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Design Issues for a Small Muon Cooling Demonstration Ring

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Title: Design Issues for a Small Muon Cooling Demonstration Ring


1
Design Issues for a Small Muon Cooling
Demonstration Ring
  • Steve Kahn
  • Brookhaven National Lab
  • Miami Muon Collider Workshop

2
Magnetic Model for the Mini Cooling Ring
  • In this talk I will concentrate on the storage
    ring aspects of the Muon Cooling Ring. Harold
    described the cooling aspects yesterday.
  • In this study we will use the four cell model
    that resulted from the last June meeting.
  • The previous presentation in June discussed the
    six cell model. Figures from the six cell model
    are available if we need them.
  • We chose the four cell model because we thought
    that it would better accommodate a ?15 cm
    aperture than the six cell model.
  • We expect that this is true, since the ratio of
    the length of the magnet to the magnet aperture
    is greater.

3
Cell Geometry Description
Based on a Sketch from A. Garren
4
Dipole Ring Parameters
5
Using TOSCA
  • Hard edge field calculations for the Garren-Kirk
    Weak Focusing Dipole Ring have shown promising
    results.
  • It is essential to examine the ring using
    realistic fields that at least obey Maxwells
    equations.
  • Tosca can supply fields from a coil and iron
    configuration.
  • We can use the program to supply a field map that
    can be used by ICOOL and GEANT.
  • Tosca itself can also track particles through the
    magnetic field that it generates.
  • This allows us to avoid the descretization error
    that comes from field maps.

6
Tosca Model
  • For the ease of calculation we initially modeled
    the dipole magnets by its coils only. This was
    for ease of calculations and is not way we would
    actually engineer the magnet if we actually built
    it.
  • This permits the field to be calculated with
    Biot-Savart integration directly. No
    finite-element mesh is necessary if iron is not
    used.
  • There are also limitations in the Tosca tracking.
  • Tosca permits only 5000 steps. This limits the
    step size to 0.5 mm. This may limit the
    ultimate precision.

7
Tosca Modeling with Iron
  • The need for iron
  • Using an iron yoke to return the flux reduces
    stray fields in areas that we dont want field.
  • It makes the field more uniform where we want the
    field.
  • It gives more control over the quality of the
    field.
  • This requires that we actually make a finite
    element mesh to solve Poissons equations.
  • This has finally been done.
  • Hopefully this has been done in a manner that is
    flexible enough for future changes that we will
    certainly have.

8
Four Cell Ring with Iron Flux Return
9
Finding the Closed Orbit using Tosca
  • We know that the closed orbit path must be in the
    xz plane and that it must have x0 at the
    x-axis from symmetry.
  • We can launch test particles with different
    Xstart.
  • The figures on the right show Xstart vs. ?x90 and
    Xstart vs ?x'90.
  • Where ?x90 and ?x'90 are the variable differences
    after 90 advance.
  • We find that the best starting values are
  • Xstart55.03362 cm for ?x90
  • Xstart55.05569 cm for ?x'90

Xstart vs. ?x90
Xstart vs. ?x'90
10
Comparison of Closed Orbits with and without Iron
Coils Only
With Iron
Note the reverse curvature between magnets
11
By Field Along the Closed Orbit Path
Coils onlyNo Iron
Coils plus Iron
Constant Hardedge Field
  • Since coil only field has large negative field
    between the magnets, it must have larger field in
    the magnet to give the same integrated bend.

12
Using the Field Map
  • We can produce a 3D field map from TOSCA.
  • We could build a GEANT model around this field
    map.
  • I will discuss this later.
  • We have decided that we can provide a field to be
    used by ICOOL.
  • ICOOL works in a beam coordinate system.
  • We know the trajectory of the reference path in
    the global coordinate system.
  • We can calculate the field and its derivatives
    along this path.
  • We can describe the field everywhere from this.
    (This is just an application of Greens theorem)

13
Representation of the Field in a Curving
Coordinate System
  • Chun-xi Wang has a magnetic field expansion
    formulism to represent the field in curved
    (Frenet-Serret) coordinate system.
  • This formulism is available in ICOOL.
  • Up-down symmetry kills off the an terms bs is
    zero since there is no solenoid component in the
    dipole magnets.
  • The bn(s) are obtained by fitting
  • to the field in the midplane orthogonal to the
    trajectory at s
  • The field is obtained from a splining the field
    grid.

14
Fourier Expansion of bn(s)
  • The bn(s) can be expanded with a Fourier series
  • These Fourier coefficients can be fed to ICOOL to
    describe the field with the BSOL 4 option.
  • We use the bn for n0 to 5.

15
Low Order Harmonics along the Reference Path for
Field Map without Iron
16
Higher Order Harmonics along the Reference Path
without Iron
17
Low Order Field Harmonics along the Reference
Path with Iron Yokes
18
(No Transcript)
19
Filtered the Harmonic Plots Truncating the
Fourier Series at 50 terms
Note the field is plotted for One Cell, not Two
20
Filtered Higher Order Harmonics Truncated to 50
terms
21
Some Comments about the Harmonic Distributions
  • The effect of the focusing in y is contained in
    the B1(s) harmonic.
  • This contains the edge focusing used in this
    ring.
  • Notice that the B1 harmonic is larger for the no
    iron model.
  • The iron model will have a larger ?y. We will
    discuss this later.
  • The higher order harmonics show large amounts of
    high frequency noise.
  • This appears to be related to the descretization
    of the mesh.
  • It is partially, but not completely, removed by
    the truncation of the Fourier series, that will
    be used to describe each field harmonic.

