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LONGITUDINAL DYNAMICS by Joël Le DuFF (LAL-Orsay) Introductory Level Course on Accelerator Physics Baden, 12-24 September 2004 CAS Baden, 12-24 September 2004 1

Longitudinal Dynamics I II III - CERN Accelerator School

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Page 1: Longitudinal Dynamics I II III - CERN Accelerator School

LONGITUDINAL DYNAMICS

by

Joël Le DuFF

(LAL-Orsay)

Introductory Level Course on Accelerator Physics Baden, 12-24 September 2004

CAS Baden, 12-24 September 2004 1

Page 2: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 2

summary

• Radio-Frequency Acceleration and Synchronism• Properties of Radio-Frequency cavities• Energy Gain• Principle of Phase Stability and Consequences• Synchronous linear accelerator• Energy-Phase oscillations• The capture phenomenon• The Synchrotron• RF cavities for Synchrotron• Dispersion Effects in a Synchrotron• Energy-Phase Equations in a Synchrotron• Phase space motions

Page 3: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 3

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)

Page 4: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 4

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

Page 5: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 5

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 , preferably along the direction of the initial momentum.

Er

eEdtdp=

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

ρBep=

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.

Page 6: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 6

Acceleration & Curvature

θo

x, rz

s

ρ

Within the assumption:

θEE →r

zBB →r

the Newton-Lorentz force:

BveEedtpd rrrr

×+=

becomes:( )

rzr uBevueEuvmudtmvd rrrr

θθθθ

θθ

ρ −=−2

ρθ

θθ

zBep

eEdtdp

=

=leading to:

Page 7: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 7

Energy Gain

In relativistic dynamics, energy and momentum satisfy the relation:

( )WEE += 0222

02 cpEE +=

Hence: vdpdE =

The rate of energy gain per unit length of acceleration (along z) is then:

zeEdtdp

dzdpvdz

dE ===

and the kinetic energy gained from the field along the z path is:

eVdzEeWdzeEdEdW zz =∫=⇒==

where V is just a potential

Page 8: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 8

Methods of Acceleration

1_ Electrostatic Field

Energy gain : W=n.e(V2-V1)

limitation : Vgenerator =Σ ViElectrostatic accelerator

2_ Radio-frequency Field

Synchronism : L=vT/2

Wideroe structurev=particle velocity T= RF period

Page 9: Longitudinal Dynamics I II III - CERN Accelerator School

Methods of Acceleration (2)

3_ Acceleration by induction

From MAXWELL EQUATIONS :

The electric field is derived from a scalar potential φ and a vector potential AThe time variation of the magnetic field H generates an electric field E

AHB

tAE

rrrr

rrr

×∇==

∂∂−∇−=

µ

φ

CAS Baden, 12-24 September 2004 9

Page 10: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 10

The advantage of Resonant Cavities

- Considering RF acceleration, it is obvious that when particles get high velocities the drift spaces get longer and one loses on the efficiency. The solution consists of using a higher operating frequency.

- The power lost by radiation, due to circulating currents on the electrodes, is proportional to the RF frequency. The solution consists of enclosing thesystem in a cavity which resonant frequency matches the RF generator frequency.

-Each such cavity can be independently powered from the RF generator.

- The electromagnetic power is now constrained in the resonant volume.

- Note however that joule losses will occur in the cavity walls (unless made of superconducting materials)

Ezr

JouHrr

ωRF

Page 11: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 11

The Pill Box Cavity

02

2

002 =

∂∂−∇ t

AA µε )( HouEA =

( )krJEz 0=

( )krJZj

H 10

−=θ

Ω==== 37762,220Zack λω

λπ

e tjω

Ez Hθ

From Maxwell’s equations one can derive the wave equations :

Solutions for E and H are oscillating modes, at discrete frequencies, of types TM ou TE. For l<2a the most simple mode, TM010, has the lowest frequency ,and has only two field components:

Page 12: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 12

The Pill Box Cavity (2)

The design of a pill-box cavity can be sophisticated in order to improve its performances:

-A nose cone can be introduced in order to concentrate the electric field around the axis,

-Round shaping of the corners allows a better distribution of the magnetic field on the surface and a reduction of the Joule losses. It also prevent from multipactoringeffects.

