S. Chao;P. Charlton;É. Chassande-Mottin;Y. Chen;A. Chincarini;A. Chiummo;H. Cho;M. 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;N. Cornish;A. Corsi;C. Costa;M. Coughlin;J. Coulon;S. Countryman;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;K. Craig;J. Creighton;T. Creighton;J. Cripe;S. Crowder;A. Cumming;L. Cunningham;E. Cuoco;C. Cutler;K. Dahl;T. D. Canton;M. Damjanic;S. Danilishin;S. D’Antonio;K. Danzmann;L. Dartez;V. Dattilo;I. Dave;H. Daveloza;M. Davier;G. Davies;E. Daw;R. Day;D. DeBra;G. Debreczeni;J. Degallaix;M. D. Laurentis;S. Deléglise;W. D. Pozzo;T. Denker;T. Dent;H. Dereli;V. Dergachev;R. Rosa;R. Derosa;R. DeSalvo;S. Dhurandhar;M. Díaz;L. Fiore;A. Lieto;I. Palma;A. Virgilio;G. Dojcinoski;V. Dolique;E. Dominguez;F. Donovan;K. Dooley;S. Doravari;R. Douglas;T. Downes;M. Drago;J. Driggers;Z. Du;M. Ducrot;S. Dwyer;T. Eberle;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;R. Essick;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;S. Fairhurst;X. Fan;Q. Fang;S. Farinon;B. Farr;W. Farr;Marc Favata;M. Fays;H. Fehrmann;M. Fejer;D. Feldbaum;I. Ferrante;E. Ferreira;F. Ferrini;F. Fidecaro;I. Fiori;R. Fisher;R. Flaminio;J. Fournier;S. Franco;S. Frasca;F. Frasconi;Z. Frei;A. Freise;R. Frey;T. Fricke;P. Fritschel;V. Frolov;S. Fuentes-Tapia;P. Fulda;M. Fyffe;J. Gair;L. Gammaitoni;S. Gaonkar;F. Garufi;A. Gatto;N. Gehrels;G. Gemme;B. Gendre;E. Génin;A. Gennai;L. Gergely;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;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;S. Grunewald;G. Guidi;C. Guido;X. Guo;K. Gushwa;E. Gustafson;R. Gustafson;J. Hacker;E. Hall;G. Hammond;M. Hanke;J. Hanks;C. Hanna;M. Hannam;J. Hanson;T. Hardwick;J. Harms;G. Harry;I. Harry;M. Hart;M. Hartman;C. Haster;K. Haughian;S. Hee;A. Heidmann;M. Heintze;G. Heinzel;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;A. Heptonstall;M. Heurs;M. Hewitson;S. Hild;D. Hoak;K. Hodge;D. Hofman;S. Hollitt;K. Holt;P. Hopkins;D. Hosken;J. Hough;E. Houston;E. Howell;Y. Hu;E. Huerta;B. Hughey;S. Husa;S. Huttner;M. Huynh;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;A. Idrisy;N. Indik;D. Ingram;R. Inta;G. Islas;J. Isler;T. Isogai;B. Iyer;K. Izumi;M. Jacobson;H. Jang;P. Jaranowski;S. Jawahar;Y. Ji;F. Jiménez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;M. Kasprzack;E. Katsavounidis;W. Katzman;H. Kaufer;S. Kaufer;T. Kaur;K. Kawabe;F. Kawazoe;F. Kéfélian;G. M. Keiser;D. Keitel;D. Kelley;W. Kells;D. Keppel;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;M. Korobko;W. Korth;I. Kowalska;D. Kozak;V. Kringel;B. Krishnan;A. Królak;C. Krueger;G. Kuehn;A. Kumar;P. Kumar;L. Kuo;A. Kutynia;M. Landry;B. Lantz;S. Larson;P. Lasky;A. Lazzarini;C. Lazzaro;J. Le;P. Leaci;S. Leavey;E. Lebigot;E. Lebigot;C. Lee;H. Lee;H. Lee;M. Leonardi;J. Leong;N. Leroy;N. Letendre;Y. Levin;B. Levine;J. Lewis;T. G. F. Li;K. Libbrecht;A. Libson;A. Lin;T. Littenberg;N. Lockerbie;V. Lockett;J. Logue;A. Lombardi;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo
我们描述了从第六次LIGO科学数据运行中对数据中连续引力波的定向搜索。这些目标是九个年轻的超新星残骸，与脉冲星无关；其中八个残骸与非脉冲疑似中子星有关。一个目标的参数不确定，足以保证两次搜索，总共十次。每一次搜索都覆盖了很宽的频率范围，以及固定天空方向的一阶和二阶频率导数。搜索使用匹配过滤F统计量在5.3-25.3天的时间跨度内一致地整合了来自两个LIGO干涉仪的数据。我们没有发现可信的引力波信号。我们将95%的置信度上限设置为本征应变为$4×10^-25$，基准椭圆度为$2×10^-7}$，r模振幅为$4×10^-5}$。这超出了能量守恒的间接极限，并在中子星椭圆度和r模振幅的理论预测范围内。
We describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target's parameters are uncertain enough to warrant two searches, for a total of ten. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering F-statistic. We found no credible gravitational-wave signals. We set 95% confidence upper limits as strong (low) as $4\times10^{-25}$ on intrinsic strain, $2\times10^{-7}$ on fiducial ellipticity, and $4\times10^{-5}$ on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.