Title: The Neutrino Factory and Muon Collider Collaboration
1The Neutrino Factory and Muon Collider
Collaboration
- RD Program
- and
- Participation in the IDS
2NFMCC Mission
To study and develop the theoretical tools, the
software simulation tools, and to carry out RD
on the hardware that is unique to the design of
Neutrino Factories and Muon Colliders
- Extensive experimental program to verify the
theoretical and simulation predictions
3Current Organization
4Collaborating Institutions
US
International
National Labs Argonne BNL Fermilab LBNL Oak
Ridge Thomas Jefferson
Universities Columbia Cornell IIT Indiana Mic
higan State Northern Illinois Princeton UC-Berkele
y UC-Davis UC-Los Angeles UC-Riverside University
of Chicago
National Labs Budker DESY INFN JINR,
Dubna KEK RAL TRIUMF
Universities Karlsruhe Imperial
College Lancaster Osaka Oxford Pohang Tel Aviv
Corporate Partners Muons Inc. Tech-X Corporation
5Core Program
Targetry RD Mercury Intense Target Experiment
(MERIT) Spokesperson Kirk
McDonald Project Manager Harold
Kirk Ionization Cooling RD MuCool and
MICE MuCool Spokesperson Alan Bross US
MICE Leader Dan Kaplan Simulations
Theory Coordinator Rick Fernow Muon Collider
Task Force Being organized now _at_ Fermilab
6Hardware Activities
7MuCool
8MuCool Program
- Mission
- Design, prototype and test all cooling channel
components (SFOFO) - 201 MHz RF Cavities, absorbers, SC solenoids
- Support MICE (cooling demonstration experiment)
- Perform high beam-power engineering test of
cooling section components
- Currently consists of 9 institutions from the US
and Japan
RF Development ANL Fermilab IIT JLAB LBNL Mississi
ppi
Absorber RD Fermilab IIT KEK NIU Mississippi Osak
a
Solenoids LBNL Mississippi
9- RD Focus of MuCool
- Component testing Fermilab
- RF Cavities
- High RF-power Testing
- Absorbers
- Technology tests
- High power-load testing
- With beam
- Magnets
10MuCool Test Area
- Facility to test all components of cooling
channel (not a test of ionization cooling) - At high beam power
- Designed to accommodate full Linac Beam
- 1.6 X 1013 p/pulse _at_15 Hz
- 2.4 X 1014 p/s
- 600 W into 35 cm LH2 absorber _at_ 400 MeV
- RF power from Linac (201 and 805 MHz test stands)
- Waveguides pipe power to MTA
11MTA
- The MTA is the focus of our Activities
- RF testing (805 and 201 MHz)
- High pressure H2 gas-filled RF
- LH2 Absorber tests
- Two parts of infrastructure yet to be completed
- Cryo Plant
- Beam Line
12MTA Hall
13MTA Hall Instrumentation
Chipmunk
Plastic Scintillator
805
CsI
201
Magnet
14Phase I of RF Cavity Closed Cell Magnetic Field
Studies (805 MHz)
- Data seem to follow universal curve
- Max stable gradient degrades quickly with B field
- Sparking limits max gradient
- Copper surfaces the problem
Gradient in MV/m
Peak Magnetic Field in T at the Window
15Phase II of 805 MHz studies
- Study breakdown and dark current characteristics
as function of gradient and applied B field in
Pillbox cavity - Curved Be window Test
- TiN coated
- Cavity has been conditioned to 32MV/m without B
field - Measurements at 2.5T
- Stable gradient limited lt 17MV/m
- Button test
- Evaluate various materials and coatings
- TiN, ALD
- W,Cu,Mo,SS,..
- Quick Change over
16New 805 MHz RF data
- Recent repeat of Max Grad with B
- No conditioning observed
17805 MHz Imaging
18RF RD 201 MHz Cavity Design
- The 201 MHz Cavity is now operating
- Reached 16MV/m at B0 (design gradient!)
