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arXiv 2409.04552hep-phastro-ph.HEhep-ex
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磁单极子搜寻的下一个前沿

The next frontiers for magnetic monopole searches

O. Gould, I. Ostrovskiy, A. Upreti

AI总结:

本文研究通过施温格过程在重离子碰撞、宇宙射线和宇宙磁场衰变中产生低质量磁单极子的可能性,提出利用下一代对撞机、工业采矿和南极冰钻基础设施及专用探测器进行搜寻,并给出可达10^{-22} cm^{-2} s^{-1} sr^{-1}量级的通量灵敏度。

摘要:

磁单极子(MMs)是具有充分理论动机的假想粒子,其发现将使麦克斯韦方程组对称化,解释电荷量子化,并探测统一理论的规范结构。近期模型预言了低质量磁单极子,重新激发了在对撞机上的搜寻。然而,大多数理论预言的是复合磁单极子,其在部分子-部分子碰撞中的产生预计会受到抑制。施温格过程——即磁单极子对在强磁场存在下隧穿真空势垒——不受这一限制。此外,施温格截面可以非微扰地计算。这些特点共同使其成为低质量磁单极子搜寻的黄金通道。我们研究了未来对撞机重离子碰撞中磁单极子的施温格产生、宇宙射线与大气碰撞中的产生,以及宇宙起源磁场衰变中的产生。我们发现下一代对撞机将提供最佳灵敏度,能够发现或排除具有TeV尺度质量的磁单极子。同时,利用工业矿石开采和南极冰钻的基础设施,可以以更快的时间尺度和仅适度的投入推进该领域。特别是,我们通过详细计算表明,所提出的实验将在宽广的洛伦兹因子范围内对低至几个单位的10^{-22} cm^{-2} s^{-1} sr^{-1}的低质量磁单极子通量具有灵敏度。我们还提议在宇宙射线观测站部署专用磁单极子探测器,以直接研究无法解释的最高能量宇宙射线是否为磁单极子。这些提议的努力将共同定义未来几十年磁单极子搜寻领域的方向。

英文摘要:

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.

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