Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

The LIGO Scientific Collaboration; the Virgo Collaboration; the KAGRA Collaboration; R Abbott; T. D Abbott; S Abraham; F Acernese; K Ackley; A Adams; C Adams; R. X Adhikari; V. B Adya; C Affeldt; D Agarwal; M Agathos; K Agatsuma; N Aggarwal; O. D Aguiar; L Aiello; A Ain; P Ajith; T Akutsu; K. M Aleman; G Allen; A Allocca; P. A Altin; A Amato; S Anand; A Ananyeva; S. B Anderson; W. G Anderson; M Ando; S. V Angelova; S Ansoldi; J. M Antelis; S Antier; S Appert; Koya Arai; Koji Arai; Y Arai; S Araki; A Araya; M. C Araya; J. S Areeda; M Arène; N Aritomi; N Arnaud; S. M Aronson; K. G Arun; H Asada; Y Asali; G Ashton; Y Aso; S. M Aston; P Astone; F Aubin; P Aufmuth; K AultONeal; C Austin; S Babak; F Badaracco; M. K. M Bader; S Bae; Y Bae; A. M Baer; S Bagnasco; Y Bai; L Baiotti; J Baird; R Bajpai; M Ball; G Ballardin; S. W Ballmer; M Bals; A Balsamo; G Baltus; S Banagiri; D Bankar; R. S Bankar; J. C Barayoga; C Barbieri; B. 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D Brown; S Brunett; G Bruno; R Bruntz; J Bryant; A Buikema; T Bulik; H. J Bulten; A Buonanno; R Buscicchio; D Buskulic; L Cadonati; M Caesar; G Cagnoli; C Cahillane; H. W CainIII; J. Calderón Bustillo; J. D Callaghan; T. A Callister; E Calloni; J. B Camp; M Canepa; M Cannavacciuolo; K. C Cannon; H Cao; J Cao; Z Cao; E Capocasa; E Capote; G Carapella; F Carbognani; J. B Carlin; M. F Carney; M Carpinelli; G Carullo; T. L Carver; J. Casanueva Diaz; C Casentini; G Castaldi; S Caudill; M Cavaglià; F Cavalier; R Cavalieri; G Cella; P Cerdá-Durán; E Cesarini; W Chaibi; K Chakravarti; B Champion; C. -H Chan; C Chan; C. L Chan; M Chan; K Chandra; P Chanial; S Chao; P Charlton; E. A Chase; E Chassande-Mottin; D Chatterjee; M Chaturvedi; K Chatziioannou; A Chen; C Chen; H. Y Chen; J Chen; K Chen; X Chen; Y. -B Chen; Y. -R Chen; Z Chen; H Cheng; C. K Cheong; H. Y Cheung; H. Y Chia; F Chiadini; C-Y Chiang; R Chierici; A Chincarini; M. L Chiofalo; A Chiummo; G Cho; H. S Cho; S Choate; R. K Choudhary; S Choudhary; N Christensen; H Chu; Q Chu; Y-K Chu; S Chua; K. W Chung; G Ciani; P Ciecielag; M Cieślar; M Cifaldi; A. A Ciobanu; R Ciolfi; F Cipriano; A Cirone; F Clara; E. N Clark; J. A Clark; L Clarke; P Clearwater; S Clesse; F Cleva; E Coccia; P. -F Cohadon; D. E Cohen; L Cohen; M Colleoni; C. G Collette; M Colpi; C. M Compton; M ConstancioJr; L Conti; S. J Cooper; P Corban; T. R Corbitt; I Cordero-Carrión; S Corezzi; K. R Corley; N Cornish; D Corre; A Corsi; S Cortese; C. A Costa; R Cotesta; M. W Coughlin; S. B Coughlin; J. -P Coulon; S. T Countryman; B Cousins; P Couvares; P. B Covas; D. M Coward; M. J Cowart; D. C Coyne; R Coyne; J. D. E Creighton; T. D Creighton; A. W Criswell; M Croquette; S. G Crowder; J. R Cudell; T. J Cullen; A Cumming; R Cummings; E Cuoco; M Curyło; T. Dal Canton; G Dálya; A Dana; L. M DaneshgaranBajastani; B D'Angelo; S. L