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Chromatic Correction Basics 3 Montague chromatic functions : A x,y are created first, and then converted into B x,y as phase advances x,y grow K 1, K 2 are normalized quadrupole and sextupole gradients, D x is dispersion function: D x = dx c.o. /d p The mantra: Kill A’s before they transform into B’s ! - difficult to achieve in both planes - horizontal correction requires 2 sextupoles 180 apart to cancel spherical aberrations B x,y are most important since they determine modulation of phase advance x,y x,y = - x,y /2, x,y are Twiss lattice functions, p is relative momentum deviation. Equations for chromatic functions MC Design Status- Y. Alexahin MC workshop 06/30/2011
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Muon Collider Lattice Design Status
Muon Collider Workshop, Telluride CO, June 27 – July 1 2011
Y. Alexahin (FNAL APC)
Lattice design - 1.5 TeV c.o.m Lattice - New 3 TeV c.o.m Lattice
Fringe Field and Multipole Errors Strong-Strong Beam-Beam Simulations Plans
Ring Lattice Requirements2
What we would like to achieve compared to other machines:
MC Tevatron LHC
Beam energy (TeV) 0.75 0.98 7
* (cm) 1 28 55
Momentum spread (%) 0.1 <0.01 0.0113
Bunch length (cm) 1 50 15
Momentum compaction factor (10^-3) 0.01 2.3 0.322
Geometric r.m.s. emittance (nm) 3.5 3 0.5
Particles / bunch (10^11) 20 2.7 1.15
Beam-beam parameter , 0.1 0.0250.01
Muon collider is by far more challenging:
much larger momentum acceptance with much smaller *
~ as large Dynamic Aperture (DA) with much stronger beam-beam effect
very small momentum compaction factor
- New ideas for IR magnets chromaticity correction needed!
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Chromatic Correction Basics3
,
,1,
22xxx
xpx
xxpx
xx
px
BAW
BA
Montague chromatic functions :
Ax,y are created first, and then converted into Bx,y as phase advances x,y grow
K1 , K2 are normalized quadrupole and sextupole gradients, Dx is dispersion function: Dx = dxc.o./dp
The mantra:
Kill A’s before they transform into B’s !
- difficult to achieve in both planes
- horizontal correction requires 2 sextupoles 180 apart to cancel spherical aberrations
Bx,y are most important since they determine modulation of phase advance x,y
xxx
xxxxx
ABKDKBA
2),(2 21
s
pxppx s
sds0 ),(1
1),(
x,y = -x,y /2 , x,y are Twiss lattice functions, p is relative momentum deviation.
Equations for chromatic functions
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Magnet Requirements4
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Distance from IP to the 1st quad = 6 m Bending field in the arcs = 10T, in large aperture IR dipoles
8T Aperture diameter > 10 max + 30 mm Quad gradient < 10T/ (/2) Quad length < 2 m, dipole length < 6 m Interconnects > (1 + 2)/2 + 16 cm (typically + 2 cm
added) FF quads horizontally displaced (if possible) to provide a
dipole component that: - generates additional dispersion for chromaticity
correction - sweeps aside decay electrons
*=1cm 1.5 TeV c.o.m. MC IR Optics
MC Design Status- Y. Alexahin MC workshop 06/30/2011
5
50 100 150 200 1000
0
1000
2000
3000
4000
5000
6000
xW
xDD
)(
)(,
cmDD
mW
x
yx
yW
)(ms
50 100 150 200
50
100
150
200
250
x
y)(
)(,
cmD
m
x
yx2S
)(ms
2/xD
3S 4S1S
essentially a focusing doublet
chromaticity correction sextupoles
6*=1cm 1.5 TeV MC FF Quads
5 10 15 20 25
2
4
6
8
Q3 Q4 Q5 B1 Q6
Q2Q1
s(m)
a(cm)
5x
5y
Parameter Unit Q1 Q2 Q3
Coil aperture mm 80 110 160
Nominal gradient T/m 250 187 -130
Nominal current kA 16.61 15.3 14.2
