Title: Muon Collider
1 FERMI NATIONAL ACCELERATOR
LABORATORY US
DEPARTMENT OF ENERGY
f
Muon Collider Ionization Cooling Issues Y.
Alexahin
FNAL Accelerator Advisory Committee meeting
December 5, 2006
2Plan of the talk
- Overview of basic ideas
- low emittance MC
- 6D ionization cooling
- PIC and REMEX
- Ongoing work
- Questions to answer
- FY07 plan
- FY08 plan and beyond
- Summary
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
3Muon Collider parameters
- Low emittance option (advanced) owing to ideas
by Yaroslav Derbenev (HCC, PIC) much lower 6D
emittances seem to be feasible than previously
thought of. - High emittance option (baseline) conceptually
follows 1999 PRSTAB Muon Collider Collaboration
report
Low Emitt. High Emitt. Energy (TeV)
0.750.75 (?7098.4) Average Luminosity
(1e34/cm2/s) 2.7 1 Average bending field
(T) 10 8.33 Mean radius (m) 361.4 363.8 Number
of IPs 4 (350m/2 each) 2 (200m each) P-driver
rep.rate (Hz) 65 60 Beam-beam parameter/IP,
? 0.052 0.1 ?? (cm) 0.5 3 Bunch length (cm),
?z 0.5 2 Number of bunches/beam,
nb 10 1 Number of muons/bunch (1e11),
N? 1 12 Norm.transverse emittance (?m),
??N 2.1 13 Energy spread () 1
0.1 Norm.longitudinal emittance (m), ?N 0.35
0.14 Total RF voltage (GV) at 800MHz 406.6
?103?c 0.26?103?c RF bucket height
() 23.9 0.6 Synchrotron tune 0.723 ?103?c
0.02?103?c ? ?- in collision / proton 0.15
/2 0.15 8GeV proton beam power (MW) 1.1 0.6
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
4Low emittance option for MC
- Low emittance pros
- smaller ?? ? smaller total number of particles
nbN? ? - ? relaxed coherent stability requirements
- ? low proton driver power
- ? low neutrino radiation
- Low emittance cons
- bb-effect limits N? ? larger nb is required ?
electrostatic separation or crossing angle - smaller ?? ? strong IR chromaticity
- ? smaller ?z is required ?
- ? small ?c ?
strong arc cell chromaticity - ? higher
?p/p for the same long. emittance
problems with momentum acceptance
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
5The roadmap to low emittance
Ionization cooling very similar to SR cooling
in e-damping rings The longitudinal damping
partition number is naturally negative at p ?
lt300MeV/c
How to make it positive see next slide. The
normalized equilibrium emittance (r.m.s.)
(overestimation for H and He)
With Z4 (Be) and the natural value of glt0 (the
final cooling stage)
so that to achieve ??2?m ??lt0.2mm is required
(for ??1). Is it feasible? Another possibility
(D.Neuffer) decelerate muons to very low ?.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
6Basic 6D Cooling
- Two ways to get ggt0
- generate large dispersion and use wedge
absorbers - generate large momentum compaction ?c gt0 in a
homogeneous absorber - The first method is realized in two schemes
- "Guggenheimed" RFOFO channel (helical or spiral
with reducing radius), estimated emittances
??N5?102 ?m , ? N1mm - straight FOFO channel with tilted solenoids,
??N5?102 ?m , ? N0.5mm - The second method in
- Helical Cooling Channel (HCC) , ??N2?102 ?m ,
? N 0.3mm - HCC is the most attractive scheme, however, it
has inherent difficulties
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
7PIC REMEX
- Basic idea of the Parametric resonance Ionization
Cooling (Y. Derbenev) - form a structure with 180? phase advance/cell
- resonantly excite beta-beating with special
lenses to obtain very small ?? at absorber plates
Lattice magnets and RF cavities not shown
- Reverse EMittance EXchange
- obtain very small ?? as described above
- enhance transverse damping by making g lt0 as
large by the absolute value as possible by
reversing the wedge angle and generating maximum
dispersion at the wedges
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
8Guggenheim RFOFO structure (R.Palmer)
- modification of the initially proposed by
V.Balbekov RFOFO ring
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
9Guggenheim RFOFO cooling simulations (R.Palmer,
A.Klier)
- Adding 804 MHz section would allow to achieve
??N7.5?102 ?m , but - no matching section designed yet (may further
increase losses surpassing 50 already) - high magnetic field may drastically limit RF
voltage (would GH2 filling help?) - shown reduction in emittances include both
cooling and initial shaving - the merit factor of the 2-stage RFOFO channel
is just (N? /?6D)fin/ (N? /?6D)ini 800
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
10HCC Simulations (K.Yonehara)
- Initial proposal
- RF cavities packed inside solenoid
- additional helical coils create rotating dipole
and quadrupole fields - As R.Palmer noted the transverse field on the
coils would exceed 103T at the last stage!
6D cooling factor in the series of HCC is 50,000
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
11HCC issues
Vladimir Kashikhin found a brilliant solution
helical solenoid! Magically, the dipole and
quadrupole components have the right values,
while the orbit goes through the centers of the
coils!
