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Transcript
PHASE STABILITY
by
Joël Le DuFF
(LAL-Orsay)
CAS on Synchrotron Radiation & Free Electron Lasers
Brunnen 2-9 July 2003
CAS
Brunnen 2-9 July 2003
1
summary
•Bibliography
•Radio-Frequency Acceleration
•Principle of Phase Stability
•Consequences of Phase Stability
•The Synchrotron
•Dispersion Effects in Synchrotron
•Energy-Phase Equations
•Longitudinal (synchrotron) Phase Space Motion
•Characteristics of the electron Synchrotron
•From Synchrotron to Linac
•Adiabatic Damping
CAS
Brunnen 2-9 July 2003
2
Bibliography : Old Books
M. Stanley Livingston
High Energy Accelerators
(Interscience Publishers, 1954)
J.J. Livingood
Principles of cyclic Particle Accelerators
(D. Van Nostrand Co Ltd , 1961)
M. Stanley Livingston and J. B. Blewett Particle Accelerators
(Mc Graw Hill Book Company, Inc 1962)
K.G. Steffen
High Energy optics
(Interscience Publisher, J. Wiley & sons, 1965)
H. Bruck
Accelerateurs circulaires de particules
(PUF, Paris 1966)
M. Stanley Livingston (editor) The development of High Energy Accelerators
(Dover Publications, Inc, N. Y. 1966)
A.A. Kolomensky & A.W. Lebedev Theory of cyclic Accelerators
(North Holland Publihers Company, Amst. 1966)
E. Persico, E. Ferrari, S.E. Segre Principles of Particles Accelerators
(W.A. Benjamin, Inc. 1968)
P.M. Lapostolle & A.L. Septier
Linear Accelerators
(North Holland Publihers Company, Amst. 1970)
A.D. Vlasov
Theory of Linear Accelerators
(Programm for scientific translations, Jerusalem 1968)
CAS
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3
Bibliography : New Books
M. Conte, W.W. Mac Kay
An Introduction to the Physics of particle Accelerators
(World Scientific, 1991)
P. J. Bryant and K. Johnsen The Principles of Circular Accelerators and Storage Rings
(Cambridge University Press, 1993)
D. A. Edwards, M. J. Syphers An Introduction to the Physics of High Energy Accelerators
(J. Wiley & sons, Inc, 1993)
H. Wiedemann
Particle Accelerator Physics
(Springer-Verlag, Berlin, 1993)
M. Reiser
Theory and Design of Charged Particles Beams
(J. Wiley & sons, 1994)
A. Chao, M. Tigner
Handbook of Accelerator Physics and Engineering
(World Scientific 1998)
K. Wille
The Physics of Particle Accelerators: An Introduction
(Oxford University Press, 2000)
E.J.N. Wilson
An introduction to Particle Accelerators
(Oxford University Press, 2001)
And CERN Accelerator Schools (CAS) Proceedings
CAS
Brunnen 2-9 July 2003
4
Main Characteristics of an Accelerator
ACCELERATION is the main job of an accelerator.
•The accelerator provides kinetic energy to charged particles, hence increasing their
momentum.
•In order to do so, it is necessary to have an electric field E, preferably along the
direction of the initial momentum.
dp
= eE
dt
BENDING is generated by a magnetic field perpendicular to the plane of the
particle trajectory. The bending radius ρ obeys to the relation :
p
= Bρ
e
FOCUSING is a second way of using a magnetic field, in which the bending
effect is used to bring the particles trajectory closer to the axis, hence
to increase the beam density.
