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2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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Page 1: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Beam Dynamics Studies of FFAG

Akira SATOOsaka University

Page 2: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Contents

PRISM FFAG studiesLarge gap FFAGExperimental studies of PoP FFAGSummary

Page 3: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

PRISM FFAG Studies

PRISM OverviewPhase Rotation

Acceptance

Page 4: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 5: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 6: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 7: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 8: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 9: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 10: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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.

Page 11: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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%

Page 12: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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.

Page 13: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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.

①②

①①

②③

Page 14: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 15: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 16: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 17: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

FFAG Magnet with Large Gap(1)

Page 18: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Dose an acceptance depend on betatron tune?

Selection of Betatron Tune

Page 19: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Long Term Acceptance (Region1)

Page 20: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Long Term Acceptance (Region2)

Page 21: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Page 22: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Page 23: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Studies of the beam dynamics in the PoP-FFAG

Beam AccelerationHorizontal acceptanceDynamic aperture

PoP FFAG

Page 24: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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Page 25: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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Beam position monitor

Page 26: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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Beam Acceleration

Page 27: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Horizontal acceptance

Page 28: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

Beam motion at the resonance conditions

Page 29: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

2002/7/04 NuFact02@Imperial College, London

150-MeV proton FFAG

With “return yoke free” magnetNow under construction

Page 30: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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

Page 31: 2002/7/04 NuFact02@Imperial College, London Beam Dynamics Studies of FFAG Akira SATO Osaka University

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.