landau(damping( - cern · 2017-09-29 ·...
TRANSCRIPT
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 1
Landau Damping part 2
Vladimir Kornilov GSI Darmstadt, Germany
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
energy transfer to resonant parKcles
2
Landau Damping
PERTURBATION
the wave
G
suppression
driving field
suppression
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon: Impedance driving field ü energy transfer: the wave ↔ the (few) resonant parKcles
Incomplete (!) mechanism of Landau Damping in beams for the end of the first part
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 3
Existence of Landau damping
driving dipole impedance here
SKll, the beams are oVen stable without an acKve miKgaKon
In any accelerator, there are many Re(Z) sources
In any beam, there are many unsuppressed eigenmodes
There must be a fundamental damping mechanism in beams
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 4
Existence of Landau damping
The beams are stable and absorb some energy
AddiKonally to Re(Z), deliberate excitaKon is oVen applied (tune measurements, opKcs control, …)
Energy is directly transferred to the beam, mostly at the beam resonant frequencies
There must be a fundamental damping mechanism in beams
Tune measurements at PS, kick every 10 ms, M.Gasior, et al, CERN
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 5
Damping
Basic consideraKon of a collecKve mode stability
change the parameters and the source of the driving mechanism
use and enhance the intrinsic damping
mechanism
Instability Stabilized mode Driven (unsuppressed) mode Mode suppressed by its drive
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 6
Another Leading Actor: Decoherence
K.Y.Ng, Physics of Intensity Dependent Beam InstabiliKes, 2006 A.Hofmann, Proc. CAS 2003, CERN-‐2006-‐002 A.Chao, Phys. Coll. Beam Instab. in High Energy Acc. 1993 A.W. Chao, et al, SSC-‐N-‐360 (1987)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 7
V.Kornilov, O.Boine-‐F., PRSTAB 15, 114201 (2012)
Decoherence
CollecKve beam oscillaKons aVer a short (one turn or shorter) kick
• Usually the beam displacement is comparable to the beam size
• In reality, signals can be very complicated
• A common diagnosKcs • Decoherence is a process
affected by many effects and mechanisms
A bunched beam Ar18+ in SIS18. Transverse signal aVer a kick
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 8
Pulse Response
-1-0.8-0.6-0.4-0.2
0 0.2 0.4 0.6 0.8
1
0 5 10 15 20
x / x
0
ωt
⟨x⟩ 8 parKcles with different frequencies Betatron oscillaKons: frequency spread
The Pulse Response is the Fourier image of BTF
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 9
Phase-‐Mixing (FilamentaKon)
x /
x x
x x
x /
x /
x /
1. 2.
3. 4.
Phase-‐mixing of non-‐correlated parKcles with a tune spread
• Beam offset oscillaKons decay
• Beam size increases (blow-‐up)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 10
Phase-‐Mixing, CoasKng Beam
-1
-0.5
0
0.5
1
0 2 4 6 8 10
Beam
Offs
et ⟨x
⟩ / x
0
Turn Number
-1
-0.5
0
0.5
1
0 2 4 6 8 10
Beam
Offs
et ⟨x
⟩ / x
0
Turn Number
Gaussian DistribuKon Lorentz DistribuKon
Q0=10.3, ξ=1, δp=0.5×10−3 Q0=10.3, ξ=1, δp=0.5×10−3
This is the case without any collecKve interacKons: phase-‐mixing of non-‐correlated parKcles
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 11
ξ=0.5 ξ=1.4 Ns=100 Qs=0.01
Phase-‐Mixing, Bunched Beam
-1
-0.5
0
0.5
1
0 50 100 150 200
bunc
h of
fset
/ σ
x0
time (turns)
Due to the parKcle synchrotron moKon, the iniKal posiKons return aVer a synchrotron period
In literature, named as “decoherence” and “recoherence”
In reality, the decoherence is very different (other effects)
dashed lines: amplitude solid lines: offset
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 12
Decoherence Landau Damping
Phase-‐mixing
Space-‐charge
Impedances
Other nonlineariKes
ChromaKcity
Octupoles
Image charges
Impedances
Decoherence
Effects Process Mechanisms
K.Y.Ng, Physics of Intensity Dependent Beam InstabiliKes, 2006 A.Hofmann, Proc. CAS 2003, CERN-‐2006-‐002 A.W. Chao, et al, SSC-‐N-‐360 (1987) V.Kornilov, O.Boine-‐F., PRSTAB 15, 114201 (2012) I.Karpov, V.Kornilov, O.Boine-‐F., PRAB 19, 124201 (2016)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 13
Decoherence Landau Damping
Phase-‐mixing
Space-‐charge
Impedances
Other nonlineariKes
ChromaKcity
Octupoles
Image charges
Impedances
Decoherence
Effects Process Mechanisms
AVer a kick, we observe the decoherence, which is a mixture of effects.