CAS
Brunnen 2-9 July 2003
5
Radio-Frequency Acceleration
Cylindrical electrodes separated by gaps and
fed by a RF generator, as shown on the Figure,
lead to an alternating electric field polarity
Synchronism condition
CAS
Brunnen 2-9 July 2003
L = v T/2
6
Radio-Frequency Acceleration (2)
L = vT/2 (π mode)
Single Gap
CAS
L = vT (2π mode)
Multi-Gap
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7
Energy Gain
r
dp
Newton-Lorentz Force
dt
r
=eE
Relativistics Dynamics
2
2
2 2
E = E0 + p c
dE
dz
=v
dp
dz
=
dp
dt
RF Acceleration
⇒
dE = vdp
∫ Eˆ z dz = Vˆ
= eE z
dE = dW = eE z dz
Ez = Eˆ z cosωRFt = Eˆ z cosΦ(t)
W = eVˆ cosΦ
⇒
CAS
W = ∫ E z dz
(neglecting transit time factor)
Brunnen 2-9 July 2003
8
Principle of Phase Stability
Let’s consider a succession of accelerating gaps, operating in the 2π mode,
for which the synchronism condition is fulfilled for a phase Φs .
For a 2π mode,
the electric field
is the same in all
gaps at any given
time.
eVs = eVˆ sinΦs
is the energy gain in one gap for the particle to reach the next
gap with the same RF phase : P1 ,P2, …… are fixed points.
If an increase in energy is transferred into an increase in velocity, M1 & N1
will move towards P1(stable), while M2 & N2 will go away from P2 (unstable).
CAS
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9
A Consequence of Phase Stability
Transverse Instability
Longitudinal phase stability means :
∂V
∂t
>0⇒
∂E z
∂z
<0
Defocusing
RF force
The divergence of the field is
zero according to Maxwell :
∇.E = 0 ⇒
∂E x ∂E z
+
=0 ⇒
∂x
∂z
∂E x
>0
∂x
External focusing (solenoid, quadrupole) is then necessary
CAS
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10
The Synchrotron
The synchrotron is a synchronous accelerator since there is a synchronous RF
phase for which the energy gain fits the increase of the magnetic field at each
turn. That implies the following operating conditions:
^
If v = c,
e V sin Φ
Energy gain per turn
Φ = Φ s = cte
Synchronous particle
ω RF = hω r
RF synchronism
ρ = cte R = cte
Constant orbit
Bρ = P ⇒ B
e
Variable magnetic field
ωr hence ωRF remain constant (ultra-relativistic e- )
CAS
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11
The Synchrotron (2)
Energy ramping is simply obtained by varying the B field:
p = eB ρ
Since:
⇒
E
2
dp
dt
= e ρ B′
2
2 2
= E0 + p c
⇒ (∆ p )turn = eρ B′Tr =
⇒
2 π e ρ R B′
v
∆E = v∆p
(∆E)turn = (∆W )turn = 2πρ RB′ = eV sin Φ s
•The number of stable synchronous particles is equal to the harmonic
number h. They are equally spaced along the circumference.
•Each synchronous particle satifies the relation p=eBρ. They have the
nominal energy and follow the nominal trajectory.
CAS
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12
Dispersion Effects in a Synchrotron
cavity
If a particle is slightly shifted in
momentum it will have a different
orbit:
α=
E
Circumference
E+δE
2πR
p dR
R dp
This is the “momentum compaction”
generated by the bending field.
If the particle is shifted in momentum it will
have also a different velocity. As a result of
both effects the revolution frequency changes:
p=particle momentum
R=synchrotron physical radius
p dfr
η=
fr dp
fr=revolution frequency
CAS
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13
Dispersion Effects in a Synchrotron (2)
p
α = dR
R dp
ds0 = ρdθ
ds = ( ρ + x )dθ
s
s0
p + dp
p
dθ
ρ
The elementary path difference
from the two orbits is:
leading to the total change in the circumference:
1
x
∫ dl = 2πdR = ∫ ρ ds0 = ρ ∫ xds0 ⇒ dR = x
Since:
dp
x = Dx
p
CAS
we get:
x
θ
ds − ds0 dl
=
= x
ds0
ds0 ρ
m
x
Dx
α=
R
Brunnen 2-9 July 2003
m
< >m means that
m
the average is
considered over
the bending
magnet only
14
Dispersion Effects in a Synchrotron (3)
η=
p dfr
fr dp
fr =
df dβ dR
βc
⇒ r=
−
2π R
fr
β
R
dp dβ d(1 − β )
−1 dβ
E0
2
⇒
=
+
p = mv = βγ
1 = (1 − β )
−
β
β
c
p
2
2
(1 − β )
1
−
2 2
1
η = 2 −α
dfr  1
dp
=  2 − α 
fr  γ
 p
γ
η=0 at the transition energy
CAS
γ tr = 1
α
Brunnen 2-9 July 2003
15
Phase Stability in an Electron Synchrotron
In an electron synchrotron γ is generally very large and:
1
η = 2 − α ≅ −α < 0
γ
(since α>0 in most cases)
Hence dp>0 translates into dfr<0, which is a consequense of a
longer orbit while the velocity remains constant=c.