Quench gradient @ 4.5 K T/m 281.5 209.0 146.0
Quench gradient @ 1.9 K T/m 307.6 228.4 159.5
Coil quench field @ 4.5 K T 12.8 13.2 13.4Coil quench field @ 1.9 K T 14.0 14.4 14.8Magnetic length m 1.5 1.7 1.7
Quads displaced horizontally by 0.1 aperture to create ~2T bending field
MC Design Status- Y. Alexahin MC workshop 06/30/2011
7*=1cm 1.5 TeV MC Lattice Performance
Qx Qy
p
p
c
DA ()
p
“Diagonal” Dynamic Aperture (Ax=Ay) vs. (constant) momentum deviation in the presence of beam-beam effect ( = 0.09/IP) for normalised emittance N=25 m
Only muons at bunch center tracked !Fractional parts of the tunes and momentum compaction factor vs. momentum deviation
beam extent
MC Design Status- Y. Alexahin MC workshop 06/30/2011
8Design Pros & Contras
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Pros: Achieves all stated goals (momentum acceptance, DA, etc.) Robust chromaticity correction scheme Small horizontal beam size allows for close shielding to intercept secondaries FF quads can be displaced horizontally to create a dipole field
Contras: Large y_max high sensitivity to magnet errors Difficult to upgrade to higher energies: it may not be possible to retain 10T pole tip field in quads with apertures > 16 cm due to mechanical problems
Triplet vs Doublet FF9
A simplified problem considered: Point-to-parallel focusing *=5mm, N=25()mmmrad, 1.5TeV/beam First quad starts at 6m from IP Continuously varying quad gradient G=8T / R_bore, R_bore= 5*Sqrt(max*N/)+15 mm
8 10 12 14 16 18 20
50 000
100 000
150 000
200 000
250 000
15 20
20 000
40 000
60 000
80 000
s s
In the case of triplet focusing max is 3 times smaller! - effect of the gradient dependence on aperture
MC Design Status- Y. Alexahin MC workshop 06/30/2011
10
Q3Q4 Q5 B1Q7
Q2Q1
s(m)
a(cm)
5x5y
Q8Q6
*=5mm 3 TeV c.o.m. MC FF Quads (Preliminary!)
Q1 Q2 Q3 Q4-Q6 Q7 Q8
aperture (mm) 80 104 130 146 146 160
gradient (T/m) -250 -192.3 153.9 136.5 -136.7 -121.4
length (m) 1.85 1.75 1.95 2.05 1.75 2.6
Aperture requirement >10 max +30 mm as in 1.5 TeV case The number of different apertures increased to 5 to follow more
closely the beam sizes Length limit < 2 m not fulfilled for Q8, it can be cut in two
pieces if necessary No horizontal displacement due to large horizontal beam size
M1
MC Design Status- Y. Alexahin MC workshop 06/30/2011
11*=5mm 3 TeV c.o.m. MC IR Optics (Preliminary!)
y (m)
x (m)
10*DDx (m)
20*Dx (m)
s (m)
Wy
chromaticity correction sextupoles
M2
s (m)
Wx
M1
MC Design Status- Y. Alexahin MC workshop 06/30/2011
12*=5mm 3 TeV MC Lattice Performance (w/o Arcs)
Large Qx= -1.65105 octupole (and decapole) correctors at M2 DA < 4 compensating octupole at M1 DA > 5
*(cm)
y*
p
x*
Qx
Qy
p
Static momentum acceptance 0.5% and Dynamic Aperture ~ 5 seem feasible – the arc sextupoles are too weak to have any effect
CSIy [m]
CSIx [m]
5
1024 turns DAFractional parts of the tunes
MC Design Status- Y. Alexahin MC workshop 06/30/2011
133 TeV MC Arc Cell
SY
DDx(m)/2
Dx (m)
SX SX
SASY
dsDDDCd
d
dsDC
C
xx
p
c
Cx
c
0
2
0
)(211
,1
x (m)y (m)
Central quad and sextupole SA control the momentum compaction factor and its derivative (via Dx and DDx) w/o significant effect on chromaticity Large -functions ratios at SX and SY sextupole locations simplify chromaticity correction Phase advance 300/ cell spherical aberrations cancelled in groups of 6 cells Large dipole packing factor small circumference (C~4.5 km with 10T dipole field)MC Design Status- Y. Alexahin MC workshop 06/30/2011
14Parameters of the Two Designs
