h. padamsee outline - cern · h. padamsee. outline • general comments on sc cavity design choices...
TRANSCRIPT
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H. Padamsee
Outline
• General comments on SC cavity design choices for accelerators• Basics of SRF cavities
– Structure Types• Basic RF Cavity Design Principles• Figures of Merit
– Gradient, Losses, Q, Shunt Impedance, Peak Fields…• Miracle of Superconductivity• SC/NC comparison for CW application• Design Aspects for Multicells• Mechanical Aspects of Cavity Design• Cavity Performance Aspects/Cavity Technology
– Multipacting, Breakdown (Quench), Field Emission, Q-Slope• Ultimate gradient possibilities• Fundamental critical fields• Wide Range of Applications
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H. Padamsee
Overall Approach
• General introduction to many workshop topics– Focus on high velocity structures – Separate tutorials on high β and low β cavity
design aspects• Important Topics not covered
– Input couplers– HOM couplers– Tuners, Vibrations, Microphonics– Cryomodules
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H. PadamseeRF Cavities: Energy for Accelerators
ILC 16,000 cavities!
Apply concepts to two examples: Storage Ring, Linear Collider
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H. PadamseeGeneral Accelerator Requirements That DriveSC Cavity Design Choices
VoltageStorage Rings
CESR-III: 7 MV, KEK-B HER: 14 MV, LEP-II: 3 GV
Duty Factor (RF on time x Repetition Rate)Storage Rings: CW
Proton Linacs: < 10%Linear Collider: 0.01 - 1%
Linear Collider: 500 - 1000 GV
Beam Current, Ave. Beam PowerStorage Rings: amp, MW
Proton Linacs: 10 - 100 mA, 1- 10 MW
Proton Linac: 1 GV SNS, ESS
Linear Collider: few ma, 10 MW
Linac-Based FEL or ERL : 500 MeV - 5 GeV
Linac-Based FEL or ERL CW
Linac-Based FEL or ERL 50 μA - 100 mA
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Cavity Design Choices
• Main Choices – RF Frequency– Operating Gradient– Operating Temperature– Number of Cells– Cell Shapes– Beam Aperture
• Optimize for Capital + Operating Cost • Best Cavity/Accelerator Performance for Least Risk• Optimizations Involve Many Trade-offs• Discuss parameters/dependencies
– But not the trade-offs
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H. PadamseeBasics for Radiofrequency Cavities
E
TM010 mode
•Add beam tube for charge to enter and exit
H
EzR
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RF accelerator cavitiesFields and Currents
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Medium and High Velocity Structures β = v/c = 0.5 -> 1
Single Cell
Multi-Cell Cavity
Squeezed Cells for v/c = 0.5
Basic Principle, v/c = 1
λ/2
βλ/2
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1300 MHz Structures for Accelerating Particles at v ~ c
Structures for Particles at v < c (SNS)For protons at 1 ~ GeV
TESLA-shape
(DESY, TTF)
Low-Loss shape (Jlab, KEK…)
Re-entrant shape (Cornell)
Structure Examples
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H. PadamseeLow Velocity Structures, β = v/c = 0.01 -> 0.2
Basic Principle
Quarter Wave
Half-Wave SpokeSplit -Ring
Inter-Digital
Niobium
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H. PadamseeLow-Velocity Structures for Heavy Ions
β = v/c : 0.28 -0.62
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Crab Cavities (Deflecting mode TM110)
• KEK-B• Possibly LHC-upgrade• Possibly Ultra-fast X-ray source
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• Accelerating voltage then is:
• Accelerating field is:
• For maximum acceleration need
so that the field always points in the same direction as the bunch traverses the cavity
Figures of MeritAccelerating Voltage/Field
(v = c Particles)
d
2Trf
Enter Exit
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Figures of Merit for SC Cavity
• Accelerating Field and Q: Eacc, Q• Stored Energy, Geometry Factor• Peak Electric and Magnetic Field Ratios
– Epk/Eacc, Hpk/Eacc
• Shunt Impedance, Geometric Shunt Impedance: Ra, Ra/Q
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H. PadamseeSingle Cell CavitiesKEK-B Cavity
Electric field high at iris
Magnetic field high at equator
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• For Eacc important parameter is Epk/Eacc,– Typically 2 - 2.6
• Make as small as possible, to avoid problems with field emission - more later.
