Reducing scattered light in LIGO's third observing run

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Autorschaft

  • The LIGO Scientific Collaboration
  • N. Bode
  • P. Booker
  • J. Liu
  • Fabian Meylahn

Organisationseinheiten

Externe Organisationen

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer025016
FachzeitschriftClassical and quantum gravity
Jahrgang38
Ausgabenummer2
Frühes Online-Datum14 Dez. 2020
PublikationsstatusVeröffentlicht - 22 Jan. 2021

Abstract

Noise due to scattered light has been a frequent disturbance in the advanced LIGO gravitational wave detectors, hindering the detection of gravitational waves. The non stationary scatter noise caused by low frequency motion can be recognized as arches in the time-frequency plane of the gravitational wave channel. In this paper, we characterize the scattering noise for LIGO and Virgo's third observing run O3 from April, 2019 to March, 2020. We find at least two different populations of scattering noise and we investigate the multiple origins of one of them as well as its mitigation. We find that relative motion between two specific surfaces is strongly correlated with the presence of scattered light and we implement a technique to reduce this motion. We also present an algorithm using a witness channel to identify the times this noise can be present in the detector.

ASJC Scopus Sachgebiete

Zitieren

Reducing scattered light in LIGO's third observing run. / The LIGO Scientific Collaboration; Bode, N.; Booker, P. et al.
in: Classical and quantum gravity, Jahrgang 38, Nr. 2, 025016, 22.01.2021.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

The LIGO Scientific Collaboration, Bode, N, Booker, P, Liu, J & Meylahn, F 2021, 'Reducing scattered light in LIGO's third observing run', Classical and quantum gravity, Jg. 38, Nr. 2, 025016. https://doi.org/10.1088/1361-6382/abc906
The LIGO Scientific Collaboration, Bode, N., Booker, P., Liu, J., & Meylahn, F. (2021). Reducing scattered light in LIGO's third observing run. Classical and quantum gravity, 38(2), Artikel 025016. https://doi.org/10.1088/1361-6382/abc906
The LIGO Scientific Collaboration, Bode N, Booker P, Liu J, Meylahn F. Reducing scattered light in LIGO's third observing run. Classical and quantum gravity. 2021 Jan 22;38(2):025016. Epub 2020 Dez 14. doi: 10.1088/1361-6382/abc906
The LIGO Scientific Collaboration ; Bode, N. ; Booker, P. et al. / Reducing scattered light in LIGO's third observing run. in: Classical and quantum gravity. 2021 ; Jahrgang 38, Nr. 2.
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abstract = "Noise due to scattered light has been a frequent disturbance in the advanced LIGO gravitational wave detectors, hindering the detection of gravitational waves. The non stationary scatter noise caused by low frequency motion can be recognized as arches in the time-frequency plane of the gravitational wave channel. In this paper, we characterize the scattering noise for LIGO and Virgo's third observing run O3 from April, 2019 to March, 2020. We find at least two different populations of scattering noise and we investigate the multiple origins of one of them as well as its mitigation. We find that relative motion between two specific surfaces is strongly correlated with the presence of scattered light and we implement a technique to reduce this motion. We also present an algorithm using a witness channel to identify the times this noise can be present in the detector.",
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Download

TY - JOUR

T1 - Reducing scattered light in LIGO's third observing run

AU - The LIGO Scientific Collaboration

AU - Soni, S.

AU - Austin, C.

AU - Effler, A.

AU - Schofield, R. M. S.

AU - Gonzalez, G.

AU - Frolov, V. V.

AU - Driggers, J. C.

AU - Pele, A.

AU - Urban, A. L.

AU - Valdes, G.

AU - Abbott, R.

AU - Adams, C.

AU - Adhikari, R. X.

AU - Ananyeva, A.

AU - Appert, S.

AU - Arai, K.

AU - Areeda, J. S.

AU - Asali, Y.

AU - Aston, S. M.

AU - Baer, A. M.

AU - Ball, M.

AU - Ballmer, S. W.

AU - Banagiri, S.

AU - Barker, D.

AU - Barsotti, L.

AU - Bartlett, J.

AU - Berger, B. K.

AU - Betzwieser, J.

AU - Bhattacharjee, D.

AU - Billingsley, G.

AU - Biscans, S.

AU - Blair, C. D.

AU - Blair, R. M.

AU - Bode, N.

AU - Booker, P.

AU - Bork, R.

AU - Bramley, A.

AU - Brooks, A. F.

AU - Buikema, A.

AU - Cahillane, C.

AU - Cannon, K. C.

AU - Ciobanu, A. A.

AU - Clara, F.

AU - Cooper, S. J.

AU - Corley, K. R.

AU - Countryman, S. T.

AU - Covas, P. B.

AU - Willke, B.

AU - Liu, J.

AU - Meylahn, Fabian

PY - 2021/1/22

Y1 - 2021/1/22

N2 - Noise due to scattered light has been a frequent disturbance in the advanced LIGO gravitational wave detectors, hindering the detection of gravitational waves. The non stationary scatter noise caused by low frequency motion can be recognized as arches in the time-frequency plane of the gravitational wave channel. In this paper, we characterize the scattering noise for LIGO and Virgo's third observing run O3 from April, 2019 to March, 2020. We find at least two different populations of scattering noise and we investigate the multiple origins of one of them as well as its mitigation. We find that relative motion between two specific surfaces is strongly correlated with the presence of scattered light and we implement a technique to reduce this motion. We also present an algorithm using a witness channel to identify the times this noise can be present in the detector.

AB - Noise due to scattered light has been a frequent disturbance in the advanced LIGO gravitational wave detectors, hindering the detection of gravitational waves. The non stationary scatter noise caused by low frequency motion can be recognized as arches in the time-frequency plane of the gravitational wave channel. In this paper, we characterize the scattering noise for LIGO and Virgo's third observing run O3 from April, 2019 to March, 2020. We find at least two different populations of scattering noise and we investigate the multiple origins of one of them as well as its mitigation. We find that relative motion between two specific surfaces is strongly correlated with the presence of scattered light and we implement a technique to reduce this motion. We also present an algorithm using a witness channel to identify the times this noise can be present in the detector.

KW - scattered light

KW - LIGO

KW - ground motion

KW - interferometry

UR - http://www.scopus.com/inward/record.url?scp=85101012170&partnerID=8YFLogxK

U2 - 10.1088/1361-6382/abc906

DO - 10.1088/1361-6382/abc906

M3 - Article

VL - 38

JO - Classical and quantum gravity

JF - Classical and quantum gravity

SN - 0264-9381

IS - 2

M1 - 025016

ER -