| Autor: |
J. Feicht, A. Fernandez-Galiana, B. B. Lane, Benno Willke, J. Hanson, P. J. Veitch, H. Yamamoto, C. L. Romel, J. H. Romie, R. L. McCarthy, Aaron Buikema, T. R. Saravanan, R. Penhorwood, N. Kijbunchoo, Beverly K. Berger, G. Mendell, S. M. Aston, A. M. Baer, Madeline Wade, D. Sigg, L. Sun, P. H. Nguyen, S. Gras, M. P. Ross, K. R. Corley, J. Zweizig, S. E. Dwyer, Haocun Yu, F. Clara, Hang Yu, C. D. Blair, P. Booker, C. Austin, T. Vo, C. M. Mow-Lowry, B. J. J. Slagmolen, G. Venugopalan, A. Effler, R. M. S. Schofield, B. Lantz, D. C. Vander-Hyde, Lu Zhang, Rana X. Adhikari, Matthew Evans, E. Payne, K. D. Giardina, T. J. N. Nelson, J. G. Rollins, Y. K. Lecoeuche, K. L. Dooley, Richard J. Abbott, G. Vajente, Lisa Barsotti, J. S. Areeda, Michael E Zucker, D. Barker, R. Schnabel, A. L. Urban, M. Laxen, L. Xiao, D. C. Coyne, L. Nuttall, D. Sellers, G. González, D. Bhattacharjee, Kipp Cannon, John R. Smith, Evan Goetz, S. McCormick, Andrew Lundgren, Michael Landry, D. V. Martynov, J. McIver, Simone Mozzon, K. Riles, James G. Bartlett, David E. McClelland, P. J. King, L. McCuller, E. L. Merilh, P. Godwin, T. Shaffer, T. Hardwick, Jonathan Richardson, J. D. Jones, S. W. Ballmer, N. A. Robertson, Richard J. Oram, E. J. Sanchez, R. Mittleman, K. E. Ramirez, A. C. Green, C. Gray, Eyal Schwartz, Rainer Weiss, P. B. Covas, A. Mullavey, J. Oberling, J. N. Leviton, Fabrice Matichard, M. Kasprzack, L. E. H. Datrier, G. Valdes, K. Merfeld, R. M. Blair, C. C. Wipf, Carrie Reinhardt Adams, A. Ananyeva, B. Weaver, S. Karki, J. Betzwieser, Z. Márka, K. Mason, C. J. Perez, S. Banagiri, Xin Chen, T. Etzel, Peter Fritschel, Aaron Viets, D. Schaetzl, G. Moreno, L. E. Sanchez, J. C. Driggers, J. R. Palamos, M. Pirello, R. Gray, R. Macas, J. Hanks, S. Márka, H. Overmier, Kenneth A. Strain, S. J. Cooper, S. Kandhasamy, C. Cahillane, Nergis Mavalvala, V. V. Frolov, J. S. Kissel, H. Radkins, Paul Fulda, N. Bode, K. A. Thorne, A. Bramley, J. A. Giaime, R. Gustafson, J. Liu, K. Kawabe, A. P. Spencer, D. D. Brown, M. Fyffe, K. Venkateswara, R. L. Ward, M. Lormand, T. J. Massinger, Kevin M. Ryan, P. Thomas, C. Vorvick, S. T. Countryman, F. Meylahn, Matthew Heintze, Richard L. Savage, A. F. Helmling-Cornell, S. Soni, A. Pele, A. A. Ciobanu, G. L. Mansell, C. Whittle, Calum Torrie, Maggie Tse, Michael Thomas, R. Bork, M. MacInnis, K. Toland, T. Mistry, Y. Asali, S. Appert, J. Warner, C. Di Fronzo, G. Billingsley, Koji Arai, Derek Davis, P. Dupej, Terry G. McRae, G. Traylor, B. Sorazu, T. Sadecki, David J. Ottaway, N. A. Holland, Rajesh Kumar, D. M. Macleod, C. Osthelder, M. Ball, A. Brooks, S. Biscans, Marek Szczepanczyk, William Parker, Eric K. Gustafson, Timothy Evans, R. K. Hasskew |
| Přispěvatelé: |
California Institute of Technology, National Science Foundation (US) |
| Rok vydání: |
2021 |
| Předmět: |
|
| Zdroj: |
Classical and Quantum Gravity
Digital.CSIC. Repositorio Institucional del CSIC
instname |
| Popis: |
Soni, S., et al. (LIGO Scientific Collaboration)
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.
LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under Cooperative Agreement No. PHY-1764464. Advanced LIGO was built under Grant No. PHY-0823459. We acknowledge support from the NSF grant PHY-1806656, PHY-1505779, and PHY-1912604. We also acknowledge the discussions with the members of Detector Characterization Group of the LIGO Scientific Collaboration. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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