• Equally important is Hpk/Eacc, to maintain SC – Typically 40 - 50 Oe/MV/m
• Hpk/Eacc can lead to premature quench problems (thermal breakdown).
• Ratios increase significantly when beam tubes are added to the cavity or when aperture is made larger.
Figures of MeritPeak Fields
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Hpk
Peak fields for low beta cavities are higherTypical
Epk/Eacc = 4 - 6
Hpk/Eacc = 60 - 200 Oe/MV/m
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H. PadamseeFigures of Merit
Dissipated Power, Stored Energy, Cavity Quality (Q)
•Surface currents (∝ H) result in dissipation proportional to the surfaceresistance (Rs):
•Stored energy is:
•Dissipation in the cavity wall given bysurface integral:
UTrf Pc
= 2 π•Define Quality (Q) as
which is ~ 2 π number of cycles it takes to dissipate the energy stored in the cavity Easy way to measure Q• Qnc ≈ 104, Qsc ≈ 1010
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Galileo, 1600 AD
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H. Padamsee
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H. Padamsee
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H. PadamseeFigures of Merit
Shunt Impedance (Ra)
•Ra/Q only depends on the cavity geometry Cavity design impacts mode excitation
• Shunt impedance (Ra) determines how much acceleration one gets for a given dissipation (analogous to Ohm’s Law)
Another important figure of merit is
To maximize acceleration, must maximize shunt impedance.
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H. PadamseeEvaluation - Analytic Expressions
For Cu: Rs = 10 mohm Q = 25,700, Ra = 5 MohmFor Nb: Rs = 10 nohm Q = 25,700,000,000, Ra = 5 Tohm!
1.5 GHz pillbox cavity, R = 7.7 cm, d = 10 cm
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H. PadamseeReal Cavities
Codes
• Adding beam tubes reduces Ra/Q by about x2 => for Cu cavities use a small beam hole.
• Peak fields also increase. – Can be a problem for high gradient cavities
• Analytic calculations are no longer possible, especially if cavity shape is changed to optimize peak fields.
• Use numerical codes.• E.g., MAFIA, MicrowaveStudio, SuperLans, CLANS,
Omega3P….
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270 ohmΩ88 ohm/cell
2.552 Oe/MV/m
Cornell SC 500 MHz
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• Example: Assume we make this cavity out of copper
• Want to operate CW at 500 MHz and
• 1 MV (3 MV/m)
• Rs = 6 mohm
Q = 45,000Ra = 4 Mohm
Pdiss = 250 kWThis would result in a overheating of copper cell. Water-cooled copper cavities at this frequency can dissipate about 40 kW.
(CW) copper cavity design is primarily driven by the requirement that losses must be kept small.
Copper Cavity ExampleCW and Low Gradient
R/Q = 89 Ohm
Rs = √ (π f μ0 ρ)f = RF frequencyρ = DC resistivity
μ0 = permeability of free space
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* DF
Want high Vacc
Depends only on geometry.Maximize this for copper cavities
Determined by the materialbeing used
If dissipation is too large,must reduce duty factor
Minimizing Losses
Pdiss =Vacc
2
Ra
Vacc2
Ra/Q * Q=* DF
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H. PadamseeOptimizing CW Copper CavitiesHigh Current Application
• Use small beam tubes• Use reentrant design to reduce
surface magnetic currents.• Ra/Q = 265 Ohm• Pdiss = 80 kW @ 3 MV/m• Still have to reduce voltage to
0.7 MV.•
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H. PadamseeSuperconductivity
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H. Padamsee
Elementary Solid State : Electrons in Solids
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H. PadamseeElectron Energy Levels
Fermi Level
Empty Levels
Occupied Levels
Normal conductor
T = 0 K
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Electron-Phonon Interaction
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Superconductivity
Fermi Level
Empty Levels
Occupied Levels
Gap
Normal conductor Superconductor (electrons form Cooper pairs)T = 0 K
For T > 0K, have some excitation of “normal” electrons
Two Fluid Model
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Simplified Explanation for Zero Resistance
• NC– Resistance to flow of electric current– Free electrons scatter off impurities, lattice vibrations
(phonons)• SC
– Cooper pairs carry all the current– Cooper pairs do not scatter off impurities due to their
coherent state – Some pairs are broken at T>0K due to phonon interaction
• But supercurrent component has zero resistance
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Superconductors: RF Resistance
• DC resistance is zero because NC electrons are shorted out by SC ones.
