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Smith, J.D.A.

Paper Title Page
TH5PFP046 Condor as a Resource for Accelerator Research 3303
 
  • J.D.A. Smith
    Cockcroft Institute, Warrington, Cheshire
  • J. Kewley
    STFC/DL, Daresbury, Warrington, Cheshire
  • C. Lingwood
    Cockcroft Institute, Lancaster University, Lancaster
  • J.W. McKenzie
    STFC/DL/ASTeC, Daresbury, Warrington, Cheshire
 
 

This work reports on the developments of a computational infrastructure framework that aids achievement of computational research objectives. Examples from a broad range of accelerator problems will be presented, along with ways in which the workflow can be modified.

 
FR5RFP041 Full Structure Simulations of ILC Collimators 4622
 
  • J.D.A. Smith
    Cockcroft Institute, Warrington, Cheshire
 
 

The prototype collimator of the ILC is simulated, to address potential issues with trapped modes and heating. A number of codes are benchmarked, and the interplay between resistive and geometric wakefields is carefully considered.

 
TU5PFP040 Novel Geometries for the LHC Crab Cavity 909
 
  • B.D.S. Hall, G. Burt
    Cockcroft Institute, Lancaster University, Lancaster
  • R. Calaga
    BNL, Upton, Long Island, New York
  • J.R. Delayen, R.A. Rimmer, H. Wang
    JLAB, Newport News, Virginia
  • J.D.A. Smith
    Lancaster University, Lancaster
 
 

In 2017 the LHC is envisioned to increase is luminosity via an upgrade. This upgrade is likely to require a large crossing angle hence a crab cavity is required to align the bunches prior to collision. There are two possible schemes for crab cavity implementation, global and local. In a global crab cavity the crab cavity is far from the IP and the bunch rotates back and forward as it traverses around the accelerator in a closed orbit. For this scheme a two cell elliptical squashed cavity at 800 MHz is preferred. To avoid any potential beam instabilities all the modes of the cavities must be damped strongly, however crab cavities have lower order and same order modes in addition to the usual higher order modes and hence a novel damping scheme must be used to provide sufficient damping of these modes. In the local scheme two crab cavities are placed at each side of the IP two start and stop rotation of the bunches. This would require crab cavities much smaller transversely than in the global scheme but the frequency cannot be increased any higher due to the long bunch length of the LHC beam. This will require a novel compact crab cavity design.