The next frontiers for magnetic monopole searches

TL;DR

This paper explores innovative methods for detecting low-mass magnetic monopoles using the Schwinger process in various high-energy environments, proposing next-generation colliders and cosmic ray experiments as promising avenues.

Contribution

It introduces the Schwinger process as a promising channel for low-mass MM searches and evaluates its potential in future colliders and cosmic ray experiments.

Findings

Next-generation colliders could discover or exclude TeV-scale MMs.

Industrial and Antarctic experiments can detect extremely low fluxes of MMs.

Dedicated detectors could investigate the role of MMs in high-energy cosmic rays.

Abstract

Magnetic monopoles (MMs) are well-motivated hypothetical particles whose discovery would symmetrize Maxwell equations, explain quantization of electric charge, and probe the gauge structure of the unified theory. Recent models predict MMs with low masses, reinvigorating searches at colliders. However, most theories predict composite MMs, whose production in parton-parton collisions is expected to be suppressed. The Schwinger process, whereby MM pairs tunnel through the vacuum barrier in the presence of a strong magnetic field, is not subject to this limitation. Additionally, the Schwinger cross section can be calculated nonperturbatively. Together, these make it a golden channel for low-mass MM searches. We investigate the Schwinger production of MMs in heavy-ion collisions at future colliders, in collisions of cosmic rays with the atmosphere, and in decay of magnetic fields of cosmic origin. We find that a next-generation collider would provide the best sensitivity, allowing one to discover or exclude MMs with TeV-scale masses. At the same time, exploiting the infrastructure of industrial ore extraction and Antarctic ice drilling could advance the field at a faster timescale and with only a modest investment. In particular, we show with detailed calculations that the proposed experiments will be sensitive to fluxes of low-mass MMs as low as a few units of 10^{-22} cm^{-2} s^{-1} sr^{-1} in a wide range of Lorentz factors. We also propose deploying dedicated MM detectors in conjunction with cosmic ray observatories to directly investigate if the unexplained, highest energy cosmic rays are MMs. Together, the proposed efforts would define the field of MM searches in the next decades.