Title: High Gradient RF Cavity R
1High Gradient RF Cavity RD for Muon Cooling
Channels
- Derun Li
- Beam Electrodynamics Group
- Center for Beam Physics
- Lawrence Berkeley National Laboratory
- DOE High Energy Physics Review
- February 18-19, 2004
2Outline
- Introduction
- High Gradient RF Cavity RD Activities
- 805 MHz cavity
- 201 MHz cavity
- Be window RD
- LBNL Responsibility for MICE
- RF and coupling coil module
- Cooling channel integration
- Summary
3Introduction
- Muon beam is unstable, and has short life-time (
2 ?s at rest) - Muon beam is created with LARGE 6-D phase space
- Muon beam manipulation must be done quickly,
including cooling - Demand for highest possible RF gradient cavities
- Technical challenges
- Requirements of RF cavity for a muon cooling
channel - High cavity shunt impedance and high accelerating
gradient - Gradient at 201 MHz 17 MV/m Kilpatrick 15
MV/m - Gradient at 805 MHz 30 MV/m Kilpatrick 26
MV/m - Normal-conducting strong external magnetic
fields preclude use of superconducting RF - Practical implementation for muons RF cavity
with irises terminated by thin low-Z material
windows - Higher shunt impedance
- Lower ratio of peak surface field to accelerating
field - Independent phase control, higher transit-time
factor - We started with experimental RD at 805 MHz cavity
4805 MHz Cavity Test Setup at Lab G of FNAL
Up to 12 MW peak power
SC Solenoid
805 MHz cavity inside the solenoid
Input RF Waveguide
5Collaboration on the 805 MHz Cavity Tests at Lab
G, Fermilab
LBNL 805 MHz cavity had been under test for
nearly two years at Lab G, Fermilab
- Exceeded its design gradient of 30 MV/m at no
magnetic field and reached up to 40 MV/m - Thin Be windows with and without TiN-coated
surface have been tested versus magnetic fields
up to 4 Tesla - No surface damage was found on the Be windows
- Little multipacting was observed accelerating
gradient limit is a function of the external
magnetic field
6 201 MHz Cavity Concept
Extruding ports
Spinning of half shells using thin Cu sheets and
e-beam welding to join the shells
Water cooling channels
Cavity design accommodates different windows
7The Cavity Body Profile
Spherical section at the equator to ease
addition of ports ( 6o) Elliptical-like (two
circles) nose to reduce peak surface field
Stiffener ring
2o tilt angle
6-mm Cu sheet permits spinning technique and
mechanical tuners similar to SCRF ones
De-mountable pre-curved Be windows to terminate
RF fields at the iris
Bolted Be window
8The Cavity Parameters
- The cavity design parameters
- Frequency 201.25 MHz
- ß 0.87
- Shunt impedance (VT2/P) 22 M?/m
- Quality factor (Q0) 53,000
- Be window radius and thickness 21-cm and 0.38-mm
- Nominal parameters for cooling channel in a
neutrino factory - Up to 17 MV/m peak accelerating field
- Peak input RF power 4.6 MW per cavity (85 of
Q0, 3t filling) - Average power dissipation per cavity 8.4 kW
- Average power dissipation per Be window 100
watts
9Spinning _at_ ACME
An example of using spinning technique !
Spinning tools
Spinning a bowl
10RF CMM Measurements at LBNL
3 CMM scans per half shell conducted at 0o, 45o,
90o, respectively.
Measured frequency 196.97 MHz (simulated
frequency 197.32 MHz)
CMM scans, RF frequency and Q measurements of
half shells Cu tape for better RF contacts.
11E-Beam Welding
Stiffener ring
Preparation for e-beam welding of the stiffener
ring (left) after the e-beam Welding (above)
12Extruding Tests at JLab
Successful extruding recently!
Extruding tests on a flat Cu plate going through
e-beam joint
Possible improvement Anneal around the extruding
area or Combination between pilot hole
dimensions and lid heights,
13201 MHz cavity status
- Four half shells have been formed by spinning
- Cu stiffener rings were e-beam welded to two half
shells - The shells were mechanically cleaned at JLab
- Shells are ready for machining prior to e beam
welding of equator joint - Equator weld fixturing has been fabricated at
LBNL - Cavity nose piece rings (Univ. of Mississippi)
have been brazed at LBNL - Conceptual design of RF loop coupler
- E-beam welding of equator joint
- Extruding four ports
- Chemical cleaning and electro-polishing of the
cavity - Pre-curved Be windows
- The cavity should be ready for test in MTA at
Fermilab this fall
14Be Windows RD
- Ideal windows
- Transparent to muon beams
- Perfect electric boundary to RF field
- No detuning of cavity frequency
- Engineering solutions
- Pre-stressed flat Be (low-Z) windows
- Pre-curved Be windows
- Grids
Window profile evolutions
A pre-curved Be window 0.25 mm thick and 21 cm
in radius
15Curved S.S. Windows
Succeeded in the S.S. window with Cu frame for
805 MHz cavity
Pre-formed at room temperature by holding foil
edge then brazing the Cu frames
A finished curved S.S. window with brazed Cu
frame
16Curved Be Window
Failed in forming Be window at room temperature
The curved Be windows can be formed at higher
temperature at Brush- Wellman Company. Purchase
order has been placed and the window will be
ready soon.
The Be foil cracked during forming at room
temperature (LBNL)
A successfully formed Be foil (Feb. 5th 2004
at Brush-Wellman)
17Components for MICE
- LBNL responsibility for MICE RF and coupling
coil module - Eight 201 MHz RF cavities with Be windows for
the cooling channel (D. Li) - SC magnet (M. Green) and system integration (S.
Virostek)
Solenoid
Magnet
Cooling Channel
Envelope
Coupling coils
RF Cavity
Cavities
Raft
Absorber
Tuning
Bellows
Eight 201 MHz cavities
LH absorber
18Summary
- LBNL provides a leadership role in muon-beam RD
- RF cavity RD
- Be window RD
- SC magnets and system integration
- Expertise that LBNL provides to MC is well
recognized - 805 MHz cavity performs well at Lab G and
provides valuable operation experience and
experimental data that will benefit accelerator
community - 805 MHz cavity and the SC magnet will be moved to
MTA, FNAL - LBNL plays leading role and is responsible for
eight 201 MHz RF cavities, two SC magnets and
system integration - 201 MHz test cavity fabrication progressing well
ready for testing this fall