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Introduction to Accelerator Physics. DESY Summer Student Lecture 2009 Winni Decking DESY –MPY-

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Page 1: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Introduction to Accelerator Physics.

DESY Summer Student Lecture 2009Winni DeckingDESY –MPY-

Page 2: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Accelerator: A Definition

Device that provides accelerated particles with defined and controllable properties:

– Particle Species (electron, proton, ion)– Energy– Direction– Time structure– Intensity– Density

Accelerators are tailored to applications needs

Employ cutting edge and special developed technology to advance parameter space in any of the above areas

Page 3: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Accelerator Applications

• Direct particle beams on specific targets or collide beams with each other

• Produce thin beams for synchrotron light

• HEP: structure of atom, standard model, …• Bombard targets to obtain new materials with different properties• Synchrotron radiation: spectroscopy, X-rat diffraction, X-ray

microscopy, crystallography (of proteins), …• Medicine: use for Positron Emission Tomography (PET), cancer

therapy, surgery• Nuclear waste transmutation (conversion of long lived into short lived

nuclides)

Page 4: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Accelerators Worldwide

courtesy W. Mondelaers, JUAS 2004

CATEGORY NUMBER

Ion implanters 7000Industry 1500Radiotherapy 7500Medical isotopes 200Hadron therapy 20non-nuclear research 1000SR sources 70Nuclear & Particle physics res. 120TOTAL 17390

Page 5: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Accelerator Physics – What’s needed

• Basic knowledge– relativistic particle dynamics– classical theory of electromagnetism (Maxwell’s equations)

• Advanced Studies– Hamiltonian mechanics, optical concepts– Quantum scattering, radiation of charged particles– Statistical mechanics– Surface physics– Computing, ….

Page 6: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

What we will do

• Historical introduction• Review of relativity• Acceleration concepts• Ring concepts• Optical Functions• Luminosity• Synchrotron Radiation

• Questions and discussions

Page 7: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Rutherford Scattering

1906 – 1913 using α particles from a radioactive source to bombard a thin gold foil:Discovery of massive, non point-like structure of the nucleus

1927 E. Rutherford says, addressing the Royal Society : “... if it were possible in the laboratory to have a supply of electrons and atoms of matter in general, of which the individual energy of motion is greater even than that of the alfa particle, .... this would open up an extraordinary new field of investigation....”

But bright sources with such energies were not yet available: man-made devices, mainly built to produce X-rays, operated at the time in the hundred KV range.

Villard X-ray Tube 1898-1905

N(θ)

θ

Thomson-Model of Atom

Measurement and Rutherford-Model

Prediction

Page 8: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Basic Principles: Relativity

Relativistic Energy

Relativistic Momentum

Relationship between Momentum and Energy

Kinetic Energy

20

2 cmmcE γ==

cmmvp γβ0==

22

211-11 βγβ −===

cv

cv

420

222 cmcpE +=

( )120

20 −=−= γcmcmET

Page 9: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Basic Principles: Relativity

Speed of Light

Electron Rest Mass

Proton Rest Mass

Electron Charge

Electron Volts

Energy in eV

Energy and rest mass

[ ]

kg1078.1eV1

eV

Joule106021.11eV

Coulomb106021.1

MeV 3.938

keV 511s

m109979.2

362

20

2

19

19

2,0

2,0

8

×=

==

×=

×=

=

=

×=

cecm

emcE

ec

mc

m

c

proton

electron

γ

Page 10: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Motion in Electric and Magnetic Fields

Equation of motion under Lorentz Force

( )BvEqdtpdF

rrrr×+==

( ) EpqcBvEpqcdtpdpc

dtdEE

cmcpErrrrrr

rr

r

222

420

222

=×+==⇒

+=

Magnetic Fields do not change the particles energy, only electric fields do!

