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New method for a continuous determination of the spin tune in storage rings and implications for precision experiments
- Source :
- Physical review letters 115(9), 094801 (2015). doi:10.1103/PhysRevLett.115.094801
- Publication Year :
- 2015
-
Abstract
- A new method to determine the spin tune is described and tested. In an ideal planar magnetic ring, the spin tune - defined as the number of spin precessions per turn - is given by $\nu_s = \gamma G$ (gamma is the Lorentz factor, $G$ the magnetic anomaly). For 970 MeV/c deuterons coherently precessing with a frequency of ~120 kHz in the Cooler Synchrotron COSY, the spin tune is deduced from the up-down asymmetry of deuteron carbon scattering. In a time interval of 2.6 s, the spin tune was determined with a precision of the order $10^{-8}$, and to $1 \cdot 10^{-10}$ for a continuous 100 s accelerator cycle. This renders the presented method a new precision tool for accelerator physics: controlling the spin motion of particles to high precision is mandatory, in particular, for the measurement of electric dipole moments of charged particles in a storage ring.<br />Comment: 6 pages, 6 figures
- Subjects :
- Accelerator Physics (physics.acc-ph)
time reversal
Cyclotron
FOS: Physical sciences
General Physics and Astronomy
Socio-culturale
Electron
01 natural sciences
7. Clean energy
law.invention
Nuclear physics
Economica
law
0103 physical sciences
ddc:550
Nuclear Experiment (nucl-ex)
010306 general physics
and other discrete symmetries
11.30.Er Charge conjugation
Nuclear Experiment
Spin-½
Accelerator physics
Physics
Spin polarization
010308 nuclear & particles physics
Charged particle
Dipole
parity
29.20.dg Cyclotrons, 11.30.Er Charge conjugation, parity, time reversal, and other discrete symmetries,13.40.Em Electric and magnetic moments
13.40.Em Electric and magnetic moments
Physics - Accelerator Physics
Atomic physics
29.20.dg Cyclotrons
Storage ring
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Physical review letters 115(9), 094801 (2015). doi:10.1103/PhysRevLett.115.094801
- Accession number :
- edsair.doi.dedup.....34abffc2fc3b5c4dfc8c25bae697a346
- Full Text :
- https://doi.org/10.1103/PhysRevLett.115.094801