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Chopper. Longitudinal dynamics. May 26, 2010 Nick Perunov , Nikolay Solyak. Input beam parameters after RFQ. Beam distribution after HINS RFQ . (Simulation for 10 mA ). Beam distribution after HINS RFQ (Simulation for 10 mA ).
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Chopper. Longitudinal dynamics. May 26, 2010 Nick Perunov, NikolaySolyak
Beam parameters after RFQ, used in TraceWin for matching between RFQ and chopperc Note : Beam parameters used in lattice design is slightlydifferent from RFQ simulations in TRACK (previous slide)
Objectives: In the first design, presented in May 19, 2010 we have observed longitudinal emittance growth after SSR0 section caused by non-linearity in the cavity. Reason is large bunch length (>90 deg for 3 sigma) in the location of buncher cavities.Goal: minimize emittance growth at the end of SSR0 section and halo formation, by reducing bunch length in chopper cavities. Revision of the longitudinal beam dynamics in Choppersection.
Chopper geometry & parameters. • Periodic structure (4 periods) • Each period = chopper, triplet, bunching cavity, beam dump. Phase advance μX=180°; μY=120°; μz~90°; • Apertures: • Chopper: 15mmx25mm; cavity Ø30mm; triplet = Ø40mm; beam dump 10-14mm • Chopper: • 0.5m long; Voltage: ±375 V; gap=15mm
Input beam parametersBeam: 325 MHz; 2.5 MeV; 10mA-peak Estimation for minimum longitudinal beam size in cavity location: where: εz- emittance; z = L perod/2 In our case: εz = 0.49 mm*mrad; z = 1.3 m: σmin = 4.2 mm = 22.5 deg (RMS)
Longitudinal 3σ envelopes • Four cases are presented here: • Version 0 (Initial) – shown May 19 presentation • V1-V4 is new versions with different cavity voltages and bunch lenghts Initial V4 V2 V1 V3 • Transverse beam dynamics are the same: • Phase advance in x-plane = 180 deg; • Phase advance in y-plane ≈ 120 deg;
Beam distribution in the exit of the chopper Initial version Version 1 Version 2 In all cases the distribution in the entrance of the chopper was Gaussian( 3 independent planes, max_size = 3.1 rms_size ) Version 4 Version 3
Beam halo. Version 1 Version 2 Initial version Version 4 Version 3
99% Emittance. Initial version Version 2 Version 1 Version 4 Version 3
Version 3 looks as the best choice. • Let’s compare two versions: Ver.0 vs. Ver.3 Details of longitudinal phase space see in next slides.