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RIS citation export for MOPF01: Final Cooling for a High Energy High Luminosity Collider

TY - UNPB
AU - Neuffer, D.V.
AU - Hart, T.L.
AU - Summers, D.J.
ED - Akers, Evelyn (Jefferson Lab), Satogata, Todd Satogata (Jefferson Lab), Schaa, Volker RW Schaa (GSI)
TI - Final Cooling for a High Energy High Luminosity Collider
J2 - Proc. of COOL2015, Newport News, VA, USA, September 28 - October 2, 2015
C1 - Newport News, VA, USA
T2 - International Workshop on Beam Cooling and Related Topics
T3 - 10
LA - english
AB - 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 an initial approach, this is obtained by transverse cooling of low-energy muons within a sequence of high field solenoids with low-frequency rf systems. Since the final cooling steps are actually emittance exchange, much of this transformation can be obtained by thick wedge absorbers at matched parameters. Other variations using quad-based cooling channels, transverse beam slicing and round to flat transforms can be used. in x-y, with transverse slicing and longitudinal recombination are discussed. Development of lowest emittance cooling with final exchange is discussed.
PB - JACoW
CP - Geneva, Switzerland
ER -