Transverse Motion 1

23
Transverse Motion 1 Eric Prebys, FNAL

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Transverse Motion 1. Eric Prebys, FNAL. The Journey Begins…. We will tackle accelerator physics the way we tackle most problems in classical physics – ie , with 18 th and 19 th century mathematics! Calculate ideal equilibrium trajectory - PowerPoint PPT Presentation

Transcript of Transverse Motion 1

Page 1: Transverse Motion 1

Transverse Motion 1Eric Prebys, FNAL

Page 2: Transverse Motion 1

The Journey Begins… We will tackle accelerator physics the way we

tackle most problems in classical physics – ie, with 18th and 19th century mathematics! Calculate ideal equilibrium trajectory Use linear approximations for deviations from this

trajectory Solve for motion Treat everything else as a perturbation to this

As we discussed in our last lecture, the linear term in the expansion of the magnetic field is associated with the quadrupole, so let’s start there…

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 2

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Quadrupole Magnets*

A positive particle coming out of the page off center in the horizontal plane will experience a restoring kick

xB

y

yB

x

)()()(

BlxB

BlxBx

lBBf

')(

*or quadrupole term in a gradient magnet

USPAS, Knoxville, TN, Jan. 20-31, 2014 3Lecture 3 - Transverse Motion 1

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What about the other plane?

pairs give net focusing in both planes -> “FODO cell”

xB

y

lBBf

')(

Defocusing!Luckily, if we place equal and opposite pairs of lenses, there will be a net focusing regardless of the order.

USPAS, Knoxville, TN, Jan. 20-31, 2014 4Lecture 3 - Transverse Motion 1

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Transfer matrices The simplest magnetic lattice consists of quadrupoles and

the spaces in between them (drifts). We can express each of these as a linear operation in phase space.

By combining these elements, we can represent an arbitrarily complex ring or line as the product of matrices.

)0(')0(

1101

')0(1)0(''

)0(

xx

fxx

xf

xx

xx

)0(')0(

101

)(')(

)0(')(')0(')0()(

xxs

sxsx

xsxsxxsx

Quadrupole:

sx

Drift:

12... MMMM NUSPAS, Knoxville, TN, Jan. 20-31, 2014 5Lecture 3 - Transverse Motion 1

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Example: FODO cell At the heart of every beam line or ring is the “FODO” cell,

consisting of a focusing and a defocusing element, separated by drifts:

The transfer matrix is then

f -fL L

fL

fL

fLL

fL

fL

f

L

f

L

1

211101

101

1101

101

2

22

M

USPAS, Knoxville, TN, Jan. 20-31, 2014 6Lecture 3 - Transverse Motion 1

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Where we’re going… It might seem like we would start by looking at beam lines and

them move on to rings, but it turns out that there is no unique treatment of a standalone beam line Depends implicitly in input beam parameters

Therefore, we will initially solve for stable motion in a ring. Rings are generally periodic, made up of more or less identical cells

In addition to simplifying the design, we’ll see that periodicity is important to stability

The simplest rings are made of dipoles and FODO cells Or “combined function magnets” which couple the two

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 7

Periodic “cell”

Our goal is to de-couple the problem into two parts

The “lattice”: a mathematical description of the machine itself, based only on the magnetic fields, which is identical for each identical cell

A mathematical description for the ensemble of particles circulating in the machine

Ncellcellcellcellring MMMMM

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Stability Criterion We can represent an arbitrarily complex ring as a

combination of individual matrices

We can express an arbitrary initial state as the sum of the eigenvectors of this matrix

After n turns, we have

Because the individual matrices have unit determinants, the product must as well, so

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 8

123... MMMMM nring

221 VVMVV 211 BAxx

BAxx

21 VVM nnn BAxx

21

21 /1

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Stability Criteria (cont’d) We can therefore express the eigenvalues as

However, if a has any real component, one of the solutions will grow exponentially, so the only stable values are

