A search for neutron to mirror neutron oscillation using neutron electric dipole moment measurements

TL;DR

This paper uses neutron electric dipole moment measurements to set new constraints on neutron to mirror neutron oscillations, providing the most stringent limits in certain magnetic field ranges and advancing the search for mirror matter.

Contribution

It introduces a novel method of constraining neutron to mirror neutron oscillations using EDM measurement data, improving existing bounds in specific magnetic field ranges.

Findings

Established a lower limit on the oscillation time constant of 5.7 seconds.

Provided the best constraints in the magnetic field range of 0.36 to 0.40 microtesla.

Constrained perturbations due to $n-n'$ oscillation using systematic analysis of precession frequency data.

Abstract

Baryon number violation is a key ingredient of baryogenesis. It has been hypothesized that there could also be a parity-conjugated copy of the standard model particles, called mirror particles. The existence of such a mirror universe has specific testable implications, especially in the domain of neutral particle oscillation, viz. the baryon number violating neutron to mirror-neutron ($n-n'$) oscillation. Consequently, there were many experiments that have searched for $n-n'$ oscillation, and imposed constraints upon the parameters that describe it. All the previous efforts searched for $n-n'$ oscillation by comparing the relative number of ultracold neutrons that survive after a period of storage for one or both of the two cases: (i) comparison of zero applied magnetic field to a non-zero applied magnetic field, and (ii) comparison where the orientation of the applied magnetic field was reversed. However, $n-n'$ oscillations also lead to variations in the precession frequency of polarized neutrons upon flipping the direction of the applied magnetic field. For the first time, we used the data from the latest search for the neutron electric dipole moment [Phys. Rev. Lett. 124, 081803 (2020)] to constrain $n-n'$ oscillation. After compensating for the systematic effects that affect the ratio of precession frequencies of ultracold neutrons and cohabiting $^{199}$Hg-atoms, chief among which was due to their motion in non-uniform magnetic field, we constrained any further perturbations due to $n-n'$ oscillation. We thereby provide a lower limit on the $n-n'$ oscillation time constant of $\tau_{nn'}/\sqrt{|\cos(\beta)|} > 5.7~$s, $0.36~\mu$T'$<B'<1.01~\mu$T' (95\% C.L.), where $\beta$ is the angle between the applied magnetic field and the ambient mirror magnetic field. This constraint is the best available in the range of $0.36~\mu$T'$<B'<0.40~\mu$T'.