2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka...
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Transcript of 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka...
![Page 1: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University.](https://reader035.fdocuments.in/reader035/viewer/2022062408/56649eb65503460f94bc07a8/html5/thumbnails/1.jpg)
2002/7/04 NuFact02@Imperial College, London
Beam Dynamics Studies of FFAG
Akira SATOOsaka University
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2002/7/04 NuFact02@Imperial College, London
Contents
PRISM FFAG studiesLarge gap FFAGExperimental studies of PoP FFAGSummary
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2002/7/04 NuFact02@Imperial College, London
PRISM FFAG Studies
PRISM OverviewPhase Rotation
Acceptance
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2002/7/04 NuFact02@Imperial College, London
PRISM Beam Characteristics
intensity : 1011-1012±/secmuon kinetic energy : 20 MeV (=68 MeV/c)
range = about 3 g
kinetic energy spread : ±0.5-1.0 MeV±a few 100 mg range width
beam repetition : about 100Hz
Search μN→eN with sensitivity of 10-18
Cf. MECO @BNL-AGS 10-16
Phase Rotated Intense Slow Muon source
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2002/7/04 NuFact02@Imperial College, London
PRISM layoutPion capture sectionDecay sectionPhase rotation section
FFAG Baseda ring instead of linear
systemsreduction of # of rf cavitiesreduction of rf power consumptioncompact not in scale
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2002/7/04 NuFact02@Imperial College, London
FFAG for Phase Rotation
synchrotron oscillation for phase rotation
not cyclotron (isochronous)
large momentum acceptancelarger than synchrotron± several 10 % is aimed
large transverse acceptancestrong focusinglarge horizontal emittancereasonable vertical emittance at low energy
Fixed Field Alternating Gradient Synchrotron
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2002/7/04 NuFact02@Imperial College, London
Phase RotationPhase Rotation = decelerate particles with high energy and accelerate particle with low energy by high-field RF
A narrow pulse structure (<1 nsec) of proton beam is needed to ensure that high-energy particles come early and low-energy one come late.
energyenergy
time time
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2002/7/04 NuFact02@Imperial College, London
Muon phase rotation was studied by the GEANT3.21 3D simulation.
except kicker parts.
GEANT3 has single precision.
Cf. Double precisionDPGeantGeant4
PRISM FFAG Simulation
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2002/7/04 NuFact02@Imperial College, London
Magnet Model and Field 3D magnetic field of FFAG magnet was calculated by TOSCA.
Field gradient was made by gap size.Magnitude of the field
D : Bz = -0.0717(r(m)/r0)5 (T)
F : Bz = +0.435(r(m)/r0)5 (T)
r0 = 5 m for 68MeV/c
1 Cell = 45.0 deg.Straight sect. = 16.49 D = 2.46 FD 間 = 0.10 F/2 = 3.00
rrin=460
rout=550cm
Half gap = 10 x (500/r)5 cm
FFAG LatticeTriplet : DFD
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2002/7/04 NuFact02@Imperial College, London
Typical Muon Track
54.4MeV/c μBecause FFAG has momentum dispersion, radius of the muon orbit becomes lager gradually.
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2002/7/04 NuFact02@Imperial College, London
01
23
45
Phase Rotation
RF : 5MHz, 128kV/mΔE/E = 20MeV+12%-10%
012
3
4
5
RF : 5MHz, 250kV/mΔE/E = 20MeV+4%-5%
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2002/7/04 NuFact02@Imperial College, London
How to realize saw toothIt is difficult to realize saw tooth with a field gradient of 250kV/m. Fit the saw tooth wave to the function:
Each RF have just sinusoidal wave.
V (t) Ansin(nt /L Bn )n1
3
phase(nsec)-100 -50 05 0 100
-2000
-1500
-1000
-500
0
500
1000
1500
2000
wave136.dat
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.6647)E = -275.00 sin( 2
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.6647)E = -275.00 sin( 2
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.9085)E = 250.00 sin( 3
Wav e Comp.
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2002/7/04 NuFact02@Imperial College, London
Simulation Result1 0
3
2
4
phase(nsec)-100 -50 05 0 100
-2000
-1500
-1000
-500
0
500
1000
1500
2000
wave136.dat
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.6647)E = -275.00 sin( 2
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.6647)E = -275.00 sin( 2
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.1569)E = 350.00 sin( 1
Wav e Comp.
phase(nsec)-100 -500 50 100
-300
-200
-100
0
100
200
300
x / L + -0.9085)E = 250.00 sin( 3
Wav e Comp.
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②
③
①
①
①
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①
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2002/7/04 NuFact02@Imperial College, London
Horizontal Phase SpaceInitial Phase
After 1 turn
After 2turns
After 3turns
After 4 turns
After 5turns
54.4 61.2 68.0 74.8 81.6MeV/c
Horizontal Acceptance 10000pi mm mrad
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2002/7/04 NuFact02@Imperial College, London
54.4 61.2 68.0 74.8 81.6MeV/c
Initial Phase
After 1 turn
After 2 turns
After 3 turns
After 4 turns
After 5 turns
Vertical Phase Space
Vertical Acceptance 2000pi mm mrad
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2002/7/04 NuFact02@Imperial College, London
Survival Rate vs. Momentum
Why do large momentum particles have low survival rate? Gap ∝ (r0/r)5
Physical aperture limits the dynamical acceptance.Lager Gap Magnet → Lager Acceptance
We Need Lager Gap Magnet !
rrin
rout
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2002/7/04 NuFact02@Imperial College, London
FFAG Magnet with Large Gap(1)
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2002/7/04 NuFact02@Imperial College, London
Dose an acceptance depend on betatron tune?
Selection of Betatron Tune
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2002/7/04 NuFact02@Imperial College, London
Long Term Acceptance (Region1)
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2002/7/04 NuFact02@Imperial College, London
Long Term Acceptance (Region2)
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2002/7/04 NuFact02@Imperial College, London
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2002/7/04 NuFact02@Imperial College, London
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2002/7/04 NuFact02@Imperial College, London
Studies of the beam dynamics in the PoP-FFAG
Beam AccelerationHorizontal acceptanceDynamic aperture
PoP FFAG
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2002/7/04 NuFact02@Imperial College, London
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2002/7/04 NuFact02@Imperial College, London
Beam position monitor
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2002/7/04 NuFact02@Imperial College, London
Beam Acceleration
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2002/7/04 NuFact02@Imperial College, London
Horizontal acceptance
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2002/7/04 NuFact02@Imperial College, London
Beam motion at the resonance conditions
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2002/7/04 NuFact02@Imperial College, London
150-MeV proton FFAG
With “return yoke free” magnetNow under construction
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2002/7/04 NuFact02@Imperial College, London
150 MeV FFAG Roadmap
23
fiscal 2002 45 Construction6789
1011 Commissioning12123 Experiment
fiscal 2003 456
Inspection by Government
making the proposalof the radioactive instrument
Permission of the commissioning
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2002/7/04 NuFact02@Imperial College, London
SummaryThe PoP FFAG worked as designed.
Proton can be accelarated in 1msec.
PRISM phase rotation was studied by GEANT3.21.
Energy spread of ΔE/E=+-5% was achieved.The present design PRISM FFAG has large acceptance : H=10000, V=2000pmm mrad. These acceptance was limited by physical aperture.
We have some idea to get lager acceptance FFAG. These will be studied soon.