Examining the (invariant) trace of the matrix

So the general stability criterion is simply

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 9

complex generalin is where;; 21 aee aa

real is where;; 21 ii ee

cos2Tr ii eeM

2Trabs M

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Example Recall our FODO cell

Our stability requirement becomes f -f

L L

fL

fL

fLL

fL

fL

M1

21

2

22

fLfL 222abs

2

USPAS, Knoxville, TN, Jan. 20-31, 2014 10Lecture 3 - Transverse Motion 1

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Twiss Parametrization We can express the transfer matrix for one period as the sum of an identity

matrix and a traceless matrix

The requirement that Det(M)=1 implies

We can already identify A=Tr(M)/2=cosμ. If we adopt the arbitrary normalization

We can identify B=sinμ and write

Note that

So we can identify it with i=sqrt(-1) and write

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 11

)()()()(

1001

),(ss

ssBAsCs

M

1))()()(( 222 sssBA

1)()()( 2 sss

sincos)()(

)()(sin

1001

cos),( JI

ssss

sCsM

IJ

)()()(0

0)()()()()(

)()()()(

)()(2

22

ssssss

ssss

ssss

)(),( sesCs JM Remember this! We’ll see it again in a few pages

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Equations of Motion General equation of motion

For the moment, we will consider motion in the horizontal (x) plane, with a reference trajectory established by the dipole fields.

Solving in this coordinate system, we have

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 12

xy

s

sBvBvyBvxBvme

BBvvvsyx

me

mBveR

RmRmdtd

dtpdBveF

xyyxxsys

yx

syx ˆˆˆ0

ˆˆˆ

xr

Reference trajectory

Particle trajectory

yysrrxrr

yyxrsrsrxryysrsrsrxrxrRyysrxryyxrxrR

yyxrR

ˆˆ2ˆˆˆˆˆ2ˆˆˆˆˆˆˆ

ˆˆˆˆˆˆˆˆ

2

2

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Equations of Motion (cont’d) Equating the x terms

Re-express in terms of path length s. Use

Rewrite equation

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 13

BBv

pBev

mvBev

mBev

rr

ys

ys

s

ys

ys

2

22

2

r

s

rtvs

svrdt

dss

Note: s measured along nominal trajectory, vs measured along actual trajectory

rv

dsd

rv

dtd

dsd

rv

dsd

dtds

dtd s

ss

;2

22

2

2

1 ;12

2

2

22

22

22

2

22

xBByxx

BB

x

rrB

Bvr

BBv

rvr

dsrd

rv

xy

ys

ysss

terms)(rearrange

) (use xr

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Equations of Motion Expand fields linearly about the nominal trajectory

Plug into equations of motion and keep only linear terms in x and y

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 14

xx

sBBxx

sBBy

ysB

xx

sBsBsyxB

yy

sByy

sBxx

sBsBsyxB

yyyyyy

x

x

xxxx

)()()()(,0,0),,(

)()()(,0,0),,(

0coupling no

dipole nocoupling no

0)(1

0)(11

112)(111

)(

2

222

2

yy

sBB

y

xx

sBB

x

xxxx

sBB

xxB

xx

sBB

x

x

y

y

y

Looks “kinda like” a harmonic oscillator

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Piecewise solution These equations are in the form

For K (gradient) constant), these equations are quite simple. For K>0, it’s just a harmonic oscillator and we write

In terms if initial conditions, we identifyand write

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 15

sKbKsKaKsx

sKbsKasKAsxcossin)('

sincoscos)(

Kxbxa 0

0 ;

0

0

cossin

sin1cos)()(

xx

sKsKK

sKK

sKsxsx

0)( xsKx

Page 16: Transverse Motion 1

For K<0, the solution becomes

For K=0 (a “drift”), the solution is simply

We can now express the transfer matrix of an arbitrarily complex beam line with

But there’s a limit to what we can do with this

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 16

0

0

coshsin

sin1cosh

)()(

xx

sKsKK

sKK

sK

sxsx

0

0

00

101

)()(

)(

xxs

sxsx

sxxsx

nMMMMM ...321

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Closed Form Solution Our linear equations of motion are in the form of a “Hill’s Equation”

