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EPJ Plus Highlight - Searching for dark matter with a haloscope

An artist’s impression of the haloscope, ready for testing at a temperature close to absolute zero. Credit: Nicolò Crescini

A new paper in EPJ Plus introduces a novel method of searching for a type of dark matter known as axions; a modified version of this technique may have useful ‘real life’ applications.

Most of the universe is now thought to consist of dark matter: mysterious substances which, because they don’t interact with light or any other kind of electromagnetic radiation, are almost impossible to detect. Physicists have been searching for it for decades, using different techniques; Nicolò Crescini, now of Institut Néel, Grenoble, France, developed a novel method of searching for one type of dark matter, axions, when working at the Laboratori Nazionali di Legnaro, Padova, Italy. This work has now been published in the journal EPJ Plus.

Axions are hypothetical particles that were introduced in the 1970s to plug a gap in the Standard Model of particle physics, namely the strong CP problem. “Studying axions is a good way of catching two birds - dark matter and the strong CP problem - with one stone, the axion,” says Crescini.

The methods used to look for axions differ from the typical particle physics experiments that involve colliding fast-moving particles in accelerators. Instead, these experiments search for weak electromagnetic anomalies that can be detected at extremely low energy and indicate axions coupling to other fundamental particles.

“Most of these experiments look for axions coupling with photons,” adds Crescini. “This approach searches for coupling with electrons, which is more challenging but can yield richer results.” It involves placing a sample of magnetic material in a very well controlled environment close to the absolute zero of temperature and monitoring it for the anomalous variations in magnetisation that might indicate axion activity. The system is a type of magnetometer known as a haloscope after the Dark Matter halo of the Milky Way.

This experiment, named QUAX (short for ‘Quaerere Axions, where ‘quaerere’ is Latin for ‘to search’), is not yet sensitive enough to be able to detect axions. “It needs to be scaled up, and more sensitive sensors need to be employed,” says Crescini. “Nevertheless, this research also has practical applications: we have patented a modified version that could be used as a commercial magnetometer.”

Crescini, N. Building instructions for a ferromagnetic axion haloscope. Eur. Phys. J. Plus 137, 338 (2022). https://doi.org/10.1140/epjp/s13360-022-02533-w

B. Fraboni and G. García López
On behalf of the authors, I gratefully acknowledge the Editors and the Editorial and Production Office for their attention in the revision and editing of the manuscript.

Davide Rotta, Università di Milano Bicocca, Italy

ISSN: 2190-5444 (Electronic Edition)

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