R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 [email protected]...

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CHESS & LEPP 103 [email protected] Introduction to Accelerator Physics Fall semester 2017 ρ κ κ κ 1 with = = e e s ds d ! ! ds R d = ! κ κ e e e e e e s R e s b s ds d s ds d ds d s ! ! ! ! ! ! ! ! × ) ( b s ds d e T e e ! ! ! ' + = κ κ ( ) κ κ κ = = e e e e ds d s s ds d ! ! ! ! 0 κ e T e b ds d ! ! ' = ( ) ' 0 T e e e e b ds d b ds d + = = ! ! ! ! κ κ ) ( s R ! ) ( ) ( ) ( s e y s e x s R r y x ! ! ! ! + + = s b e x e T x y e T y x r ! ! ! ! ) 1 ( ) ' ' ( ) ' ' ( ' κ κ + + + + = Accumulated torsion angle T The Frenet Coordinate System

Transcript of R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 [email protected]...

Page 1: R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 Georg.Hoffstaetter@Cornell.edu Introduction to Accelerator Physics Fall semester 2017 ρ κ κ κ 1 ds d e s =

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ρκκ κ

1with =−= eesdsd !!

dsRd =!

κ

κ

eeeeee

sRe

sb

sdsd

sdsd

dsd

s

!!!

!!!

!!

×≡

−≡

≡ )(

bsdsd eTee !!! '+=κκ

( ) κκκ −⋅=⋅= eeee dsd

ssdsd !!!!0

κeTebdsd !! '−=

( ) '0 Teeee bdsd

bdsd +⋅=⋅=

!!!!κκ

)(sR!

)()()( seysexsRr yx!!!!

++=

sb exeTxyeTyxr !!!! )1()''()''(' κκ ++++−=

Accumulated torsion angle T

The Frenet Coordinate System

Page 2: R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 Georg.Hoffstaetter@Cornell.edu Introduction to Accelerator Physics Fall semester 2017 ρ κ κ κ 1 ds d e s =

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yyxxsdsd eee !!!

κκ −−=

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

by

bx!!!

!!!

+≡

−≡

κ

κ

sysydsd

sxsxdsd

eeTeeeTe!!!

!!!

κκ

κκ

==

==

)sin()cos(

)(sR!

)()()( seysexsRr yx!!!!

++=

dds!r = x ' !ex + y '

!ey + (1+ xκ x + yκ y )!es

The Curvi-linear System

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ppsrsrsph

mdtd

dsd !!"!"!

=== −−γ111

FFsps

epppeppeppp

sphm

dtd

syyxxsyysyxxsxdsd

!!"!"

!!!!

γ

κκκκ

===

+++−+−=−− 11

''' )()()(

s

h

yxyxdsd eyxeyexr !

""#""$%!!! )1('' κκ ++++=

⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜

+

+=

⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜

ysyphm

xsxphm

yph

xph

y

x

pFpFpp

ppyx

s

s

s

s

κ

κγ

γ

'

'

''

sphmst γ== −1' !

FppEpcpmcpcE

sph

dsd

dsd

dpd

!!!!

⋅==+= 2222 )()('

222 )()( mcpcE +=

Phase Space ODE

ddt!p =!F

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),,,,,( δτbyaxz =!

0

00

0

2

00

0

00

)()(,,,pEtt

vctt

EEE

pp

bppa yx −=−=

−=== τδ

01

00

00

00'

0

2

0

0

2

''

''

','',''

pKKKE

pKEKKt

pKbpKypKapKx

KpKx

vc

Et

vc

E

yb

xa

xx

px

ττ

δδ

δ

τ

−∂=∂−=⇒∂−=

∂=∂=⇒∂=−

⎩⎨⎧

−∂=∂=

−∂=∂=⇒

⎭⎬⎫

−∂=

∂=

New Hamiltonian:

0~ pKH =

Using a reference momentum p0 and a reference time t0:

Usually p0 is the design momentum of the beam And t0 is the time at which the bunch center is at “s”.

x'xa ≈

sΔ≈τ

6 Dimensional Phase Space

Page 5: R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 Georg.Hoffstaetter@Cornell.edu Introduction to Accelerator Physics Fall semester 2017 ρ κ κ κ 1 ds d e s =

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Only magnetic fields: 0=E!

