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https://doi.org/10.18429/JACoW-IPAC2015-WEPWA064
Title Ionization Cooling Channels in COSY Infinity
Authors
  • B.T. Loseth, M. Berz
    MSU, East Lansing, Michigan, USA
  • P. Snopokpresenter
    Illinois Institute of Technology, Chicago, Illinois, USA
Abstract Ionization cooling is a method to reduce the emittance of a beam through the use of absorbers, rf cavities, and strong solenoids for focusing, arranged into a condensed lattice. By tuning lattice parameters, it is possible to construct a staged cooling channel in which the beam emittance is always considerably greater than the minimum value. In the late stages of the cooling channel, space charge effects can become a significant obstacle to further emittance reduction once the beam becomes sufficiently condensed. A method has been implemented in COSY Infinity, a beam dynamics simulation and analysis code, which efficiently and accurately calculates the self-fields of all particles on each other based on a variant of the Fast Multipole Method (FMM). In this paper, we present simulations of a muon ionization cooling channel performed in COSY, utilizing the FMM, benchmarked against G4beamline, a standard code for muon beam analysis, in order to investigate the significance of space charge effects.
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Conference IPAC2015, Richmond, VA, USA
Series International Particle Accelerator Conference (6th)
Proceedings Link to full IPAC2015 Proccedings
Session Wednesday Posters (Washington)
Date 06-May-15   16:00–18:00
Main Classification 3: Alternative Particle Sources and Acceleration Techniques
Sub Classification A09 - Muon Accelerators and Neutrino Factories
Keywords emittance, space-charge, simulation, multipole, solenoid
Publisher JACoW, Geneva, Switzerland
Editors Stuart Henderson (ANL, Argonne, IL, USA); Evelyn Akers (Jlab, Newport News, VA, USA); Todd Satogata (JLab, Newport News, VA, USA); Volker R.W. Schaa (GSI, Darmstadt, Germany)
ISBN 978-3-95450-168-7
Published June 2015
Copyright
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cc Creative Commons Attribution 3.0