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1 1 - - 1 1 LA-UR 09-01205 US Particle Accelerator School 2009 US Particle Accelerator School 2009 University of New Mexico University of New Mexico - - Albuquerque NM Albuquerque NM Theory and Practice of Free-Electron Lasers Particle Accelerator School Day 1 Dinh Nguyen, Steven Russell & Nathan Moody Los Alamos National Laboratory

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  • 11--11LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Theory and Practice ofFree-Electron Lasers

    Particle Accelerator SchoolDay 1

    Dinh Nguyen, Steven Russell& Nathan Moody

    Los Alamos National Laboratory

  • 11--22LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Course Content

    1. Introduction to Free-Electron Lasers2. Basics of Relativistic Dynamics3. One-dimensional Theory of FEL4. Optical Architectures5. Wigglers6. RF Linear Accelerators7. Electron Injectors

    Chapter

    ChapterChapter

    ChapterChapter

    Chapter

    Chapter

  • 11--33LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Course Schedule

    ElectronInjectorsRF LinacOptical Architectures1-D FEL Theory

    SimulationLab

    SimulationLab

    SimulationLab

    SimulationLab

    Final Exam

    Lab Report DueRF LinacWigglersOptical Architectures1-D FEL Theory

    Final ExamRF LinacWigglersOptical Architectures

    Intro. to FEL

    Relativistic Dynamics

    FridayThursdayWednesdayTuesdayMonday9:00

    10:45

    12:151:15

    3:15

    5:30

    10:30

    3:30

  • 11--44LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Chapter 1Introduction to Free-Electron Lasers

  • 11--55LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Introduction to Free-Electron Lasers

    • The nature of light• Gaussian beam• Laser beam emittance• Longitudinal coherence• How a quantum laser works• How an FEL works• Basic features of FEL• RF-linac FEL• Fourth-generation Light Sources• Applications of FEL

  • 11--66LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    We can treat the EM wave as a sinusoidal plane wave. In our convention, the electric field is in the x direction and magnetic field in the y direction. For a wave travelling in the positive z direction, the fields are given below

    where k = wavenumber in m-1= angular frequency in s-1= phase in radians

    Light can be described as bothparticles (photons) and waves

    • Light consists of photons each having energy where h = Planck’s constant (h = 6.626 x 10-34 J-s) and = frequency of the light; Photon energy can be calculated from wavelength as follows

    hvE

    1.24( )

    eV

    E

    v c

    82.9979 10 mcs

    B

    E

    • Light can also be described as a travelling electromagnetic (EM) wave.

    c

    12.4(Å)keV

    E

    0

    0

    ˆ( , ) cos( )ˆ( , ) cos( )

    z t E kz tz t B kz t

    E xB y

  • 11--77LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Gaussian Laser Beam

    rms radius in x

    -4.0 -3.0 -2.0 -1.0 0.0 1.0 2.0 3.0 4.0

    w

    x

    x

    Intensity

    .135 I0

    I0

    2 22 2

    2

    2( , )x yw wPI x y e e

    w

    2 xw

    22

    ( , )

    ( , )x

    I x y x dxdy

    I x y dxdy

    1/e2 radius

    2 2ln 2 xFWHM

    Full width at half max (FWHM)

    FWHM

    2.355 xFWHM

  • 11--88LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Gaussian Beam Propagation

    0w

    Diffraction limit

    22 2

    0 21R

    zw wz

    Parabolic expansion of 1/e2 radius with z

    0w

    At large z the divergence angle scales with /w0

    The product of the waist radius and converging angle of a diffraction limited beam is the wavelength divided by . Focusing the beam to small spots requires large angles.

    20

    Rwz

    Rayleigh length

  • 11--99LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Laser Beam Emittance

    dxxdz

    ( , )x x

    photonsz

    ' 4x x

    Photon beam emittance

    ( , )x x

    x

    xconverging

    x

    xwaist

    x

    xdiverging

    0' 4 4rms x x

    wA

    Light phase space area = times x(rms radius) times x’ (rms angle)

  • 11--1010LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Longitudinal Coherence

    If and are the full-width at half max (FWHM), the transform limit becomes

    4 2 0 2 40

    5 108

    1 109

    1.5 109

    2 109

    g t( )

    ttime (ps)

    inte

    nsity

    (W/c

    m2 )

    Coherence length

    Fourier transform

    4 2 0 2 40

    0.2

    0.4

    0.6

    0.8

    1

    0

    f ( )

    55 frequency (THz)

    An optical pulse with length is fully coherent if its coherence length ≥ 2 c

    0.44 2 2

    4ln 2

    0 0t

    t t

    I I e I e

    2

    cL

    Gaussian pulse

  • 11--1111LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    How a quantum laser works

    An external source of energy excites electrons from the ground state to an excited state

    Electrons from excited state decay to a metastable energy level with long lifetime (transition from this level to the ground state is quantum mechanically forbidden) → population inversion

    A co-propagating light beam stimulates emission of radiation → amplification of co-propagating light beam (Light Amplification by Stimulated Emission of Radiation)

    g

    em

    Absorption Population Inversion Stimulated Emission

  • 11--1212LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    How an FEL works