Technical challenge: provide large enough electric fields

Page 11: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Electrostatic Accelerators

Cockroft & Walton:

qUrddUqrdFE

dUqEqF

b

a

b

a∫∫ ===Δ

==

rrr

rr

useful unit charge×voltage = eV

1932: First particle beam (protons) produced for nuclear reactions: splitting of Li-nuclei with a proton beam of 400 keV

Today: Proton Pre-accelerator at PSI (Villingen)

Page 12: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Electrostatic Accelerators

Van de Graaff:• Mechanical transport of charges

creates high voltages• Maximum potential around 20 MV

(needs already SF6 gas surrounding to prevent discharges)

Today: 12 MV-Tandem van de GraaffAccelerator at MPI Heidelberg

Page 13: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Linear Accelerators (Basic Principle)

Wideroe (1928): apply acceleration voltage several times to particle beam

• acceleration of the particle in the gap between the tubes

• voltage has to be „flipped“ to get the right sign in the next gap RF voltage shield the particle in drift tubes during the negative half wave of the RF voltagevary the tube length with increasing energy/velocity

+ + + +-̶ -̶-̶

Page 14: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

0* * *sinn sE n q U ψ=Energy gained after n acceleration gaps

n number of gaps between the drift tubesq charge of the particleU0 Peak voltage of the RF SystemΨS synchronous phase of the particle

Kinetic energy of the particles21 *

2n nE m v= valid for non relativistic particles ...

=> velocity of the particle

02 2* * * *sinn Sn

E n q Uvm m

ψ= =

Acceleration in the Wideroe Structure

shielding of the particles during the negative half wave of the RF

t

U0 Length of the n-th drift tube:1* *

2 2RF

n n nRF

l v vτν

= =

Page 15: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

988totalE MeV=

310 /p MeV c=

2 2 2 2 40E c p m c= +

20k in to ta lE E m c= −

50kinE MeV=

Examples

DESY proton linac (LINAC III)

GSI Unilac

E ≈ 20 MeV per Nukleonβ ≈ 0.04 … 0.6 Protons/Ions

Page 16: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Acceleration in RF fields

Traveling wave structure:

• Particles in phase with waveform• Reduce phase velocity in

waveguide with irises

Example: SLAC 2 mile LINAC

E up to 50 GeVin operation since mid 60’sElectrons/Positronsν = 2.8 GHz, 35 MV/m

Page 17: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Klystron

courtesy E. Jensen, RF for LINACS, CAS 2005

• Energy/velocity modulated electron beam in first resonator

• After drift density modulation• Electric field extracted in

second resonator

Page 18: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

What is relativistic?

Electrons: β > 0.99 at 3.7 MeV

Protons: β > 0.99 at 6.7 GeV

Page 19: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Motion in a constant B-field (E=0)

• Energy stays constant• Spiraling trajectory along the uniform magnetic fieldLorentz Force

Zentrifugal Force

* ( )F q v B→ → →

= ×

2*m vFρ

=

2** * * /m vq v B B p qρρ

= → =

Page 20: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Cyclotron

Uses magnetic field to force particles to pass through accelerating fields at regular intervals

Cyclotron:• Constant B-field• Time for one revolution

• Constant revolution frequency = constant accelerating frequency

• Works only if m=const => non-relativistic particles• Large momentum => large magnets

2 2* z

mTv q Bρπ π= =

12 * .zz z

q B constT m

π ωω = = → =

qpB =ρ* E. Lawrence and his first

cyclotron

Page 21: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Synchrotron

• Varying B-field• Constant ρ

• Increase B-field synchronous to momentum p

Where is the acceleration?• RF field in accelerating cavity with the right (synchronous) phase

qpB =ρ*

Increase B → decreases ρ → particle comes early → gains more energy

0 sin( )p eUq φΔ =

Page 22: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Synchrotron

Synchronous accelerator where there is a synchronous RF phase for which the energy gain fits the increase of B-field at each turn.

revolution time

revolution frequency

RF frequencyh = harmonic number

=number of possible bunches

Magnetic rigidity

Page 23: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Technical design of a dipole magnet:a magnet with two flat, parallel pole shoescreates a homogeneous dipole field

0 00

0 0,

*FeFe

B BH Hμ μ μ

= =

Maxwells equations: DH jt

δδ

∇× = +r

r r r

n*I = number of coil windings, each carrying the current I

μr = rel. permeability of the material,μr (Fe) ≈ 3000

00

*nIBh

μ=

the magnetic field B depends on *the current* the number of windings* the gap height

