Ultralight vector dark matter search using data from the KAGRA O3GK run

verfasst von: LIGO Scientific, Virgo, and KAGRA Collaborations , L. Zhang, H. Hansen, C. A. Rose, V. B. Adya, L. Sun, J. Zhang, Y. Zhang, M. Brinkmann, M. Carlassara, P. Chakraborty, K. Danzmann, M. Heurs, N. Johny, J. Junker, N. Knust, J. Lehmann, H. Lück, M. Matiushechkina, M. Nery, B. W. Schulte, H. Vahlbruch, D. Wilken, B. Willke, D. S. Wu, S. Bose, A. K. Mishra, A. More, T. Klinger, R. Jones, C. Chatterjee, X. Chen, R. N. Lang, S. Danilishin, J. S. Hennig, H. P. Cheng, S. K. Gupta, R. Zhang, H. Pham, S. Roy, S. Schmidt, P. Nguyen, J. Z. Wang, A. Dasgupta, D. D. Brown, Y. Zheng, S. Bhowmick, T. G.F. Li, P. Schmidt, H. Wu, Y. Lee, Y. Yang, X. Li, K. Yamamoto, Y. Xu, S. Roy, H. Guo, A. Singh, S. Kim, H. M. Lee, M. H. Kim, H. M. Lee, J. R. Sanders, Christoph Affeldt, Fabio Bergamin, Aparna Bisht, Nina Bode, Phillip Booker, Andreas Borchers, Eike Brockmüller, Jonathan Carter, Shrobana Ghosh, S. Hochheim, Wolfgang Kastaun, Fawad Khan, Philip Koch, Volker Kringel, G. Kuehn, James Lough, R. R. Maciy, Fabian Meylahn, Severin Nadji, F. Ohme, G. Pascale, M. Schneewind, B. F. Schutz, J. Venneberg, J. von Wrangel, Michael Weinert, F. Wellmann, Peter Weßels
Abstract: Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for Formula Presented gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the Formula Presented gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation timescale of DM.
Organisationseinheit(en): Institut für Künstliche Intelligenz
QuantumFrontiers
Institut für Gravitationsphysik
Externe Organisation(en): California Institute of Technology (Caltech)
National Science Foundation (NSF)
University of Wisconsin Milwaukee
Australian National University
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Inter-University Centre for Astronomy and Astrophysics India
University of Glasgow
University of Western Australia
Massachusetts Institute of Technology (MIT)
Maastricht University
Nationaal instituut voor subatomaire fysica (Nikhef)
University of Florida
Utrecht University
University of Oregon
University of Michigan
Institute for Plasma Research
University of Adelaide
Missouri University of Science and Technology
Colorado State University
KU Leuven
The Chinese University of Hong Kong
University of Birmingham
National Tsing Hua University
National Central University
Department of Electrophysics
National Yang Ming Chiao Tung University (NSTC)
University of Toyama
Universität Zürich (UZH)
Stony Brook University (SBU)
Center for Computational Astrophysics
Flatiron Institute
University of Utah
University of Mississippi
Department of Astronomy and Space Science
Chungnam National University
Seoul National University
Sungkyunkwan University
Inje University
Marquette University
Cardiff University
Typ: Artikel
Journal: Physical Review D
Band: 110
Seiten: 1-21
Anzahl der Seiten: 21
ISSN: 2470-0010
Publikationsdatum: 15.08.2024
Publikationsstatus: Veröffentlicht
Peer-reviewed: Ja
ASJC Scopus Sachgebiete: Kern- und Hochenergiephysik
Elektronische Version(en): https://doi.org/10.1103/PhysRevD.110.042001 (Zugang: Geschlossen)

BibTeX

@article{811ca63e44494c799ca5fe8a967c7b5a,
title = "Ultralight vector dark matter search using data from the KAGRA O3GK run",
abstract = "Among the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for Formula Presented gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the Formula Presented gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation timescale of DM.",
author = "{LIGO Scientific, Virgo, and KAGRA Collaborations} and L. Zhang and H. Hansen and Rose, {C. A.} and Adya, {V. B.} and L. Sun and J. Zhang and Y. Zhang and M. Brinkmann and M. Carlassara and P. Chakraborty and K. Danzmann and M. Heurs and N. Johny and J. Junker and N. Knust and J. Lehmann and H. L{\"u}ck and M. Matiushechkina and M. Nery and Schulte, {B. W.} and H. Vahlbruch and D. Wilken and B. Willke and Wu, {D. S.} and S. Bose and Mishra, {A. K.} and A. More and T. Klinger and R. Jones and C. Chatterjee and X. Chen and Lang, {R. N.} and S. Danilishin and Hennig, {J. S.} and Cheng, {H. P.} and Gupta, {S. K.} and R. Zhang and H. Pham and S. Roy and S. Schmidt and P. Nguyen and Wang, {J. Z.} and A. Dasgupta and Brown, {D. D.} and Y. Zheng and S. Bhowmick and Li, {T. G.F.} and P. Schmidt and H. Wu and Y. Lee and Y. Yang and X. Li and K. Yamamoto and Y. Xu and S. Roy and H. Guo and A. Singh and S. Kim and Lee, {H. M.} and Kim, {M. H.} and Lee, {H. M.} and Sanders, {J. R.} and Christoph Affeldt and Fabio Bergamin and Aparna Bisht and Nina Bode and Phillip Booker and Andreas Borchers and Eike Brockm{\"u}ller and Jonathan Carter and Shrobana Ghosh and S. Hochheim and Wolfgang Kastaun and Fawad Khan and Philip Koch and Volker Kringel and G. Kuehn and James Lough and Maciy, {R. R.} and Fabian Meylahn and Severin Nadji and F. Ohme and G. Pascale and M. Schneewind and Schutz, {B. F.} and J. Venneberg and {von Wrangel}, J. and Michael Weinert and F. Wellmann and Peter We{\ss}els",
note = "Publisher Copyright: {\textcopyright} 2024 American Physical Society.",
year = "2024",
month = aug,
day = "15",
doi = "10.1103/PhysRevD.110.042001",
language = "English",
volume = "110",
pages = "1--21",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Institute of Physics",
number = "4",
}

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Ultralight vector dark matter search using data from the KAGRA O3GK run

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