A good cavity is a cavity which efficiently transforms the RF power into accelerating voltage.

Page 13: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 13

Transit Time Factor

tgVtEEz ωω coscos0 ==

vtz=

Oscillating field at frequency ω and which amplitude is assumed to be constant all along the gap:

Consider a particle passing through the middle of the gap at time t=0 :

dzvz

geVW

g

g∫=∆

2/

2/cosωThe total energy gain is:

angletransitvgωθ=

factortimetransitTeVTeVW ==∆ 2/2/sin

θθ

( 0 < T < 1 )

Page 14: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 14

Transit Time Factor (2)

Consider the most general case and make use of complex notations:

( ) dzezEeE tjgze

ω∫ℜ=∆ 0

( ) ⎥⎦

⎤⎢⎣

⎡∫ℜ=∆ − dzezEeeE v

zjgz

je

p ωψ0

( ) ⎥⎦

⎤⎢⎣

⎡∫ℜ=∆ − g v

zj

zjj

e dzezEeeeE ip

0

ωψψ

( ) φω

cos0∫=∆ g vzj

z dzezEeE( )( )∫

∫= g

z

g tjz

dzzEdzezE

T0

pvzt ψωω −=

ip ψψφ −=

Ψp is the phase of the particle entering the gap with respect to the RF.

and considering the phase which yields the maximum energy gain:

Introducing:

Page 15: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 15

Important Parameters of Accelerating Cavities

Shunt Impedance

RVPd

2=Relationship between gap

voltage and wall losses.

Quality Factor

Relationship between stored energy in the volume and dissipated power on the walls.P

WQd

sω=W

VQR

sω2

=

Filling Time

ωτ Q=WQdtWdP s

sd

ω=−=Exponential decay of the stored energy due to losses.

Page 16: Longitudinal Dynamics I II III - CERN Accelerator School

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.

is the energy gain in one gap for the particle to reach the nextgap with the same RF phase: P1 ,P2, …… are fixed points.sVeseV Φ= sinˆ

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 Baden, 12-24 September 2004 16

Page 17: Longitudinal Dynamics I II III - CERN Accelerator School

A Consequence of Phase StabilityTransverse Instability

00 <∂

∂⇒>

z

zE

t

VLongitudinal phase stability means :

defocusing RF force

000. >∂∂

⇒=∂∂

+∂∂

⇒=∇x

Ez

Ex

EE xzxThe divergence of the field iszero according to Maxwell :

External focusing (solenoid, quadrupole) is then necessary

CAS Baden, 12-24 September 2004 17

Page 18: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 18

The Traveling Wave Case

( )

( )0

0 cos

ttvz

vk

kztEE

RF

RFz

−=

=

−=

ϕ

ωω

velocityparticlev

velocityphasev

=

=ϕThe particle travels along with the wave, and k represents the wave propagation factor.

⎟⎠

⎞⎜⎝

⎛−−= 00 cos φωω

ϕtv

vtEE RFRFz

00 cosφϕ EEandvv z ==If synchronism satisfied:

where φ0 is the RF phase seen by the particle.

Page 19: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 19

Multi-gaps Accelerating Structures:A- Low Kinetic Energy Linac (protons,ions)

Mode 2π L= vT = βλMode π L= vT/2In « WIDEROE » structure radiated power ∝ ω CV

In order to reduce the radiated power the gap is enclosed in a resonant volume at the operating frequency. A common wall can be suppressed if no circulating current in itfor the chosen mode.ALVAREZ structure

Page 20: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 20

CERN Proton Linac

Page 21: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 21

Multi-gaps Accelerating Structures:B- High Energy Electron Linac

- When particles gets ultra-relativistic (v~c) the drift tubes become very long unless the operating frequency is increased. Late 40’s the development of radar led to high power transmitters (klystrons) at very high frequencies (3 GHz).

- Next came the idea of suppressing the drift tubes using traveling waves. However to get a continuous acceleration the phase velocity of the wave needs to be adjusted to the particle velocity.

solution: slow wave guide with irises iris loaded structure

Page 22: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 22

Iris Loaded Structure for Electron Linac

Photo of a CGR-MeV structure

4.5 m long copper structure, equipped with matched input and output couplers. Cells are low temperature brazed and a stainless steel envelope ensures proper vacuum.