    Electrons in an FEL are not bound to atoms or molecules. The “free” electrons traverse a series of alternating magnets, called a “wiggler,” and radiate light at wavelengths depending on electrons’ energy, wiggler period and magnetic field.

    light (electromagnetic wave)

    v┴

    v║Bwy z

    x

    wigglermagnets

    electron trajectory

    unbunched electron beam pulse

    bunched electron beam pulse

  • 11--1313LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    How an FEL works (cont’d)

    The wiggler induces transverse sinusoidal velocity in electron beam

    Energy exchange occurs between the transverse electron current and transverse electric field of a co-propagating light beam

    Depending on the phase of the light beam with the electrons’ wiggling motion, some electrons gain energy while others lose energy → energy modulation →bunching of electrons along the axial direction into microbunches with period equal to an optical wavelength

    Microbunched electron beams radiate coherently at higher power →amplification of the co-propagating light beam.

    Note: The subscript ┴ denotes transverse and s stands for signal.

    sW e E

  • 11--1414LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Basic features of FEL• Wavelength tunable• Diffraction limited optical beam• Longitudinally and transversely coherent• High power (GW peak, 100kW to MW average)• Efficient (with energy recovery)

    0.1nm 1nm 10nm 100nm 1 10 100 1mm 10mm 100mm

    Gamma X-rays VUV IR THz mm-wave waveVisible

    Eb 10GeV 1GeV 100MeV 10MeV 1MeV 100keV

  • 11--1515LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Wavelength Tunability

    22 12w

    wa

    w wiggler period resonant wavelength

    relativistic factoraw (also Krms) rms wiggler parameter

    0 00

    0.662w ww

    eBa B T cmk m c

    20

    1 2T T MeVm c

    For electrons (m0c2 = 0.511 MeV)

    Select coarse wavelength by choosing the electron beam energy, wiggler period and wiggler magnetic field. Fine-tune wavelength by adjusting electron beam energy or wiggler magnetic field.

    Another convention uses peak parameter K2

    2 12 2w K

    0

    0

    2 ww

    eBK ak m c

  • 11--1616LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Radio-frequency Linac FEL

    Electron Injector

    RF Linac

    Bunch Compressor

    Wiggler

    FEL Beam

    Beam Dump

    Single-pass AmplifierSelf-Amplified Spontaneous Emission (SASE)

    Electron Injector

    Energy Recovery Linac

    Beam Dump

    Booster

    Wiggler

    Outcoupler High Reflector

    FELOscillator

  • 11--1717LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    RF-Linac FEL Pulse Structure

    FEL macropulseTmacro

    1RF

    RF

    tf

    n tRF

    FEL micropulses

    RF wave train

  • 11--1818LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Temporal & Spectral StructuresSASE FEL have spiky temporal and spectral features.

    Unsaturated oscillator/amplifier FEL have smooth temporal and spectral profiles.Oscillator/Amplifiertime domain

    Oscillator/Amplifierspectraldomain

    SASEtime domain

    SASEspectraldomain

  • 11--1919LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    FEL optical beam properties

    • Intensity

    2p

    x y

    N hvB

    t

    20

    2 pN hvIw t

    2p

    x y

    Nt

    B

    W/m2

    W/cm2

    photons/(m2 s 0.1% BW)

    1

    wN

    • Brightness

    • Spectral bandwidth

    • Brilliance

  • 11--2020LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    InjectorInjectorat 2at 2--km pointkm point

    1 km S1 km S--band band linaclinac

    ee TransportTransport

    UndulatorUndulatorExperiment HallExperiment Hall

    4th Generation Light Source (4GLS)

    Peak brilliance of linac-based 4th generation light sources (XFEL) is 8-10 orders of magnitude higher than that of 3rd generation light sources and >20 orders of magnitude above Bremsstrahlung sources.

    Linac Coherent Light Source (LCLS)

  • 11--2121LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Some examples of 4GLS

    250 fs80 fs75 fsBunch length

    1.5 cm1.3 (1.838)

    50 m

    3.56 cm2.33 (3.3)

    200 m

    3 cm2.62 (3.7)

    55 m

    Wiggler periodaw (K)Length

    2 m1.4 m0.4 mrms emittance

    1 nC1 nC0.25 nCBunch charge

    Pulsed DC gunCeB6 thermionic

    L-band RF gunCs2Te photocathode

    NCRF, 2.856 GHzCu photocathode

    Gun type, frequencyCathode

    NCRF, 5.712 GHz0.75 km

    SRF, 1.3 GHz3.4 km

    NCRF, 2.856 GHz1 km

    Linac type, frequencyLength

    8 GeV20 GeV14.3 GeVBeam energy

    0.1 nm12.4 keV

    0.1 nm12.4 keV

    0.15 nm8 keV

    WavelengthX-ray energy

    Spring-8HyogoJapan

    DESYHamburgGermany

    SLACPalo Alto, CA

    USA

    InstitutionLocationCountry

    SCSSEuropean XFELLCLS

  • 11--2222LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Peak brilliance of 4GLSPulse energy ~ 1 mJ

    Photon energy ~ 1 keV

    # of photons ~ 1013

    rms emittance ~ 10-4 m

    rms bunch length ~ 10-13 s

    Energy spread ~ 0.01% BW

    Brilliance ~ 1033 (s m2 0.1% BW)-1

  • 11--2323LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    High-average-power FEL

    • Ground-based FEL Program (Boeing/LANL, LLNL/TRW)

    • Energy-recovery FEL (e.g. Jefferson Lab FEL)

    Jefferson Lab FEL holds the world record in cw average power (14 kW).

