Front End Capture/Phase Rotation & Cooling Studies
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Front EndCapture/Phase Rotation& Cooling Studies David NeufferCary Yoshikawa
December 2008
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0utlineIntroduction -Factory Front endCapture and -E rotation High Frequency buncher/rotation Study 2B -FactoryShorter version -Factory+-- Collider
Discussion
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Variations tried Study 2A ISS baselineShorter bunch train examplenB= 10Better for Collider; as good for -Factory ICOOL/G4Beamline simulations Study of accepted particlesRf cavities in solenoids? Use magnetic insulation ASOL latticeNot too bad Variations Higher energy capture ??
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Study2B June 2004 scenario (ISS)Drift 110.7mBunch -51m(1/) =0.00812 rf freq., 110MV330 MHz 230MHz-E Rotate 54m (416MV total)15 rf freq. 230 202 MHzP1=280 , P2=154 NV = 18.032Match and cool (80m)0.75 m cells, 0.02m LiHCaptures both + and -~0.2 /(24 GeV p)
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Study 2B ICOOL simulation (NB=18)s = 1ms=109m s=166ms= 216m-4060500MeV/c0DriftBunchRotate500MeV/c0
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Features/Flaws of Study 2B Front EndFairly long system ~300m long (217 in B/R) Produces long trains of ~200 MHz bunches~80m long (~50 bunches)Transverse cooling is ~2 in x and y, no longitudinal coolingInitial Cooling is relatively weak ? -Requires rf within magnetic fields in current lattice, rf design; 12 MV/m at B = ~2T, 200MHzMTA/MICE experiments to determine if practical
For Collider (Palmer)Select peak 21 bunchesRecombine after cooling~1/2 lost
-4060m500 MeV/c
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Shorter Bunch train example Reduce drift, buncher, rotator to get shorter bunch train:217m 125m 57m drift, 31m buncher, 36m rotatorRf voltages up to 15MV/m (2/3)Obtains ~0.26 /p24 in ref. acceptanceSlightly better ? ~0.24 /p for Study 2B baseline80+ m bunchtrain reduced to < 50mn: 18 -> 10 -3040m500MeV/c
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Further iteration/optimizationMatch to 201.25 MHz cooling channelReoptimize phase, frequencyf = 201.25 MHz, = 30, Obtain shorter bunch train
Choose ~best 12 bunches ~ 21 bunch train for Collider at NB= 18 case~12 bunches (~18m)~0.2 /pref in best 12 bunchesDensest bunches are ~twice as dense as NB = 18 case
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Details of ICOOL model (NB=10)Drift 56.4mB=2TBunch- 31.5mPref,1=280MeV/c, Pref,2 =154 MeV/c, nrf = 10 Vrf 0 to 15MV/m (0.5m rf, 0.25m drift) cells 360 MHz 240MHz-E Rotate 36m Vrf = 15MV/m (0.5m rf, 0.25m drift) cellsNV = 10.07 (240 -> 201.5 MHz)Match and cool (80m)Old ICOOL transverse match to ASOL (should redo)Pref= 220MeV/c, frf = 201.25 MHz 0.75 m cells, 0.02m LiH, 0.5m rf, 16.00MV/m, rf =30Better cooling possible (H2, stronger focussing)
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Simulations (NB=10)-30m30m500 MeV/c0Drift andBunchs = 89ms = 1mRotates = 125ms = 219mCool
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Front end simulationsInitial beam is 8GeV protons, 1ns bunch length
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Comparisons of ICOOL and G4BLSimulations of front end and cooling agreeICOOL and G4Beamline results can be matched
Buncher rotator cooler sequence can be developed in both codes
Method Captures both + and -
But some differencesdE/dx is larger in ICOOL Phasing of rf cavities uses different model
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12.9 m43.5 m31.5 m36 mdriftbuncherrotatorcaptureMC Front End Layout in G4beamline
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G4BeamlineICOOLPi+/Mu+Pi-/Mu-Rotator End
