Ultralight vector dark matter search using data from the KAGRA O3GK run
Cosmology and Nongalactic Astrophysics
2024-03-06 v1 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
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 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 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 time scale of DM.
Keywords
Cite
@article{arxiv.2403.03004,
title = {Ultralight vector dark matter search using data from the KAGRA O3GK run},
author = {The LIGO Scientific Collaboration and the Virgo Collaboration and the KAGRA Collaboration and A. G. Abac and R. Abbott and H. Abe and I. Abouelfettouh and F. Acernese and K. Ackley and C. Adamcewicz and S. Adhicary and N. Adhikari and R. X. Adhikari and V. K. Adkins and V. B. Adya and C. Affeldt and D. Agarwal and M. Agathos and O. D. Aguiar and I. Aguilar and L. Aiello and A. Ain and P. Ajith and T. Akutsu and S. Albanesi and R. A. Alfaidi and A. Al-Jodah and C. Alléné and A. Allocca and S. Al-Shammari and P. A. Altin and S. Alvarez-Lopez and A. Amato and L. Amez-Droz and A. Amorosi and C. Amra and S. Anand and A. Ananyeva and S. B. Anderson and W. G. Anderson and M. Andia and M. Ando and T. Andrade and N. Andres and M. Andrés-Carcasona and T. Andrić and J. Anglin and S. Ansoldi and J. M. Antelis and S. Antier and M. Aoumi and E. Z. Appavuravther and S. Appert and S. K. Apple and K. Arai and A. Araya and M. C. Araya and J. S. Areeda and N. Aritomi and F. Armato and N. 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Yang and L. -C. Yang and Y. Yang and Z. Yarbrough and S. -W. Yeh and A. B. Yelikar and S. M. C. Yeung and X. Yin and J. Yokoyama and T. Yokozawa and J. Yoo and H. Yu and H. Yuzurihara and A. Zadrożny and A. J. Zannelli and M. Zanolin and M. Zeeshan and T. Zelenova and J. -P. Zendri and M. Zeoli and M. Zerrad and M. Zevin and A. C. Zhang and J. Zhang and L. Zhang and R. Zhang and T. Zhang and Y. Zhang and C. Zhao and Yue Zhao and Yuhang Zhao and Y. Zheng and H. Zhong and S. Zhong and R. Zhou and Z. -H. Zhu and M. E. Zucker and J. Zweizig and T. Fujimori and H. Fujimoto and T. Fujita and Y. Manita and I. Obata and H. Takidera},
journal= {arXiv preprint arXiv:2403.03004},
year = {2024}
}
Comments
20 pages, 5 figures