We do not observe pure Landau Damping. (infinitesimal perturbaKons)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
energy transfer to resonant parKcles
decoherence
14
Landau Damping of 1st Type
eigenmode PERTURBATION
the wave
⟨x⟩
suppression
G
beam offset
driving field
suppression
suppression
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon: Impedance driving field ü energy transfer: the wave ↔ the (few) resonant parKcles
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 15
Landau Damping: the wave & the tune spread
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
0
0.2
0.4
0.6
0.8
1
-3 -2 -1 0 1 2 3ψ
p
∆Q / δQξ
16
Landau Damping
0
0.2
0.4
0.6
0.8
1
-3 -2 -1 0 1 2 3
ψp
10-3 ∆p / p0
resonant parKcles from both sides contribute to the energy transfer, thus f(ω)
Momentum spread translates into tune spread
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 17
Landau Damping
Loss of Landau damping due to coherent tune shiV
0.0 0.2 0.4 0.6 0.8 1.0 1.2Im(∆Q) / δQ
ξ
-4
-2
0
2
4
Re(∆
Q) /
δQ
ξ
STABLE
UNSTABLE
0
0.2
0.4
0.6
0.8
1
-3 -2 -1 0 1 2 3 4 5 6
Parti
cle
Dis
tribu
tion
∆Q / δQξ
there is sKll tune spread, but no resonant parKcles for this wave → no Landau damping
impedance tune shiV
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
-6
-4
-2
0
2
4
0 0.2 0.4 0.6 0.8 1
Re(∆
Q) /
δQξ
Im(∆Q) / δQξ
∆Qsc = 2 δQξ
no space charge
18
Landau Damping
impedance tune shiV
Loss of Landau damping due to space-‐charge
-‐
0
0.2
0.4
0.6
0.8
1
-6 -5 -4 -3 -2 -1 0 1 2
Parti
cle
Dis
tribu
tion
∆Q / δQξ
there is sKll tune spread, but no resonant parKcles for this wave → no Landau damping
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 19
Landau Damping
Loss of Landau damping due to space-‐charge
Coherent dipole oscillaKons of four O8+ bunches in the SIS18 of GSI Darmstadt at the injecKon energy 11.4 MeV/u O.Boine-‐F., T.Shukla, PRSTAB 8, 034201 (2005)
there is sKll tune spread, but no resonant parKcles for this wave → no Landau damping
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 20
Landau Damping
Some analyKcal models or simulaKons predict Landau anKdamping:
unstable oscillaKons for zero or negaKve impedance
No anKdamping for Gaussian-‐like distribuKons!
D.Pestrikov, NIM A 562, 65 (2006) V.Kornilov, et al, PRSTAB 11, 014201 (2008) A.Burov, V.Lebedev, PRSTAB 12, 034201 (2009)
Remark 1
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 21
Landau Damping
a tune spread does not automaKcally means Landau Damping
Remark 2
0
0.2
0.4
0.6
0.8
1
-4 -3 -2 -1 0 1 2 3 4
Parti
cle
Dis
tribu
tion
∆Q / δQξ
k=1
Head-‐tail modes in bunches: • there is a tune spread
(due to chromaKcity ξ) • the coherent frequency overlaps
with the incoherent spectrum sKll, there is NO Landau Damping!
