Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching 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. C Barish; D Barker; P Barneo; 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; S Biscans; M Bischi; S Biscoveanu; A Bisht; B Biswas; M Bitossi; M. -A Bizouard; J. K Blackburn; J Blackman; C. D Blair; D. G Blair; R. M Blair; F Bobba; N Bode; M Boer; G Bogaert; M Boldrini; 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. R Brady; A Bramley; A Branch; M Branchesi; J. E Brau; M Breschi; T Briant; J. H Briggs; A Brillet; M Brinkmann; P Brockill; A. F Brooks; J Brooks; D. D Brown; S Brunett; G Bruno; R Bruntz; J Bryant; A Buikema; T Bulik; H. J Bulten; A Buonanno; R Buscicchio; D Buskulic; R. L Byer; 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; 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. 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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; A Sergeev; 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. 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doi:10.48550/arxiv.2104.14417

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Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching 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

07/01/2022

DOI: https://doi.org/10.48550/arxiv.2104.14417

摘要

Physics - General Relativity and Quantum Cosmology

Physics - High Energy Astrophysical Phenomena

ApJ 922 71 (2021) We present a search for continuous gravitational-wave emission due to r-modes in the pulsar PSR J0537-6910 using data from the LIGO-Virgo Collaboration observing run O3. PSR J0537-6910 is a young energetic X-ray pulsar and is the most frequent glitcher known. The inter-glitch braking index of the pulsar suggests that gravitational-wave emission due to r-mode oscillations may play an important role in the spin evolution of this pulsar. Theoretical models confirm this possibility and predict emission at a level that can be probed by ground-based detectors. In order to explore this scenario, we search for r-mode emission in the epochs between glitches by using a contemporaneous timing ephemeris obtained from NICER data. We do not detect any signals in the theoretically expected band of 86-97 Hz, and report upper limits on the amplitude of the gravitational waves. Our results improve on previous amplitude upper limits from r-modes in J0537-6910 by a factor of up to 3 and place stringent constraints on theoretical models for r-mode driven spin-down in PSR J0537-6910, especially for higher frequencies at which our results reach below the spin-down limit defined by energy conservation.

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題名: Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching 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
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
S Biscans
M Bischi
S Biscoveanu
A Bisht
B Biswas
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J Blackman
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M Boer
G Bogaert
M Boldrini
F Bondu
E Bonilla
R Bonnand
P Booker
B. A Boom
R Bork
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N Bose
S Bose
V Bossilkov
V Boudart
Y Bouffanais
A Bozzi
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M Zhan
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T Enoto
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學術資源類型: 預印本
出版資訊: arXiv.org
語言: 英語

Constraints from LIGO O3 data on gravitational-wave emission due to r-modes in the glitching pulsar PSR J0537-6910

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