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https://doi.org/10.18429/JACoW-IPAC2015-TUBD2
Title Final Cooling For a High-luminosity High-energy Lepton Collider
Authors
  • D.V. Neuffer
    Fermilab, Batavia, Illinois, USA
  • T.L. Hart, D.J. Summers
    UMiss, University, Mississippi, USA
  • H. K. Sayed
    BNL, Upton, Long Island, New York, USA
Abstract The final cooling system for a high-energy high-luminosity muon collider requires reduction of the transverse emittance by an order of magnitude to ~0.00003 m (rms, N), while allowing longitudinal emittance increase to ~0.1m. In the present baseline approach, this is obtained by transverse cooling of low-energy muons within a sequence of high field solenoids with low-frequency rf systems. Recent studies of such systems are presented. Since the final cooling steps are actually emittance exchange a variant form of that final system can be obtained by a round to flat transform in x-y, with transverse slicing of the enlarged flat transverse dimension followed by longitudinal recombination of the sliced bunchlets. Development of final exchange following lowest-emittance cooling is discussed.
Funding Fermilab is operated by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the U. S. Department of Energy.
Paper download TUBD2.PDF [0.692 MB / 3 pages]
Slides download TUBD2_TALK.PDF [1.976 MB]
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Conference IPAC2015, Richmond, VA, USA
Series International Particle Accelerator Conference (6th)
Proceedings Link to full IPAC2015 Proccedings
Session Contributed Orals (MC1)
Date 05-May-15   15:00–16:00
Main Classification 1: Circular and Linear Colliders
Sub Classification A02 - Lepton Colliders
Keywords emittance, collider, luminosity, solenoid, linac
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
Copyright © 2015 by JACoW, Geneva, Switzerland     CC-BY Creative Commons License
cc Creative Commons Attribution 3.0