  • 11--2424LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Applications of FEL and 4GLSFEL Features Wavelengths Examples of applications

    • Ultrashort tunable pulses– Medicine 1-6 m Laser surgery– Physics XUV Ultrafast spectroscopy– Chemistry XUV, UV Chemical dynamics– Biology X-rays Protein structures

    • High peak power– High-density physics X-rays Warm dense matter– Materials sciences near-IR Laser machining

    • High average power– Directed energy IR Defense– Space near-IR Power beaming– Material processing UV Lithography

  • 11--2525LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Chapter 2Basics of Relativistic Dynamics

  • 11--2626LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Basics of Relativistic Dynamics• Special relativity• Lorentz transformation• Relativistic Doppler shifts• Wavelength dependence on angle• Relativistic velocity, momentum & energy• Lorentz force law• Curvilinear coordinate system• Linear beam dynamics• Emittance• Emittance & energy spread requirements

  • 11--2727LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Special Relativity

    1. All inertial frames are completely equivalent with regard to physical phenomena

    2. The speed of light in vacuum is the same for all observers in inertial frames of reference.

    Beam Framey’

    x’

    z’

    v

    Lab Framey

    x

    z

    e- beam

  • 11--2828LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Lorentz Transformation

    ( )( )

    '''

    '

    x xy yz z ct

    ct ct z

    g b

    g b

    ==

    = -

    = -2

    11

    c

    gb

    ub

    =-

    =Transverse dimensions are unchanged.

    Lorentz factor

    Velocity relative to c

    Lengths of moving objects along direction of motion appear to becontracted in the Lab frame by a factor (Lorentz-FitzGerald contraction)

    Clocks in the moving objects run slower by as observed in the Lab frame (time dilation).

    x

    y

    z

    y’

    x’

    z’

    cBeam coordinates

    Labcoordinates

  • 11--2929LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Wiggler period contracts in beam frame

    Lab frame

    y

    x

    z

    w

    x’

    z’

    y’

    Beam framew

    ' ww

    ll

    g=

    Wiggler period in beam frame

  • 11--3030LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Lorentz Transformation of Fields

    ( )( )

    '

    '

    '

    x x z y

    y y z x

    z z

    E E B

    E E B

    E E

    g u

    g u

    = +

    = -

    =

    Electric field

    Transverse electric and magnetic fields are different in the beam frame. Pure electric (and magnetic) fields in the Lab frame transform into mixed electric and magnetic fields in the beam frame. Longitudinal (along the direction of motion) electric and magnetic fields remain the same.

    '2

    '2

    '

    zx x y

    zy y x

    z z

    B B Ec

    B B Ec

    B B

    ug

    ug

    æ ö÷ç= - ÷ç ÷çè øæ ö÷ç= + ÷ç ÷çè ø

    =

    Magnetic field

  • 11--3131LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Electromagnetic Field Transformation

    x’

    z’

    y’

    Beam frameF’ = -e (E’ + v’ x B)

    B’

    E’

    F = -e (v x B)B

    Lab framey

    x

    z

    v

    Wiggler magnetic field deflects electrons in x direction

    Electromagnetic field deflects electrons in x’ direction

    v’ ~ 0 in beam frameForce is almost entirely due to electric field

    Force is due to magnetic field in Lab frame

  • 11--3232LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Radiation in Beam Frame

    x’

    z’

    y’

    Beam frame Wiggler electromagnetic wave behaves like virtual photons impinging on the electrons

    B’

    E’

    ''ww

    c cgn

    l l» =

    Real photons are scattered off the electrons. They can also be seen in the beam frame as circular waves radiated from the electrons at frequency ’

    Lorentz contraction causes ’ to be increased by a factor of compared to Lab frame

    View from the top

  • 11--3333LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Useful Relativistic Relations

    2

    2

    2

    2

    112

    112

    1 112

    1 112

    bg

    bg

    b g

    b g

    » -

    - »

    » +

    - »

    Approximations for ~ 1Exact relations

    22

    22

    2 2 2

    11

    11

    1

    gb

    bg

    b g g

    =-

    = -

    = -

    2 2 2

    1 1 1b g b

    = -

  • 11--3434LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Lorentz Transformation ofFrequency and Angle

    ( )

    '

    1 cosn

    ng b q

    =-

    Relativistic Doppler shift depends on Lab frame observation angle

    '

    2n

    ng

    =

    Forward ()

    '2n gn=

    Use approximation 211

    2b

    g- »

    Relativistic Doppler shift in the forward direction

    Backward ( = )

