Frictional Cooling MC Collaboration Meeting June 11-12/2003 - PowerPoint PPT Presentation

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Frictional Cooling MC Collaboration Meeting June 11-12/2003

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... n=15 orbit, then cascades down to n=1. Transition n=2 n=1 releases 2.2 KeV x-ray. ... can provide a consistent picture under various experimental conditions ... – PowerPoint PPT presentation

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Title: Frictional Cooling MC Collaboration Meeting June 11-12/2003


1
Frictional CoolingMC Collaboration MeetingJune
11-12/2003
Raphael Galea
2
Frictional 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
3
Problems/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 )

4
Trajectories 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
5
Results 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 !!
6
Summary 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
  1. Punch through protons
  2. Cooled protons

TOFT0-(Tsi-TMCP)
speed
Kinetic energy
8
Add windows
300nm
721KeV p
Add gas
No gas/grid/windows Extract time offsets
0.06atm
9
Cool protons???
MC exp
Flat constant Background
Background exponential with mgt0
10
Problems/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
11
Lab situated at MPI-WHI in Munich
Sharper peak in Energy than peak from measuring
time.
12
Future 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
13
Conclusions
  • 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.
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