july 28, 2004k. yonehara, nufact'04 osaka1 high pressure rf cavities for muon beam cooling...
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July 28, 2004 K. Yonehara, NuFact'04 Osaka 1
High pressure RF cavitiesfor muon beam cooling
Katsuya Yonehara
Illinois Institute of Technology
NuFact04 in Osaka 7/28/04
July 28, 2004 K. Yonehara, NuFact'04 Osaka 2
Muon accelerators
• Muon colliders (Energy frontier machine)– No limitation by synchrotron radiation
• Radiation (beam-strahlung) factor (m/me)2 ~ 40,000
– 1/10 energy/footprint of proton colliders• Energy of interaction is full energy of produced
particle since s are fundamental particles.
• Neutrino factories (Muon storage ring)– Exciting new physics
July 28, 2004 K. Yonehara, NuFact'04 Osaka 3
Six muon projectsPromoted by Muons, Inc., July, 2004
• High-pressure gaseous hydrogen RF cavity• MANX (Muon collider And Neutrino factory
eXperiment)• 6-Dimensional helical cooling channel
– see MuCoolNote0284
• Hydrogen cryostat• Phase ionization cooling• Cryogenic pulsed power compressor
See “http://www.cap.bnl.gov/mumu/conf/MC-040127/johnson-MC.pdf “for below three items
July 28, 2004 K. Yonehara, NuFact'04 Osaka 4
Muon ionization cooling
Step 1: Beam energy loss dE/dx in transverse and longitudinal directions
Step 2: Longitudinal energy replaced by RF electric acceleration field
# A strong solenoidal magnetic field is required to make a low in cooling material.
Cooling material
Step 1
Step 2
This method is only available for muons.
Py
Pz
July 28, 2004 K. Yonehara, NuFact'04 Osaka 5
Properties of gaseous hydrogen
• Best cooling material– Highest (X0 dE/ds)2
• High heat capacity– Cools Be RF windows effectively
• Low critical temperature– 33 K
July 28, 2004 K. Yonehara, NuFact'04 Osaka 6
Advantages of high pressuregaseous hydrogen in an RF cavity
• Dense GH2 suppresses high-voltage breakdown– Small mean free path inhibits avalanches
(Paschen’s law)
• Gas acts as an energy absorber– Needed for ionization cooling
July 28, 2004 K. Yonehara, NuFact'04 Osaka 7
Phase I research
• Build cryogenic HP RF test cell– Need special sealing technology on every joint
(ex. RF feed line, pickup coil, etc)– Good pressure seal and RF seal
• Measure RF breakdown voltage vs. pressure– The data should follow Paschen’s law, relating
breakdown voltage to gas density, over a range of temperatures, and pressures.
– Compare helium and hydrogen.
July 28, 2004 K. Yonehara, NuFact'04 Osaka 8
Collaborators
R. E. Hartline, R. P. Johnson, M. Kuchnir,
T.J. RobertsMuons, Inc.
C. M. Ankenbrandt, A. Moretti, M. PopovicFermi National Accel. Lab
M. Alsharo’a, D.M. Kaplan, K. YoneharaIllinois Institute of Tech.
July 28, 2004 K. Yonehara, NuFact'04 Osaka 9
HP RF cavity
Electrode (“knob”)replaceable
Metal sealing (use Aluminum gasket) RF feed line
All surfaces arecopper plated
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Test Cell
July 28, 2004 K. Yonehara, NuFact'04 Osaka 11
Experiment
July 28, 2004 K. Yonehara, NuFact'04 Osaka 12
Frequency shift
P vs f, GH2 @77K 11/19/03
frequency = -7E-07P2 - 0.0263P + 805
794
796
798
800
802
804
806
0 100 200 300 400
P (PSIA)
TC
fre
qu
ency
(M
Hz)
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11/19/03 Lab G Results, Molybdenum Electrode
H2 vs He RF breakdown at 77K, 800MHz
0
10
20
30
40
50
60
70
80
0 100 200 300 400 500 600
Pressure (PSIA)
Max
Sta
ble
Gra
die
nt
(MV
/m)
Linear Paschen Gas Linear Paschen Gas Breakdown RegionBreakdown Region
Metallic Surface Metallic Surface Breakdown RegionBreakdown Region
Waveguide BreakdownWaveguide Breakdown
Hydrogen Hydrogen
HeliumHelium
Fast conditioning: 3 h from 70 to 80 Fast conditioning: 3 h from 70 to 80 MV/mMV/m
July 28, 2004 K. Yonehara, NuFact'04 Osaka 14
Results
• 80 MV/m surface gradient achieved• Fast conditioning (Last 15 MV/m in 3 h)• Note that the resonant frequency diminishes with
pressure since the dielectric constant depends on density. As the klystron was tuned to follow the cavity resonant frequency, a resonance in the wave guide caused breakdown before the power reached the cavity i.e. the dip in the previous plot.
