32
2002/7/02 NuFact02@Imperial College, London Muon Phase Rotation at PRISM FFAG Akira SATO Osaka University

Muon Phase Rotation at PRISM FFAG

  • Upload
    santo

  • View
    50

  • Download
    2

Embed Size (px)

DESCRIPTION

Muon Phase Rotation at PRISM FFAG. Akira SATO Osaka University. Contents. PRISM Overview Tracking Simulation by Geant3.21 Phase rotation Acceptance of FFAG Muon decay - survival rate Large Gap FFAG Betatron tune dependence Summary. PRISM Beam Characteristics. - PowerPoint PPT Presentation

Citation preview

Page 1: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Muon Phase Rotation at PRISM FFAG

Akira SATOOsaka University

Page 2: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

ContentsPRISM OverviewTracking Simulation by Geant3.21

Phase rotationAcceptance of FFAGMuon decay - survival rate

Large Gap FFAGBetatron tune dependence

Summary

Page 3: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 4: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 5: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 6: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 7: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Simulation of the PRISM Phase Rotator

By GEANT3.21 Full simulationMuon decay -> intensityInteraction -> background

Acceptance studyPhase rotation studyMuon survival rate

Page 8: Muon Phase Rotation at PRISM FFAG

2002/7/02 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

Simulation Setup

Page 9: Muon Phase Rotation at PRISM FFAG

2002/7/02 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: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

RF modelingTotal # of RF cavity : 12

4gaps/cavity

RF wave field type:SinusoidalSaw tooth

25cm

2 m

Page 11: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

100 cm

Information @θ =0

(r,θ,z)momentumToFParticle ID

θ

θ =0

Page 12: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Muon injectionMuon was injected from θ=0momentum: 68MeV/c+-20%54.4, 61.2, 68.0, 74.8, 81.6MeV/c

Phase space:r : r(p)+-8 cmur : 0+-0.2 rad.z : 0+-16 cmuz : 0+-0.08 rad.

Timing :Arrival time to solenoid exit is taken into account.

10ns 10ns

81.6

71.2

68.0

61.2

54.4MeV/c

t=0,+-5ns

Page 13: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Typical Muon Track

54.4MeV/c μBecause FFAG has momentum dispersion, radius of the muon orbit becomes lager gradually.

Page 14: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Phase Rotation Study

SinusoidalSaw tooth

Page 15: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

01

23

45

Sinusoidal RFRF : 5MHz, 128kV/m

Energy spread after 5turnsΔp/p = 68MeV/c+8%-6%ΔE/E

= 20MeV+12%-10%

Page 16: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

012

3

4

5

Saw tooth RF RF : 5MHz, 250kV/m

Energy spread after

5turnsΔp/p

= 68MeV/c+2%-2%ΔE/E

= 20MeV+4%-5%

Page 17: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 18: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 19: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Acceptance Study

Horizontal acceptanceVertical acceptance

Survival rateLarge gap FFAG

Page 20: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 21: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 22: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Muon surviving -

e-

decay

Surviving rate after 5turns : 60%e- contamination : < 1/1600

Decay OFF

Decay ON

# of surviving muon after 5 turns

Page 23: Muon Phase Rotation at PRISM FFAG

2002/7/02 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 24: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

FFAG Magnet with Large Gap(1)

Page 25: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Dose an acceptance depend on betatron tune?

Selection of Betatron Tune

Page 26: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Long Term Acceptance (Region1)

Page 27: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Long Term Acceptance (Region2)

Page 28: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

5 turns Acceptance- Number of lost particle

Region1 Region2

FFAG acceptance depends on betatron tune.

Page 29: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Surviving Rate (Region2)

Page 30: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Page 31: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

Page 32: Muon Phase Rotation at PRISM FFAG

2002/7/02 NuFact02@Imperial College, London

SummaryPRISM phase rotation was studied by GEANT3.21.We can achieve energy spread of ΔE/E=+-5% after phase rotation.Even present design PRISM FFAG has large acceptance : H=10000, V=2000mm mrad. These acceptance was limited by physical aperture.We have some idea to get lager acceptance. These will be studied soon.