USPAS Lecture 26 - Cornell Universitydugan/USPAS/Lect26.pdf · · 2001-12-03yy y p 1 2 0 10 0 01...
Transcript of USPAS Lecture 26 - Cornell Universitydugan/USPAS/Lect26.pdf · · 2001-12-03yy y p 1 2 0 10 0 01...
12/3/01 USPAS Lecture 26 1
LECTURE 26Collective instabilities;
Rigid beam transverse multibunch instability
The macroparticle model used in the previous lecture can beapplied to the important case of multiple bunches in a common
vacuum chamber. Long-range wakefields will couple themotion of the bunches together and can lead to tune shifts and
instabilities.
As we saw above, the wake fields generated by themacroparticle can be expressed in terms of a transverse
integrated force exerted at the location of the impedance.rF t ieI t mr r m m Zm
mm⊥
− ⊥= −( ) ( )( ) ( ) ˆ cos ˆ sin1 φ φ φ ω
12/3/01 USPAS Lecture 26 2
For m=1, and in the vertical direction, we have
F t ieI t Zy( ) ( )= ( )⊥1 1 ω
To use the above equation, we need to know the Fourierspectrum of the dipole moment of the current. As discussed in
Lecture 25, the wake force is
F tiNe
Ty i p Q t Z p Q
y i p Q t Z p Q
y y yp
y y
( ) ˜ exp
˜ exp*
= − +( )( ) +( )( )+ − −( )( ) −( )( )
⊥
=−∞
∞
⊥
∑2
00 0 1 0
0 0 1 0
2ω ω
ω ω
in which y y i yy= + ′β . Using the symmetry property
Z Z1 1⊥ ⊥= − −( ) ( )*ω ω .
12/3/01 USPAS Lecture 26 3
The integrated force, summed over all harmonics, can bewritten as
F tiNe
Ty i p Q t Z p Q c cy y y
p
( ) ˜ exp . .= − +( )( ) +( )( ) +⊥
=−∞
∞
∑2
00 0 1 02
ω ω
c.c represents the complex conjugate-dropped for now, addedback in equation of motion
This is the integrated force due to a single macroparticle.Suppose now that we have 2 bunches (macroparticles), of equalcharge. We’ll label the first bunch 0, and the second (trailing)
bunch 1. The wake force due to bunch 0 can be written as
F tiNe
Ty t ip t Z p Qy y
p0
2
00 0 1 02
( ) = ( ) −( ) +( )( )⊥
=−∞
∞
∑˜ exp ω ω
12/3/01 USPAS Lecture 26 4
in which ˜ ˜ expy t y iQ ty( ) = −( )0 0ω
Suppose that bunch 1 trails bunch 0 by the time interval t t= 01.
t
0 1
t0 1(n+1)T0
0 1
t0 1
nT0
Since it arrives at the impedance at t nT t= +0 01, its current isgiven by
I tNeT
ip t tp
00
0 01( ) exp= − −( )( )=−∞
∞
∑ ω
12/3/01 USPAS Lecture 26 5
and its betatron oscillation can be written as
˜ ˜ expy t y iQ t ty1 10 0 01( ) = − −( )( )ω
so the force created by its wake is given by
F tiNe
Ty iQ t t
ip t t Z p Q
y y
yp
1
2
010 0 01
0 01 1 0
2( ) = − −( )( ) ×
− −( )( ) +( )( )⊥
=−∞
∞
∑
˜ exp
exp
ω
ω ω
Bunch 0 arrives at the impedance at time t T T= −... , , ,...0 00 andfeels the total wake force
12/3/01 USPAS Lecture 26 6
F F nT F nT
iNeT
y i Q n Z p Q
