First search for dark photon dark matter with a MADMAX prototype

J. Egge, D. Leppla-Weber, S. Knirck, B. Ary dos Santos Garcia, D. Bergermann, A. Caldwell, V. Dabhi, C. Diaconu, J. Diehl, G. Dvali, M. Ekmedžić, F. Gallo, E. Garutti, S. Heyminck, F. Hubaut, A. Ivanov, J. Jochum, P. Karst, M. Kramer, D. Kreikemeyer-Lorenzo, C. Krieger, C. Lee, A. Lindner, J. P. A. Maldonado, B. Majorovits, S. Martens, A. Martini, A. Miyazaki, E. Öz, P. Pralavorio, G. Raffelt, A. Ringwald, J. Redondo, S. Roset, N. Salama, J. Schaffran, A. Schmidt, F. Steffen, C. Strandhagen, I. Usherov, H. Wang, G. Wieching, G. Cancelo, M. Di Federico, G. Hoshino, L. Stefanazzi
{"title":"First search for dark photon dark matter with a MADMAX prototype","authors":"J. Egge, D. Leppla-Weber, S. Knirck, B. Ary dos Santos Garcia, D. Bergermann, A. Caldwell, V. Dabhi, C. Diaconu, J. Diehl, G. Dvali, M. Ekmedžić, F. Gallo, E. Garutti, S. Heyminck, F. Hubaut, A. Ivanov, J. Jochum, P. Karst, M. Kramer, D. Kreikemeyer-Lorenzo, C. Krieger, C. Lee, A. Lindner, J. P. A. Maldonado, B. Majorovits, S. Martens, A. Martini, A. Miyazaki, E. Öz, P. Pralavorio, G. Raffelt, A. Ringwald, J. Redondo, S. Roset, N. Salama, J. Schaffran, A. Schmidt, F. Steffen, C. Strandhagen, I. Usherov, H. Wang, G. Wieching, G. Cancelo, M. Di Federico, G. Hoshino, L. Stefanazzi","doi":"arxiv-2408.02368","DOIUrl":null,"url":null,"abstract":"We report the first result from a dark photon dark matter search in the mass\nrange from ${78.62}$ to $83.95~\\mathrm{\\mu eV}/c^2$ with a dielectric haloscope\nprototype for MADMAX (Magnetized Disc and Mirror Axion eXperiment). Putative\ndark photons would convert to observable photons within a stack consisting of\nthree sapphire disks and a mirror. The emitted power of this system is received\nby an antenna and successively digitized using a low-noise receiver. No dark\nphoton signal has been observed. Assuming unpolarized dark photon dark matter\nwith a local density of $\\rho_{\\chi}=0.3~\\mathrm{GeV/cm^3}$ we exclude a dark\nphoton to photon mixing parameter $\\chi > 3.0 \\times 10^{-12}$ over the full\nmass range and $\\chi > 1.2 \\times 10^{-13}$ at a mass of $80.57~\\mathrm{\\mu\neV}/c^2$ with a 95\\% confidence level. This is the first physics result from a\nMADMAX prototype and exceeds previous constraints on $\\chi$ in this mass range\nby up to almost three orders of magnitude.","PeriodicalId":501374,"journal":{"name":"arXiv - PHYS - Instrumentation and Detectors","volume":"26 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Detectors","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.02368","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

We report the first result from a dark photon dark matter search in the mass range from ${78.62}$ to $83.95~\mathrm{\mu eV}/c^2$ with a dielectric haloscope prototype for MADMAX (Magnetized Disc and Mirror Axion eXperiment). Putative dark photons would convert to observable photons within a stack consisting of three sapphire disks and a mirror. The emitted power of this system is received by an antenna and successively digitized using a low-noise receiver. No dark photon signal has been observed. Assuming unpolarized dark photon dark matter with a local density of $\rho_{\chi}=0.3~\mathrm{GeV/cm^3}$ we exclude a dark photon to photon mixing parameter $\chi > 3.0 \times 10^{-12}$ over the full mass range and $\chi > 1.2 \times 10^{-13}$ at a mass of $80.57~\mathrm{\mu eV}/c^2$ with a 95\% confidence level. This is the first physics result from a MADMAX prototype and exceeds previous constraints on $\chi$ in this mass range by up to almost three orders of magnitude.
利用 MADMAX 原型机首次搜索暗光子暗物质
我们报告了在{78.62}$到83.95~\mathrm\{mu eV}/c^2$ 的质量范围内,利用MADMAX(Magnetized Disc and Mirror Axion eXperiment)的介质半透明原型进行暗光子暗物质搜索的第一个结果。暗光子将在由三个蓝宝石盘和一面镜子组成的堆栈中转换成可观测的光子。该系统的发射功率由天线接收,并通过低噪声接收器连续数字化。没有观测到暗光子信号。假设非极化暗光子暗物质的局部密度为$\rrho_{\chi}=0.3~\mathrm{GeV/cm^3}$,我们排除了在全质量范围内暗光子与光子的混合参数为$\chi > 3.0 \times 10^{-12}$,以及在质量为$80.57~\mathrm\{mueV}/c^2$时为$\chi > 1.2 \times 10^{-13}$,置信度为95%。这是来自MADMAX原型的第一个物理学结果,并且在这个质量范围内超过了以前对$\chi$的约束,几乎达到了三个数量级。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信