    ( )' 1 cosn g b q n= -

    For >>1 Lorentz transformation yields 1/ emission angle

    ( ) ( )22 '1 cos 1 cos 1 cosq g b q q- = - -1/'1 cosq

    qg

    -=

    For small angles

  • 11--3535LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Longitudinal Doppler Shift (Forward)

    x’

    z’

    y’

    Beam frame

    2

    2 ' 2

    2w

    w

    c

    c

    gn gn g

    l

    gn

    l

    æ ö÷ç ÷= = ç ÷ç ÷çè ø

    =

    22wllg

    =Combined effect of Lorentz contraction and Doppler shift gives a factor of 2 increase in frequency

    2 'n gn=

    Doppler effect causes up-shift in frequency and narrowing of emission angle

    Consider radiation emitted in the forward direction (same direction as electrons)

    Lab framey

    x

    z

  • 11--3636LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Longitudinal Doppler Shift (Backward)

    x’

    z’

    y’

    Beam frame

    ' 12 2 2w w

    c cn gn

    g g l l

    æ ö÷ç ÷= = =ç ÷ç ÷çè ø

    2 wl l=

    Lorentz contraction is negated by Doppler shift. Frequency is reduced by a factor of 2.

    Doppler effect causes down-shift in frequency

    Lab framey

    x

    z

    Consider radiation emitted in the backward direction (opposite to beam direction)

    '

    2n

    ng

    =

  • 11--3737LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Wavelength Dependence on Angle

    ( )2 22 12wll g qg

    » +

    Forward wave

    ( )1wl l b= +Backward wave

    The wavelength of wiggler (undulator) radiation depends on emission angle. Shortest wavelengths are radiated in the forward direction ( = 0). Radiation at larger angles have longer wavelengths. The opening half angle of wiggler radiation, is given by

    w

    2 waqg

    =

  • 11--3838LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Relativistic Energy & Momentum2 2 2

    0 0E T m c mc m cg= + = =

    Multiply by c and square

    Energy is in unit of MeV or GeV.Momentum is in unit of MeV/c or GeV/c

    Total energy

    Kinetic energy

    Momentum

    ( ) ( )2 20 0 1T m m c m c g= - = -

    0p m m cu bg= =

    ( ) ( ) ( )( )2 22 2 2 2 2 20 01cp m c m cb g g= = -

    Energy right triangle ( ) ( )222 20E cp m c= +moc2

    cpE

  • 11--3939LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Parameter Variation Table

    d

    d

    dpp

    d

    dpp

    d

    1

    1

    1

    2

    2 2

    2

    1 2 2

    1

    2

    1

    2

  • 11--4040LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Relative velocity differencesbecome smaller at high energy

    0

    0.2

    0.4

    0.6

    0.8

    1

    1 2 3 4 5 6 7 8 9 10

    2 2

    1d db gb b g g

    =

    Most electron accelerators are speed-of-light (=1) machinesAt large , it becomes very hard to perform ballistic bunch compression because all electrons travel nearly at the speed of light.

  • 11--4141LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Relative momentum change issame as energy spread at high energy

    2

    1dp dp

    gb g

    =

    0

    2

    4

    6

    8

    10

    12

    1 2 3 4 5 6 7 8 9 10

    p (m

    oc)

    Bunch compression via momentum spread can be done at any energyGiven sufficient energy spread and dispersive elements such as magnetic chicanes, electron bunches can be compressed to ultrashort pulses.

  • 11--4242LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Lorentz Force Law

    e F E v B

    In MKS units, e = 1.6 x 10-19 coulomb, electric field is in volts/m and magnetic field is in tesla.

    Electric force acts on electrons along their direction of motionand thus changes the electrons’ kinetic energy.

    Magnetic force is perpendicular to direction of motion and does not change the electrons’ kinetic energy. Magnetic field can be used to change momentum, i.e. bend electron beams.

    T d e d F s E s

    p dt e dt F B

  • 11--4343LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Bending Relativistic Beams

    0

    tan

    tan

    1

    b

    b

    b

    pp

    p F t e B t eB sEp m cc

    s ecB sE

    ecBE

    q

    u

    bg

    qr

    r

    ^

    ^

    =

    = D =- D =- D

    = =

    D - D= =

    =

    bend radius

    11 ( )299.8

    b

    B TmE MeV

    1299.8 b

    B T m E MeV

    Magnetic rigidity

    incident beamdipole magnet

    bent beam

    Bend angle and radiuss

    p┴

    p║

  • 11--4444LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Curvilinear Coordinate

    y

    x

    y

    Trajectory ofreference particle

    s

    x

    Electrons travel in the s direction. Use (x, y, s) coordinate system to follow the reference electron, an ideal particle at the beam center with a curvilinear trajectory. The reference particle trajectory takes into account only pure dipole fields along the beam line. The x and y of the reference trajectory are thus affected only by the placement and strength of the dipole magnets.