iNeT
y i Q ntT
ip t Z p Q
y n y y
y yp
y yp
0 0 0 1 0
2
000 1 0
2
001
01
00 01 1 0
22
22
,
˜ exp
˜ exp exp
= ( ) + ( ) =
= −( ) +( )( ) +
− −
( ) +( )( )
⊥
=−∞
∞
⊥
=
∑π ω
π ω ω−∞−∞
∞
∑
Let us defineˆ ( ) ˜ exp ˜ ( )
ˆ ( ) ˜ exp ˜ ( )
y n y iQ n y n
y n y iQ ntT
y nT
y
y
0 00 0
1 0101
01 0
2
2
= −( ) =
= − −
=
π
π
12/3/01 USPAS Lecture 26 7
ˆ , ˆy n y n0 1( ) ( ) are the y variables of bunch 0,1 when bunch 0crosses the location of the impedance. These are sometimes
called the “snapshot” position of the bunch. ˆ , ˆy n y n0 1( ) ( )describe the bunch displacements and slopes, not at the same
location, but at the same time at different locations (the locationof the impedance, for bunch 0; a distance ct01 behind bunch 0,
for bunch 1).Then we have
FiNe
T
y n Z p Q
y n iptT
Z p Qy n
yp
yp
0
2
0
0 1 0
101
01 0
22
,
ˆ ( )
ˆ ( ) exp
=
+( )( ) +
+( )( )
⊥
=−∞
∞
⊥
=−∞
∞
∑
∑
ω
π ω
12/3/01 USPAS Lecture 26 8
We now insert this into the betatron equation of motion. Theunperturbed betatron equation for the 0th bunch, written in
terms of turn number, has the form
dydn
iQ yy
ˆˆ 0
02= − π
The effect of the integrated force is to produce a change in y0
given by ∆ ∆ˆ , ,y i y iF
pvi
F
m cy yy n
yy n
0 00 0
02= ′ = =β β βγ
. Hence the
equation of motion becomes
12/3/01 USPAS Lecture 26 9
dydn
iQ y iiNe
m c Ty A y A y B y B
A Z p Q
B iptT
Z p Q
y y
yp
yp
ˆˆ ˆ ˆ ˆ ˆ
exp
* * * *00
2
02
00 0 1 1
1 0
01
01 0
22
2
= − + − + −( )
= +( )( )
=
+( )( )
⊥
=−∞
∞
⊥
=−∞
∞
∑
∑
π βγ
ω
π ω
Now let us consider the motion of bunch 1. Since bunch 1 trailsbunch 0, it crosses the impedance at the time nT t0 01+ and feels
the force
12/3/01 USPAS Lecture 26 10
F F nT t F nT t
iNeT
y n i QtT
ip t Z p Q
iNeT
y n Z p Q
iNe
y n y y
y yp
yp
1 0 0 01 1 0 01
2
00
01
00 01 1 0
2
01 1 0
2
22
2
,
˜ exp exp
˜
= +( ) + +( ) =
( ) −
−( ) +( )( ) +
( ) +( )( )
=
⊥
=−∞
∞
⊥
=−∞
∞
∑
∑
π ω ω
ω
222
2
0
01
00 1
01
01 0
Ti Q
tT
y B y A
B i ptT
Z p Q
y
yp
exp ˆ ˆ
exp
−
′ +( )
′ = −
+( )( )⊥
=−∞
∞
∑
π
π ω
12/3/01 USPAS Lecture 26 11
We now insert this into the betatron equation of motion forbunch 1. The unperturbed betatron equation for bunch 1,
written in terms of turn number, has the form
dydn
iQ yy
ˆˆ 1
12= − π
The effect of the integrated force is to produce a change in y1
given by
∆ ∆ˆ exp exp,y i y iQtT
iF
m ciQ
tTy y y
y ny1 1
01
0
1
02
01
0
2 2= ′
=
β π βγ
π . Hence
the equation of motion becomes
dydn
iQ y iiNe
m c Ty A y A y B y By y
ˆˆ ˆ ˆ ˆ ˆ* * * *1
1
2
02
01 1 0 02
2= − + − + ′ − ′( )
π βγ
12/3/01 USPAS Lecture 26 12
This, and the equation for bunch 0, are a set of coupleddifferential equations, for the 2 bunches. We can rewrite these