Danilishin; S D'Antonio; K Danzmann; C Darsow-Fromm; A Dasgupta; L. E. H Datrier; V Dattilo; I Dave; M Davier; G. S Davies; D Davis; E. J Daw; R Dean; M Deenadayalan; J Degallaix; M De Laurentis; S Deléglise; V Del Favero; F De Lillo; N De Lillo; W Del Pozzo; L. M DeMarchi; F De Matteis; V D'Emilio; N Demos; T Dent; A Depasse; R De Pietri; R De Rosa; C De Rossi; R DeSalvo; R De Simone; S Dhurandhar; M. C Díaz; M Diaz-OrtizJr; N. A Didio; T Dietrich; L Di Fiore; C Di Fronzo; C Di Giorgio; F Di Giovanni; T Di Girolamo; A Di Lieto; B Ding; S Di Pace; I Di Palma; F Di Renzo; A. K Divakarla; A Dmitriev; Z Doctor; L D'Onofrio; F Donovan; K. L Dooley; S Doravari; I Dorrington; M Drago; J. C Driggers; Y Drori; Z Du; J. -G Ducoin; P Dupej; O Durante; D D'Urso; P. -A Duverne; S. E Dwyer; P. J Easter; M Ebersold; G Eddolls; B Edelman; T. B Edo; O Edy; A Effler; S Eguchi; J Eichholz; S. S Eikenberry; M Eisenmann; R. A Eisenstein; A Ejlli; Y Enomoto; L Errico; R. C Essick; H Estellés; D Estevez; Z Etienne; T Etzel; M Evans; T. M Evans; B. E Ewing; V Fafone; H Fair; S Fairhurst; X Fan; A. M Farah; S Farinon; B Farr; W. M Farr; N. W Farrow; E. J Fauchon-Jones; M Favata; M Fays; M Fazio; J Feicht; M. M Fejer; F Feng; E Fenyvesi; D. L Ferguson; A Fernandez-Galiana; I Ferrante; T. A Ferreira; F Fidecaro; P Figura; I Fiori; M Fishbach; R. P Fisher; J. M Fishner; R Fittipaldi; V Fiumara; R Flaminio; E Floden; E Flynn; H Fong; J. A Font; B Fornal; P. W. F Forsyth; A Franke; S Frasca; F Frasconi; C Frederick; Z Frei; A Freise; R Frey; P Fritschel; V. V Frolov; G. G Fronzé; Y Fujii; Y Fujikawa; M Fukunaga; M Fukushima; P Fulda; M Fyffe; H. A Gabbard; B. U Gadre; S. M Gaebel; J. R Gair; J Gais; S Galaudage; R Gamba; D Ganapathy; A Ganguly; D Gao; S. G Gaonkar; B Garaventa; C García-Núñez; C García-Quirós; F Garufi; B Gateley; S Gaudio; V Gayathri; G Ge; G Gemme; A Gennai; J George; L Gergely; P Gewecke; S Ghonge; Abhirup Ghosh; Archisman Ghosh; Shaon Ghosh; Shrobana Ghosh; Sourath Ghosh; B Giacomazzo; L Giacoppo; J. A Giaime; K. D Giardina; D. 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H Reitze; P Relton; P Rettegno; F Ricci; C. J Richardson; J. W Richardson; L Richardson; P. M Ricker; G Riemenschneider; K Riles; M Rizzo; N. A Robertson; R Robie; F Robinet; A Rocchi; J. A Rocha; S Rodriguez; R. D Rodriguez-Soto; L Rolland; J. G Rollins; V. J Roma; M Romanelli; R Romano; C. L Romel; A Romero; I. M Romero-Shaw; J. H Romie; C. A Rose; D Rosińska; S. G Rosofsky; M. P Ross; S Rowan; S. J Rowlinson; Santosh Roy; Soumen 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. S Salafia; L Salconi; M Saleem; F Salemi; A Samajdar; E. J Sanchez; J. H Sanchez; L. E Sanchez; N Sanchis-Gual; J. R Sanders; A Sanuy; T. R Saravanan; N Sarin; B Sassolas; H Satari; S Sato; T Sato; O Sauter; R. L Savage; V Savant; T Sawada; D Sawant; H. L Sawant; S Sayah; D Schaetzl; M Scheel; J