    For other electrons, define x’ and y’ as the slopes of x and y with respect to s

    dxxds

    dyyds

  • 11--4545LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Paraxial Rays & Trace SpaceParaxial ray approximation deals with non-crossing trajectories near the axis.

    z( , )x x

    x

    x’

    x

    x’

    x

    x’

    In a drift space, converging beams come to a waist and then diverge

  • 11--4646LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Lorentz Forces

    20

    y yecB eBxm c p

    0

    x xeB eBym c p

    Lorentz force in x2

    0 2 y yd xm e B ecBdt

    2

    0 2 x xd ym e B ecBdt

    Lorentz force in y

    1dx dxxds c dt

    2 2

    2 2 2

    1d x d xxds c dt

    Slope of x with respect to s

    Curvature of x with respect to s

  • 11--4747LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Quadrupole LensA quadrupole is a focusing element in one plane (e.g., x) and defocusing in the other plane (e.g., y). Its magnetic field, and thus the focusing force, increases linearly with distance from the center. .

    Quadrupole

    x

    y

    Quadrupole field

    Before quadrupole

    x

    x’

    x

    x’Quadrupole focusing After drift

    x

    x’

  • 11--4848LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Linear Beam Dynamics

    0xx K x 0yy K y Mathieu-Hill Equations

    Linear beam dynamics is valid if the restoring forces in x and y are linear.Quadrupoles are linear focusing (and defocusing) elements since the restoring forces are linear with distance from the center.

    A system of alternating focusing and defocusing quadrupoles separated by drift space (abbreviated FODO) is used to transport electron beams.

    Rx

    Ry

  • 11--4949LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Phase space concept

    Beams are treated as a statistical distribution of particles in x’-x (also in y’-yand -ct) phase space (trace space, to be exact). We can draw an ellipsearound the particles such that 50% of the particles are found within the ellipse. The area of this ellipse is a measure of rms spread of electron distribution in phase space. The rms emittance is area of the ellipse divided by . Emittance has dimension of length (e.g. microns) since x’ is dimensionless. Traditionally, emittance has unit of mm-mrad.

    rmsA

    x

    xwaist

    x

    xconverging

    x

    xdiverging

  • 11--5050LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Beam Emittance

    22 2,rms x x x xx

    Emittance is defined using ensemble averages, denoted by < >, of x2 and x’ 2 and x’-x correlation. The correlation vanishes at the waist (upright ellipse) and rms beam emittance becomes xx’ where is the rms radius in x and is the rms spread in x’.

    Ensemble average of x2 Ensemble average of x’2 x’-x Correlation

    2x x

    2x x

    22 01

    1 Nj

    jx x x

    N 22

    1

    1 Nj

    j

    x xN

    01

    1 Nj j

    jxx x x x

    N

    Root-mean-square x emittance (for y emittance, replace x with y)

  • 11--5151LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Liouville’s Theorem

    If the beam is accelerated, emittance (defined by x and x’) is not a conserved quantity because x’ decreases as the axial momentum increases by .

    n u

    Liouville’s theorem : In the absence of non-linear forces or acceleration, the beam ellipse area in x-px phase space is conserved. If the forces acting on the beam are linear, its emittance is also conserved.

    .xx p const

    px

    pz

    x’ = px/pzpxpz

    x’ = px/pz accelerated

    By accelerating the beam (increasing pz), we reduce the “un-normalized”emittance (also known as Lab frame emittance). The conserved quantity is the normalized emittance, un-normalized emittance multiplied by . Normalized emittance is used to specify the quality of electron beams regardless of energy.

  • 11--5252LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Electron Beam Emittance Requirement

    4n

    At a fixed wavelength and beam energy, the required normalized rms emittance for FEL is

    Accelerating the electron beam reduces its un-normalized emittance (adiabatic damping). Beams with large (bad) normalized emittance need to be accelerated to high energy.

    nu

    Electrons’ phase-space area must be less than photons’ phase space area for efficient energy exchange between electrons and photons

    x

    x

    photons

    electrons

    x

    x

    x

    x

    4e uA

  • 11--5353LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Energy Spread Requirement

    c t

    Electron beam’s energy spread must be smaller than the electrons’velocity spread over the interaction length.

    For oscillator FEL, interaction length ~ wiggler length

    For SASE and amplifier FEL, interaction length ~ gain length

    Uncompressed electron beams have small energy spread and low peak current. Compressed beams have high current and large energy spread.

    c t

    12 wN

  • 11--5454LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Chapter 31-D Theory of FEL

  • 11--5555LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    One-dimensional Theory of FEL• Transverse motion in a wiggler• Figure 8 motion and harmonics• Pendulum equation• FEL bunching• Bunched beam radiation• Spontaneous emission spectrum• Madey’s theorem• Low-gain FEL• Synchrotron oscillation• Saturation• Extraction efficiency• High-gain FEL• Self-consistent FEL equations

  • 11--5656LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Equations of Motion 0ˆ cosy wB yB k z

    wwk

    2

    Byy

    x

    zvz

    0 ˆˆ cosx z o wF m x e z y B k z

    For most FEL, vx is much smaller than vz . We can ignore the second force equation and consider only motion in x (the wiggle plane).

