Abstract

The nEDM apparatus at PSI has been used to search for different dark matter signatures utilizing its high sensitivity to shifts in the neutron precession frequency and its well-controlled low magnetic field at the \muμT level. Such a shift could be interpreted as a consequence of a short-range spin-dependent interaction that could possibly be mediated by axions or axion-like particles, or as an axion-induced oscillating electric dipole moment of the neutron. Another search, based on so-called UCN disappearance measurements, targeted previously reported signals of neutron to mirror-neutron oscillations. These dark matter searches confirmed and improved previous results, as detailed in this review.

Highlights

  • Apart from searching for the electric dipole moment of the neutron, the neutron electric dipole moment (nEDM) apparatus at PSI (Section 27 [1]) is an excellent tool to search for signatures of dark matter particles

  • ultracold neutrons (UCN) disappearance experiments were conducted with this apparatus [4] to search for dark matter signatures

  • It has been proposed starting from the fifties that there could be a mirror copy of the Standard Model (SM) particles, restoring parity conservation in the weak interaction on the global level

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Summary

28.1 Introduction

Apart from searching for the electric dipole moment of the neutron, the nEDM apparatus at PSI (Section 27 [1]) is an excellent tool to search for signatures of dark matter particles. The first potential signature studied was a high precision measurement of the shift in the ratio of the spin-precession frequencies of ultracold neutrons (UCN) and 199Hg atoms. UCN disappearance experiments were conducted with this apparatus [4] to search for dark matter signatures It has been proposed starting from the fifties that there could be a mirror copy of the Standard Model (SM) particles, restoring parity conservation in the weak interaction on the global level. A comparison to previous constraints on model parameters will be given

28.2 Search for axion-like particles
28.3 Search for mirror neutrons
28.4 Outlook
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