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":"利用 MADMAX 原型机首次搜索暗光子暗物质","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":"{\"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}","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}
First search for dark photon dark matter with a MADMAX prototype
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.