    Lorentz force laws

    0 ˆ ˆ cosz x o wF m z e x y B k z

  • 11--5757LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Equations of Motion (cont’d)

    x

    z

    cc

    x z x 2z zdx x xdt

    0

    coso weBx k zm c

    Small-angle approximation: transverse motion is small; axial velocity is almost c

    Rewrite Lorentz force equation in term of second derivative with respect to z

    Lorentz force equation

    2

    20

    cosz o wed xx B k z

    dt m

    2

    2 2 2z

    d z x xxdz c

    Transverse accelerationTransverse velocity

    Second derivative of x with respect to z ( ) coso wB z B k zConsider only on-axis magnetic field

  • 11--5858LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Solution to Transverse EOMIntegrate Lorentz force equation once to obtain deflection angle

    0

    00

    0

    cos

    sin

    2 sin

    ow

    ow

    w

    ww

    eBx k z dzm ceBx k z xk m c

    ax k z x

    Integrate again to obtain position

    0

    0 0

    2 sin

    2 cos

    ww

    ww

    w

    ax k z x dz

    ax k z x z xk

    Transverse motion is periodic with wiggler wavenumber kw. Wiggler magnetic force is harmonic oscillator’s restoring force. Transverse motion in the absence of field errors is given by

    2 0wx k x 2w

    w

    k

    x’0 = initial deflection anglex0 = initial position

    Wiggler wavenumber

  • 11--5959LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    B field, deflection and position

    Wiggler magnetic field

    + error - error

    First integral of field (deflection)

    Second integral of field (position)

    2cos sinwo w waB k z dz k z

    2cos coswo w ww

    aB k z dz dz k zk

    coso wB k z

  • 11--6060LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Transverse and longitudinal velocities

    2 sinwx wca k z

    2 2 2 2

    22 2 2 2

    2

    22 2 2

    2 2

    2 sin

    211 sin

    z x

    wz w

    wz w

    c

    ac k z

    ac k z

    2 2

    2 2

    11 cos 2

    2 2w w

    z w

    a ac k z

    Transverse velocity is oscillatory with period equal to the wiggler period

    Longitudinal velocity

    Axial velocity oscillates with a period equal to one-half the wiggler period

    vx

    vz

    v = c

    2

    2 cos 22w

    z z wca k z

    Find the square root and use small x approximation (1 + x)½ ≈ 1 + ½ x

    ( )( )2 2211 1 2 sin

    2z w wc a k zu

    g

    é ùê ú= - +ê úë û

    ( ) ( )22sin 1 cos 2w wk z k z= -Use sine squared identity

  • 11--6161LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Figure 8 MotionIn the reference frame that travels at the electrons’ average axial velocity, vz as given by 2

    2

    11

    2w

    z

    ac

    Electrons’ transverse and axial motions are coupled. At zero crossing, transverse speed is at a maximum and axial speed a minimum. At the edges, transverse speed is zero and axial speed is at a maximum. Electrons’motion on the x-z plane follows the figure 8.

    ' ' '

    2' ' '

    ' 2

    2 sin

    cos 22

    x

    z

    ww

    ww

    w

    ca k z

    ca k zk

    Motion in reference electron’s rest frame

    Figure 8 motion gives rise to harmonicsin spontaneous (incoherent) radiation

  • 11--6262LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Energy exchange betweenelectrons and FEL beam

    sdW j Edt

    sinw wecaj ecx k z

    Transverse electron current Plane-wave transverse electric field

    ,0( , ) cos( )s sE z t E kz t

    2

    0 0 sin cos( )w wd m c eca E k z kz t

    dt

    2

    0 0 sin2

    ww

    d m c eca E k k z tdt

    Rate of energy exchange depends on the phase of the “ponderomotive wave”

  • 11--6363LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Resonance ConditionQuestion: How can an optical wave traveling at the speed of light interact with slower electrons in a fast wave device (e.g., FEL)?

    Answer: If the optical wave slips ahead of the electrons exactly one wavelength every wiggler period, the sum of wiggler phase and optical phase is constant, and energy exchange can occur.

    .

    0

    w

    wz

    k k z t constd k kdz

    2

    2

    12

    ww

    ak k

    2

    2

    12

    ww

    a

    w

    ww

    z

    c

    Resonance wavelength satisfies this condition

    2

    22

    2

    1211

    2

    ww

    w

    akk k k ka

  • 11--6464LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Ponderomotive phase = -/2kwz = 0

    kz - t = -/2

    (kw + k)z – t = -/2

    j

    Eskwz =

    kz - t = -3/2

    (kw + k)z – t = -/2

    Es

    j

    0dWdt

    Electrons gain energy

    j

    Es

    Electrons gain energy (light is absorbed)

    Optical wave slips ahead by every w

  • 11--6565LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Ponderomotive phase = 0

    j

    Es

    j

    Es

    No energy gain or loss

    Optical wave slips ahead one

    j

    Eskwz =

    kz - t = -

    (kw + k)z – t = 0

    kwz = 0

    kz - t = 0

    (kw + k)z – t = 00dW

    dt

    No energy gain or loss

  • 11--6666LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Ponderomotive phase = /2

    j

    Es

    kwz = 0

    kz - t = /2

    kwz =

    kz - t = -/2

    j

    Es

    Electrons lose energy (FEL gains energy)