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
energy transfer to resonant parKcles
decoherence
22
Landau Damping of 1st Type
eigenmode PERTURBATION
the wave
⟨x⟩
suppression
G
beam offset
driving field
suppression
suppression
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon: Impedance driving field ü energy transfer: the wave ↔ the (few) resonant parKcles
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 23
Landau Damping in Beams of 2nd type
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
For example, an octupole magnet: First-‐order frequency shiV of the anharmonic oscillaKons Amplitude-‐dependent betatron tune shiVs
24
Landau Damping of 2nd type Different situaKon from ξ+δp:
Tune spread due to amplitude-‐dependent tune shiVs
SchemaKc yoke profile of an octupole magnet
N
N
N
N
S
S
S
S
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 25
Decoherence
0
0.5
1
1.5
2
2.5
3
0 20 40 60 80 100
∆x0 = 2 σx∆x0 = σx
ε / ε
0
turn number
0
0.5
1
1.5
2
0 20 40 60 80 100
∆x0 = 2 σx
∆x0 = σx
A ⟨x⟩
/ σ
x
turn number
A.W. Chao, et al, SSC-‐N-‐360 (1987) V.Kornilov, O.Boine-‐F., PRSTAB 15, 114201 (2012) I.Karpov, V.Kornilov, O.Boine-‐F., PRAB 19, 124201 (2016)
Phase-‐Mixing is very different from the chromaKcity case
• No recoherence • Kick amplitude dependent • AnalyKcal model for:
OscillaKon amplitude
Transverse emigance
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
Amplitude-‐dependent betatron tune shiVs in a lapce: Every parKcle has a different amplitude (Jx, Jy) → tune spread → Landau damping?
26
Landau Damping of 2nd type
-100
-50
0
50
100
0 50 100 150 200
x iωt
∆ωi / Ω = 0.03∆ωi / Ω = 0.01ωi = Ω
Tune spread due to amplitude-‐dependent tune shiVs
Ωcoh
The resonant parKcles driV away in tune from the resonance as they get excited
-0.04
-0.02
0
0.02
0.04
0.06
0 0.5 1 1.5 2 2.5 3 3.5 4
∆Q
x
ax / a0
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017
-0.04
-0.02
0
0.02
0.04
0.06
0 0.5 1 1.5 2 2.5 3 3.5 4
∆Q
x
ax / a0
27
Landau Damping of 2nd type
0
0.2
0.4
0.6
0.8
1
0 0.5 1 1.5 2 2.5 3 3.5 4
ψx
ax / a0
a(Ωcoh)
ParKcle excitaKon for amplitude-‐dependent tune shiVs
a(Ωcoh)
We already guess: the distribuKon slope (df/da) might be involved
-100
-50
0
50
100
0 50 100 150 200
x i
ωt
∆ωi / Ω = 0.03∆ωi / Ω = 0.01ωi = Ω
Once the parKcle is driven away from the resonance, the energy is transferred back to the wave
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 28
Landau Damping of 2nd type
L.Laslet, V.Neil, A.Sessler, 1965 D.Möhl, H.Schönauer, 1974 J.Berg, F.Ruggiero, CERN SL-‐96-‐71 AP 1996
ΔQcoh : coherent no-‐damping tune shiV imposed by an impedance ΔQex(Jx,Jy) : external (lapce) incoherent tune shiVs
The resulKng damping is a complicated 2D convoluKon of the distribuKon df(Jx,Jy)/dJx and tune shiVs ΔQext(Jx,Jy)
The dispersion relaKon
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 29
Landau Damping of 2nd type
energy transfer to resonant parKcles
decoherence eigenmode PERTURBATION
the wave
⟨x⟩
suppression
G
beam offset
driving field
suppression
suppression
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon: Impedance driving field ü energy transfer: the wave ↔ the (few) resonant parKcles
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 30
Landau Damping of 2nd type
-0.2
-0.1
0
0.1
0.2
-0.2 -0.1 0 0.1 0.2
∆Q
y ( ×
10−
3 )
∆Qx ( × 10−3 )
0 0.005
0.01 0.015
0.02 0.025
0.03 0.035
0.04
-0.6 -0.4 -0.2 0 0.2 0.4 0.6Im
(∆Q
) ( ×
10−
3 )Re(∆Q) ( × 10−3 )
stable
unstable
Octupole Tune Footprint ResulKng Stability Diagram
An example of the applicaKon: Beam stability studies for FCC
V.Kornilov, FCC Week 2017, Berlin
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 31
Landau Damping of 2nd type
Dynamic Aperture
Landau Damping
A balance is necessary
Octupoles are the essenKal part of the beam stability in many machines
Drawback: octupoles, like other nonlineariKes, can reduce Dynamic Aperture and LifeKme.
