Magnetic monopole noise.
basic_science · Level V
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- Record sourced from PubMed, PMID 31270461.
- Also identified by DOI 10.1038/s41586-019-1358-1.
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Abstract
Magnetic monopoles<sup>1-3</sup> 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)<sup>4</sup>. Following the theoretical prediction that emergent magnetic monopoles should exist in several lanthanide pyrochlore magnetic insulators<sup>5,6</sup>, including Dy<sub>2</sub>Ti<sub>2</sub>O<sub>7</sub>, the SQUID technique has been proposed for their direct detection<sup>6</sup>. 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<sup>7,8</sup>. 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 Dy<sub>2</sub>Ti<sub>2</sub>O<sub>7</sub> crystals. We detect almost all of the features of magnetic-flux noise predicted for magnetic monopole plasmas<sup>7,8</sup>, 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 Dy<sub>2</sub>Ti<sub>2</sub>O<sub>7</sub> is in the millisecond range, magnetic monopole flux noise amplified by SQUID is audible to humans.