    Optical wave slips ahead by every w

    (kw + k)z – t = /2

    (kw + k)z – t = /2

    j

    Es

    0dWdt

    Electrons lose energy

  • 11--6767LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Ponderomotive WaveThe electrons interact with the so-called ponderomotive wave with frequency and wavenumber kw + k. The ponderomotive wave is synchronous with the resonant electrons, i.e. those at the zero phase of the ponderomotive wave. The ponderomotive phase velocity, divided by kw + k, is slightly less than the speed of light. The phase of the ponderomotive wave is defined by average arrival time of the electrons

    wk k z t

    wz

    d k kdz

    Taking derivative with respect to z

    Average electron axial velocity 2

    2

    112

    wz

    ac

    2k

    where

  • 11--6868LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Phase Equation

    2 wR

    d kdz

    2 2

    2 2

    1 11

    2 2w w

    w w

    a ad k k k kdz c

    Evolution of phase along the wiggler

    1RR R

    Define an energy difference relative to the resonant energy R

    The phase of individual electrons evolves along the wiggler according to their energy difference relative to the resonance energy

    2

    2R

    w wd k kdz

    Using the definition for resonance condition in k space 22 12w wRkk a

    2

    1 2RR

  • 11--6969LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Energy Exchange Equation

    sins wcka addt

    Rewrite the above equation in terms of derivative with respect to z of the energy difference relative to the resonant energy, R

    2 sins w

    R R

    ka addz

    Energy exchange rate depends on the phase of electrons in the ponderomotive potential. Electrons with phase between –and 0 gain energy. Electrons with phase between 0 and lose energy.

    ,02

    0

    ss

    eEa

    km cDefine a dimensionless signal field parameter, as

    The energy of an electron relative to the resonance energy evolves according to the sine of its phase in the ponderomotive wave

  • 11--7070LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Coupled First-OrderDifferential Equations

    2 sin

    2

    s w

    R R

    wR

    ka addz

    d kdz

    sinv a

    v

    Evolution of relative energy difference and phase along the wiggler

    Define new variables, and a

    22

    2 w

    R

    s w

    R

    k

    v

    ka aa

    Pendulum equations

    Rate of energy gain/loss along z

    Rate of phase change along z

    angular phase

    = angular velocity

    |a| = height of potential well

    = oscillation frequency

  • 11--7171LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Hamiltonian SystemHamiltonian mechanics is useful in representing beam physics because it relies on something being conservative. In the case of a pendulum, the conserved quantity is the total energy of the system of two canonical conjugate variables , the angular momentum, and , the angular phase.

    2

    cos2

    H a

    Hamiltonian = Total energy

    Potential energyKinetic energy

    Hamiltonian equations

    sinH a

    H

  • 11--7272LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Pendulum Equations

    sinv a

    sinv a

    v

    Coupled non-linear 1st order differential equations

    Particles rotate clockwise in phase space as the rate of change of is proportional to -sin and the rate of change of is . Particles follow elliptical trajectories each of which corresponds to a constant energy. Higher energies occupy larger ellipses up to phase angle of ± .

  • 11--7373LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Small-angle Solutions

    2v

    v

    2 0

    The small-angle oscillation frequency is known as the synchrotron frequency 0. The synchrotron frequency is proportional to the square root of dimensionless optical field (fourth root of intensity).

    01

    s wR

    ka ag

    W =

    0sin

    Small-angle approximation, i.e. sin ~ leads to harmonic solutions with oscillation frequency , square root of |a|

    Second-order differential equation

    and its solution

  • 11--7474LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Large-angle Close-orbit Solutions

    Solutions corresponding to large-angle oscillations can be solved numerically. The large-angle oscillation frequency is lower than the small-angle synchrotron frequency and approaches zero at = ± Oscillation frequency is given by

    where K : elliptic function. 20 02

    sin2

    K

    p

    zW

    =æ öæ öW ÷ç ÷ç ÷÷ç ç ÷÷ç ÷ç è øè ø

    20

    0

    116zW

    » -W

    Oscillation frequency for initial angle up to

  • 11--7575LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Separatrix

    Motion at the two nodes, , vanishes. These are unstable equilibrium points, corresponding to the pendulum at the top. The separatrix is the boundary separating trapped and un-trapped trajectories. The region inside the separatrix is called the “bucket.” The bucket height is proportional to the square root of the optical field (fourth root of optical intensity).

    Separatrix for a uniform wiggler

    0 2 cos 1v Bucket half-height

    max 21s w

    w

    a ava

  • 11--7676LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Laser Field and Bucket Height

    ,02

    0

    ss

    eEa

    km cDimensionless optical (signal) field parameter, as

    The electric field of the FEL beam depends on the optical intensity and free space impedance ,0 02s LE Z I

    Laser intensity depends on power and mode radius20

    2 LL

    PIw

    1 x 10-3max

    3 x 10-6as

    6 x 1010Electric field (V/m)

    5 x 1014Intensity (W/cm2)

    1.5 x 1010Peak power (W)

    X-ray FEL at 1.5 Å

    0 377Z

    max 21s w

    w

    a aa

    Bucket half-height

  • 11--7777LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Open Orbits

    Motion has large angular velocity. The pendulum rolls over the top and librates about the pivot point. The corresponding phase space trajectories are not elliptical. These represent un-trapped electrons outside the “bucket.” The un-trapped electrons also provide FEL gain. The electrons at small phases near the top of the “bucket” flow down into the “troughs”and lose energy to the optical field. As the optical field grows, the bucket also grows in height and eventually capture these electrons.

