论文标题

搜索质量m $ _a = 43〜μ $ ev的质量的无形斧头暗物质与Quax-$aγ$实验

Search for invisible axion dark matter of mass m$_a=43~μ$eV with the QUAX--$aγ$ experiment

论文作者

Alesini, D., Braggio, C., Carugno, G., Crescini, N., D'Agostino, D., Di Gioacchino, D., Di Vora, R., Falferi, P., Gambardella, U., Gatti, C., Iannone, G., Ligi, C., Lombardi, A., Maccarrone, G., Ortolan, A., Pengo, R., Rettaroli, A., Ruoso, G., Taffarello, L., Tocci, S.

论文摘要

Quax-$aγ$实验的吊带板由8.1 T磁铁内的无氧高导热率CU组成,并冷却至$ \ sim200 $ MK,用于搜索带有质量$ $ M_A \ simeq43〜μ \ simeq43〜μ \ text {ev {ev {ev} $的银河系轴的搜索。共振腔发出的功率用约瑟夫森参数放大器扩增,其噪声波动在标准量子极限处。 With the data collected in about 1 h at the cavity frequency $ν_c=10.40176$ GHz, the experiment reaches the sensitivity necessary for the detection of galactic QCD-axion, setting the $90\%$ confidence level limit to the axion-photon coupling $g_{aγγ}<0.639\times10^{-13}$ GeV$^{-1}$.

A haloscope of the QUAX--$aγ$ experiment composed of an oxygen-free high thermal conductivity-Cu cavity inside an 8.1 T magnet and cooled to $\sim200$ mK is put in operation for the search of galactic axion with mass $m_a\simeq43~μ\text{eV}$. The power emitted by the resonant cavity is amplified with a Josephson parametric amplifier whose noise fluctuations are at the standard quantum limit. With the data collected in about 1 h at the cavity frequency $ν_c=10.40176$ GHz, the experiment reaches the sensitivity necessary for the detection of galactic QCD-axion, setting the $90\%$ confidence level limit to the axion-photon coupling $g_{aγγ}<0.639\times10^{-13}$ GeV$^{-1}$.

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