( ) nIHlHhsdHdanH FeFeA

=+==×∇ ∫∫ ** 0rrrrr

Magnetic Dipole Fields

Page 24: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Dipole Fields and Max. Energies

For high energy machines (γ >> 1)

pcEcmcpE ≈⇒+= 420

222

]m[]T[3.0** ρρρ ××≈⇒=⇒= BEceEBq

pB

Technologynormal conducting: Bmax ≈ 2 Tsuper conducting : Bmax ≈ 7 T

Size (= money)

Page 25: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Example: HERA p

920 GeV Proton storage ringdipole magnetsN = 416, l = 8.8m, ρ=580 m, B = 5.5 Ttotal length 6.3 km (3.6 km dipoles)1990 till 2007

Page 26: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Example LHC

7 TeV Proton storage ringdipole magnetsρ=2810 m, B = 8.3 Ttotal length 27 km (17.6 km dipoles)turns on now !!!!!!!!!

Page 27: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

HEP: The energy frontier

ILC

SPEAR, DORIS (charm quark, τ lepton)

CESR, DORIS II

HERA

Page 28: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Synchrotron Radiation

• Particles radiate when accelerated, particle moving in a dipole is accelerated centrifugally and emits radiation tangential to the trajectory

• Total energy loss after one turn:

• Ratio of proton to electron mass is 1836• At the same energy and radius: ΔΕelectron :ΔΕproton≈1013

[ ]4

20

18

GeV/c]GeV[

]m[10034.6GeV][/ ⎟

⎟⎠

⎞⎜⎜⎝

⎛×=Δ

mErevE

ρ

B

Page 29: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Synchrotron Radiation

• Example HERA electron ring– E = 27 GeV– B = 0.16 T, ρ=580 m– ΔΕ≈ 80 MeV– Lots of RF stations and power installed in HERA-e

• Example HERA proton ring– E = 920 GeV– B = 5.5 T, ρ=580 m– ΔΕ≈ 10 eV– RF only needed for longitudinal focusing and acceleration

Page 30: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Linear Collider

e+ e-

15 km

For a Ecm = 500 GeV:

Effective gradient: 35 MV/m

Huge International Collaboration: ILC

No Bends, but lots of RF!

Page 31: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

TESLA Superconducting RF technology

•1.3 GHZ niobium cavities•2 K•23 MV/m for XFEL•35 MV/m for ILC•10 Hz•TTF linac

accelerator gradient MV/m30 4020

AC55 AC56AC57 AC58AC59 AC60AC61 AC62AC63 AC64AC65 AC66AC67 AC68AC69 AC79

1011

0 10109

1010

30 4020

AC55 AC56AC57 AC58AC59 AC60AC61 AC62AC63 AC64AC65 AC66AC67 AC68AC69 AC79

1011

0 10109

1010

23.6 MV/mun

load

ed q

ualit

y fa

ctor

Page 32: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Cavity String and Module Assembly

cold mass with cavities, magnet / BPM, HOM abs. beam pipe, valve

The XFEL accelerator module is based on the 3rd cryomodulegeneration tested at the TESLA Test Facility and designed by INFN.

Already 10 cryomodules have been built and commissioned for the TTF Linac.

Length 12.2 mTotal weight 7.8 t

Page 33: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Luminosity

.* reactR L= Σ production rate of (scattering) events is determinedby the cross section Σreactand a parameter L that is given by the design of the accelerator: … the luminosity

p-Bunch

e-BunchIP 2 σ

3*10^10 particles

7*10^10 particles

x yπ σ σ∗ ∗= 0 n b

I I1 e pL *24 e f

Page 34: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Synchrotron Radiation

• Radiation is produced in a narrow light cone of angle

• Radiation spot size depends thus on electron energy and beam size at source point

• A quality measure for synchrotron radiation is the brilliance (or brightness in US literature):Photon flux (per 0.1 % bandwidth) normalized with the total horizontal

and vertical photon source size and divergence

c vand electronsfor ]keV[

5111≈=≈

Eγθ

''24 yyxx

FBσσσσπ

=

Page 35: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Brightness Comparison