- Still a number of problems to be solved
- how far down this helix can be scaled? Is helix
period of 20cm (with Bs15T) technically
feasible? - a principal solution for the RF structure which
can fit inside the HCC has yet to be found - segmented HCC with RF cavities between solenoid
sections was proposed but not demonstrated to
provide adequate cooling
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
12REMEX with HTS solenoids (R.Palmer)
It is possible to obtain ??N10 ?m in a
solenoidal focusing channel with LH2 absorber
Simulations of cooling in a channel with 6
solenoids (no RF yet) gave ??N25 ?m . To achieve
emittances for the low emittance MC option this
channel must be followed by a stronger focusing
channel with short solid absorbers.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
13Mixed Lattice for PIC/REMEX channels (A.Bogacz)
absorber
10T solenoid
quads
dipoles
This mixed quadrupole-solenoid focusing lattice
provides ?? 1.4cm at the absorber center. Large
dispersion function gives the possibility of
chromatic correction (not demonstrated yet). By
reducing dimensions and increasing field strength
one may hope to get ?? in the mm range.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
14Questions to answer
- Collider ring
- correction of chromatic perturbations
(chromatic beta-beating, nonlinear chromaticity
and momentum compaction factor) - radiation shielding necessary to protect the
superconducting magnets and detectors at specific
for the particular design beam intensity and
sizes - field quality of the magnets which have the
required aperture and field strength (magnets
being developed for the LHC luminosity upgrade is
a good first approximation) - dynamic aperture with realistic field and
alignment errors - beam-beam effects
- suppression of coherent instabilities at given
bunch intensity, length, momentum compaction and
lattice functions. - 6D cooling channel
- scalability of the proposed by V.Kashikhin HCC
technical solution to the helix period of 20cm
(with Bs15T) - principal solution for the RF structure which
can fit inside the HCC
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
15Questions to answer
- 6D cooling channel (continued)
- ability of gas-filled cavities to support
high-gradient RF field in the presence of
ionizing beam - end-to-end simulation of the "Guggenheimed"
RFOFO channel to prove its competitiveness - proof-of-principle study of the FOFO channel
with tilted solenoids followed by cooling
simulations. - PIC / REMEX
- optics design for different stages (solenoidal
vs quadrupole and mixed focusing) - compensation of chromatic and spherical
aberrations - space charge effects
- Proton driver, Pion production, Muon RF capture,
Bunch coalescing, Acceleration - There is little doubt in feasibility of these
elements of the complex, - there are a number of options for each of them
which should be studied and compared, - but only after the principal solution for the
collider ring and the cooling channel is chosen.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
16FY07 plan
- Physics analysis and computer simulations of
different schemes for the basic 6D cooling
channel and PIC/REMEX channel. - Side-by-side comparison of the obtained results
with the aim of choosing the 6D cooling channel
baseline scheme compatible with the chosen
collider option. - Analysis of implications of different options
for the muon collider (low emittance vs. high
emittance, electrostatic separation in one ring
vs. double ring) resulting in a presumably
optimal choice of parameters. - Collider ring optics design for the chosen
option. - Preliminary analysis of the technical
feasibility and physical validity of the proposed
design (momentum acceptance, medium-term dynamic
aperture, coherent stability). - Formulating requirements to the proton driver
and other systems of the complex. - Consistent scheme(s) of the muon collider
complex.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
17FY08 plan and beyond
- Upgrade of the muon production and RF capture
systems design - Analysis, selection and preliminary design of
muon acceleration systems (RLA vs. FFAG for the
first stage, RLA vs. fast ramping synchrotrons
for subsequent stages) - Extensive simulation studies and design
optimization of all essential systems of the
collider complex. - Analysis of radiological issues for appropriate
choice of the collider orientation and depth - Cost estimates
- Draft conceptual design report
- Optimistically, the conceptual design will be
finished in 2009
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
18Summary
- The Muon Collider for c.o.m. energy 1.5-2TeV
seems doable with present day technology and can
be accomodated on the Fermilab site - Extensive design and simulation work is
necessary for all parts of the complex with the
1999 PRSTAB Muon Collider Collaboration report
being a good first approximation
- The requested funding for this work seems
adequate taking into account heavy contribution
from other labs especially BNL, JLab and MuonsInc.
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
19Backup slides Emittance diagram
Emittance evolution in R.Palmers muon cooling
scheme
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
20Backup slides straight FOFO channel (Y.Alexahin)
tilted solenoids
straight solenoids
RF cavities
y/L
z/L
x/L
Closed orbit at ? 0.01 (dispersion follows the
same pattern)
- Phase advance over the 4-solenoid period is
above 2? ? resonant dispersion generation - Cooling by combination of GH2 and Li wedges in
high-dispersion locations for damping repartition - The scheme requires RF cavities operation in
high magnetic field (hopefully GH2 will help)
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006
21Backup slides collider ring optics
- Two optics designs so far
- prepared for 1999 PRSTAB Muon Collider
Collaboration report by Carol Johnstone et al.
? 3mm, peak ?max1.5 ?105m, ?c - 9.2?10-5.
Requires further work on chromatic correction,
the momentum acceptance is just (- 1.2?10-4,
1.6?10-4). - more conventional design by A.Bogacz ? 1cm,
peak ?max4.8 ?103m (but with the distance from
IP to the first quad just 2m), ?c 2?10-4
IR and a few arc cells in the design by A.Bogacz
Muon Collider Ionization Cooling Issues - Y.
Alexahin, FNAL December 5,
2006