Speaker
Description
The final cooling performance for the muon collider is strongly dependent on absorber length, beam kinetic energy and energy spread. This paper explores the role of energy-time correlations in longitudinal emittance growth within the absorber. This process is significant as it dictates the efficiency of the longitudinal rotation required between final cooling cells. Minimizing longitudinal emittance is crucial as it ensures a reduced energy spread at the muon collider, which is required to allow for efficient chromaticity correction, and further improving luminosity.
Another consideration is that the longitudinal emittance growth has a strong correlation with action, particularly due to high-field solenoid dynamics. This paper shows how this correlation changes throughout the cooling channel, including the impact of the liquid hydrogen absorbers.
Funding Agency
Endorsed by the IMCC
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