July 28, 2004 K. Yonehara, NuFact'04 Osaka 15
Plan I: Observe breakdown• Study metal surface breakdown
– Change electrode material• Cu, Mo, Cr, Be (ref. Perry Wilson)
• Optical approach– Use glass fiber optics
• Good transmission efficiency from UV to VIS region• Insensitive to temperature
– Use photo diode• Good sensitivity from UV to VIS region• Insensitive to magnetic field
– Use C fiber ferrule for optical feedthrough• Sealing test has been done under 1600 PSI GHe• Yet to do the same test at cryogenic temperature
July 28, 2004 K. Yonehara, NuFact'04 Osaka 16
Plan I setup
NPT-SWG1/8
C fiber ferrule
Fiber optics(D 500 microns)
Change electrodes materials
July 28, 2004 K. Yonehara, NuFact'04 Osaka 17
Plan II: Test with proton beam
• What is breakdown voltage with ionizing radiation? We expect;– Fast ion recombination in HP GH2
• Much shorter than the RF period
– RF breakdown is suppressed• Extrapolating from our measurement ~700 MV/m at
one half of LH2 density
July 28, 2004 K. Yonehara, NuFact'04 Osaka 18
Hopes for HP RF cavity
• Higher gradients than with vacuum• Less dependence on metallic surfaces
– Dark currents, x-rays diminished– Very short conditioning times already seen
• Easier path to closed-cell RF design– Hydrogen cooling of Be windows
• Can be used for 6D cooling and acceleration– Homogeneous absorber concept– Implies HF for muon acceleration (1.6 GHz)
July 28, 2004 K. Yonehara, NuFact'04 Osaka 19
Present activities for HP RF Phase II project
• Studying RF breakdown with Cu, Mo, Cr, Be electrodes 50:85:112:194 (Perry Wilson)
• Planning Test Cell for Operation in the 5 Tesla solenoid at 1600 PSI (~ 110 atm) and 77K
• Working on MTA Beamline– Want radiation test of GH2 RF in 2005
• Constructing simple MTA beam line (reference; MuCoolNote0287, 0294)
July 28, 2004 K. Yonehara, NuFact'04 Osaka 20
MANX project
• This is a first project using the high pressure gaseous RF cavities
• Muons, Inc. are funding phase I
July 28, 2004 K. Yonehara, NuFact'04 Osaka 21
MANX is GH2 version of MICE
Scifi Tracker Regions
Matching coils
Spectrometer solenoid 2
Cooling solenoids 1 & 2
High Pressure H2
RF cavities
July 28, 2004 K. Yonehara, NuFact'04 Osaka 22
Summary for HP GH2 RF
• GH2 an enabling technology for machines
– High gradient RF for less-expensive, more efficient beam cooling
– Emittance exchange with homogeneous absorber• 6D cooling makes Muon Collider possible
– Maybe ionization cooling parametric resonances for higher luminosity
• 6D cooling for less expensive acceleration for Neutrino Factory
July 28, 2004 K. Yonehara, NuFact'04 Osaka 23
6-Dimensional helical cooling channel
Design and feasible study of 6D HCC by using ICOOL and G4BL
July 28, 2004 K. Yonehara, NuFact'04 Osaka 24
Helix cooling channel
Bcouples with vz
Bzcouples with v
HPGH2 filled RF cavity
Helix + Solenoid coilsOne segment
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Helical Dipole Magnet
Warm spin rotatorfor AGS ring at BNL
July 28, 2004 K. Yonehara, NuFact'04 Osaka 26
Simulation results in ICOOL 1
Reference orbit
Particle orbit
z
xy
Bx, By
z
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Simulation results in ICOOL
No cooling material Multiple scattering on
No multiple scattering
transverse longitudinal 6-d
N = 500 muons
July 28, 2004 K. Yonehara, NuFact'04 Osaka 28
Possible origin of RF off-phase
July 28, 2004 K. Yonehara, NuFact'04 Osaka 29
Summary for 6D HCC• Analytical investigation by Ya S. Derbenev and
R.P. Johnson– Cooling factor: ~106
• First cooling effects were observed in ICOOL– Cooling factor: >106 without multiple scattering– : ~20 with multiple scattering– Need tilting RF cavities
• Progress on G4BL– Install ICOOL helix field and tested– Test basic parameters (compare with ICOOL): dE/ds,
Multiple scattering angle, range: a few % discrepancy