A delayed particle with respect to the synchronous one will
get closer to it if it gets a smaller energy increase when
going through the cavity, since then it will go faster around
the machine because of a smaller path.
Consequently the stable synchronous phase has to sit on the
negative slope of the RF voltage ( π-φs )
CAS
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16
Phase Stability in an Electron Synchrotron (2)
Radiation loss:
Ur ∝
Es
4
ρ
Es
Es-Ur
cavity
hν
Stable synchr. particle
CAS
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17
Longitudinal Dynamics
It is also often called “ synchrotron motion”.
The RF acceleration process clearly emphasizes two coupled
variables, the energy gained by the particle and the RF
phase experienced by the same particle. Since there is a
well defined synchronous particle which has always the same
phase φs, and the nominal energy Es, it is sufficient to follow
other particles with respect to that particle. So let’s
introduce the following reduced variables:
revolution frequency :
∆fr = fr – frs
particle RF phase
∆φ = φ - φs
:
particle momentum :
∆p = p - ps
particle energy
:
∆E = E – Es
azimuth angle
:
∆θ = θ - θs
CAS
Brunnen 2-9 July 2003
18
First Energy-Phase Equation
f RF = hf r
R
θ
⇒ ∆φ = − h∆θ
with θ = ∫ ωr dt
For a given particle with respect to the reference one:
dφ
∆ωr = d (∆θ ) = − 1 d (∆φ ) = − 1
dt
h dt
h dt
Since:
one gets:
η=
ps  dωr 
Es  dωr 
=
≅ −α




ωrs  dp s ωrs  dE s
(electron case)
∆E = 1 dφ = R φ&
Es ωrsα h dt cα h
CAS
Brunnen 2-9 July 2003
19
Second Energy-Phase Equation
eVˆ sin φ
(∆E )turn = eVˆ(sin φ − sin φs )
The energy gained by a particle at each turn is:
and when compare to the reference one:
The rate of relative energy gain can be approximated to first order:
d(∆E )
≅ (∆E )turn frs = c eVˆ(sin φ − sin φs)
dt
2πR
leading to the second energy-phase equation:
d  ∆E  = ceVˆ (sin φ − sin φ )
s
dt  Es  2πREs
CAS
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20
Small Amplitude Oscillations
d  ∆E  = ceVˆ (sin φ − sin φ ) ≅ ceVˆ cos φs ∆φ
s
dt  Es  2πREs
2πREs
(for small ∆φ)
∆E = 1 dφ = R φ& ⇒ φ&& = cαh d  ∆E 
Es ωrsα h dt cα h
R dt  Es 
By combining the two equations one gets a second order linear
differential equation:
ˆ cos φ
α
he
V
c


s
Ω2s = − 
2πEs
 R
2
φ&& + Ω2s ∆φ = 0
Since α>0,stable oscillations mean cos φs<0, which correspond to
the negative slope of the RF as mentioned already ( π/2 < φs < π )
CAS
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21
Large Amplitude Oscillations
For larger phase (or energy) deviations from the reference the
second order differential equation is non-linear:
Ω2s
&
&
(
φ+
sin φ − sin φs ) = 0
cos φs
(Ωs as previously defined)
Multiplying by φ& and integrating gives an invariant of the motion:
φ&2
Ω2s
(cos φ + φ sin φs ) = I
−
2 cos φs
which for small amplitudes reduces to:
2
&
2
(
)
∆φ
φ
+ Ω2s
=I
2
2
(the variable is ∆φ and φs is constant)
Similar equations exist for the second variable : ∆E∝dφ/dt
CAS
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22
Large Amplitude Oscillations (2)
When φ reaches π-φs the force goes
to zero and beyond it becomes non
restoring. Hence π-φs is an extreme
amplitude for a stable motion which
φ&
in the phase space(
, ∆φ ) is shown
Ωs
as closed trajectories.