Scheuer; A Schindler-Tyka; P Schmidt; R Schnabel; M Schneewind; R. M. S Schofield; A Schönbeck; B. W Schulte; B. F Schutz; E Schwartz; J Scott; S. M Scott; M Seglar-Arroyo; E Seidel; T Sekiguchi; Y Sekiguchi; D Sellers; A. S Sengupta; N Sennett; D Sentenac; E. G Seo; V Sequino; Y Setyawati; T Shaffer; M. S Shahriar; B Shams; L Shao; S Sharifi; A Sharma; P Sharma; P Shawhan; N. S Shcheblanov; H Shen; S Shibagaki; M Shikauchi; R Shimizu; T Shimoda; K Shimode; R Shink; H Shinkai; T Shishido; A Shoda; D. H Shoemaker; D. M Shoemaker; K Shukla; S ShyamSundar; M Sieniawska; D Sigg; L. P Singer; D Singh; N Singh; A Singha; A. M Sintes; V Sipala; V Skliris; B. J. J Slagmolen; T. J Slaven-Blair; J Smetana; J. R Smith; R. J. E Smith; S. N Somala; K Somiya; E. J Son; K Soni; S Soni; B Sorazu; V Sordini; F Sorrentino; N Sorrentino; H Sotani; R Soulard; T Souradeep; E Sowell; V Spagnuolo; A. P Spencer; M Spera; A. K Srivastava; V Srivastava; K Staats; C Stachie; D. A Steer; J Steinlechner; S Steinlechner; D. J Stops; M Stover; K. A Strain; L. C Strang; G Stratta; A Strunk; R Sturani; A. L Stuver; J Südbeck; S Sudhagar; V Sudhir; R Sugimoto; H. G Suh; T. Z Summerscales; H Sun; L Sun; S Sunil; A Sur; J Suresh; P. J Sutton; Takamasa Suzuki; Toshikazu Suzuki; B. L Swinkels; M. J Szczepańczyk; P Szewczyk; M Tacca; H Tagoshi; S. C 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. J Tanasijczuk; S Tanioka; D. B Tanner; D Tao; A Tapia; E. N. Tapia San Martin; J. D Tasson; S Telada; R Tenorio; L Terkowski; M Test; M. P Thirugnanasambandam; M Thomas; P Thomas; J. E Thompson; S. R Thondapu; K. A Thorne; E Thrane; Shubhanshu Tiwari; Srishti Tiwari; V Tiwari; K Toland; A. E Tolley; T Tomaru; Y Tomigami; T Tomura; M Tonelli; A Torres-Forné; C. I Torrie; I. Tosta e Melo; D Töyrä; A Trapananti; F Travasso; G Traylor; M. C Tringali; A Tripathee; L Troiano; A Trovato; L Trozzo; R. J Trudeau; D. S Tsai; D Tsai; K. 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Y Washington; J Watchi; B Weaver; L Wei; M Weinert; A. J Weinstein; R Weiss; C. M Weller; F Wellmann; L Wen; P Weßels; J. W Westhouse; K Wette; J. T Whelan; D. D White; B. F Whiting; C Whittle; D Wilken; D Williams; M. J Williams; A. R Williamson; J. L Willis; B Willke; D. J Wilson; W Winkler; C. C Wipf; T Wlodarczyk; G Woan; J Woehler; J. K Wofford; I. C. F Wong; J Wrangel; C Wu; D. S Wu; H Wu; S Wu; D. M Wysocki; L Xiao; W-R Xu; T Yamada; H Yamamoto; Kazuhiro Yamamoto; Kohei Yamamoto; T Yamamoto; K Yamashita; R Yamazaki; F. W Yang; L Yang; Yang Yang; Yi Yang; Z Yang; M. J Yap; D. W Yeeles; A. B Yelikar; M Ying; K Yokogawa; J Yokoyama; T Yokozawa; A Yoon; T Yoshioka; Hang Yu; Haocun Yu; H Yuzurihara; A Zadrożny; M Zanolin; S Zeidler; T Zelenova; J. -P 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. J Zhu; Z. -H Zhu; M. E Zucker; J Zweizig; D Antonopoulou; Z Arzoumanian; T Enoto; C. M Espinoza; S Guillot

