Keyword: plasma
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MOPF06 Quantification of the Electron Plasma in TItan's Cooler Penning Trap electron, ion, detector, TRIUMF 39
 
  • B.A. Kootte, B. Barquest, U. Chowdhury, J. Even, M. Good, A.A. Kwiatkowski, D. Lascar, K.G. Leach, A. Lennarz, D.A. Short
    TRIUMF, Canada's National Laboratory for Particle and Nuclear Physics, Vancouver, Canada
  • M. Alanssari
    Universität Muenster, Physikalisches Institut, Muenster, Germany
  • C. Andreoiu
    SFU, Burnaby, BC, Canada
  • J. Bale, J. Dilling, A. Finlay, A.A. Gallant, E. Leistenschneider
    UBC & TRIUMF, Vancouver, British Columbia, Canada
  • D. Frekers
    Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany
  • G. Gwinner
    University of Manitoba, Manitoba, Canada
  • R. Klawitter
    Heidelberg University, Physics Institute, Heidelberg, Germany
  • T.T. Li
    UW/Physics, Waterloo, Ontario, Canada
  • A.J. Mayer
    University of Calgary, NW Calgary, Alberta, Canada
  • R. Schupp
    MPI, Muenchen, Germany
 
  Funding: Funded by Natural Sciences and Engineering Research Council of Canada (NSERC)
Modern rare isotope facilities provide beams of shortlived radionuclides primarily for studies in the field of nuclear structure, nuclear astrophysics, and low energy particle physics. At these facilities, many activities such as re-acceleration, improvement of resolving power, and precision experimental measurements require charge breeding of ions. However, the charge breeding process can increase the energy spread of an ion bunch, adversely affecting the experiment. A Cooler Penning Trap (CPET) is being developed to address such an energy spread by means of sympathetic electron cooling of the Highly Charged Ion bunches to . 1 eV/q. Recent work has focused on developing a strategy to effectively detect the trapped electron plasma without obstructing the passage of ions through the beamline. The first offline tests demonstrate the ability to trap and detect more than 108 electrons. This was achieved by using a novel wire mesh detector as a diagnostic tool for the electrons.
* E.M. Burbidge et al, Rev Mod Phys, 29 547 (1957)
** V.V. Simon et al, Phys Rev C, 85 064308 (2012)
*** Z. Ke et al, Hyp Int, 173 103 (2006)
**** U. Chowdhury et al, AIP Conf Proc, 1640 120 (2015)
 
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TUWAUD03 Study of Helical Cooling Channel for Intense Muon Source cavity, simulation, solenoid, emittance 72
 
  • K. Yonehara
    Fermilab, Batavia, Illinois, USA
  • Y.S. Derbenev
    JLab, Newport News, Virginia, USA
  • R.P. Johnson
    Muons, Inc, Illinois, USA
 
  Linear beam dynamics of muons in a helical cooling channel is non-trivial. Betatron oscillation in the channel is induced by coupling of motions in xyz-planes. As a result, the analytic eigen values are very complicated. The cooling decrements are controlled by tuning coupling strength. The helical dynamic parameters are translated into the conventional accelerator physics term. Non-linear dynamics in the helical channel is studied by using the conventional accelerator technique. The beam-plasma interaction in a high-pressure hydrogen gas-filled RF cavity is a new physics process and important to design the cooling channel. Machine development of helical beam elements is also shown in this presentation.  
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THWCR04 RF Technologies for Ionization Cooling Channels cavity, vacuum, electron, ion 145
 
  • B.T. Freemire, Y. Torun
    IIT, Chicago, Illinois, USA
  • D.L. Bowring, A. Moretti, A.V. Tollestrup, K. Yonehara
    Fermilab, Batavia, Illinois, USA
  • A.V. Kochemirovskiy
    University of Chicago, Chicago, Illinois, USA
  • D. Stratakis
    BNL, Upton, Long Island, New York, USA
 
  Funding: Fermilab Research Alliance, LLC under Contract No. DE-AC02-07CH11359
Ionization cooling is the preferred method of cooling a muon beam for the purposes of a bright muon source. This process works by sending a muon beam through an absorbing material and replacing the lost longitudinal momentum with radio frequency (RF) cavities. To maximize the effect of cooling, a small optical beta function is required at the locations of the absorbers. Strong focusing is therefore required, and as a result normal conducting RF cavities must operate in external magnetic fields on the order of 10 Tesla. Vacuum and high pressure gas filled RF test cells have been studied at the MuCool Test Area at Fermilab. Methods for mitigating breakdown in both test cells, as well as the effect of plasma loading in the gas filled test cell have been investigated. The results of these tests, as well as the current status of the two leading muon cooling channel designs, will be presented.
 
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