Pilot bunch and co-magnetometry of polarized particles stored in a ring
J. Slim, F. Rathmann, A. Andres, V. Hejny, A. Nass, A. Kacharava, P., Lenisa, N.N. Nikolaev, J. Pretz, A. Saleev, V. Shmakova, H. Soltner, F., Abusaif, A. Aggarwal, A. Aksentev, B. Alberdi, L. Barion, I. Bekman, M., Bey\ss, C. B\"ohme, B. Breitkreutz, N. Canale, G. Ciullo

TL;DR
This paper introduces a method using a pilot bunch as a co-magnetometer in storage rings to monitor and compensate for magnetic field fluctuations, enhancing precision in spin-resonance experiments.
Contribution
The paper presents a novel shielding technique that allows a pilot bunch to serve as a real-time co-magnetometer, improving control of spin precession in storage ring experiments.
Findings
Successfully demonstrated shielding of a pilot bunch from high-frequency fields.
The pilot bunch effectively tracked magnetic fluctuations on a one-second timescale.
Potential applications in electric dipole moment searches and future spin physics facilities.
Abstract
In polarization experiments at storage rings, one of the challenges is to maintain the spin-resonance condition of a radio-frequency spin rotator with the spin-precessions of the orbiting particles. Time-dependent variations of the magnetic fields of ring elements lead to unwanted variations of the spin precession frequency. We report here on a solution to this problem by shielding (or masking) one of the bunches stored in the ring from the high-frequency fields of the spin rotator, so that the masked pilot bunch acts as a co-magnetometer for the other signal bunch, tracking fluctuations in the ring on a time scale of about one second. While the new method was developed primarily for searches of electric dipole moments of charged particles, it may have far-reaching implications for future spin physics facilities, such as the EIC and NICA.
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Taxonomy
TopicsAtomic and Subatomic Physics Research · Dark Matter and Cosmic Phenomena · Particle Accelerators and Free-Electron Lasers
