Computing for accelerator physics Ilya Agapov, 7/12/09, DESY ...

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Longterm stability, dynamic aperture Poincare section <strong>for</strong> linear (left) and nonlinear maps (right) Determining stability <strong>for</strong> largeamplitude particles requires longterm tracking Symplectic integrators to avoid large error accumulation Long term stability under influence of small random perturbations (RF noise, scattering) requires sofisticated computeintensive techniques (e.g. 6D FokkerPlanck equation) Spin dynamics in storage rings Codes: COSY, PTC,… Julia Set
Page 1 and 2: Computing for accelerator physics I
Page 3 and 4: Areas where computing plays a role
Page 5 and 6: Linear accelerators Injectorts for
Page 8 and 9: Plasmawakefield acceleration Use
Page 10 and 11: EM field calculations LHC main quad
Page 12 and 13: CST particle studio Collimator wake
Page 14 and 15: Wakefield code ECHO (TU Darmstadt /
Page 16 and 17: Beam optics Accelerator dimensions
Page 18 and 19: Linear optics A typical parametriza
Page 20: Steering (PLACET code, D.Schulte, A
Page 27 and 28: Collective effects a computational
Page 29 and 30: BDSIM Complicated geometries are p
Page 31 and 32: Start to end simulations Several c
Page 33 and 34: For complex machines the control sy
Page 35 and 36: Operator console - virtual mode 35
Page 37 and 38: Example: injection and dump commiss
Page 39 and 40: CMS beam crossing (from CERN logboo
Page 41: Conclusion Electromagnetic codes s

Computing for accelerator physics Ilya Agapov, 7/12/09, DESY ...

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