If K is a constant >0, then so try a solution of the form

If we plug this into the equation, we get

Coefficients must independently vanish, so the sin term gives

If we re-express our general solution

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 17

)()( ;0)( sKCsKxsKx Consider only periodic systems at the moment

)(cos)()( ssAwsx

0sin)2(cos)( 2 wwAKwwwAKxx

222

by mutliply '0'202wkwwwwww w

sincos

sincossincos

1221

1221

21

wkAwA

wkAwA

wAwAwAwAxAAwx

sKAsx cos)(

)()( BUT ),()( assume

sCsswCsw

03

2

Kwwkw

We’ll see this much later

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Solving for periodic motion Plug in initial condition (s=0Ψ=0) Define phase advances over one period

and we have

But wait! We’ve seen this before…

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 18

kwxwxA

wxA

002

01

)(cos);(sin CCCS

0

0

2

2

2

0

2

2

20

200

0

0

2

0

02

00

/

1)()(

'

)('

)(

xx

SkwwCS

kwkww

Sk

wSkwwC

CxCx

xSkwwCSx

kw

wk

Sw

kxkwx

kwwxCxCx

xSk

wxSkwwC

Sk

wwxwxCxCx

This form will make sense in a minute

Page 19: Transverse Motion 1

Recall the Twiss representation of a Period We showed a flew slides ago, that we could write

We quickly identify

We also showed some time ago that a requirement of the Hill’s Equation was that

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 19

sin)(cossin)(sin)(sin)(cos

)()()()(

sin1001

cos),(

ssss

ssss

sCsM

)()(1)(

)(21

21)(

)(

2

2

2

sss

dssd

kw

dsd

kwws

kws

dss

Csw

k Cs

s

0

0)(

1)()(

12

)(C

Phase advance over one period

Super important!Remember forever!

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Closing the Loop We’ve got a general equation of motion in terms of initial

conditions and a single “betatron function” β(s)

β(s) is a parameter of the machine, but we still don’t know its form! Important note!

(s) (and therefore (s) and Υ(s)) are defined to have the periodicity of the machine!

In general Ψ(s) (and therefore x(s)) DO NOT! Indeed, we’ll see it’s very bad if they do

So far, we have used the lattice functions at a point s to propagate the particle to the same point in the next period of the machine. We now generalize this to transport the beam from one point to another, knowing only initial conditions and the lattice functions at both points

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 20

)(

)( ;)(cos)()(0s

sdssssAsx

)(sin)(cos)()(

1

)(sin)()()(cos)()(

121)(

)(cos)()(

ssss

A

sds

sdsAsds

sds

Asx

ssAsx

cellcellNs

ds

21

)(21

Define “tune” as the number of pseudo-oscillations around the ring

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We use this to define the trigonometric terms at the initial point as

We can then use the sum angle formulas to define the trigonometric terms at any point Ψ(s1) as

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 21

0

00

0000

0000

)(sin

1)(cos

Ax

AxsS

AxsC

sincossin1

sincos)(sin)(sin

sinsincos1

sincos)(cos)(cos

00

0

0

00

00011

00

0

0

00

00011

Ax

AAx

CSsSs

Ax

AAx

SCsCs

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General Transfer Matrix We plug the previous angular identities for C1 and S1 into the

general transport equations

And (after a little tedious algebra) we find

This is a mess, but we’ll oftenrestrict ourselves to the extremaof , where

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 22

1111

1

11111

1cos

SCAx

CAAx

021

dsd

0

0

1

0

10

100

1

1

1

cossin1

sincos

xx

xx

Page 23: Transverse Motion 1

About the Tune The tune is the number of oscillations that a particle makes

around equilibrium in one orbit. For a round machine, we can approximate

Note also that in general

USPAS, Knoxville, TN, Jan. 20-31, 2014Lecture 3 - Transverse Motion 1 23

RRds

2

21

21

yx