doi:10.48550/arxiv.2012.12926

預印本

Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration, R Abbott, T. D Abbott, S Abraham, F Acernese, K Ackley, A Adams, C Adams, …

arXiv.org

10/06/2021

DOI: https://doi.org/10.48550/arxiv.2012.12926

摘要

Physics - General Relativity and Quantum Cosmology

Physics - High Energy Astrophysical Phenomena

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency. We find no signal, however, and report our upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of two and limit gravitational waves from thel=m=2mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is limited to less than about 3e-5, which is the third best constraint for any young pulsar.

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詳細資料

題名: Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910
創作者：: The LIGO Scientific Collaboration
the Virgo Collaboration
the KAGRA Collaboration
R Abbott
T. D Abbott
S Abraham
F Acernese
K Ackley
A Adams
C Adams
R. X Adhikari
V. B Adya
C Affeldt
D Agarwal
M Agathos
K Agatsuma
N Aggarwal
O. D Aguiar
L Aiello
A Ain
P Ajith
T Akutsu
K. M Aleman
G Allen
A Allocca
P. A Altin
A Amato
S Anand
A Ananyeva
S. B Anderson
W. G Anderson
M Ando
S. V Angelova
S Ansoldi
J. M Antelis
S Antier
S Appert
Koya Arai
Koji Arai
Y Arai
S Araki
A Araya
M. C Araya
J. S Areeda
M Arène
N Aritomi
N Arnaud
S. M Aronson
K. G Arun
H Asada
Y Asali
G Ashton
Y Aso
S. M Aston
P Astone
F Aubin
P Aufmuth
K AultONeal
C Austin
S Babak
F Badaracco
M. K. M Bader
S Bae
Y Bae
A. M Baer
S Bagnasco
Y Bai
L Baiotti
J Baird
R Bajpai
M Ball
G Ballardin
S. W Ballmer
M Bals
A Balsamo
G Baltus
S Banagiri
D Bankar
R. S Bankar
J. C Barayoga
C Barbieri
B. C Barish
D Barker
P Barneo
S Barnum
F Barone
B Barr
L Barsotti
M Barsuglia
D Barta
J Bartlett
M. A Barton
I Bartos
R Bassiri
A Basti
M Bawaj
J. C Bayley
A. C Baylor
M Bazzan
B Bécsy
V. M Bedakihale
M Bejger
I Belahcene
V Benedetto
D Beniwal
M. G Benjamin
T. F Bennett
J. D Bentley
M BenYaala
F Bergamin
B. K Berger
S Bernuzzi
D Bersanetti
A Bertolini
J Betzwieser
R Bhandare
A. V Bhandari
D Bhattacharjee
S Bhaumik
J Bidler
I. A Bilenko
G Billingsley
R Birney
O Birnholtz
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M Bischi
S Biscoveanu
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J Blackman
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D. G Blair
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M Boer
G Bogaert
M Boldrini
F Bondu
E Bonilla
R Bonnand
P Booker
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R Bork
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V Bossilkov
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A Bozzi
C Bradaschia
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A Bramley
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A Zadrożny
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T Zelenova
J. -P Zendri
M Zevin
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R Zhang
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T Enoto
C. M Espinoza
S Guillot
學術資源類型: 預印本
出版資訊: arXiv.org
語言: 英語

Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

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