• RF resistance small but finite because Cooper pairs have inertia nc electrons “see” an electric field. More resistance the more NC electrons
are excitedMore resistance the more the sc pairs are jiggled around
1.5 GHz
Residual resistance
Compare with Cu: Rs ~ 10 mΩ
Choose Nb becausea) Has high Tc, Hc low Rsb) Easy to fabricate
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for T < 0.5Tc
London penetration depth Coherence length of Cooper
pairs Fermi velocity
Energy gap electron mean free path
Tc = SC transition temperature
R s = A( λL, ξ0 , l) f 2 e (- Δ 0 /kT)
λL
ξ0
v F
Δ 0
l
R bcs = 3x 10 -4 [ f (GHz)1.5
]2
( 1T
) e -(17.67/T)
Low Field Frequency and Temperature Dependence of Rs
Good fitting function
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Cavity Q0
• 120 C bake• Lowers electron mean free path and increases BCS Q
Kneisel et alCiovati et al
1.8 K
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Superconducting Cavity
• Recalculate Pdiss with SC Nb at 4.2 K, 1 MV, and 500 MHz.
Q = 2 x 109 (Rs ≈ 15 nΩ) Ra= 5.3 x 1011
Pdiss= 1.9 W!Pac= 660 W = AC power (Frig. efficiency = 1/350)Include cryostat losses, transfer lines, etc.Pacincreases, but is still 10-100 times less than that of Cu cavities.
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H. PadamseeA challenge of the SC option is cryogenics
Refrigerator efficiencies are low
And one has to add other heat contributions from conduction, radiation, helium distribution.
Carnot efficiency of frigand technical efficiency of frig machinery
ηCarnot = 4.5300 - 4.5
= 0.015
ηtechnical = 0.20ηtotal = 0.003 = 1/333
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H. PadamseeSRF Requirements & Limitations
• Cryogenic system.
Hi Tech:Ultra-clean preparation and
assembly required
Max Eacc = 50 MV/mMore Later
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SC Advantages
• Power consumption is much less operating cost savings, better conversion of ac power to beam power.
• CW operation at higher gradient possible Less klystron power required capital cost saving
• Need fewer cavities for CW operation Less beam disruption
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Copper cavity shape
Design Comparison
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CW RF Cavities for Storage Rings
Copper Cavity: PEP-II
Superconducting Cavity: CESR-III
Fundamental differences due to difference in wall losses
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(Some) Further SC Advantages
• Freedom to adapt design better to the accelerator requirements allows, for example, the beam-tube size to be increased:– Reduces the interaction of the beam
with the cavity (scales as size3) The beam quality is better preserved (important for, e.g., FELs).
– HOMs are removed more easily better beam stability more current accelerated (important for, e.g., B-factories)
– Reduce the amount of beam scraping less activation in, e.g., proton
machines (important for, e.g., SNS, Neutrino factory)
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H. PadamseeAdditional Design Aspects for Multi-cell Cavities
Standing Wave Mode
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H. Padamsee
9-cell cavity
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H. PadamseeDispersion Relation
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H. PadamseeCircuit Model of MultiCells
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H. Padamsee
Mode spacing increases with stronger cell to cell coupling kMode spacing decreases with increasing number of cells N
Solve the circuit equations for mode frequenciesDispersion Relation
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H. Padamsee
Field Flatness
• Stronger cell-to-cell coupling (k) and smaller number of cells N means – Field flatness is less
sensitive to mechanical differences between cells
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H. Padamsee
Tuning for Right Frequency and Field Profile
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H. PadamseeIn Addition to EM PropertiesMechanical Properties Are Also
Important to Cavity Design
• Cavity should not collapse or deform too much under atmospheric load
• Shape– avoid flat regions– Elliptical profile is stronger
• Choose sufficient wall thickness• Use tuner to bring to right frequency
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H. Padamsee
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H. PadamseeDetuning, Problem for pulsed operation as for TESLA
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H. Padamsee
11
10
9
80 25 50 MV/m
Accelerating Field
Residual losses
Multipacting
Field emission
Thermal breakdown
Fundamental Quench
Ideal
10
10
10
10
Q
Grain boundaries
Oxide interface
Cavity Performance Characterization
Most Important : Q vs E curve
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H. Padamsee
Critical Fields
• Superconductors only remain in the superconducting state if the applied field is less than the critical magnetic field Hc (2000 Oe for Nb for DC)
• But! Phase transition requires some time (1 μs?) to nucleate sc-nc transition.