Page 23: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 23

Energy-phase Equations

- Rate of energy gain for the synchronous particle:

sss eEdt

dpdzdE φsin0==

- Rate of energy gain for a non-synchronous particle, expressed in reduced variables, and :ss EEWWw −=−= sφφϕ −=

( )[ ] ( )ϕϕφφϕφ smalleEeEdzdw

sss .cossinsin 00 ≈−+=

- Rate of change of the phase with respect to the synchronous one:

( )ss

RF

sRF

sRF vv

vvvdzdt

dzdt

dzd −−≅⎟

⎠⎞

⎜⎝⎛ −=⎟

⎠⎞

⎜⎝⎛

⎟⎠⎞⎜

⎝⎛−= 2

11 ωωωϕ

( ) ( ) 30

22

2ss

ss

ss vmwccvvγ

βββββ ≅−≅−=−Since:

Page 24: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 24

Energy-phase Oscillations

wvmdz

dss

RF33

0 γωϕ −=one gets:

Combining the two first order equations into a second order one:

022

2

=Ω+ ϕϕsdz

d33

0

02 cosss

sRFs vm

eEγ

φω=Ωwith

Stable harmonic oscillations imply:

realands 02 >Ω

hence: 0cos >sφAnd since acceleration also means: 0sin >sφ

One finally gets the results: 20 πφ << s

Page 25: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 25

The Capture Problem

- Previous results show that at ultra-relativistic energies (γ >> 1) the longitudinal motion is frozen. Since this is rapidly the case for electrons, all traveling wave structures can be made identical (phase velocity=c).

- Hence the question is: can we capture low kinetic electrons energies (γ < 1), as they come out from a gun, using an iris loaded structure matched to c ?

( )tEEz φsin0=e-

β0 < 1vϕ=c

gun structureThe electron entering the structure, with velocity v < c, is not synchronous with the wave. The path difference, after a time dt, between the wave and the particle is: ( )dtvcdz −=Since:

cvkfactornpropagatiowithkzt RFRFRF

ωωωφϕ==−=

φπλ

φω ddcdz g

RF 2== ( )βλπφ −= 12 cdt

dg

one gets: and

Page 26: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 26

The Capture Problem (2)

( ) ( )( )

φβ

ββγ sin1

021

200 eEdt

dcmdtdcmmvdt

d =⎟⎟⎟

⎜⎜⎜

−==

From Newton-Lorentz:

Introducing a suitable variable:

αφα 2

0

0 sinsincmeE

dtd −=the equation becomes:

2112coscos

21

0

0

0

20

0 ≤⎟⎠⎞

⎜⎝⎛+−=− ββ

λπφφ Ee

cmg

ααα

λπφφ deE

cmdg

20

20

sincos12sin −=−

dtd

dd

dtd α

αφφ =Using

Integrating from t0 to t

(from β=β0 to β=1)21

0

02

00 1

1⎟⎠⎞

⎜⎝⎛+−≥ ββ

λπ

gecmECapture condition

Page 27: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 27

Improved Capture With Pre-buncher

A long bunch coming from the gun enters an RF cavity; the reference particle is the one which has no velocity change. The others get accelerated or decelerated. After a distance L bunch gets shorter while energies are spread:bunching effect. This short bunch can now be captured more efficiently by a TW structure (vϕ=c).

Page 28: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 28

Improved Capture With Pre-buncher (2)

The bunching effect is a space modulation that results from a velocity modulation and is similar to the phase stability phenomenon. Let’s look at particles in the vicinity of the reference one and use a classical approach.

Energy gain as a function of cavity crossing time:

φφ 00002

0 sin21 eVeVvvmvmW ≈=∆=⎟

⎠⎞⎜

⎝⎛∆=∆

00

0vm

eVv φ=∆

Perfect linear bunching will occur after a time delay τ, corresponding to a distance L, when the path difference is compensated between a particle and the reference one:

RFvtvzv ω

φτ 00. ==∆=∆ (assuming the reference particle enters the cavity at time t=0)

Since L = vτ one gets:

RFeVWvL ω0

02=

Page 29: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 29

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

⇒=

==

=

=Φ=Φ

Φ

ρ

ρ

ωω

sin^

Energy gain per turn

Synchronous particle

RF synchronism

Constant orbit

Variable magnetic field

If v = c, ωr hence ωRF remain constant (ultra-relativistic e- )

