New results from HAYSTAC’s phase II operation with a squeezed state receiver

New results from HAYSTAC’s phase II operation with a squeezed state receiver
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DOI:
10.1103/physrevd.107.072007
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发表时间:
2023-01
期刊:
影响因子:
5
通讯作者:
H. C. M. J. Jewell;A. Leder;K. Backes;Xiran Bai;K. Bibber;B. Brubaker;S. Cahn;A. Droster;Maryam H. Esmat;Sumita Ghosh;Eleanor Graham;G. Hilton;H. Jackson;C. Laffan;S. Lamoreaux;K. Lehnert;S. Lewis;M. Malnou;R. Maruyama;D. Palken;N. Rapidis;E. Ruddy;M. Simanovskaia;Sukhman Singh;D. Speller;L. Vale;H. Wang;Y. Zhu
H. C. M. J. Jewell;A. Leder;K. Backes;Xiran Bai;K. Bibber;B. Brubaker;S. Cahn;A. Droster;Maryam H. Esmat;Sumita Ghosh;Eleanor Graham;G. Hilton;H. Jackson;C. Laffan;S. Lamoreaux;K. Lehnert;S. Lewis;M. Malnou;R. Maruyama;D. Palken;N. Rapidis;E. Ruddy;M. Simanovskaia;Sukhman Singh;D. Speller;L. Vale;H. Wang;Y. Zhu
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
H. C. M. J. Jewell;A. Leder;K. Backes;Xiran Bai;K. Bibber;B. Brubaker;S. Cahn;A. Droster;Maryam H. Esmat;Sumita Ghosh;Eleanor Graham;G. Hilton;H. Jackson;C. Laffan;S. Lamoreaux;K. Lehnert;S. Lewis;M. Malnou;R. Maruyama;D. Palken;N. Rapidis;E. Ruddy;M. Simanovskaia;Sukhman Singh;D. Speller;L. Vale;H. Wang;Y. Zhu

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利用Haystac实验的压缩态接收器,对质量为10 ev/c的暗物质轴子进行了搜索,获得了亚量子限幅噪声。这份报告详细介绍了以前用来搜索质量范围为16.96-17.12美元和17.14-17.28美元的轴子的实验的设计和操作细节。这些升级包括对数据采集程序的改进,将有效停滞时间减少了5倍,使扫描新区域的速度提高了1.6倍,并具有相当的灵敏度。在$18.44-18.71 eV/c^{2}$($4.459-4.523$GHz)范围内没有发现显著的轴子信号证据,导致轴子-光子耦合的总上限排除在$90\$水平。
A search for dark matter axions with masses $>10 \mu eV/c^{2}$ has been performed using the HAYSTAC experiment's squeezed state receiver to achieve sub-quantum limited noise. This report includes details of the design and operation of the experiment previously used to search for axions in the mass ranges $16.96-17.12$ and $17.14-17.28 \mu eV/c^{2}$($4.100-4.140$GHz) and $4.145-4.178$GHz) as well as upgrades to facilitate an extended search at higher masses. These upgrades include improvements to the data acquisition routine which have reduced the effective dead time by a factor of 5, allowing for the new region to be scanned $\sim$1.6 times faster with comparable sensitivity. No statistically significant evidence of an axion signal is found in the range $18.44-18.71\mu eV/c^{2}$($4.459-4.523$GHz), leading to an aggregate upper limit exclusion at the $90\%$ level on the axion-photon coupling of $2.06\times g_{\gamma}^{KSVZ}$.