CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le...

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CAS Chios, 18-30 September 2011 1 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator Physics Course Chios, 18-30 September 2011

Transcript of CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le...

Page 1: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 1

LONGITUDINAL DYNAMICS

Frank Tecker

based on the course byJoël Le Duff

Many Thanks!

CAS on Intermediate Level Accelerator Physics Course

Chios, 18-30 September 2011

Page 2: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 2

Summary

•Radio-Frequency Acceleration and Synchronism Condition

•Principle of Phase Stability and Consequences•The Synchrotron•Dispersion Effects in Synchrotron•Energy-Phase Equations•Longitudinal Phase Space Motion•Stationary Bucket•Injection Matching•From Synchrotron to Linac•Adiabatic Damping•Dynamics in the vicinity of transition energy

Page 3: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 3

Bibliography

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

Page 4: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 4

Main Characteristics of an Accelerator

ACCELERATION is the main job of an accelerator.• It provides kinetic energy to charged particles, hence increasing their

momentum. • In order to do so, it is necessary to have an electric field , preferably along the

direction of the initial momentum.dp

dt=eEz

BENDING is generated by a magnetic field perpendicular to the plane of the particle trajectory. The bending radius obeys to the relation :

Be

p

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.

E

Newton-Lorentz Force on a charged particle:

rF

dpdt

eE +

B( )

2nd term always perpendicular to motion => no acceleration

B [Tm] ≈p[GeV/c]

0.3in practical units:

Page 5: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 5

Radio-Frequency Acceleration

Cylindrical electrodes (drift tubes) separated by gaps and fed by a RF generator, as shown above, lead to an alternating electric field polarity

Synchronism condition L = v T/2 v = particle velocityT = RF period

D.Schulte

Similar for standing wave cavity as shown

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CAS Chios, 18-30 September 2011 6

Radio-Frequency Acceleration (2)

L = vT/2 (π mode) L = vT (2π mode)

Single Gap Multi-Gap

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CAS Chios, 18-30 September 2011 7

Energy Gain

RF Acceleration

(neglecting transit time factor)

The field will change during the passage of the particle through the cavity=> effective energy gain is lower

Newton-Lorentz Force Relativistics Dynamics

cpEE 222

02 + dpvdE

dE

dz=v

dpdz

=dpdt

=eEz

dE=dW=eEzdz W =e Ez dz∫

Ez =Ez sinω RFt= Ez sinφ t( )

Ez dz=V∫

sinVeW

rF =

drp

dt=e

rE +

rv×

rB( )

2nd term always perpendicular to motion => no acceleration

p =mv=Ec2 βc=β

Ec=βγm0c

2

11

γβ

c

v γ =E

E0

=m

m0

=1

1 − β 2

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CAS Chios, 18-30 September 2011 8

Transit time factor

In the general case, the transit time factor is:

Ta =E1(s,r) cos ωRF

sv

⎛⎝⎜

⎞⎠⎟

ds−∞

+∞

E1(s,r) ds−∞

+∞

Defined as: Ta eneγy γain o paticle ωith vβc

m axim um eneγy γain (paticle ωith v→ ∞)

const.),(1 g

VrsE RF

• Ta < 1• Ta 1 for g 0, smaller ωRF

Important for low velocities (ions)

E(s,r, t) =E1(s,r)⋅E2 (t)

Examplefor g=βλ/3:

for

Simple modeluniform field:

Ta =sinωRFg2v

ωRFg2v

follows:

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CAS Chios, 18-30 September 2011 9

Let’s consider a succession of accelerating gaps, operating in the 2π mode, for which the synchronism condition is fulfilled for a phase s .

For a 2π mode, the electric field is the same in all gaps at any given time.

sVeseV sinˆ 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.

Principle of Phase Stability (Linac)

If an energy increase is transferred into a velocity increase => M1 & N1 will move towards P1 => stable M2 & N2 will go away from P2 => unstable

(Highly relativistic particles have no significant velocity change)

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CAS Chios, 18-30 September 2011 10

00

z

zE

t

VLongitudinal phase stability means :

The divergence of the field is zero according to Maxwell : 000.