Page 36: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Transverse Beam Dynamics

To describe the motion of particles, each particle is characterized within a six-dimensional phase space (x,x’, y,y’,s,p)– x its horizontal (vertical) position– x’ its horizontal (vertical) slope– s its longitudinal position along the accelerator– p its momentum

IAll particles having the design momentum p will fly happily along the accelerator with (0,0, 0,0,s,pnom)

The trouble starts when– p ≠ pnom

– x,x’, y,y ≠ 0– dipoles are introduced

Page 37: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Focusing

Magnet imperfections, misalignments, gravitation, earth magnetic field, ….

Particles will not stay on a stable circular orbit (or follow a long straight pass) => need a magnet with increasing B-field away from the centre axis

four iron pole shoes of hyperbolic contour

ygFxgF

ygBxgB

yx

xy

* ,*

* ,*

=−=

=−=

focusing in one plane, defocusing in the other

02

2 nIgRμ

=

Page 38: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Focusing

Put many quadrupoles in a row – motion is confined‘FODO’ structure

Net focusing effect

Page 39: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Momentum: p = 920 GeV/c

Bending field: B = 5.5 Tesla

Quadrupol Gradient G= 110 T/m

k = 33.64*10-3 /m2

1/ρ = 1.7 *10-3 /m

1/B B

p q Bρ ρ= =

normalise magnet fields to momentum (remember: B*ρ = p / q )

Dipole Magnet Quadrupole Magnet

:/gk

p q=

Example: HERA p Ring

Focusing forces and particle trajectories

Page 40: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Under the influence of the focusing and defocusing forces the differential equation of the particles trajectory can be developed:

'' * 0x k x+ = horizontal plane

vert. plane: k k⇒ −if we assume ....* linear retrieving force* constant magnetic field* first oder terms of displacement x

... we get the general solution (hor. focusing magnet):

00( ) *cos( ) *sin( )xx s x ks ks

k′

= +

0 0( ) *sin( ) *cos( )x s x k ks x ks′ ′= − +

: dxxds

′ =

x = distance of a single particleto the center of the beam

Equation of Motion

Page 41: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

0

*' 's

x xM

x x⎛ ⎞ ⎛ ⎞

=⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠Matrices of lattice elements

⎟⎟⎟

⎜⎜⎜

−=

)l*Kcos()l*Ksin(K

)l*Ksin(K

)l*Kcos(MQF

1

⎟⎟⎟

⎜⎜⎜

⎛=

)l*Kcosh()l*Ksinh(K

)l*Ksinh(K

)l*Kcosh(MQD

1

10 1Drift

lM

⎛ ⎞= ⎜ ⎟

⎝ ⎠

Hor. focusing Quadrupole

Hor. defocusing Quadrupole

Drift spare

formalism is only valid within onelattice element where k = const

in reality: k = k(s)

Matrix Formalism

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Accelerator Physics Winni Decking

* we can calculate the trajectory of a single particle within a singlelattice element

* for any starting conditions x0, x´0* we can combine these piecewise solutions together and get the

trajectory for the complete storage ring

1 1 1 2* * * * ......lattice QF D QD D QFM M M M M M=

courtesy: K. Wille

Example: storage ring for beginners

Dipole magnets and QF & QD quadrupole lenses

Combination of Elements

Page 43: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

tracking one particle through the storage ring

Page 44: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

( ) * ( ) *cos( ( ) )x s s sε β ψ φ= +

β(s) given by focusing properties of the lattice ↔ quadrupoles

ε beam emittance = intrinsic beam parameter, cannot be changed by the foc. properties.