Mid-plane symmetry: ),,(),,(,),,(),,( syxBsyxBsyxBsyxB yyxx −=−−=

0',)('

')()1())(1(

'

''

11)(

21

1)'(

1)(

0

0

00

00

00000

02220

=−=−==

=⇒++−=++++−=

+−=+==

=⇒====

++

−−+

δκτ

κδκκδκκ

κκκκ

x

ykbkxxkx

Bqvpa

byax

pE

vh

vpE

dsttd

pp

ysvpx

pp

xdtd

vph

pepp

pp

ppdpp

ppp

s

s

s

s

s

xxs

x

yx

x

z

x

!!

δκκ xxyxkbaH −+−++= 222122

212

212

21 )(

Hamiltonian:

Simplified Equation of Motion

xksyxByksyxB qp

qp

yqp

x000 1),,(,),,( +== ρ

Linearization in :

0,0

0

0

0

0

0 →→ −−−vvv

EEE

pppHighly relativistic :

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zsFz !! )('=

0z!

Linear equation of motion:

Matrix solution of the starting condition 0)0( zz !!=

01drift )( zLMz !!=

01drift2quad )()( zLMLMz !!=

01drift2quad3drift )()()( zLMLMLMz !!=

01drift2quad3drift4bend )()()()( zLMLMLMLMz !!=

Bend

Quadrupole

Matrix Solutions

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⎟⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜⎜

=

⎟⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜⎜

000

0

''''''

b

a

byax

δ

τ

0

0

0

0

00

00

1001

00

010

10

0010

1

zs

s

bsbyasax

byax

!

⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜

=

⎟⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜⎜

+

+

=

⎟⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜⎜

δ

τ

δ

τ

Note that in nonlinear expansion so that the drift does not have a linear transport map even though is completely linear.

ax ≠'

sxxsx '00)( +=

The Drift

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x ''+ x κ 2 = δκ

y '' = 0τ ' + xκ = 0

)sin()cos('' 2 sBsAxxx HHH κκκ +=⇒−=Homogeneous solution:

κδκκκκκκ

κκκκκκ

κκ

κδ

+−=+−−=

+++−=

+=

=

xsBsAxx

sBsAsBsAxssBssAx

220

)cos(')sin('''

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

!!!!! "!!!!! #$

!!!! "!!!! #$

Variation of constants:

⎟⎟⎠

⎞⎜⎜⎝

⎛=⎟⎟

⎞⎜⎜⎝

⎛⎟⎟⎠

⎞⎜⎜⎝

− δκκ

κκ 0''

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

ssss

(natural ring focusing)

The Dipole Equation of Motion

Page 9: R s κ with κ ! ! ! ! 0 e −κhoff/LECTURES/17F...CHESS & LEPP 103 Georg.Hoffstaetter@Cornell.edu Introduction to Accelerator Physics Fall semester 2017 ρ κ κ κ 1 ds d e s =

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⎟⎟⎟⎟⎟⎟⎟

⎜⎜⎜⎜⎜⎜⎜

−−−

=

−−

10])[sin(1

000

]1)[cos()sin(

010

10

)sin(0)]cos(1[0

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

11

11

κκκκκκ

κ

κκκκκ

κκ κ

ssss

sss

ssss

M

)sin()cos(with)sin()cos(1 sBsAx

BA

ss

BA

H

H κκκ

κκδ +=⎟⎟

⎞⎜⎜⎝

⎛+⎟⎟⎠

⎞⎜⎜⎝

⎛=⎟⎟⎠

⎞⎜⎜⎝

⎛ −

⎟⎟⎠

⎞⎜⎜⎝

⎛⎟⎟⎠

⎞⎜⎜⎝

⎛ −=⎟⎟

⎞⎜⎜⎝

δκκ

κκ 0)cos()sin()sin()cos(

''

ssss

BA

κτ x−='

The Dipole