Dark photon constraints from a 7.139 GHz cavity haloscope experiment

Fuente: arXiv
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Main Authors: He, Dong, Fan, Jie, Gao, Xin, Gao, Yu, Houston, Nick, Ji, Zhongqing, Jin, Yirong, Li, Chuang, Li, Jinmian, Li, Tianjun, Liu, Shi-hang, Niu, Jia-Shu, Peng, Zhihui, Sun, Liang, Sun, Zheng, Wang, Jia, Wei, Puxian, Wu, Lina, Xiang, Zhongchen, Yang, Qiaoli, Zhang, Chi, Zhang, Wenxing, Zhang, Xin, Zheng, Dongning, Zheng, Ruifeng, Zhou, Jian-yong
Format: Preprint
Published: 2024
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author He, Dong
Fan, Jie
Gao, Xin
Gao, Yu
Houston, Nick
Ji, Zhongqing
Jin, Yirong
Li, Chuang
Li, Jinmian
Li, Tianjun
Liu, Shi-hang
Niu, Jia-Shu
Peng, Zhihui
Sun, Liang
Sun, Zheng
Wang, Jia
Wei, Puxian
Wu, Lina
Xiang, Zhongchen
Yang, Qiaoli
Zhang, Chi
Zhang, Wenxing
Zhang, Xin
Zheng, Dongning
Zheng, Ruifeng
Zhou, Jian-yong
author_facet He, Dong
Fan, Jie
Gao, Xin
Gao, Yu
Houston, Nick
Ji, Zhongqing
Jin, Yirong
Li, Chuang
Li, Jinmian
Li, Tianjun
Liu, Shi-hang
Niu, Jia-Shu
Peng, Zhihui
Sun, Liang
Sun, Zheng
Wang, Jia
Wei, Puxian
Wu, Lina
Xiang, Zhongchen
Yang, Qiaoli
Zhang, Chi
Zhang, Wenxing
Zhang, Xin
Zheng, Dongning
Zheng, Ruifeng
Zhou, Jian-yong
contents The dark photon is a promising candidate for the dark matter which comprises most of the matter in our visible Universe. Via kinetic mixing with the Standard Model it can also be resonantly converted to photons in an electromagnetic cavity, offering novel experimental possibilities for the discovery and study of dark matter. We report the results of a pathfinder dark photon dark matter cavity search experiment performed at Hunan Normal University and the Institute of Physics, Chinese Academy of Sciences, representing the first stage of the APEX (Axion and dark Photon EXperiment) program. Finding no statistically significant excess, we place an upper limit on the kinetic mixing parameter $|χ|<3.7\times 10^{-13}$ around $m_A\simeq 29.5$ $μ$eV at 90% confidence level. This result exceeds other constraints on dark photon dark matter in this frequency range by roughly an order of magnitude.
format Preprint
id arxiv_https___arxiv_org_abs_2404_00908
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Dark photon constraints from a 7.139 GHz cavity haloscope experiment
He, Dong
Fan, Jie
Gao, Xin
Gao, Yu
Houston, Nick
Ji, Zhongqing
Jin, Yirong
Li, Chuang
Li, Jinmian
Li, Tianjun
Liu, Shi-hang
Niu, Jia-Shu
Peng, Zhihui
Sun, Liang
Sun, Zheng
Wang, Jia
Wei, Puxian
Wu, Lina
Xiang, Zhongchen
Yang, Qiaoli
Zhang, Chi
Zhang, Wenxing
Zhang, Xin
Zheng, Dongning
Zheng, Ruifeng
Zhou, Jian-yong
High Energy Physics - Experiment
High Energy Physics - Phenomenology
The dark photon is a promising candidate for the dark matter which comprises most of the matter in our visible Universe. Via kinetic mixing with the Standard Model it can also be resonantly converted to photons in an electromagnetic cavity, offering novel experimental possibilities for the discovery and study of dark matter. We report the results of a pathfinder dark photon dark matter cavity search experiment performed at Hunan Normal University and the Institute of Physics, Chinese Academy of Sciences, representing the first stage of the APEX (Axion and dark Photon EXperiment) program. Finding no statistically significant excess, we place an upper limit on the kinetic mixing parameter $|χ|<3.7\times 10^{-13}$ around $m_A\simeq 29.5$ $μ$eV at 90% confidence level. This result exceeds other constraints on dark photon dark matter in this frequency range by roughly an order of magnitude.
title Dark photon constraints from a 7.139 GHz cavity haloscope experiment
topic High Energy Physics - Experiment
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2404.00908