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 32
X.Buffat, et al, PRSTAB 17, 111002 (2014)
Amplitude-‐Dependent Detuning
Another source of amplitude-‐dependent tune-‐shiVs: Tune-‐spread due to Beam-‐Beam effects produces Landau Damping
Tune Footprints ResulKng Stability Diagrams
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 33
Landau Damping in Beams of 3rd type
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 34
Landau Damping of 3rd type
Ωcoh
ωinc Electric field of the self-‐field space charge
Different situaKon: Wave−ParKcel interacKon is due to space-‐charge
0
0.5
1
1.5
2
0 1 2 3 4 5 6
∆Q
sc / ∆
QKV
ax / σx
Space-‐charge tune shiV
For the resonant parKcles Qinc≈Qcoh , wave↔parKcles energy transfer should be possible
tune spread
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 35
Landau Damping of 3rd type
L.Lasleg, V.Neil, A.Sessler, 1965 D.Möhl, H.Schönauer, 1974
f(Jx,Jy,p) ΔQcoh : no-‐damping coherent tune shiV imposed ΔQex(Jx,Jy,p) : external (lapce) incoherent tune shiV ΔQsc(Jx,Jy) : space-‐charge tune shiV
The dispersion relaKon
The resulKng damping is a complicated 2D convoluKon of the distribuKon df(Jx,Jy)/dJx and tune shiVs ΔQsc(Jx,Jy), ΔQext(Jx,Jy)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 36
Landau Damping of 3rd type
V.Kornilov, O.Boine-‐F, I.Hofmann, PRSTAB 11, 014201 (2008) E.Metral, F.Ruggiero, CERN-‐AB-‐2004-‐025 (2004)
SoluKon examples
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 37
Landau Damping of 3rd type
L.Lasleg, V.Neil, A.Sessler, 1965 D.Möhl, H.Schönauer, 1974
V.Kornilov, O.Boine-‐F, I.Hofmann, PRSTAB 11, 014201 (2008) A.Burov, V.Lebedev, PRSTAB 12, 034201 (2009)
ΔQex=0: no pole, no damping! Momentum conservaKon in a closed system
The dispersion relaKon
Even if Ωcoh is inside the spectrum, and there are resonant parKcles Qinc≈Qcoh ,
there is no Landau damping in coasKng beams only due to space-‐charge
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 38
Landau Damping
a tune spread does not automaKcally means Landau Damping
Remark
Thus, we discussed two examples: 1. Head-‐tail modes and the chromaKcity tune-‐spread 2. Nonlinear space-‐charge in coasKng beams • there is a tune spread • the coherent frequency overlaps
with the incoherent spectrum sKll, there is NO Landau Damping! 0
0.2
0.4
0.6
0.8
1
-4 -3 -2 -1 0 1 2 3 4
Parti
cle
Dis
tribu
tion
∆Q / δQξ
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 39
Landau Damping of 3rd type
energy transfer to resonant parKcles
decoherence eigenmode PERTURBATION
the wave
⟨x⟩
suppression
beam offset
over space charge
suppression
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon: E-‐field of Space-‐charge ü energy transfer: the wave ↔ the (few) resonant parKcles
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 40
Landau Damping of 3rd type
Main ingredients of Landau damping: ü wave−parKcle collisionless interacKon:
the electric field of space-‐charge ü energy transfer: the wave ↔ the (few) resonant parKcles in addiKon, the decoherence, other ΔQex(Jx,Jy,p), the mix with G
THE WAVE faster
resonant parKcles
slower resonant parKcles
ENERGY
over electric field
If simplified, very similar to Landau damping in plasma:
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 41
Landau Damping of 3rd type
Landau damping in bunches • There is damping due to only
space charge • Space-‐charge tune spread due
to longitudinal bunch profile
A.Burov, PRSTAB 12, 044202 (2009) V.Balbekov, PRSTAB 12, 124402 (2009) V.Kornilov, O.Boine-‐F, PRSTAB 13, 114201 (2010)
Vladimir Kornilov, The CERN Accelerator School, London, UK, Sept 3-‐15, 2017 42
Landau Damping in beams
• Waves: collecKve oscillaKons in a medium of parKcles • Wave ↔ parKcles collisionless interacKon • Dispersion relaKon and Stability Diagram • Decoherence is a result of Phase-‐Mixing, Landau damping, etc • CollecKve Frequency ↔ Tune Spread • Tune spreads of different nature produce
different types of Landau damping • A tune spread does not automaKcally means Landau Damping • A special role of Space-‐Charge as a provider of a tune spread
and the wave↔parKcles interacKon