equations as
dydn
iQ y y y y y
dydn
iQ y y y y y
y A A B B
y A A B B
ˆˆ ˆ ˆ ˆ ˆ
ˆˆ ˆ ˆ ˆ ˆ
* * * *
* * * *
00 0 0 1 1
11 1 1 0 0
2
2
= − − + − +
= − − + − +′ ′
π
π
Γ Γ Γ Γ
Γ Γ Γ Γ
in which
Γ Γ ΓAy
By
ByANe
m c T
BNe
m c T
B Ne
m c T= = =
′′
2
02
0
2
02
0
2
02
02 2 2
βγ
βγ
βγ
We will treat the wake effects as a small perturbation: that is,we assume that
12/3/01 USPAS Lecture 26 13
Γ2
1πQy
<< , and take the motion of the two bunches to have the
form
ˆ ˆ exp, ,y n y i n0 1 00 01( ) = −( )Ω
with Ω = + <<2 1π δ δQy ,
In this case, the complex conjugate terms in the aboveequations have the approximate forms
ˆ ˆ exp ˆˆ
ˆexp,
*,
*,
,*
,
y n y i Q n y ny
yi Q ny y0 1 00 01 0 1
00 01
00 01
2 4( ) ≈ ( ) ≈ ( ) ( )
π π
12/3/01 USPAS Lecture 26 14
For Γ
21
πQy
<< , these rapidly oscillating terms may be omitted
from the equations, which then simplify to the set of coupledequations
dydn
iQ y y y
dydn
iQ y y y
y A B
y A B
ˆˆ ˆ ˆ
ˆˆ ˆ ˆ
00 0 1
11 1 0
2
2
= − − −
= − − − ′
π
π
Γ Γ
Γ Γ
or, in matrix form,
dydn
yiQ
iQy A B
B y A
ˆˆ,
rr′ = =
− − −− − −
′
M M2
2
ππ
Γ ΓΓ Γ
12/3/01 USPAS Lecture 26 15
There will be a set of normal modes ζ m, for which theequations of motion decouple:
ˆr ry = Sζ
The normal mode eqations are
S MS S MSddn
ddn
′ = ′ = =−r
rr
r rζ ζ ζ ζ ζ 1 Λ
The matrix Λ =
λλ
0
1
0
0
in which λ0 and λ1 are the eigenvalues of the matrix M. For the
matrix given above, the eigenvalues are
λ πi y A B BiQ= − − ± ′2 Γ Γ Γ
12/3/01 USPAS Lecture 26 16
The eigenvectors in the ( ˆ , ˆy y0 1) basis are
r rζ ζ1 2
12 1
12 1
= ′
= −
′
BB
BB,
We have, for each normal mode, the equation
ddn
ii i
′ =ζ λζ
Assuming a solution of the form
ζ ζi i in in( ) ˜ exp= −( )0 Ω . Using
ddn
iii i i i
′ = − =ζ ζ λζΩ .
The normal mode frequencies are
12/3/01 USPAS Lecture 26 17
Ω Γ Γ Γi i y A B Bi Q i i= = − ± ′λ π2
Using the definitions of Γ and A, B from above, these become
12/3/01 USPAS Lecture 26 18
Ω Γ Γ Γi y A B B
y
y
yp
py
Q i
i Ne
m c TA BB
i Ne
m c T
Z p Q
i p ptT
Z p Q Z
− = − ( )
= − ± ′( )
= − ×
+( )( ) ±
− ′( )
+( )( )
′
⊥
=−∞
∞
′ =−∞
∞⊥
∑
∑
2
2
2
2
2
02
0
2
02
0
1 0
01
01 0
π
βγ
βγ
ω
π ω
m
exp 11 0⊥
=−∞
∞
′ +( )( )
∑ p Qyp
ω
Consider the special case when tT
010
2= . Then
12/3/01 USPAS Lecture 26 19
exp exp2 1 101
0π πi p p
tT
i p p p p− ′( )
= − ′( )( ) = −( ) −( ) ′
Ωi yy p
yp
Qi Ne
m c TZ p Q− = − ± −( )( ) +( )( )
⊥
=−∞
∞
∑22
1 12
02
01 0π
βγ
ω
The eigenvectors are
r rζ ζ
ζ ζ
0 1
0 0 1 1 0 1
12
1
112
1
1=
=−
⇒
= + = − +
,
ˆ ˆ , ˆ ˆ y y y y
In the sum mode, both bunches oscillate in phase; in thedifference mode, the two bunches oscillate out of phase.
