This work describes a quadrupole cooling channel designed to cool initial emittances of 15-20 cm (normalized) by a factor of two in each transverse plane. Its application is clearly as the most upstream stage of cooling and, being a linear channel with no bends, serves to reduce the large transverse beam size before introduction into emittance exchange channels or ring coolers. As will be shown, this channel cools efficiently and beyond the momentum reach of a solenoidal precooler. It uses large bore, normal-conducting quadrupoles with fringe-field and other higher-order effects fully included in the simulations. Some of the attractions of such a channel are that superconducting magnetic elements are not required and rf cavities and absorbers can be placed entirely in the region between quadrupoles, thus removing the difficulty of inserting them within magnetic elements. There is a marked reduction, at least, in the component cost and technical difficulty of such a channel.
C. J. Johnstone: Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510, USA. Email: cjj@fnal.gov.
M. Berz: Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA. Email: berz@msu.edu.,
D. Errede, K. Makino: Department of Physics, University of Illinois at Urbana-Champaign, 1110 W. Green Street, Urbana, IL 61801-3080, USA. Email: derrede@uiuc.edu, makino@uiuc.edu.
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