+

x

E

z

E

x

EE xzx

defocusing RF force

External focusing (solenoid, quadrupole) is then necessary

A Consequence of Phase Stability

Transverse focusing fields at the entrance and defocusing at the exit of the cavity.Electrostatic case: Energy gain inside the cavity leads to focusingRF case: Field increases during passage => transverse defocusing!

Page 11: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 11

Circular accelerators: 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:

BePB

cteRcte

h

cte

Ve

rRF

s

ωω

sin^

Energy gain per turn

Synchronous particle

RF synchronism (h - harmonic number)

Constant orbit

Variable magnetic fieldIf v≈c, wr hence wRF remain constant (ultra-relativistic

e- )

B

injection extraction

r

R

E

Bending magnet

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CAS Chios, 18-30 September 2011 12

Energy ramping is simply obtained by varying the B field (frequency follows v):

p =eB ⇒

dp

dt=e &B ⇒ (Δp)turn = eρ &BTr =

2π eρ R &B

v

Since: E2 =E0

2 + p2c2 ⇒ ΔE =vΔp

•The number of stable synchronous particles is equal to the harmonic number h. They are equally spaced along the circumference.•Each synchronous particle satisfies the relation p=eB. They

have the nominal energy and follow the nominal trajectory.

The Synchrotron (2)

turnΔE( ) =

sΔW( ) =2π eρ R &B=eV sin sϕ

Stable phase φs changes during energy ramping

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CAS Chios, 18-30 September 2011 13

Dispersion Effects in a Synchrotron

If a particle is slightly shifted in momentum it will have a different orbit and the length is different.

The “momentum compaction factor” is defined as:

a =p

L

dL

dp

If the particle is shifted in momentum it will have also a different velocity. As a result of both effects the revolution frequency changes:

dpdf

fp r

rh

p=particle momentum

R=synchrotron physical radius

fr=revolution frequency

E+E

E

cavity

Circumference

2R a =dL

Ldp

p

h =

d frfr

d pp

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CAS Chios, 18-30 September 2011 14

Dispersion Effects in a Synchrotron (2)

a =p

L

dL

dp

x

0ss

pdpp +

d

x

ds0 =dds= + x( )d

The elementary path difference from the two orbits is: dl

ds0

=ds−ds0

ds0=

x=

Dx

dpp

leading to the total change in the circumference:dL = dl

C∫ =

x∫ ds0 =

Dx

dpp

ds0∫

With ρ=∞ in straight sections we get:

RD

mxa

< >m means that the average is considered over the bending magnet only

definition of dispersion Dx

a =1

L

Dx (s)

ρ (s)ds0

C∫

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CAS Chios, 18-30 September 2011 15

Dispersion Effects in a Synchrotron (3)

dfr

fr

=hdpp

fr =βc2pR

⇒dfrfr

=dββ

−dRR

=dββ

−adpp

p mvβγE0

c⇒

dpp

dββ

+d 1−β 2( )

−12

1−β 2( )−1

2 1−β 2( )

−1

γ 21 24 34

dββ

pdp

fdf

r

r

aγ2

1 aγh 2

1

=0 at the transition energy a

γ 1tr

definition of momentum

compaction factor

Page 16: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 16

Phase Stability in a Synchrotron

From the definition of it is clear that an increase in energy gives- below transition (η > 0) a higher revolution frequency (increase in velocity dominates) while - above transition (η < 0) a lower revolution frequency (v c and longer path) where the momentum compaction (generally > 0) dominates.

Stable synchr. Particle for < 0

> 0

Crossing transition during acceleration makes the previous stable synchronous phase unstable. RF system needs to make a ‘phase jump’.

