Emittance Growth in the NLCTA First Chicane
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}{sub 0} = 5 {micro}m for instance). These simulation results agree with the experimental observations.
- Authors:
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1022482
- Report Number(s):
- SLAC-PUB-14323
TRN: US1104379
- DOE Contract Number:
- AC02-76SF00515
- Resource Type:
- Technical Report
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 43 PARTICLE ACCELERATORS; DIPOLES; LINEAR COLLIDERS; MAGNETS; QUADRUPOLES; SIMULATION; Accelerators,ACCPHY
Citation Formats
Sun, Yipeng, Adolphsen, Chris, and /SLAC. Emittance Growth in the NLCTA First Chicane. United States: N. p., 2011.
Web. doi:10.2172/1022482.
Sun, Yipeng, Adolphsen, Chris, & /SLAC. Emittance Growth in the NLCTA First Chicane. United States. https://doi.org/10.2172/1022482
Sun, Yipeng, Adolphsen, Chris, and /SLAC. 2011.
"Emittance Growth in the NLCTA First Chicane". United States. https://doi.org/10.2172/1022482. https://www.osti.gov/servlets/purl/1022482.
@article{osti_1022482,
title = {Emittance Growth in the NLCTA First Chicane},
author = {Sun, Yipeng and Adolphsen, Chris and /SLAC},
abstractNote = {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}{sub 0} = 5 {micro}m for instance). These simulation results agree with the experimental observations.},
doi = {10.2172/1022482},
url = {https://www.osti.gov/biblio/1022482},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Fri Aug 19 00:00:00 EDT 2011},
month = {Fri Aug 19 00:00:00 EDT 2011}
}
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