Equation of the separatrix:
φ&2
Ω2s
Ω2s
(cos φ + φ sin φs ) = − cos φ (cos(π − φs ) + (π − φs )sin φs )
−
2 cos φs
s
Second value φm where the separatrix crosses the horizontal axis:
cos φm + φm sin φs = cos(π − φs ) + (π − φs )sin φs
CAS
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23
Energy Acceptance
From the equation of motion it is seen that φ& reaches an extremum
when φ&& = 0 , hence corresponding to φ = φs.
Introducing this value into the equation of the separatrix gives:
2
φ&max
= 2Ω2s{2 + (2φs − π ) tan φs }
That translates into an acceptance in energy:
 ∆E  = m− eVˆ G(φ )
 E 
 παhE
s 
s
 s max


1
2
G(φs ) = [2 cos φs + (2φs − π )sin φs ]
This “RF acceptance” depends strongly on φs and plays an important role
for the electron capture at injection, and the stored beam lifetime.
CAS
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24
RF Acceptance versus Synchronous Phase
As the synchronous phase
gets closer to 90º the
area of stable motion
(closed trajectories) gets
smaller. These areas are
often called “BUCKET”.
The number of circulating
buckets is equal to “h”.
The phase extension is
maximum close to 180º
but the synchronous phase
will be slightly different
to compensate for
radiation losses. The RF
acceptance will increase
with the RF voltage.
CAS
Brunnen 2-9 July 2003
25
From Synchrotron to Linac
In the linac there is no bending magnets, hence there is no
dispersion effects on the orbit and α=0.
Provided the cavities are periodically spaced to fulfill the
synchronism condition, the longitudinal dynamics treatment remains
valid and one ends up with a phase oscillation frequency Ωs=0. In
other words the distance in phase between particles is frozen while
energies change which is a consequence of constant velocities c.
Hence in an ultra-relativistic electron linac it is important to inject
a short bunch on the crest of the RF voltage such that the bunch
length will stay short and the relative energy spread small.
However when the particle energy is too low (v«c), the factor 1/γ2
in η is no more negligible and energy and phase are coupled
together again leading to a longitudinal oscillation with Ωs∝γ-3. Note
that in the case of a linac, the term c/R which appears in the
writing of Ωs is directly related to the RF angular frequency.
Moreover in a linac the equivallent h will be equal to 1.
CAS
Brunnen 2-9 July 2003
26
Adiabatic Damping
Though there are many physical processes that can damp the
longitudinal oscillation amplitudes, one is directly generated by the
acceleration process itself. It will happen in the electron synchrotron
when ramping the energy but not in the ultra-relativistic electron
linac which does not show any oscillation.
As a matter of fact, when Es varies with time, one needs to be more
careful in combining the two first order energy-phase equations in
one second order equation:
The damping coefficient is
proportional to the rate of
energy variation and from the
definition of Ωs one has:
&
E&s
Ω
= −2 s
Es
Ωs
CAS
( )
d E φ& = −Ω2E ∆φ
s s
dt s
Esφ&& + E&sφ& + Ω2s Es ∆φ = 0
&
E
φ&& + s φ& + Ω2s( Es )∆φ = 0
Es
Brunnen 2-9 July 2003
27