Novel Accelerator and Detector Systems

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Presentation transcript:

Novel Accelerator and Detector Systems Roger Ruber ruber@tsl.uu.se CAI Workshop 28 September 2007

Novel Detector Systems WASA ATLAS MEG Roger Ruber, CAI Workshop, 28 September 2008

ATLAS: How to Meet the Requirements? To provide high field while minimizing wall material Develop high strength conductor Ni-doped Aluminium-stabilizer: mechanical reinforcement while keeping quench stability Integrate solenoid in common cryostat with LAr calorimeter Sophisticated design work: high strength G10 triangular support structure (sliding) 3D current & cryogenics feeding pure Al-strip quench propagator courtesy A. Yamamoto Roger Ruber, CAI Workshop, 28 September 2008

Novel Accelerator Systems Circular vs. Linear Collider circular accelerator → synchrotron loss higher acc. gradient → shorter linac Power Production klystron → maintenance cost two-beam acceleration Accelerating Gradient superconducting → limit ~50 MV/m (Bc) normal conducting → RF break down CTF3 international test facility power production & high gradient cost energy Circular Collider Linear drive beam main beam RF power pulsed RF power source d RF load Electric field RF wall currents courtesy H. Braun Roger Ruber, CAI Workshop, 28 September 2008

physics phenomena to be investigated RF Break Down reliability issue operation stability beam stability (kick) structure damage conditioning to reach nominal damage in high field areas physics phenomena to be investigated electron & ion currents, radiation (visible, UV, X-ray) microscopy & DC break down © CERN 30 GHz © CERN Roger Ruber, CAI Workshop, 28 September 2008

contact ruber@tsl.uu.se Summary Broad physics & engineering experience Project management & collaboration with CERN, KEK & industry Looking for collaborators in particle & accelerator physics material science & surface physics electromagnetism electronics software & control design, construction & engineering … contact ruber@tsl.uu.se Roger Ruber, CAI Workshop, 28 September 2008