12/3/01 USPAS Lecture 26 20
The general case
Let there be M bunches in the machine, with the labelsy y yM0 1 1, ,..., − . Let the time separation between the bunches be
as shown below
mkt
0 1
t 0k
nT0
2 k m M-1
t
t0m
Following from above, the force due to the mth bunch, is givenby
12/3/01 USPAS Lecture 26 21
F tiNe
Ty iQ t t
ip t t Z p Q
ym m y m
m yp
( ) ˜ exp
exp
= − −( )( ) ×
− −( )( ) +( )( )⊥
=−∞
∞
∑
2
00 0 0
0 0 1 0
22π ω
ω ω
The force on the kth bunch due to the mth bunch is
F n F nT t
iNeT
y iQ nt t
T
i ptT
Z p Q
yk m ym k
m ym k
mky
p
, ( ) ( )
˜ exp
exp
= + =
− − −
×
+( )( )⊥
=−∞
∞
∑
0 0
2
00
0 0
0
01 0
22
2
π
π ω
in which
12/3/01 USPAS Lecture 26 22
t t tmk m k= −0 0
Using ˆ ( ) ˜ expy n y iQ ntTm m y
m= − −
2 0
0
π , the force on the kth
bunch is
F niNe
Ty n iQ
tT
i ptT
Z p Q
yk m m yk
mky
p
, ( ) ˜ exp
exp
= ( ) −
×
+( )( )⊥
=−∞
∞
∑
2
0
0
0
01 0
22
2
π
π ω
The total force on the kth bunch is
12/3/01 USPAS Lecture 26 23
F niNe
TiQ
tT
y n
i ptT
Z p Q
yk yk
mm
M
mky
p
( ) exp ˜
exp
= −
× ( )
+( )( )=
−
⊥
=−∞
∞
∑
∑
2
0
0
0 0
1
01 0
22
2
π
π ω
We now insert this into the betatron equation of motion forbunch k. The unperturbed betatron equation for bunch k, written
in terms of turn number, has the form
dydn
iQ yky k
ˆˆ = −2π
The effect of the integrated force is to produce a change in yk
given by
12/3/01 USPAS Lecture 26 24
∆ ∆ˆ exp expy i y iQtT
iF n
m ciQ
tTk y k y
ky
yky
k= ′
=( )
β π βγ
π2 20
0 02
0
0
. Hence
the equation of motion becomes
dydn
iQ y
N e
m c Ty n
i ptT
Z p Q
ky k
ym
m
M
mky
p
ˆˆ
˜
exp
= − −× ( )
+( )( )
=
−
⊥
=−∞
∞
∑
∑2
2
2
2
02
0 0
1
01 0
π
βγ
π ω
This is a set of M coupled differential equations for the Mbunches. In matrix form, it can be written as
12/3/01 USPAS Lecture 26 25
dydn
y
iQN e
m c Ti p
tT
Z p Qkm y kmy mk
yp
ˆˆ,
exp
rr
=
= − −
+( )( )⊥
=−∞
∞
∑
M
M 22
22
02
0 01 0π δ
βγ
π ω
There will be a set of M normal modes ζ m, for which theequations of motion decouple:
r ry = Sζ
S MS S MSddn
ddn
′ = ′ = =−r
rr
r rζ ζ ζ ζ ζ 1 Λ
The matrix Λ ij ij i= δ λ contains the eigenvalues λi of the matrix
M.
12/3/01 USPAS Lecture 26 26
As in the two-bunch case, the normal mode frequencies aregiven by the eigenvalues of M:
Ωi ii= λ
For any bunch spacing and impedance, the matrix given abovemay be diagonalized numerically and the normal mode
frequencies obtained. However, a general analytical solution forthe normal mode frequencies for M bunches is only possible in
special cases.
For example, suppose that the M bunches are uniformlydistributed around the ring.