• For RF can exceed Hc up to the superheating field.
For typical v = c cavities this is achieved at an accelerating field of Eacc ≈ 50 MV/m.
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H. Padamsee
Hc
DC Critical Magnetic fields
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H. PadamseeMeissner Effect
• Magnetic fields are screened by surface currents in the SC perfect diamagnetism
• SC goes normal conducting when the energy needed for shielding exceeds that gained by being superconducting.
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H. Padamsee
Critical RF Magnetic Field
• What is the relationship between the RF critical magnetic field and the familiar DC critical magnetic fields?
• Is Hrf– Hc1, Hc, Hsh?– How does it depend on temperature?– How does it depend on
• Ginzburg-Landau parameter κ = λ/ξ?– Nb: κ ~1, Νb3Sn: κ ~ 20..
DC Critical Fields
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H. PadamseeCornell Experimental Status (1996)
Measured RF Critical Field for : Nb3Sn Using High Pulse Power(Calibrated results with Nb)
Nb3Sn Hc1
Best single cell Nb cavity result
Best single cell Nb3Sn cavity result
Cavities Prepared by BCPQ-slope limit?
G-L TheoryPrediction
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H. PadamseeTheoretical RF Electric Field
• No known theoretical limit• In SC test cavities, SC survives up to
– Epk = Pulsed 220 MV/m– 145 MV/m CW over cm2 area
• Single cell 1300 MHz accelerator cavity to Epk = 120 MV/m, CW (55 x 2.2)
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H. PadamseeEvolution of Cavity Gradients (1970 – 2009)
And SRF Technology Over 4 DecadesSteady progress in Gradients due to basic understanding of limiting phenomena and invention of effective cures
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H. PadamseeThermometry Has Been the Key
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H. Padamsee
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H. Padamsee
11
10
9
80 25 50 MV/m
Accelerating Field
Residual losses
Multipacting
Field emission
Thermal breakdown
Quench
Ideal
10
10
10
10
Q
Grain boundaries
Oxide interface
Cavity Performance Characterization
Most Important : Q vs E curve
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H. Padamsee
Multipacting
Thermal breakdown
Field Emission
Stone Age
RRR = 250
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H. Padamsee
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H. Padamsee
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H. Padamsee
1 4log(ΔT [mK])
Heating at sub-mm size defects leads to quench of superconductivity
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H. Padamsee
Cu
0.2 mm Ta defect, 15 MV/m
50 μm, with S, Ca, Cl, and K, 11 MV/m
A chemical stain 440 μm in diameter. K, Cl, and P, 3. 4 MV/m
500 x 200 microns pit
Sub-mm Nb welding ball, avoidable
50 micron Cu particle fell into cavity
Museum of Defects Causing Quench
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H. PadamseeImprove Bulk Thermal Conductivity (and RRR) by raising purity
to avoid Quench
RRR: Residual resistance ratio = resistivity at room temperature divided by the resistivity at 4.2 K (in the normal conducting state!). κT scales ≈ linearly with RRR.
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H. Padamsee
Niobium Purification
Interstitial O, N and C are the major impurities limiting Nb RRR
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H. PadamseeTypical Progress in RRR (at Tokyo Denkai)
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H. PadamseeField Emission
•Acceleration of electrons, heating wall, X-rays
•Impacting electrons produce line heating detected by thermometry.
1200 mK0
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H. PadamseeMuseum of Known Field Emitters 0.5 to 10 microns
Note the sharp features on the Particles.