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G4BeamlineICOOLPi+/Mu+Pi-/Mu-Cool End
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Reduce number of independent frequenciesInitial example had different rf frequency for each cavityBuncher- 42 cavities -31.5m 360to 240 MHzRotator- 48 cavities -36m240 to 202 MHz
Reduce # by 1/3 14 in buncher; 16 in rotatorNearly as good capture (
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Accepted particlesAccepted particles fit final beam cuts:AX + Ay < 0.03mAL < 0.2m
Initial beam has momenta from ~75 to ~600 MeV/cFinal beam is ~200 to 300 MeV/c
Transverse emittance is cooled from ~0.014 to ~0.0036 600 MeV/c600MeV/c0 MeV/c0 MeV/c
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Accepted Longitudinal distros1m135m135m196m196m-30m40m600 MeV/c600 MeV/c0 MeV/c0 MeV/c
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Accepted Beam propertiesFor study 2A acceptance means several cuts:AX + Ay < 0.03mAL < 0.2mFor beam within acceptances, t, N,rms = 0.0036m (from ~0.007)L, N,rms = ~0.04m (from ~0.09)
Emittances are much smaller than the full-beam emittances xrms = 6cm (all-beam)xrms = 3.6cm (accepted-beam)
-30cm+30cm-30cm+30cm
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Variations - focusing Buncher and Rotator have rf within 2T fieldsField too strong for rf field ??Axial field within pill-box cavities
Solutions ??Open-cell cavities ??magnetically insulated cavitiesAlternating Solenoid lattice is approximately magnetically insulatedUse ASOL throughout buncher/rotator/cooler
Use gas-filled rf cavitiesASOL lattice
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Use ASOL lattice rather than 2TStudy 2A ASOLBmax= 2.8T, *=0.7m,Pmin= 81MeV/c2T for initial driftLow energy beam is lost (P < 100MeV/c)Bunch train is truncatedOK for collider
Also tried weaker focusing ASOLBmax= 1.83T, *=1.1m,Pmax = 54 MeV/c1.33 T for initial driftMatch scaled from 2A match
+ -B(z)
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2T -> ASOL
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ASOL-1.33T 56m62m133m193m
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First ASOL results Simulation results2.8T ASOL0.18 /24 GeV p0.059 /8 GeV p Cools to 0.0075m1.8T ASOL0.198 /24 GeV p0.064 /8 GeV p~10% more than stronger focussingCools to 0.0085m
Baseline (2T -> ASOL) had~0.25 /24 GeV p~0.08 /8 GeV p
Weaker-focusing ASOL has ~10% better acceptance than 2.8T latticeLonger bunch train
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Variant-capture at 0.28 GeV/c0.01.0GeV/c1.0GeV/c0.02T 2.8T ASOL-30m+40m-30m+40m1.0GeV/cs=59ms=66ms=126ms=200m
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Capture at 280 MeV/cCaptures more muons than 220 MeV/c For 2.T -> 2.8T latticeBut in larger phase space areaLess cooling for given dE/ds sBetter for colliderShorter, more dense bunch trainIf followed by longitudinal cooling
220 MeV/c280 MeV/c
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Higher-Energy Simulation resultsHigher energy capture improves capture for high-field latticeCooling is slower
Not as good for low-field latticeWeaker focusing reduces coolingFor High field lattice:2.8T ASOL8GeV beam 0.065 /p in t
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DiscussionHigh frequency phase-energy rotation + cooling has been explored
Shorter system better for Collider Shorter bunch train; denser bunches
magnetic insulated lattice could be used rather than B = 2 or 1.75 T latticeSlightly worse performance (?)~10 to 20% worse for neutrino factory Ok for Collider Particles lost are at end of bunch train
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Any Questions?
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Project X Status
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High-frequency Buncher and -E RotatorForm bunches first
-E rotate bunches