ε, Φ = integration constantsdetermined by initial conditions

The ‘Beta’ Function

equation of motion ( ) ( ) ( ) 0x s k s x s′′ − =

restoring force ≠ const, we expect a kind of quasi harmonick(s) = depending on the position s oscillation: amplitude & phase will dependk(s+L) = k(s), periodic function on the position s in the ring

Solution in the form

Page 45: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Transverse Phase Space

• Under linear forces, any particle moves on an ellipse in phase space• Ellipses shear in magnets, but their area is preserved

• General equation of ellipse is• with α,β,γ functions of the distance and ε constant• Area of ellipse is πε• Statistical definitions of emittance (for nonlinear beams)

– area covering 95% of all particles– 222 xxxx ′−′=ε

εγαβ =+′+′ 22 2 xxxx

Page 46: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

βεσ *=

( ) * ( ) *cos( ( ) )x s s sε β ψ φ= + max. amplitude of all particle trajectories

( ) * ( )x s sε β=

Beam Dimension:

determined by two parameters

x

ε in phase space= area

The ‘Beta’ Function

Page 47: DESY Summer Student Lecture 2009 Winni Decking DESY –MPY- · Accelerator Physics Winni Decking Accelerators Worldwide courtesy W. Mondelaers, JUAS 2004 CATEGORY NUMBER Ion implanters

Accelerator Physics Winni Decking

Emittance

• Storage rings:– electron storage rings: equilibrium between quantum excitation of

synchrotron radiation and longitudinal damping (source independent)

– proton storage rings: source size and energy (εN=ε×γ)• Linacs:

– source size and energy

x’+Δx’

Ps+ΔPs

Px

Ps

Pxx’

Acceleration

Δx’ ≈ -x’ Δp/p0 200 400 600 800 1000

0

10

20

30

40

50

60

Energie [GeV ]

Stra

hlgr

össe

im B

ogen

[mm

]

S trahlro hr

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Accelerator Physics Winni Decking

Undulator Radiation

Simulation of radiation coming from

an electron traveling on a racetrack trajectory

an electron traveling through an undulator (an array of alternating bending magnets)

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Accelerator Physics Winni Decking

Synchrotron Light Source PETRA III

E = 6 GeVε = 1 nm radC = 2.3 kmρ = 200 mStart in 2009

P ~ N

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Accelerator Physics Winni Decking

PETRA III Optics

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Accelerator Physics Winni Decking

Linear Accelerator based Self Amplification of Spontaneous Emission (SASE) Free Electron Lasers (FELs) in the hard X-Ray regime (~0.85 - 60 Å)

Need excellent electron beam quality:

• low emittance• low energy spread• extremely high charge density

Modulation of the electron charge density with the (synchrotron radiation) field

⇒ ‘micro-bunching’⇒ more and more electrons radiate

in phase until saturation is reached

SASE FEL

P ~ N2

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Accelerator Physics Winni Decking

European X-Ray Free Electron Laser (XFEL)

3.3 km

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Accelerator Physics Winni Decking

Further Issues

• Self Fields (particles interacting with each other)– repelling forces of same-charge particles limit particle density– higher energy helps

• Interaction with surroundings– Fields and image charges of particle beams interact with vacuum

chamber walls, creating additional fields– Act back on same bunch or next bunch => Instability

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Accelerator Physics Winni Decking

Summary

• Accelerator Physics is a very broad and interesting field • Upcoming big accelerators are the LHC (this year), the ILC (2015 ?),

and many FELs (European XFEL, LCLS, Spring8-XFEL …)• Future of the field towards more tailored and specialized devices• Novel acceleration techniques (plasma acceleration) are on the horizon

and desperately needed to advance the energy frontier

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Accelerator Physics Winni Decking

Acknowledgments

• This talk based on material from– Bernhard Holzer (previous summer student lectures)– Chris Prior (CAS 2004 and 2006)– Daniel Brandt (CAS 2006)

• Further Reading– CERN Accelerator School Proceedings http://cas.web.cern.ch/cas/– E. Wilson: Introduction to Accelerators– S.Y. Lee: Accelerator Physics– H. Wiedemann: Accelerator Physics 1&2– K. Wille: Beschleunigerphysik– ….

• Accelerator Physics Programs– MAD-X http://mad.home.cern.ch/mad/– elegant

http://www.aps.anl.gov/Accelerator_Systems_Division/Operations_Analysis/oagPackages.shtml