M.apollonioCM17 -CERN- (22/2 - 25/2 2007)1 Single Particle Amplitude M. Apollonio – University of...
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m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 1
Single Particle Amplitude
M. Apollonio – University of Oxford
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 2
amplitude: is a single particle concept
Consider first a 2D case
)(
02
z
xx
)(1)(
))(cos()()(
zz
zzAzx
field strength
222
2
22
4
22
ssccA
x
scAcxx
cAx
(1)
(3)
(2)
0442 222
c=cos()
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 3
)(zA
))(cos()( zzA
x
x’
area=
A
A: for a linear system this is a constant of the motion (Liouville’s theorem)
: describes the optical propertiesof the channel
x
z
envelope
motion of a particle in the lattice
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 4
2
22
1
2
2
xxxxA
: optical Twiss parameters
1
1
B
xBxA T
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 5
if the beam is gaussian and matched there is a relationbetween V and B
BVxxxx
xxxx
here B and describe beam envelope properties.B can be inferred from Vand A too ...
... A is still a single particle amplitude BUT describes a level of constant probability for a gaussian distributed beam
xVxA T 1
V: covariance matrix of the beam
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 6
x
emittance: RMS amplitudeproperty of the beamit can be derived from the COVARIANCE MATRIX of the beam
emittance/amplitude are normalizedmultipling by a factor p/mc
optical parameters: from the covariance matrix OR from our knowledge of the magnetic field
x’
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 7
from 2D to 4D
(x,x’,y,y’)
solenoidal field introduces couplings (assume x=y)
yy
yy
xx
xx
B
00
00
00
00
ppp
ppp
ppp
ppp
B
0
0
0
0
4
ppp
ppp
ppp
ppp
B
0
0
0
0
4
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 8
we can still think about single particle amplitude but weneed to be a little more careful ...
p
ppp
pp
ppppp xyyxyyxxyxyxA
222
2222
1
2
22
xBxA Tp
14
... and take into account (x-y) correlations
the definition of 4D A from a cov. mat. V is different w.r.t. the 2D case because of a (possible) non-zero canonical angular momentum
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 9
NORMALIZED amplitudes (x,x’,y,y’) (x,px,y,py)
xypyxpyx
z
pzp
np ypxpypxppp
pyxp
mA
221 2222
xyTyxTyx
z
TzT
nT ypxpypxppp
pyxp
mA
221 2222
l=<Lcan>/2mcN T=pV1+l2 T=pV1+l2
the single particle amplitude isindependent from the beam
we can use this variable to characterize cooling and transmissionthrough the channel
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 10
profile plot
reg-2 ~ centre of 1st tracker reg-92 ~ centre of 2nd tracker
cooling
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 11
=3.0 cm rad
PZ=200 MeV/c, abs=42 cm
coolingN
2/N
1
N2/
N1
=2.0 cm rad
N2/
N1
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 12
amplitude vs aperture
p = 200
MeV/c R (cm) (cm) Anmax (cm)
Absorber 15 42 10.1
RF 21 110 7.6
Tracker 15 33 12.9 AnMAX = p/mc R2/
in a focus/unif. field the max allowed amplitude has a very simple expression
in a general case it is more complicated but still the same concept we can study transmission as a function of amplitude
AnMAX = p/mc R2/
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 13
PZ=200 MeV/c, abs=42 cm=0.6cm rad
=1.0cm rad
transmission through MICEstep VI
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 14
MICE STEP VI ~90m of MICE Channel
RF ABS tracker
A (m rad) A (m rad)
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 15
AnMAX
physical aperture R
we can define the max allowed amplitude at the end of the channel
useful for the acceleration stage in the NF
m.apollonio CM17 -CERN- (22/2 - 25/2 2007) 16
conclusion
amplitude has been introduced as a single particle property MICE is a capable of measuring single particle kinematic
parameters which, combined with the optical functions, allow to define the amplitude of each muon
idependent from beam useful to study the specific effects of scraping ...
TRANSMISSION ... and COOLING:
definable as an increase of the phase space density (rather than an emittance reduction)
useful to understand the fraction transmissable to the stage after the NF front-end