Page 30: Longitudinal Dynamics I II III - CERN Accelerator School

The Synchrotron (2)

Energy ramping is simply obtained by varying the B field:

v

BRerTBeturnpBe

dtdp

eBp′

=′=∆⇒′=⇒=ρπ

ρρρ2

)(

pvEcpEE ∆=∆⇒+=222

02Since:

( ) ( ) φρπ ssturn VeRBeWE sinˆ'2 ==∆=∆

•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 Baden, 12-24 September 2004 30

Page 31: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 31

The Synchrotron (3)During the energy ramping, the RF frequency increases to follow the increase of the revolution frequency :

hence :

),( sRF

r RBh

ωωω ==

)()(

2

2

1)()(

2

1

2

)()(tB

sR

r

tsE

ec

h

tRFftB

m

e

sR

tv

h

tRFf

πππ=⇒><==

Since , the RF frequency must follow the variation of the

B field with the law : which asymptotically tends

towards when B becomes large compare to (m0c2 / 2πr) which corresponds to

v c (pc >> m0c2 ). In practice the B field can follow the law:

2220

2cpcmE +=

21

2)(

2)/

20(

2)(

2

)(

⎭⎬⎫

⎩⎨⎧

+=

tBecrcm

tB

sR

c

h

tRFf

π

Rcfr π2

tBtB

tB2

2sin)cos1(

2)(

ωω =−=

Page 32: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 32

Single Gap Types Cavities

Pill-box variantsnoses disks

Coaxial cavityType λ/4

Page 33: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 33

Ferrite Loaded Cavities

- Ferrite toroids are placed around the beam tube which allow to reach lower frequencies at reasonable size.

- Polarizing the ferrites will change the resonant frequency, hence satisfying energy ramping in protons and ions synchrotrons.

Page 34: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 34

High Q cavities for e- Synchrotrons

Page 35: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 35

LEP 2: 2x100 GeV with SC cavities

Page 36: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 36

Dispersion Effects in a Synchrotron

cavity

Circumference

2πR

If a particle is slightly shifted in momentum it will have a different orbit:

dpdR

Rp=αE

This is the “momentum compaction” generated by the bending field.

E+δE

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

r=ηp=particle momentum

R=synchrotron physical radius

fr=revolution frequency

Page 37: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 37

Dispersion Effects in a Synchrotron (2)

θ

0ss

pdpp +

dθx( ) θρ

θρdxds

dds+=

=0dpdR

Rp=α

The elementary path difference from the two orbits is:

ρx

dsdl

dsdsds ==−

00

0

leading to the total change in the circumference:< >m means that the average is considered over the bending magnet only

mm

xdRxdsdsxdRdl =⇒∫=∫ ∫== 0012 ρρπ

RD

mx=αpdpDx x=Since: we get:

Page 38: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 38

Dispersion Effects in a Synchrotron (3)

RdRd

fdf

Rcf

r

rr −=⇒= β

βπβ

2dpdf

fp r

r=η

( )( )

( ) βββ

ββ

βββγ ddd

pdp

cEmvp 12

21

2

21

20 1

11 −

−=−

−+=⇒==

αγη −= 21

pdp

fdf

r

r ⎟⎠⎞

⎜⎝⎛ −= αγ 2

1

αγ 1=trη=0 at the transition energy

Page 39: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 39

Phase Stability in a Synchrotron

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

Stable synchr. Particle for η<0

η > 0

Page 40: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 40

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 followother 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

Page 41: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 41

First Energy-Phase Equation

θR

∫=∆−=∆⇒= dtwithhhff rrRF ωθθφ

For a given particle with respect to the reference one:

( ) ( ) dtd

hdtd

hdtd

rφφθω 11 −=∆−=∆=∆

cpEE 2220

2 +=

pRpvE srss ∆=∆=∆ ωs

r

rs

s

dpdp

⎟⎠⎞

⎜⎝⎛= ω

ωηSince: and

( ) φηωφ

ηωω&

rs

ss

rs

ss

rs hRp

dtd

hRpE −=∆−=∆one gets:

