Magnetic monopole noise

被引:47
|
作者
Dusad, Ritika [1 ]
Kirschner, Franziska K. K. [2 ]
Hoke, Jesse C. [1 ,3 ]
Roberts, Benjamin R. [1 ]
Eyal, Anna [1 ,4 ]
Flicker, Felix [5 ]
Luke, Graeme M. [6 ,7 ,8 ]
Blundell, Stephen J. [2 ]
Davis, J. C. Seamus [1 ,2 ,9 ]
机构
[1] Cornell Univ, Dept Phys, Ithaca, NY 14853 USA
[2] Univ Oxford, Clarendon Lab, Oxford, England
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[4] Technion Israel Inst Technol, Dept Phys, Haifa, Israel
[5] Rudolf Peierls Ctr Theoret Phys, Clarendon Lab, Oxford, England
[6] McMaster Univ, Brockhouse Inst Mat Res, Hamilton, ON, Canada
[7] McMaster Univ, Dept Phys, Hamilton, ON, Canada
[8] Canadian Inst Adv Res, Toronto, ON, Canada
[9] Univ Coll Cork, Dept Phys, Cork, Ireland
基金
英国工程与自然科学研究理事会; 爱尔兰科学基金会; 欧洲研究理事会;
关键词
SPIN ICE; EQUILIBRIUM NOISE; SPECTRUM; CHARGE; STATE;
D O I
10.1038/s41586-019-1358-1
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Magnetic monopoles(1-3) 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)(4). Following the theoretical prediction that emergent magnetic monopoles should exist in several lanthanide pyrochlore magnetic insulators(5,6), including Dy2Ti2O7, the SQUID technique has been proposed for their direct detection(6). 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(7,8). 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 Dy2Ti2O7 crystals. We detect almost all of the features of magnetic-flux noise predicted for magnetic monopole plasmas(7,8), 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 Dy2Ti2O7 is in the millisecond range, magnetic monopole flux noise amplified by SQUID is audible to humans.
引用
收藏
页码:234 / +
页数:14
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