Abstract

Relativistic millicharged particles ($\chi_q$) have been proposed in various extensions to the Standard Model of particle physics. We consider the scenarios where they are produced at nuclear reactor core and via interactions of cosmic-rays with the earth's atmosphere. Millicharged particles could also be candidates for dark matter, and become relativistic through acceleration by supernova explosion shock waves. The atomic ionization cross section of $\chi_q$ with matter are derived with the equivalent photon approximation. Smoking-gun signatures with significant enhancement in the differential cross section are identified. New limits on the mass and charge of $\chi_q$ are derived, using data taken with a point-contact germanium detector with 500g mass functioning at an energy threshold of 300~eV at the Kuo-Sheng Reactor Neutrino Laboratory.

Highlights

  • The origin of electric charge quantization is one of the profound intriguing mysteries of the nature [1]

  • The atomic ionization cross section of χq with matter are derived with the equivalent photon approximation

  • New limits on the mass and charge of χq are derived, using data taken with a point-contact germanium detector with 500 g mass functioning at an energy threshold of 300 eV at the Kuo-Sheng Reactor Neutrino Laboratory

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Summary

INTRODUCTION

The origin of electric charge quantization is one of the profound intriguing mysteries of the nature [1]. Despite consistency of charge quantization with all experimental data, the absence of evidence for magnetic monopoles and grand unification continues to motivate searches for the existence of nonquantized charged particles commonly known as millicharged particles and denoted by χq with mass mχq in this article [5].

Nuclear reactor χ q
Atmospheric χ q
Dark cosmic rays—DM-χ q
ATOMIC IONIZATION WITH MILLICHARGED PARTICLES
EXPERIMENTAL CONSTRAINTS
Reactor-χ q
Atmospheric-χ q
Dark cosmic ray DM-χ q
Findings
CONCLUSION AND PROSPECTS

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