22
Determining the Dynamic Aperture
  • For the x-Px (y-Py) phase space we launch n
    tracks, each track starting 1 cm apart along the
    x (y) axis.
  • The position in x-Px (y-Py) phase space is
    sampled after every cell.
  • The stable orbits form ellipses the unstable
    ones have trajectories that are lost.
  • A measure of the size of the stable phase space
    is the number of rings.

23
Horizontal Dynamic Aperture (x vs. px)Without
Iron
24
Vertical Dynamic Aperture (y vs. py)Without Iron
25
Dynamic Aperture with the Iron Yoke
y vs. Py
x vs. Px
All harmonics
No sex and above
26
Measure Dynamic ApertureCounting Rings
Old Table without Iron
New Table with Iron
27
Calculating Transfer Matrices
  • By launching particles on trajectories at small
    variations from the closed orbit in each of the
    transverse directions and observing the phase
    variables after a period we can obtain the
    associated transfer matrix.
  • Particles were launched with
  • ?x 1 mm
  • ?x' 10 mr
  • ?y 1 mm
  • ?y' 10 mr

28
90 Transfer Matrix
  • This is the transfer matrix for transversing a
    quarter turn
  • This should be compared to the 22 matrix to
    obtain the twiss variables

29
Storage Ring Parameters
  • The table below shows the Twiss Parameters as
    seen in ICOOL for both the realistic and hardedge
    models. These were calculated in a manner
    similar to those shown before
  • Both ICOOL models look reasonably comparable to
    the original SYNCH and TOSCA models.
  • This is extremely encouraging and says that the
    realistic fields do not significantly alter the
    lattice!
  • Note that realistic on this transparency is coil
    only, no Iron!

30
A Comparison of the Lattice for the Cases with
and without Iron
  • The ?x is similar between the three cases.
  • ??y is different for the case with Iron. The
    larger??y for the iron case is consistent with a
    smaller B1 that we seen for iron previously. We
    do not have enough vertical focusing.
  • Some attempt was made to scale the B1 term alone
    to see if one could reduce ?y. We could reduce it
    to 65 cm (which also reduced ?y to 101), but
    not much beyond that.

31
Field on the Vertical Symmetry Cross Plane
The figures show By on the symmetry plane for 3
cases where the horizontal extent of the magnet
aperture is varied. The vertical aperture is 30
cm. The field is shown at y0, 5, 10, 14 cm.
32
Vertical Field for the Three Cases Compared
33
Field on Mid-plane Section. Does the
half-aperture size affect the field shape?
34
Top View of Muon Cooling Ring from Blackboard
35
We Have a Possible Design of What This Ring Might
Look Like
  • It should have a double containment.
  • The inner containment would contain the beam
    channel and the interior part of the RF cavities
    and would contain the pressurized H2 gas.
  • The RF would have thin windows which could be a
    grid of Be to provide a boundary condition.
  • This containment would minimized the volume of H2
    gas required.
  • This should impress the safety committee.
  • The outer containment would be in liquid N2 at
    70K.
  • This would provide the cryogenic temperature for
    the H2.
  • The pole part of the magnet would be inside this
    containment.

36
Section View Through the Magnet Vertical Mid-plane
37
More Containment
  • The magnet flux return would be outside of the
    liquid N2 vessel.
  • It would be a small increase in the reluctance
    path to jump the 3/8 stainless steel vessel
    wall.
  • The warm copper coils could surround the flux
    return.
  • This would permit simple water cooling for the
    coils.
  • Some insulation separating the coils from the
    iron flux return might be necessary.

38
Section View Through the RF Cavity
39
Kicker Scenarios
  • A kicker to insert a muon beam with the desired
    size would require a more aggressive kicker than
    Palmer designed for the RFoFo ring. See table.
  • It would require a similar stored energy.
  • We would need a kicker rise time of 7 ns instead
    of 50 ns.
  • This has got to be expensive, even if possible!

Before Kick
After Kick
40
Proton Beam Insertion
  • Insert a proton beam and let it interact.
  • This is probably the most realistic scenario.
  • We need to know the production spectrum for 400
    MeV protons. (Mars or Geant4)
  • Will this produce sufficient ? to get the desired
    ? beam that we need.
  • We need to verify this in Geant.
  • We need to optimize where to inject protons to
    obtain the best muon beam at the desired radius
    and momentum.
  • Select negative particles to reduce background.

41
Pion or Muon Beam Insertion
  • Bring higher momentum ? or ? beam to outer edge
    of ring and let the beam loose energy by dE/dx
    loss until it is on orbit and on momentum.
  • Romulus Godang is working on some version of
    this.
  • These schemes need to be simulated to see if
    they can be made to work.

42
Field Maps
  • We have 3D field maps of the field with and
    without iron ready for explotation.
  • We have a Geant4 model of the 4 cell ring which
    will use these field maps.
  • This is necessary for more than checking ICOOL
    which we all know is right.
  • The errors in the field grow rapidly with the
    distance from the closed orbit. In the
    determination of the dynamic aperture it is not
    clear if we are measuring the breakdown in the
    parameterization of the of the field as an
    expansion around the closed orbit or the true
    aperture.
  • The errors in Geant based on a field map should
    be more uniform over the aperture.

43
Geant4 Model of Cooling Ring Using Hardedge
Fields.
Muon with Reference momentum circulating in
Storage Ring Mode.
RF cavity
Detector Planes
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