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Talman, R.M.

Paper Title Page
MOP101 Simulation of Emittance Growth Using the UAL String Space Charge Model 308
  • R.M. Talman
    CLASSE, Ithaca, New York
  • N. Malitsky
    BNL, Upton, Long Island, New York
  • F. Stulle
    CERN, Geneva

Evolution of short intense electron bunches passing through bunch-compressing beamlines is simulated using the UAL (Unified Accelerator Libraries) string space charge formulation. Excellent agreement is obtained with results obtained experimentally at CTF-II, the CERN "Compact Linear Collider'' test facility. The 40 MeV energy of these data is low enough for Coulomb and Biot-Savart forces to be important and high enough for coherent synchrotron radiation and centrifugal space charge forces to be important. UAL results are also compared with CSRtrack results for emittance growth in a 40 MeV 'standard' chicane. Vertical space charge forces are found to be important in this (low energy) case.