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

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • LIGO Scientific, Virgo, and KAGRA Collaborations
  • 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
  • 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

Externe Organisationen

  • 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
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer042001
Seiten (von - bis)1-21
Seitenumfang21
FachzeitschriftPhysical Review D
Jahrgang110
Ausgabenummer4
PublikationsstatusVeröffentlicht - 15 Aug. 2024

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.

ASJC Scopus Sachgebiete

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Ultralight vector dark matter search using data from the KAGRA O3GK run. / LIGO Scientific, Virgo, and KAGRA Collaborations ; Brinkmann, M.; Carlassara, M. et al.
in: Physical Review D, Jahrgang 110, Nr. 4, 042001, 15.08.2024, S. 1-21.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

LIGO Scientific, Virgo, and KAGRA Collaborations, Brinkmann, M, Carlassara, M, Chakraborty, P, Danzmann, K, Heurs, M, Johny, N, Junker, J, Knust, N, Lehmann, J, Lück, H, Matiushechkina, M, Nery, M, Schulte, BW, Vahlbruch, H, Wilken, D, Willke, B, Wu, DS, Affeldt, C, Bergamin, F, Bisht, A, Bode, N, Booker, P, Borchers, A, Brockmüller, E, Carter, J, Ghosh, S, Hochheim, S, Kastaun, W, Khan, F, Koch, P, Kringel, V, Kuehn, G, Lough, J, Maciy, RR, Meylahn, F, Nadji, S, Ohme, F, Pascale, G, Schneewind, M, Schutz, BF, Venneberg, J, von Wrangel, J, Weinert, M, Wellmann, F & Weßels, P 2024, 'Ultralight vector dark matter search using data from the KAGRA O3GK run', Physical Review D, Jg. 110, Nr. 4, 042001, S. 1-21. https://doi.org/10.1103/PhysRevD.110.042001
LIGO Scientific, Virgo, and KAGRA Collaborations, Brinkmann, M., Carlassara, M., Chakraborty, P., Danzmann, K., Heurs, M., Johny, N., Junker, J., Knust, N., Lehmann, J., Lück, H., Matiushechkina, M., Nery, M., Schulte, B. W., Vahlbruch, H., Wilken, D., Willke, B., Wu, D. S., Affeldt, C., ... Weßels, P. (2024). Ultralight vector dark matter search using data from the KAGRA O3GK run. Physical Review D, 110(4), 1-21. Artikel 042001. https://doi.org/10.1103/PhysRevD.110.042001
LIGO Scientific, Virgo, and KAGRA Collaborations, Brinkmann M, Carlassara M, Chakraborty P, Danzmann K, Heurs M et al. Ultralight vector dark matter search using data from the KAGRA O3GK run. Physical Review D. 2024 Aug 15;110(4):1-21. 042001. doi: 10.1103/PhysRevD.110.042001
LIGO Scientific, Virgo, and KAGRA Collaborations ; Brinkmann, M. ; Carlassara, M. et al. / Ultralight vector dark matter search using data from the KAGRA O3GK run. in: Physical Review D. 2024 ; Jahrgang 110, Nr. 4. S. 1-21.
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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.",
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language = "English",
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Download

TY - JOUR

T1 - Ultralight vector dark matter search using data from the KAGRA O3GK run

AU - LIGO Scientific, Virgo, and KAGRA Collaborations

AU - Zhang, L.

AU - Hansen, H.

AU - Rose, C. A.

AU - Adya, V. B.

AU - Sun, L.

AU - Zhang, J.

AU - Zhang, Y.

AU - Brinkmann, M.

AU - Carlassara, M.

AU - Chakraborty, P.

AU - Danzmann, K.

AU - Heurs, M.

AU - Johny, N.

AU - Junker, J.

AU - Knust, N.

AU - Lehmann, J.

AU - Lück, H.

AU - Matiushechkina, M.

AU - Nery, M.

AU - Schulte, B. W.

AU - Vahlbruch, H.

AU - Wilken, D.

AU - Willke, B.

AU - Wu, D. S.

AU - Bose, S.

AU - Mishra, A. K.

AU - More, A.

AU - Klinger, T.

AU - Jones, R.

AU - Chatterjee, C.

AU - Chen, X.

AU - Lang, R. N.

AU - Danilishin, S.

AU - Hennig, J. S.

AU - Cheng, H. P.

AU - Gupta, S. K.

AU - Zhang, R.

AU - Pham, H.

AU - Roy, S.

AU - Schmidt, S.

AU - Nguyen, P.

AU - Wang, J. Z.

AU - Dasgupta, A.

AU - Brown, D. D.

AU - Zheng, Y.

AU - Bhowmick, S.

AU - Li, T. G.F.

AU - Schmidt, P.

AU - Wu, H.

AU - Lee, Y.

AU - Yang, Y.

AU - Li, X.

AU - Yamamoto, K.

AU - Xu, Y.

AU - Roy, S.

AU - Guo, H.

AU - Singh, A.

AU - Kim, S.

AU - Lee, H. M.

AU - Kim, M. H.

AU - Lee, H. M.

AU - Sanders, J. R.

AU - Affeldt, Christoph

AU - Bergamin, Fabio

AU - Bisht, Aparna

AU - Bode, Nina

AU - Booker, Phillip

AU - Borchers, Andreas

AU - Brockmüller, Eike

AU - Carter, Jonathan

AU - Ghosh, Shrobana

AU - Hochheim, S.

AU - Kastaun, Wolfgang

AU - Khan, Fawad

AU - Koch, Philip

AU - Kringel, Volker

AU - Kuehn, G.

AU - Lough, James

AU - Maciy, R. R.

AU - Meylahn, Fabian

AU - Nadji, Severin

AU - Ohme, F.

AU - Pascale, G.

AU - Schneewind, M.

AU - Schutz, B. F.

AU - Venneberg, J.

AU - von Wrangel, J.

AU - Weinert, Michael

AU - Wellmann, F.

AU - Weßels, Peter

N1 - Publisher Copyright: © 2024 American Physical Society.

PY - 2024/8/15

Y1 - 2024/8/15

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=85203240430&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.110.042001

DO - 10.1103/PhysRevD.110.042001

M3 - Article

AN - SCOPUS:85203240430

VL - 110

SP - 1

EP - 21

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 4

M1 - 042001

ER -

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