(a) Sub-micron field emitting particles found on sample prepared with 9-cell cavity
(b) Al particle found at a field emission site in the dc field emission scanning apparatus and subsequently analyzed with the SEM
(c) Field emitting particle found with thermometry followed by dissection of a 1.5 GHz cavity. Carbon, oxygen, iron, chromium, and nickel were among the foreign elements detected
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H. Padamsee
TTF-I (2001)
Field Emission Tamed, HPR
CEBAF (1995)
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H. Padamsee100 atm jet water rinsing
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H. PadamseeHPR and Assembly at Cornell in Class 100 Clean Room < 100 particles/cu.ft > 1 μm
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H. Padamsee
All RF Processing of Field Emission Means to Burn off Remaining Electron Emitters by SparkingRF Processing Can be Enhanced With High Power RF
1 MW, 200 μsec pulses
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H. PadamseeCW Low Power RF Processing of Carbon Emitter Planted in 6
GHz Cavity
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H. PadamseePush for High Gradients : Cornell, FNAL, DESY Collaboration
Gradients > 25 MV/m in Three 5-cell 1300 MHz Cavities
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H. Padamsee
Best 12 9-cells
TTF-I (2001)
BCP treated
TTF-2 (now FLASH) 2008
EP and bake
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H. Padamsee
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H. Padamsee
Best Performance Results
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H. Padamsee
• Yield at 35 MV/m is low• Spread is high:
– Quench– Field emission
• Best 9-cell CavitiesAbout one dozen
Outstanding Issues for Highest Gradient Applications: e.g. ILC
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H. Padamsee
Yield Must Rise
TTF- 2001 EraBCP TreatmentHigh Field Q-slopeLimit
FLASH/TTF-II
2008 Era
Electropolishing and Baking
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H. Padamsee
9-cell DESY Cavities Prepared by EP and Baking
Field Emission Limited Cavities
0
2
4
6
8
10
12
14
16
18
5--10 10 - -15 15-20 20-25 25-30 30-35 35-40 40-45
Eacc (MV/m)
Series1FE Limited
Quench Limited
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H. PadamseeImpact of SRF on Accelerators for Science
Existing and Future Applications
• Low energy nuclear physics, for nuclear shape, spin, vibration…– Heavy ion linacs
• Medium energy nuclear physics, structure of nucleus, quark-gluon physics
– Recirculating linac• Nuclear astrophysics, for understanding the creation of elements
– Facility for rare isotope beams (FRIB) • X-Ray Light Sources for life science, materials science &
engineering– Storage rings, free electron lasers, energy recovery linacs
• Spallation neutron source for materials science and engineering, life science, biotechnology, condensed matter physics, chemistry
– High intensity proton linac• Future High Intensity Proton Sources for
– Nuclear waste transmutation, energy amplifier, power generation from Thorium
• High energy physics for fundamental nature of matter, space-time– Electron-positron storage ring colliders, linear collider, proton linacs for
neutrinos
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H. PadamseeSRF Has Become a Core Technology Worldwide for a Variety of Accelerators
Total > 7 GV installed (>3 GV still in operation: CEBAF, SNS, FLASH)LEP-II was 3.5 GV, later de-commissioned for LHC
• HEP– Now: LHC, CESR-TA, KEK-B, Beijing Tau-charm Factory– Future: LHC-crab-crossing, ILC, Project X, CERN-SPL, Neutrino Factory, JPARC-
Upgrade (neutrino beam line) Muon Collider• NP
– Low Energy– Now: ATLAS (Argonne), ALPI (INFN Legnaro Italy) , ISAC-II (TRIUMF), IUAC (Delhi)– Medium Energy Nuclear-Astrophysics– Now: CEBAF, 12GeV Upgrade, – Nuclear Astrophysics– Future: FRIB (MSU), ISAC-II (TRIUMF), Spiral-2, CERN ISOLDE Upgrade, Eurisol,
RHIC-II, eRHIC, ELIC• BES X-rays
– Now: FLASH, X-FEL, CHESS, Canadian Light Source, DIAMOND, SOLEIL,Taiwan Light Source, Beijing Light Source (Tau-charm Factory), Shangai Light Source, Jlab-FEL/ERL, Rossendorf-FEL
– Future: NSLS-II, Cornell-ERL, KEK-ERL, BESSY-ERL, WIFEL (Wisconsin), ARC-EN-CIEL, Pohang Light Source, Peking University,…
• BES: Neutron Sources– SNS, SNS upgrade,– Future: ESS (Sweden)
• Other High Intensity Proton Sources for – INFN, KAERI, Indian Laboratories at Indore, Mumbai and Kolkata