 DOCUMENT METADATASLAC Publication: SLAC-PUB-14323
SLAC Release Date: August 19, 2011
Emittance Growth in the NLCTA First Chicane
Sun, Yipeng.
In this paper, the emittance growth in the NLCTA (Next Linear Collider Test Accelerator) first chicane region is evaluated by simulation studies. It is demonstrated that the higher order fields of the chicane dipole magnet and the dipole corrector magnet (which is attached on the quadrupoles) are the main contributions for the emittance growth, especially for the case with a large initial emittance (gamma\epsilon _0 = 5 mu m for instance). These simulation results agree with the experimental obs... Show Full Abstract
In this paper, the emittance growth in the NLCTA (Next Linear Collider Test Accelerator) first chicane region is evaluated by simulation studies. It is demonstrated that the higher order fields of the chicane dipole magnet and the dipole corrector magnet (which is attached on the quadrupoles) are the main contributions for the emittance growth, especially for the case with a large initial emittance (gamma\epsilon _0 = 5 mu m for instance). These simulation results agree with the experimental observations. Show Partial Abstract
Download File:
|
