C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure, G. Carosi, A. S. Chou, C. Cisneros, John Clarke, E. J. Daw, N. Du, L. D. Duffy, T. A. Dyson, C. Gaikwad, J. R. Gleason, C. Goodman, M. Goryachev, M. Guzzetti, C. Hanretty, E. Hartman, A. T. Hipp, J. Hoffman, M. Hollister, R. Khatiwada, S. Knirck, C. L. Kuo, E. Lentz, B. T. McAllister, C. Mostyn, K. Murch, N. S. Oblath, M. G. Perry, A. Quiskamp, N. Robertson, L. J Rosenberg, S. Ruppert, G. Rybka, I. Siddiqi, P. Sikivie, J. Sinnis, M. E. Solano, A. Sonnenschein, N. S. Sullivan, D. B. Tanner, M. S. Taubman, M. E. Tobar, M. O. Withers, N. Woollett, D. Zhang
{"title":"利用Dine-Fischler-Srednicki-Zhitnitsky发现能力进行3.3微伏左右的轴子暗物质实验","authors":"C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure, G. Carosi, A. S. Chou, C. Cisneros, John Clarke, E. J. Daw, N. Du, L. D. Duffy, T. A. Dyson, C. Gaikwad, J. R. Gleason, C. Goodman, M. Goryachev, M. Guzzetti, C. Hanretty, E. Hartman, A. T. Hipp, J. Hoffman, M. Hollister, R. Khatiwada, S. Knirck, C. L. Kuo, E. Lentz, B. T. McAllister, C. Mostyn, K. Murch, N. S. Oblath, M. G. Perry, A. Quiskamp, N. Robertson, L. J Rosenberg, S. Ruppert, G. Rybka, I. Siddiqi, P. Sikivie, J. Sinnis, M. E. Solano, A. Sonnenschein, N. S. Sullivan, D. B. Tanner, M. S. Taubman, M. E. Tobar, M. O. Withers, N. Woollett, D. Zhang","doi":"arxiv-2408.15227","DOIUrl":null,"url":null,"abstract":"We report the results of a QCD axion dark matter search with discovery\nability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion\nhaloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise\nJosephson parametric amplifier cooled by a dilution refrigerator. This work\nexcludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to\n3.34 {\\mu}eV, assuming a standard halo model with a local energy density of\n0.45 GeV/cc made up 100% of axions.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":"26 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Axion Dark Matter eXperiment around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability\",\"authors\":\"C. Bartram, C. Boutan, T. Braine, J. H. Buckley, T. J. Caligiure, G. Carosi, A. S. Chou, C. Cisneros, John Clarke, E. J. Daw, N. Du, L. D. Duffy, T. A. Dyson, C. Gaikwad, J. R. Gleason, C. Goodman, M. Goryachev, M. Guzzetti, C. Hanretty, E. Hartman, A. T. Hipp, J. Hoffman, M. Hollister, R. Khatiwada, S. Knirck, C. L. Kuo, E. Lentz, B. T. McAllister, C. Mostyn, K. Murch, N. S. Oblath, M. G. Perry, A. Quiskamp, N. Robertson, L. J Rosenberg, S. Ruppert, G. Rybka, I. Siddiqi, P. Sikivie, J. Sinnis, M. E. Solano, A. Sonnenschein, N. S. Sullivan, D. B. Tanner, M. S. Taubman, M. E. Tobar, M. O. Withers, N. Woollett, D. Zhang\",\"doi\":\"arxiv-2408.15227\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We report the results of a QCD axion dark matter search with discovery\\nability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion\\nhaloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise\\nJosephson parametric amplifier cooled by a dilution refrigerator. This work\\nexcludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to\\n3.34 {\\\\mu}eV, assuming a standard halo model with a local energy density of\\n0.45 GeV/cc made up 100% of axions.\",\"PeriodicalId\":501181,\"journal\":{\"name\":\"arXiv - PHYS - High Energy Physics - Experiment\",\"volume\":\"26 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-08-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - High Energy Physics - Experiment\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2408.15227\",\"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 - High Energy Physics - Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.15227","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Axion Dark Matter eXperiment around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability
We report the results of a QCD axion dark matter search with discovery
ability for Dine-Fischler-Srednicki-Zhitnitsky (DFSZ) axions using an axion
haloscope. Sub-Kelvin noise temperatures are reached with an ultra low-noise
Josephson parametric amplifier cooled by a dilution refrigerator. This work
excludes (with a 90% confidence level) DFSZ axions with masses between 3.27 to
3.34 {\mu}eV, assuming a standard halo model with a local energy density of
0.45 GeV/cc made up 100% of axions.
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