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 νs=γG (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⋅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.

New Method for a Continuous Determination of the Spin Tune in Storage Rings and Implications for Precision Experiments

BERTELLI, Susanna;CIULLO, Giuseppe;CONTALBRIGO, Marco;GUIDOBONI, Greta;LENISA, Paolo;PESCE, Andrea;STATERA, Marco;
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 νs=γG (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⋅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.
2015
Eversmann, D.; Hejny, V.; Hinder, F.; Kacharava, A.; Pretz, J.; Rathmann, F.; Rosenthal, M.; Trinkel, F.; Andrianov, S.; Augustyniak, W.; Bagdasarian,...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/2336235
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