19X-ray rates From 201 MHz Cavity
B0
20201 Program
- Conditioning 201 Cavity through multipacting
- Observed at very low field
- This is now ready to begin
- Configuration shown to right
- Allows for approximately 2T on axis at window
facing magnet - Magnet operating in solenoid mode at 5T (max)
- Field falls off rapidly in both r and z
- We have also full azimuthal coverage to measure
x-ray rates - Thin and totally absorbing plastic scintillator
counters - Spectroscopy - NaI
21High Pressure H2 Filled Cavity WorkMuons Inc
- High Pressure Test Cell
- Study breakdown properties of materials in H2
- Just finished run in B field
- No degradation in M.S.G. up to 3.5T
22Absorber Design Issues
- 2D Transverse Cooling
- and
- Figure of merit MLRdEm/ds
- M2 (4D cooling) for different absorbers
H2 is clearly Best - Neglecting Engineering
Issues Windows, Safety
23Convective Absorber Activities
- First Round of studies of the KEK absorber
performed in the MTA - GHe used to input power
24Convective Absorber Activities II
25Convective Absorber Activities III
- Next Round of tests will use a modified absorber
- Test
- Electrical Heater
- New Temperature sensors
- LH liquid level sensor
Instrumentation will be used in MICE
Absorber Body being modified in Lab 6 at Fermilab
26LiH Test Program
- Produce encapsulating cast (not pressed) samples
- Small disk (5-10 cm) for intense radiation
exposure - Look at Material stability primarily
- Temperature Profile
- Large disk (30 cm) for detailed thermal
conductivity studies - External Cooling Internal Heating
- Potential absorber for MICE Phase I
- Non-instrumented, no cooling
27MICE
28Muon Ionization Cooling Experiment MICE
Beam Diffuser
29US MICE
- Tracker Module
- Solenoids
- Fiber ribbons
- VLPC System
- VLPCs, Cryostats and cryo-support equipment,
AFEIIt (front-end readout board), VME memory
modules, power supplies, cables, etc - Absorber Focus Coil Module
- LH2 and vacuum safety windows
- Fabrication and QC
- RF Module
- Coupling Coils
- RF Cavities
- Particle ID
- Upstream Cerenkov
30MuCool and MICE
- MuCool Collaboration interface to MICE
- Design Optimization/develop of Study II cooling
channel - Simulations
- Detailed engineering
- Full component design
- Systems integration
- Safety
- RF cavity development, fabrication, and test
- 201 MHz operation in B field
- Absorber development, fabrication, and test
- Ends with KEK prototype tests
- MuCool will prototype and test cooling hardware
including MICE pieces for which the collaboration
is responsible
31MERIT
32MERIT Mercury Intense Target
- Test of Hg-Jet target in magnetic field (15T)
- Submitted to CERN April, 2004 (approved April
2005) - Located in TT2A tunnel to ISR, in nTOF beam line
- First beam Summer, 2007
- Test 50 Hz operation at 24 GeV Þ 4 MW
33(No Transcript)
34Movies of viewport 2, SMD camera, 0.1 ms/frame
ORNL 2006 Nov 28 runs 10 m/s
ORNL 2006 Nov 29 run, uprighted image
Nozzle C 20 m/s
nozzle A before reaming
nozzle A after reaming
35Merit Instrumentation
- Developed Full Mars Simulation
- Particle fluxes, energy deposition, absorbed dose
and residual activity in the experimental hall - Absorbed dose and activation of mercury system
- Secondary particle production
- Study/define diagnostics needed for experiment
- Radiation load in components
- Radiation shielding
- Particle production in secondary beam
36Design and Simulation
37Design and Simulation -Some Specific Areas of
Study
m Capture/Bunch/Rotation/Cool
Linear nonscaling FFAG
? Energy
? Time
Two fixed point acceleration half synchrotron
oscillation path between fixed points
H2 filled cavities
38Design and Simulation - Acceleration
39NF Detector - Design and Simulation
- Looking at Totally-Active Sampling Detector
- Scintillator Based
- Magnetized
- 0.5T
40Totally Active Segmented Detector
Simulation of a Totally Active Scintillating
Detector (TASD) using Nona and Minerna concepts
with Geant4
- 3333 Modules (X and Y plane)
- Each plane contains 1000 slabs
- Total 6.7M channels
- Momenta between 100 MeV/c to 15 GeV/c
- Magnetic field considered 0.5 T
- Reconstructed position resolution 4.5 mm
41TASD Performance
Muon reconstructed efficiency
Muon charge mis-ID rate
42Large Magnetic Volumes
Possible magnet schemes
- Warm coil magnets
- Total cost 5m x 10 50M (.1-.2T)
- Problem operational cost (gt13M/year with
factor of 3 uncertainty)
- Superconducting coil magnet cost extrapolation
formulas - Use stored energy 14M/module
- Use magnetic volume 60M/module
- GEM magnet extrapolation 69 M/module
x10 modules!
43Large Magnetic Volumes II
- Cost Driver is not stored energy Vacuum Loading
for vacuum insulated cryostats (A. Herve, CERN) - P0 0.33 S0.8 (Price of equivalent zero energy)
- P P0 0.17 E0.7 (Total Price of magnet)
- S Surface of the cryostat
- V Mean magnetized volume
- E Stored energy
- Must get rid of vacuum loading
- Foam Insulated
- High Tc SC
- SC Pipe
SC Pipe?
44Back to the Future - VLHC
3 Æ
SC Transmission Line
45Magnetic cavern design
1 m iron wall thickness. 2.4 T peak field in
the iron.
46B in XZ cross-section
Better field uniformity with iron in the end
sections
47Parameters
100 kA op demonstrated
1000/m Þ 50M
48US NFMCC 5 Year Budget Plan
Base Program funds remain as in FY06 BNL
(0.9M) Fermilab (0.6M) LBNL (0.3M)
For FY07 - DOE has asked what we would do with
additional funds if a 10 or 20 budget
increase were forthcoming. This is on the total
including base (3.6M)
Note The Advanced Accelerator RD Sub-panel
recommended that a doubling of our funds would
be appropriate. Our Muon Technical Advisory
Council recommended a similar scenario
49NFMCC Participation in the IDS
- Areas of Interest
- Proton Driver
- BNL, Fermilab
- Targetry
- BNL, Fermilab, Princeton
- Capture and phase rotation
- Fermilab
- Cooling
- BNL, Fermilab, IIT, LBNL, UCLA, UC Riverside
- Acceleration
- BNL, Fermilab, TJNL
- Detector Design and Simulation
- Fermilab, IIT, University of Mississippi
- Our level of effort, however, will depend on our
budget in the out years. But there is some
reason to be optimistic