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磁单极子噪声。

Magnetic monopole noise.

机构信息

Department of Physics, Cornell University, Ithaca, NY, USA.

Clarendon Laboratory, University of Oxford, Oxford, UK.

出版信息

Nature. 2019 Jul;571(7764):234-239. doi: 10.1038/s41586-019-1358-1. Epub 2019 Jul 3.

DOI:10.1038/s41586-019-1358-1
PMID:31270461
Abstract

Magnetic monopoles are hypothetical elementary particles with quantized magnetic charge. In principle, a magnetic monopole can be detected by the quantized jump in magnetic flux that it generates upon passage through a superconducting quantum interference device (SQUID). Following the theoretical prediction that emergent magnetic monopoles should exist in several lanthanide pyrochlore magnetic insulators, including DyTiO, the SQUID technique has been proposed for their direct detection. However, this approach has been hindered by the high number density and the generation-recombination fluctuations expected of such thermally generated monopoles. Recently, theoretical advances have enabled the prediction of the spectral density of magnetic-flux noise from monopole generation-recombination fluctuations in these materials. Here we report the development of a SQUID-based flux noise spectrometer and measurements of the frequency and temperature dependence of magnetic-flux noise generated by DyTiO crystals. We detect almost all of the features of magnetic-flux noise predicted for magnetic monopole plasmas, including the existence of intense magnetization noise and its characteristic frequency and temperature dependence. Moreover, comparisons of simulated and measured correlation functions of the magnetic-flux noise indicate that the motions of magnetic charges are strongly correlated. Intriguingly, because the generation-recombination time constant for DyTiO is in the millisecond range, magnetic monopole flux noise amplified by SQUID is audible to humans.

摘要

磁单极子是假设的具有量子磁荷的基本粒子。原则上,磁单极子可以通过其在穿过超导量子干涉装置 (SQUID) 时产生的磁通量量子化跳跃来检测。在理论预测指出,包括 DyTiO 在内的几种镧系 pyrochlore 磁性绝缘体中应该存在涌现磁单极子之后,人们提出了使用 SQUID 技术对其进行直接检测。然而,这种方法受到了预期的热产生单极子的高密度和产生-复合波动的阻碍。最近,理论上的进展使得能够预测这些材料中单极子产生-复合波动的磁通噪声的谱密度。在这里,我们报告了一种基于 SQUID 的磁通噪声光谱仪的开发以及对 DyTiO 晶体产生的磁通噪声的频率和温度依赖性的测量。我们检测到几乎所有预测的磁单极子等离子体磁通噪声的特征,包括强烈的磁化噪声及其特征频率和温度依赖性的存在。此外,磁通噪声的模拟和测量相关函数的比较表明,磁荷的运动是强相关的。有趣的是,由于 DyTiO 的产生-复合时间常数在毫秒范围内,因此 SQUID 放大的磁单极子磁通噪声对人类来说是可听的。

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