12/3/01 USPAS Lecture 26 27
Then, we can write
tm
MTm0 0
1= −( )
and
Mkm y kmy
yp
iQN e
m c Ti p
m kM
Z p Q= − − −
+( )( )⊥
=−∞
∞
∑22
22
02
01 0π δ
βγ
π ωexp
By analogy with the 2-bunch case, the matrix which gives thenormal modes has the form
SM
iabMab =
1 2exp
π
and the eigenvalue matrix is then
12/3/01 USPAS Lecture 26 28
Λab akm
M
k
M
km mb
y aby
yp
k
M
m
M
S M S
iQN e
m c TZ p Q
MiamM
i pm k
Mikb
M
=
= − − +( )( ) ×
−
−
−
=
−
=
−
⊥
=−∞
∞
=
−
=
−
∑∑
∑
∑∑
1
0
1
0
1
2
02
01 0
0
1
0
1
22
1 22
2
π δβ
γω
π π πexp exp exp
Using the identity
exp , 20
1
π δimi jM
Mm
M
i j rM
−
=
=
−
−∑where r is any integer, we find
12/3/01 USPAS Lecture 26 29
1 22
2
12 2
2
0
1
0
1
0
1
0
1
MiamM
i pm k
Mikb
M
Mim
p aM
ikb p
M
imb a
M
k
M
m
M
k
M
m
M
p b rM
exp exp exp
exp exp
exp,
−
−
= −
−
= −
=
−
=
−
=
−
=
−
+
∑∑
∑∑
π π π
π π
δ πmm
M
p b rM b aM=
−
+∑ =0
1
δ δ, ,
so the eigenvalues are
λ πβ
γωm y
yy
r
iQNM e
m c TZ rM m Q= − − + +( )( )⊥
=−∞
∞
∑22
2
02
01 0
12/3/01 USPAS Lecture 26 30
and the normal mode frequencies are
Ωm yy
yr
QiNM e
m c TZ rM m Q− = − + +( )( )⊥
=−∞
∞
∑22
2
02
01 0π
βγ
ω
The tune shift and damping rate for mode m are related toΩm yQ− 2π by
Ω ∆m y m mQ Q i− = −2 2π π α
so the tune shift is
∆QNMe
m c TZ rM m Qm
yy
r
= + +( )( )
⊥
=−∞
∞
∑βπ γ
ω2
02
01 04
Im
and the damping rate is
12/3/01 USPAS Lecture 26 31
αβ
γωm
yy
r
NMe
m c TZ rM m Q= + +( )( )
⊥
=−∞
∞
∑2
02
01 02
Re
The eigenmodes are
ζ πb ba
a
M
a aa
M
S yM
iabM
y= = −
−
=
−
=
−
∑ ∑1
0
1
0
11 2ˆ exp ˆ
The damping rate (or instability growth rate, if it is negative)for the multibunch instability is proportional to the total numberof bunches, that is, the total current. The impedance is sampledat frequencies spaced by Mω0, rather than ω0, as in the single
bunch case. If the frequency structure of the impedance is muchbroader than Mω0, then the sparse sampling roughly cancelsthe factor of M in front, and the damping or growth rates are
roughly the same for multiple bunches as for one bunch.
12/3/01 USPAS Lecture 26 32
(This is because the wakefields for a broadband impedance areshort range, and do not couple the bunches together).
But if the impedance is narrow-band compared to Mω0 (long-range wakefield), then the bunches are strongly coupled and themultibunch growth rates can be M times larger than for a single
bunch.
Example: the transverse resistive wall instability. Theimpedance is (Lecture 19, p 23)
Z Ci
b
c1 3
212
⊥ = − ( )( )
sgnω ωωπ
ω µσ
The impedance enters the damping rate in the form
12/3/01 USPAS Lecture 26 33
Re Z pM m QCb
c pM m Q
pM m Qyp
y
yp1 0 3
2
02⊥
=−∞
∞
=−∞
∞
+ +( )( )[ ] =+ +
+ +∑ ∑ωπ
µω σ
The multibunch mode which is most strongly driven will be theone for which the denominator is the smallest. The denominator
is pM m n+ + + ∆β, in which n is the integral part of the tune.Consider, for example, the Tevatron Collider, with M=36
bunches, and an integral tune of n=19. The denominator will be36 19p m+ + + ∆β, which is just ∆β for p=-1 if the mode number
is m=17. Thus, the mode m=17 will be the dominantmultibunch mode. The snapshot mode pattern for m=17,
ˆ expyia
aa
M
=
=
−
∑16
17180
1 π
12/3/01 USPAS Lecture 26 34
is shown below:
5 10 15 20 25 30 35
-0.15
-0.1
-0.05
0.05
0.1
0.15
This is a low frequency oscillation, which can be easily dampedwith a narrow band feedback system.
12/3/01 USPAS Lecture 26 35
The damping rate per turn is
αβ
π γµ
ω σ β= ( )M Ne c
b m cfy
2 2
30
202
∆
in which f ∆β( ) is the function defined in Lecture 25. Taking
the fractional tune to be ∆β=-0.4, and with other parameters for
the Tevatron as follows:
βy=100 m, N=1011, b=2.5 cm, γ=103, T0=21 µs,
σ=3.5x107 Ω-1m-1 (aluminum), we find a damping time ofT0 3 2α
= − . s. (a weak instability). This is a gross overestimate,
in fact, since most of the Tevatron vacuum chamber is cold, andthe resistance is therefore much less than assumed above.
12/3/01 USPAS Lecture 26 36