Page 17: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 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 s, 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 : = - s

particle momentum : p = p - ps

particle energy : E = E – Es

azimuth angle : = - s

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CAS Chios, 18-30 September 2011 18

First Energy-Phase Equation

fRF =hfr ⇒ Δφ=−hΔ with = ω r dt∫

For a given particle with respect to the reference one:

( ) ( )dtd

hdtd

hdtd

rω 11 ΔΔΔ

Since:

h =ps

ω rs

dω r

dp

⎝⎜⎞

⎠⎟s

one gets:

( ) hω

hωω

rs

ss

rs

ss

rs hRp

dtd

hRpE ΔΔ

and

2E = 02E + 2p 2c

ΔE = vsΔp = ω rsRsΔp

particle ahead arrives earlier=> smaller RF phase

qs

Dq

R

v

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CAS Chios, 18-30 September 2011 19

Second Energy-Phase Equation

The rate of energy gained by a particle is: p

ω2

sinˆ rVedtdE

The rate of relative energy gain with respect to the reference particle is then:

2pΔ

&Eω r

⎝⎜

⎠⎟ eV(sinφ−sinφs)

leads to the second energy-phase equation:

2pddt

ΔEω rs

⎝⎜⎞

⎠⎟=eV sinφ−sinφs( )

Δ &ETr( ) ≅ &EΔTr + Trs Δ &E = ΔE &Tr + Trs Δ &E =

d

dtTrs ΔE( )

Expanding the left-hand side to first order:

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CAS Chios, 18-30 September 2011 20

Equations of Longitudinal Motion

( )srs

VeEdtd ωp sinsinˆ2

( ) hω

hωω

rs

ss

rs

ss

rs hRp

dtd

hRpE ΔΔ

deriving and combining

( ) 0sinsin2

ˆ +

srs

ss Vedtd

hpR

dtd p

This second order equation is non linear. Moreover the parameters within the bracket are in general slowly varying with time.

We will study some cases later…

Page 21: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 21

Hamiltonian of Longitudinal Motion

( )sVedt

dW sinsinˆ

WRp

hdtd

ss

rshωp

21

Introducing a new convenient variable, W, leads to the 1st order equations:

pREW srs

Δ

Δ pωp 22

The two variables ,W are canonical since these equations of motion can be derived from a Hamiltonian H(,W,t):

WH

dtd

Hdt

dW

( ) ( ) WpRhVetWH

ss

rssss

2

41sincoscosˆ,, hωp

Page 22: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 22

Small Amplitude Oscillations

( ) 0sinsincos

2

+ ss

s

(for small )

&&φ+s

2Δφ = 0

ss

srss pR

Vehp

hω2

cosˆ2with

Let’s assume constant parameters Rs, ps, s and :

( ) ΔΔ+ ssss cossinsinsinsin

Consider now small phase deviations from the reference particle:

and the corresponding linearized motion reduces to a harmonic oscillation:

where s is the synchrotron angular frequency

Page 23: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 23

Stability is obtained when s is real and so s2 positive:

s2 =

e VRFη hω s

2π Rs ps

cosφs ⇒ Ωs2 > 0 ⇔ η cosφs > 0

2

pp

2

3p

VRF

cos (fs)

acceleration deceleration

0h 0h0h 0hStable in the region if

Stability condition for ϕs

< tr < tr > tr > tr

Page 24: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 24

Large Amplitude Oscillations

For larger phase (or energy) deviations from the reference the second order differential equation is non-linear:

( ) 0sinsincos

2+ s

s

s (s as previously defined)

Multiplying by and integrating gives an invariant of the motion:

( ) Iss

s sincos

cos222

which for small amplitudes reduces to:

&φ2

2+ Ωs

2 Δφ( )2

2= ′I (the variable is , and s is constant)

Similar equations exist for the second variable : Ed/dt

Page 25: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 25

Large Amplitude Oscillations (2)

( ) ( ) ( )( )ssss

ss

s

s pp sincos

cossincos

cos2222

++

( ) ( ) ssssmm pp sincossincos ++

Second value m where the separatrix crosses the horizontal axis:

Equation of the separatrix:

When reaches -s the force goes to zero and beyond it becomes non restoring.Hence -s is an extreme amplitude for a stable motion which in the

phase space( ) is shown as

closed trajectories.