Page 42: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 42

Second Energy-Phase Equation

The rate of energy gained by a particle is: πωφ 2sinˆ rVedt

dE=

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

)sin(sinˆ2 sr

VeE φφωπ −=⎟⎠⎞⎜

⎝⎛∆ &

Expanding the left hand side to first order:

( ) ( )ETdtdETTEETTETE rsrsrrsrr ∆=∆+∆=∆+∆≅∆ &&&&&

leads to the second energy-phase equation:

( )srs

VeEdtd φφωπ sinsinˆ2 −=⎟

⎠⎞

⎜⎝⎛ ∆

Page 43: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 43

Equations of Longitudinal Motion

( )srs

VeEdtd φφωπ sinsinˆ2 −=⎟

⎠⎞

⎜⎝⎛ ∆( ) φηω

φηωω

&rs

ss

rs

ss

rs hRp

dtd

hRpE −=∆−=∆

deriving and combining

( ) 0sinsin2ˆ =−+⎥⎦

⎤⎢⎣⎡

srs

ss Vedtd

hpR

dtd φφπ

φηω

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

Page 44: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 44

Small Amplitude Oscillations

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

ss

srss pR

Vehπ

φηω2

cosˆ2=Ω( ) 0sinsincos

2=−Ω+ s

ss φφφφ&& with

Consider now small phase deviations from the reference particle:

( ) φφφφφφφ ∆≅−∆+=− ssss cossinsinsinsin (for small ∆φ)

and the corresponding linearized motion reduces to a harmonic oscillation:

02 =∆Ω+ φφ s&& stable for and Ωs real02>Ωs

γ < γtr η > 0 0 < φs < π/2 sinφs > 0

γ > γtr η < 0 π/2 < φs < π sinφs > 0

Page 45: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 45

Large Amplitude Oscillations

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

( ) 0sinsincos2

=−Ω+ ss

s φφφφ&& (Ωs as previously defined)

Multiplying by and integrating gives an invariant of the motion:φ&

( ) Iss

s =+Ω− φφφφφ sincoscos2

22&

which for small amplitudes reduces to:

( ) Is =∆Ω+ 222

22 φφ& (the variable is ∆φ and φs is constant)

Similar equations exist for the second variable : ∆E∝dφ/dt

Page 46: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 46

Large Amplitude Oscillations (2)

Equation of the separatrix:

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

in the phase space( ) is shown

as closed trajectories.

φφ ∆Ω ,s

&

( ) ( ) ( )( )ssss

ss

s

s φφπφπφφφφφφ sincoscossincoscos2

222−+−Ω−=+Ω−

&

Second value φm where the separatrix crosses the horizontal axis:

( ) ( ) ssssmm φφπφπφφφ sincossincos −+−=+

Page 47: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 47

Energy Acceptance

From the equation of motion it is seen that reaches an extremum when , hence corresponding to .

Introducing this value into the equation of the separatrix gives:

φ&0=φ&& sφφ =

( ) sss φπφφ tan222 22max −+Ω=&

That translates into an acceptance in energy:

( )⎭⎬⎫

⎩⎨⎧−=⎟

⎠⎞⎜

⎝⎛ ∆ φηπβ s

ssG

EhVe

EE ˆ 2

1

maxm

( ) ( )[ ]φπφφφ ssssG sin2cos2 −+=

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

Page 48: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 48

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

Page 49: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 49

Potential Energy Function

( )φφ Fdtd =2

2

( ) φφ ∂∂−= UF

( ) ( ) FdFU ss

s00

2sincoscos −∫ +Ω−=−= φ φφφφφφ

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 50: Longitudinal Dynamics I II III - CERN Accelerator School

CAS Baden, 12-24 September 2004 50

Ions in Circular Accelerators

Er = A E0

m = γ mr

P = m v

E = γ Er

A =atomic number

Q =charge state

q = Q e

W = E – Er

P = q B r

E2 = p2c2 + Er2

( )222 rBcqEE r =−

( )22

02 rBceAQEA

WA

W⎟⎠⎞

⎜⎝⎛=⎟

⎠⎞⎜

⎝⎛ +

⎥⎦⎤

⎢⎣⎡ +−== r

drB

dBE

EEdEdW r22

Moreover:

dr/r = 0 synchrotron dB/B = 0 cyclotron