Author: Butler, K.R.
Paper Title Page
WEP109 Simulations of Electron Cloud Induced Instabilities and Emittance Growth for CesrTA 1683
 
  • K.G. Sonnad, K.R. Butler
    Cornell University, Ithaca, New York, USA
  • G. Dugan, M.A. Palmer
    CLASSE, Ithaca, New York, USA
  • M.T.F. Pivi
    SLAC, Menlo Park, California, USA
 
  Funding: US Department of Energy DE-FC02-08ER41538, National Science Foundation PHY-0734867
We present results of a series of studies obtained using the simulation code CMAD to study how electron clouds affect the dynamics of positron beams in CesrTA. The study complements ongoing experiments dedicated for studying the same phenomena. The simulation involves tracking positrons through the CesrTA lattice and simultaneously computing the force exerted due to space charge of the electrons on each of the tracked positrons. The electrons themselves are allowed to evolve under the influence of the positrons. Several results bear a close resemblance to what has been observed experimentally.