Title: Frictional Cooling MC Collaboration Meeting June 11-12/2003
1Frictional CoolingMC Collaboration MeetingJune
11-12/2003
Raphael Galea
2Frictional Cooling
Ionization stops, muon too slow
Nuclear scattering, excitation, charge exchange,
ionization
- Bring muons to a kinetic energy (T) where dE/dx
increases with T - Constant E-field applied to muons resulting in
equilibrium energy - Big issue how to maintain efficiency
- First studied by Kottmann et al., PSI
-
1/?2 from ionization
3Problems/comments
- large dE/dx _at_ low kinetic energy
- ? low average density (gas)
- Apply E ? B to get below the dE/dx peak
-
- m has the problem of Muonium formation
- s(Mm) dominates over e-stripping in all
gases except He - m- has the problem of Atomic capture
- s small below electron binding energy, but
not known - Slow muons dont go far before decaying
- d 10 cm sqrt(T) T in eV
- so extract sideways (E ? B )
4Trajectories in detailed simulation
Transverse motion
Motion controlled by B field
Fluctuations in energy results in emittance
Lorentz angle drift, with nuclear scattering
Final stages of muon trajectory in gas cell
5Results of simulations to this point
Phase rotation sections
Cooling cells
- He gas is used for m, H2 for m-. There is a
nearly uniform 5T Bz field everywhere, and Ex 5
MeV/m in gas cell region - Electronic energy loss treated as continuous,
individual nuclear scattering taken into account
since these yield large angles.
- Full MARS target simulation, optimized for low
energy muon yield 2 GeV protons on Cu/W with
proton beam transverse to solenoids (capture low
energy pion cloud).
Not to scale !!
6Summary of Simulations
- Incorporate scattering cross sections into the
cooling program - Born Approx. for Tgt2KeV
- Classical Scattering Tlt2KeV
- Include m- capture cross section using
calculations of Cohen (Phys. Rev. A. Vol 62
022512-1)
- Difference in m m- energy loss rates at dE/dx
peak - Due to extra processes charge exchange
- Barkas Effect parameterized data from Agnello et.
al. (Phys. Rev. Lett. 74 (1995) 371) - Only used for the electronic part of dE/dx
- Energy loss in thin windows
- For RARAF setup proton transmitted energy
spectrum is input from SRIM, simulating protons
through Si detector - (J.F. Ziegler http//www.srim.org)
Cooling factors of 105-107!!!
7- Assumed initial conditions
- 20nm C windows
- 700KeV protons
- 0.04atm He
- Punch through protons
- Cooled protons
TOFT0-(Tsi-TMCP)
speed
Kinetic energy
8Add windows
300nm
721KeV p
Add gas
No gas/grid/windows Extract time offsets
0.06atm
9Cool protons???
MC exp
Flat constant Background
Background exponential with mgt0
10Problems/Things to investigate
- Extraction of ms through window in gas cell
- Must be very thin to pass low energy ms
- Must be reasonably gas tight
- Can we apply high electric fields in gas cell
without breakdown (large number of free
electrons, ions) ? Plasma generation ? screening
of field. - Reacceleration bunch compression for injection
into storage ring - The m- capture cross section depends very
sensitively on kinetic energy falls off sharply
for kinetic energies greater than e- binding
energy. NO DATA simulations use theoretical
calculation -
RD with industry?
1 student 1 Postdocgroup is growing
11Lab situated at MPI-WHI in Munich
Sharper peak in Energy than peak from measuring
time.
12Future Plans
- Frictional cooling tests at MPI with 5T
Solenoid, alpha source - Study gas breakdown in high E,B fields
- RD on thin windows
- Beam tests with muons to measure ? capture cross
section - ?-H ? H? e?s
- muon initially captured in n15 orbit, then
cascades down to n1. Transition n2?n1
releases 2.2 KeV x-ray.
Si drift detector Developed my MPI HLL
13Conclusions
- No clear sign of cooling but this is expected
from lack of Magnetic field geometric MCP
acceptance alone - The Monte Carlo simulation can provide a
consistent picture under various experimental
conditions - Can use the detailed simulations to evaluate Muon
Collider based on frictional cooling performance
with more confidence.still want to demonstrate
the cooling - Work at MPI on further cooling demonstration
experiment using an existing 5T Solenoid and
develop the m- capture measurement
A lot of interesting work and results to come.