Operated by JSA for the U.S. Department of Energy Thomas Jefferson National Accelerator Facility Lecture 9 Coupled Betatron Motion II 1 Betatron Motion with Coupling of Horizontal and Vertical Degrees of Freedom – Part II USPAS, Fort Collins, CO, June 10-21, 2013 Alex Bogacz, Geoff Krafft and Timofey Zolkin
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Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 1
Betatron Motion with Coupling of
Horizontal and Vertical Degrees of
Freedom – Part II
USPAS, Fort Collins, CO, June 10-21, 2013
Alex Bogacz, Geoff Krafft and Timofey Zolkin
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 2
Outline
Practical Examples:
Spin Rotator for Figure-8 Collider ring
Vertex-to-plane adapter for electron cooling (Fermilab)
Ionization cooling channel for Neutrino Factory and Muon Collider
Generalized vertex-to-plane transformer insert
V. Lebedev, A. Bogacz, ‘Betatron Motion with Coupling of Horizontal
solenoid 4.16 m solenoid 4.16 m decoupling quad insert
BL = 28.7 Tesla m
M = C
C 0
0
17.9032 0
15
0
5
0
BE
TA
_X
&Y
[m]
BETA_1X BETA_2Y BETA_1Y BETA_2X
USPAS, Fort Collins, CO, June 10-21, 2013
Hisham Sayed, PhD Thesis
ODU, 2011
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 10
solenoid 4.16 m solenoid 4.16 m decoupling quad insert
BL = 28.7 Tesla m
M = C
C 0
0
17.9032 0
1
5
0
1
-1
BE
TA
_X
&Y
[m]
DIS
P_X
&Y
[m]
BETA_X BETA_Y DISP_X DISP_Y
Locally decoupled solenoid pair
USPAS, Fort Collins, CO, June 10-21, 2013
Hisham Sayed, PhD Thesis
ODU, 2011
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 11
Universal Spin Rotator Optics
4.4 0 8.8 0
Spin rotator ~ 46 m
BL = 11.9 Tesla m BL = 28.7 Tesla m
3 7 42 8 8
M o n S e p 0 6 1 7 : 4 4 : 4 5 2 0 1 0 O p t i M - M A I N : - C : \ W o r k i n g \ E L I C \ M E I C \ O p t i c s \ 5 G e V E l e c t e . R i n g \ h a l f _ r i n g _ i n _ s t r a i g h t _ 1 2
30
0
1-
1
BE
TA
_X
&Y
[m
]
DI
SP
_X
&Y
[m
]
B E T A _ XB E T A _ YD I S P _ XD I S P _ Y
374 288
30
0
1
-1
BE
TA
_X
&Y
[m]
DIS
P_X
&Y
[m]
BETA_X BETA_Y DISP_X DISP_Y
5 GeV
USPAS, Fort Collins, CO, June 10-21, 2013
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 12 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
A single-particle phase-space trajectory along the
beam orbit can be expressed as:
,)(ˆ)(ˆRe)(ˆ))((
22
))((
112211 sisi
esess vvx
One can rewrite the above equations in the following compact form
)()(ˆ)(ˆ sss aVx
where
)(ˆ),(ˆ),(ˆ),(ˆ)(ˆ 2211 sssss vvvvV
))(sin(
))(cos(
))(sin(
))(cos(
)(
222
222
111
111
s
s
s
s
sa
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 13 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
In the case of axially symmetric focusing the eigen-vectors reduce to:
2
2
2
2
ˆ
ii
i
i
1v ,
2
2
2
2
ˆ2
i
ii
i
v
2
1
2
1
00
2
1
2
1
00
V̂
here we used that u = 1/2, 1 = 2 = /2
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 14 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Cooling Description
Ionization cooling due to energy loss in a thin absorber can be
described as:
p
p ,
here the longitudinal energy restoration by immediate re-
acceleration is assumed
Using canonical variables the above cooling equation can be written
as:
inout xRRx ˆ
1000
0100
0010
0001
ˆ 1
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 15 USPAS, Fort Collins, CO, June 10-21, 2013
Canonical variables
.2
,2
xR
yp
yR
xp
y
x
PceBR s / - longitudinal magnetic field
Relation between geometrical and canonical variables
Rxx̂ ,
where
1002
0100
0210
0001
,,ˆ
R
R
y
x
p
y
p
x
y
x
y
xRxx
,
A ‘cap’ denotes transfer matrices and vectors related to the canonical variables.
Hamiltonian formulation - equations of motion
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 16 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Employing amplitude vector representation: )()(ˆ)(ˆ sss aVx , one can
rewrite the cooling equation as:
inout aVRRaV ˆ
1000
0100
0010
0001
ˆ 1
and finally
inout aVRRVa ˆ
1000
0100
0010
0001
ˆ 11
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 17 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Carrying out the above calculation explicitly one obtains:
inout
RR
RR
RR
RR
aa
2
1
2
12
1
2
12
1
2
12
1
2
1
1000
0100
0010
0001
2D emittances after cooling are given by the following formula:
)(sin1cos211
)(sin1cos211
2
212
22
2
2
211
22
1
43
21
ORRaa
ORRaa
outout
outout
where 2121
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 18 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Two alternative descriptions of cooling
After passing through a thin absorber one computes
a new 4D phase space
new partial emittances
new beta-functions
Or one can compute everything relative to the unperturbed beta-
functions
Seems like more convenient approach, although partial
emittances (actions) depend on betatron phases
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 19 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
If cooling effect of one absorber is sufficiently small one
can perform averaging over betatron phases. That
yields
R
R
1
1
22
11
ds
dp
p
R
ds
d
ds
dp
p
R
ds
d
0
2
2
0
1
1
11
11
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 20 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Canonical momentum of a single particle
2ˆ
0000
0000
0100
1000
ˆˆ
0000
0000
0100
1000
ˆ 21aVaVxxMTT
xy ypxp
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 21 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Second order moments of the Gaussian distribution
(Note that for a single particle - 2/rms and we use rms. emittances below)
0
,2
,4
41
,
,
21
21
21
222
21
21
22
yx
xy
yx
yx
ppxy
Mypxp
pp
ypxp
yx
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 22 USPAS, Fort Collins, CO, June 10-21, 2013
Ionization Cooling in an Axially Symmetric Channel
Beta-function for Particle Motion with Axial-symmetric Solenoidal
Focusing
Equation for the square root of the beta-function is similar to the
equation for Floque-function in the case of uncoupled motion:
04
1
43
2
2
2R
ds
d .
The standard recipe determines the alpha-function:
ds
d
2
1
Operated by JSA for the U.S. Department of Energy
Thomas Jefferson National Accelerator Facility
Lecture 9 Coupled Betatron Motion II 23 USPAS, Fort Collins, CO, June 10-21, 2013