&φs

, Δφ

Area within this separatrix is called “RF bucket”.

Page 26: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 26

Energy Acceptance

From the equation of motion it is seen that reaches an extreme

when , hence corresponding to .

Introducing this value into the equation of the separatrix gives:

0 s

&φmax

2 = 2Ωs2 2 + 2φs − π( ) tanφs{ }

That translates into an acceptance in energy:

This “RF acceptance” depends strongly on s and plays an important role for the capture at injection, and the stored beam lifetime.

max

ΔE

sE⎛⎝⎜

⎞⎠⎟

mβ −eV

phh sEG sφ( )

G sφ( )= 2cos sφ + 2 sφ −p( )sin sφ⎡⎣ ⎤⎦

Page 27: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 27

RF Acceptance versus Synchronous Phase

The areas of stable motion (closed trajectories) are called “BUCKET”.

As the synchronous phase gets closer to 90º the buckets gets smaller.

The number of circulating buckets is equal to “h”.

The phase extension of the bucket is maximum for s =180º (or 0°) which correspond to no acceleration . The RF acceptance increases with the RF voltage.

Page 28: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 28

Potential Energy Function

( ) Fdtd 2

2

( ) UF

( ) ( ) FdFU ss

s00

2

sincoscos

∫ +

The longitudinal motion is produced by a force that can be derived from a scalar potential:

The sum of the potential energy and kinetic energy is constant and by analogy represents the total energy of a non-dissipative system.

Page 29: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 29

Stationnary Bucket - Separatrix

This is the case sins=0 (no acceleration) which means s=0 or . The equation of the separatrix for s= (above transition) becomes:

+ 222

cos2 ss

2sin22

222

s

Replacing the phase derivative by the canonical variable W:

ωh

p rs

ss

rs hRpEW 22 Δ

and introducing the expression for s leads to the following equation for the separatrix:

W =±2Cc

−eV sE2phh

sinφ2

=±Wbk sinφ2with C=2Rs

W

0 2

Wbk

Page 30: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 30

Stationnary Bucket (2)

Setting = in the previous equation gives the height of the bucket:

The area of the bucket is:

bkA =8Wbk =16Cc

−eV sE2phh

∫ p 202 dWAbk

Since: p 20 4

2sin d

one gets:

hp hEVe

cCW s

bk 2

ˆ2

8AW bk

bk

ΔEmax =ωrs

2πWbk = β s 2

−eVRFEs

πηh

This results in the maximum energy acceptance:

Page 31: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 31

Bunch Matching into a Stationnary Bucket

A particle trajectory inside the separatrix is described by the equation:

W

0 2

Wbk

Wb

m 2-m

( ) Iss

s sincos

cos2

22 s= Is + cos2

22

mss coscos

222

2

+

( ) coscos2 ms

W Wbk2cos m2

− 2cos2

The points where the trajectory crosses the axis are symmetric with respect to s=

cos(φ) =2cos2φ2−1

φ

Page 32: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 32

Bunch Matching into a Stationnary Bucket (2)

Setting in the previous formula allows to calculate the bunch height:

2cos

8mbk

bAW bW = bkW cos mφ

2= bkW sin

φ2

or:

b

ΔE

sE⎛⎝⎜

⎞⎠⎟=

RF

ΔE

sE⎛⎝⎜

⎞⎠⎟

cos mφ2

=RF

ΔE

sE⎛⎝⎜

⎞⎠⎟

sinφ2

This formula shows that for a given bunch energy spread the proper matching of a shorter bunch (m close to , small)will require a bigger RF acceptance, hence a higher voltage

φ

W bkA16

φ2− 2Δφ( )2

16W

bkA φ⎛

⎝⎜⎞

⎠⎟+

2Δφφ

⎝⎜⎞

⎠⎟=1

bA =p16 bkA φ2

For small oscillation amplitudes the equation of the ellipse reduces to:

Ellipse area is called longitudinal emittance

Page 33: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 33

Effect of a MismatchInjected bunch: short length and large energy spreadafter 1/4 synchrotron period: longer bunch with a smaller energy spread. W W

For larger amplitudes, the angular phase space motion is slower (1/8 period shown below) => can lead to filamentation and emittance growth

stationary bucket accelerating bucket

Page 34: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 34

Capture of a Debunched Beam with Fast Turn-On

Page 35: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 35

Capture of a Debunched Beam with Adiabatic Turn-On

Page 36: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 36

From Synchrotron to Linac

In the linac there is no bending magnets, hence there is no dispersion effects on the orbit and =0 and =1/2.

sRC p2

sRC p2

cavity

Ez

s or z

lβ RFhC

lβ RF

Page 37: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 37

From Synchrotron to Linac (2)

Moreover one has:

Since in the linac =0 and =1/2, the longitudinal frequency becomes:

pRVeh

ss

srss p

ωγ2

cosˆ22

vmpERVh sssRFs 002ˆ γpωω

leading to:

vmEe

s

sRFs γ

ω3

0

02 cos

Since in a linac the independent variable is z rather than t one gets by using

in terms of ϕ(z):

vmEe

s s

sRF33

0

02

cos2γ

ωlp

0 sγ

dz =vsdt

The longitudinal distribution is fixed for higher energy!

Page 38: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 38

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 synchrotron, even ultra-relativistic, 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:

( )

( ) 0

0

2

2

2

Δ++

Δ++

Δ

sss

s

ssss

sss

EEE

EEE

EEdtd

The damping coefficient is proportional to the rate of energy variation and from the definition of s one has:

s

s

s

s

EE

2

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CAS Chios, 18-30 September 2011 39

Adiabatic Damping (2)

∫ .constdWI

( ) WpRhVetWH

ss

rss

22

41cos

),,( ωhp Δ

tWW s cosˆ

( ) ts sin

So far it was assumed that parameters related to the acceleration process were constant. Let’s consider now that they vary slowly with respect to the period of longitudinal oscillation (adiabaticity).

For small amplitude oscillations the hamiltonian reduces to:

with

Under adiabatic conditions the Boltzman-Ehrenfest theorem states that the action integral remains constant:

(W, are canonical variables)

WpR

hWH

dtd

ss

rsωhp

21

dtWpRhdt

dtdWI

ss

rs 2

21 ωhp

Since:

the action integral becomes:

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CAS Chios, 18-30 September 2011 40

Adiabatic Damping (3)

leads to:

s

WdtWˆ 2

2 pPrevious integral over one period:

2

2

constWpR

hIsss

rs

ωh

From the quadratic form of the hamiltonian one gets the relation:

ωh

p ˆ2ˆ Δrs

sss

hRp

W

Finally under adiabatic conditions the long term evolution of the oscillation amplitudes is shown to be:

EVRE

s

sss

4/1

2

4/1

cosˆˆ

Δ

h EEorW s

4/1ˆˆ Δ

W ⋅Δφ=invariant

Page 41: CAS Chios, 18-30 September 20111 LONGITUDINAL DYNAMICS Frank Tecker based on the course by Joël Le Duff Many Thanks! CAS on Intermediate Level Accelerator.

CAS Chios, 18-30 September 2011 41

Dynamics in the Vicinity of Transition Energy

one gets:

γγaγ

h 222

1 tIntroducing in the previous expressions:

Δ

γγγ

224/1

cosˆ1ˆ t

sV

Δ

γγγ

224/1

cosˆ1ˆ t

sVE

γγγ

22

2/1

cosˆ t

ss V

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CAS Chios, 18-30 September 2011 42

Dynamics in the Vicinity of Transition Energy (2)

In fact close to transition, adiabatic solution are not valid since parameters change too fast. A proper treatment would show that:

will not go to zero

E will not go to infinityt

t t

s Δ

EEs

ˆ