s (TeV) 1.5 3* (cm) (bare lattice) 1 0.5_max (km) 48 94Av. Luminosity / IP (1034/cm2/s) 1.25 4.4Max. bending field (T) 10 10Av. bending field in arcs (T) 8.3 8.4Circumference (km) 2.5 (2.7) 4.5No. of IPs 2 2Repetition Rate (Hz) 15 12Beam-beam parameter / IP 0.087 0.087Beam size @ IP (m) 6 3Bunch length (cm) 1 0.5No. bunches / beam 1 1No. muons/bunch (1012) 2 2Norm. Trans. Emit. (m) 25 25Energy spread (%) 0.1 0.1Norm. long. Emit. (m) 0.07 0.07Total RF voltage (MV) at 800MHz 20 250
hCP
fhNn
f repb
~21
4
2
0L
P – average muon beam power (~ )
4Nr
C – collider circumference (~ if B=const)
– muon lifetime (~ )
* – beta-function at IP
– beam-beam parameter
0.5 1 1.5 2
0.6
0.7
0.8
0.9
h
z /
“Hour-glass factor”
MC Design Status- Y. Alexahin MC workshop 06/30/2011
What’s Next? 15
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Triplet FF solves the problem with large y_max, but lacks some nice features of the doublet FF associated with small x With triplet FF the major concern is horizontal beam stability, whereas with doublet FF it is for the vertical plane Is a compromise possible? For 3 TeV we must know what gradients can be realistically achieved in large aperture quads, G(A) curve is needed from magnet designers For 1.5 TeV case we may try to optimize y_max/ x_max ratio and reduce * Optimization should be performed with account of systematic and random magnet errors and their correction strategy - a lot of work to do! Extra manpower is needed!
Fringe Field in IR quads (V.Kapin)16
1024 turns DA for 1.5TeV lattice in units of initial coordinates at IP without (left) and with quadrupole fringe fields: center - embedded in MAD-X PTC hard-edge approximation, right - maps produced by COSY. Only vertical motion suffers due to y_max>> x_max PTC underestimates the effect
y0 (m)
x0 (m)
MC Design Status- Y. Alexahin MC workshop 06/30/2011
y0 (m)
x0 (m)
IR Open-Midplane Dipole Nonlinearities (V.Kapin)17
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Rref=40mm
b1=10000
b3=-5.875
b5=-18.320
b7=-17.105
IR dipole coil cross-section and good field region
Effect of multipole components on DA in 1.5TeV case: decapole is most detrimental
18
MC Design Status- Y. Alexahin MC workshop 06/30/2011
DA in the plane of initial particle coordinates:. left - no multipole errors, center -sextupole error added, right - sextupole corrector placed at the 1st y maximum. Effect of the sextupole error can also be compensated with octupole (Netepenko) Sextupole error affects both x- and y-motion
Correction of IR Dipole Nonlinearities (V.Kapin)
50 100 150 200
50
100
150
200
250
x
y)(
)(,
cmD
m
x
yx2S
)(ms
2/xD
3S 4S1S
SC1
Strong-Strong BB Simulations (K.Ohmi) 19
MC Design Status- Y. Alexahin MC workshop 06/30/2011
Very fast luminosity degradation (by 15%) observed, most likely due to initial mismatch Dr. Ohmi will come at Fermilab in October to do more studies.
Plans20
Lattice design: - complete 1.5TeV design with new tuning & collimation sections - finish the 3TeV design
Fringe fields & Multipoles: - include realistic long. profile (Enge function) in MAD-X (F.Schmidt, CERN) or borrow from COSY-Infinity (V.Kapin) - nonlinear corrector arrangement for fringe field and multipole error correction (V.Kapin, F.Schmidt)
Strong-Strong Beam-Beam Simulations: - K.Ohmi (KEK) will come at Fermilab in October - A.Valishev and E.Stern (FNAL) also promised to look
Self-Consistent Longitudinal Dynamics: - V.Balbekov & L.Vorobiev (FNAL GS) can address it (using ORBIT?)
MC Design Status- Y. Alexahin MC workshop 06/30/2011