  • 11--7878LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    2 0 220

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    1 PHSP.11

    i

    2 0 220

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    1 PHSP.11

    i

    4 6 820

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.75 .75 PHSP.11

    i

    2 4 6 820

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.6 .6 PHSP.11

    i

    2 4 620

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.5 .5 PHSP.11

    i

    2 4 620

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.422 .422 PHSP.11

    i

    2 4 620

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.365 .365 PHSP.11

    i

    2 4 620

    10

    0

    10

    20Phase Space

    Theta

    Ener

    gy

    20

    20

    PHSP.10

    i

    2.3 .3 PHSP.11

    i

    Synchrotron Oscillation Animation

    2w

  • 11--7979LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Synchrotron Oscillation Animation

    2 4 6

    50

    0

    50

    Phase Space

    Theta

    Ener

    gy

    60

    60

    PHSP.10

    i

    2.3 .3 PHSP.11

    i

    2 4 6

    50

    0

    50

    Phase Space

    Theta

    Ener

    gy

    60

    60

    PHSP.10

    i

    2.15 .15 PHSP.11

    i

    0 2 4 6

    50

    0

    50

    Phase Space

    Theta

    Ener

    gy

    60

    60

    PHSP.10

    i

    2. . PHSP.11

    i

    0 2 4

    50

    0

    50

    Phase Space

    Theta

    Ener

    gy

    60

    60

    PHSP.10

    i

    1.85 .15 PHSP.11

    i

    0 2 4

    50

    0

    50

    Phase Space

    Theta

    Ener

    gy

    60

    60

    PHSP.10

    i

    1.8 .2 PHSP.11

    i

    2w

    Change scale

  • 11--8080LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    MicrobunchingThe FEL interaction causes the electrons to gain or lose energy, depending on their ponderomotive phase. Electrons with positive ponderomotivephase lose energy and migrate to the bottom of the bucket. Electrons with negative ponderomotive phase gain energy and move to the top of the bucket. The resulting energy modulation causes the electrons to develop density modulation with period of the radiation wavelength. The bunched electrons radiate higher power, i.e. it amplifies the electromagnetic wave. As the electric field of the electromagnetic wave increases, the height of the bucket also increases. When the electrons are completely bunched, FEL power is saturated. Microbunching is responsible for harmonic generation (the Fourier transform of short bunches has high frequency components).

    Courtesy of S. Reiche

  • 11--8181LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Radiation from bunched beam

    e

    incoherent e

    E NI N

    (a)w

    (b)2

    e

    coherent e

    E N

    I N

    Electrons at the wiggler entrance are randomly distributed (a). Randomly distributed electrons radiate incoherently, i.e. the electric fields of Ne randomly distributed wave trains with Nw (Nw is the number of wiggler periods and is the wavelength) add incoherently. The total electric field is proportional with square root of Ne. The spontaneous radiation intensity scales with Ne.

    Near saturation, the electrons are bunched into microbunches with bunch length z less than radiation wavelength (b). The electric fields of Ne wave trains scales with Ne, and the coherent radiation intensity scales with Ne2.

    Nw

    Nw

    lb lb lb

    z

  • 11--8282LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Spontaneous Emission

    [ ]

    222 2 22

    20

    sin 2( )2 1

    w e ww

    w

    e N N adW JJ ad d c a

    gw pe

    æ öDæ ö ÷ç÷ ÷ç ç÷ ÷= ç ç÷ ÷ç ç÷ç ÷W + Dè ø ç ÷è ø

    Spectral and angular energy fluence of spontaneous emission radiation from a planar wiggler as a function of frequency detuning from resonance condition

    2 wN

    Spontaneous emission is peaked at zero detuning (resonant wavelength)

    Frequency detuning

    20 15 10 5 0 5 10 15 200

    0.125

    0.25

    f ( )

    2sin 2

    1

    wNwwD

    =

    ( ) ( ) ( )0 1JJ J Jx x x= -

    ( )2

    12 4

    JJ x xxé ù » - -ë û

    ( )2

    22 1w

    w

    aa

    x =+Approximation for small

    Difference between J0 and J1 Bessel functions

  • 11--8383LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Spontaneous Emission (cont’d)Consider only photons within coherent spectral bandwidth and solid angle

    2

    w wNpl

    pql

    =

    2

    0

    14 137e

    ca

    pe= »

    where = fine structure constant

    [ ]2

    22( ) 1

    photon ww

    e w

    N aJJ aN a

    paæ ö÷ç ÷= ç ÷ç ÷ç +è ø

    Number of coherent spontaneous photons per electron does not depend on Nw

    For typical values of aw, on average we need 200 electrons to generate 1 spontaneous photon within coherent angle and bandwidth

    1

    wNwwD

    =

    Coherent spectral bandwidth Solid angle

    wLl

    q=

    Coherent angle

  • 11--8484LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Madey’s TheoremMadey’s Theorem: The small-signal gain spectrum (gain versus energy detuning) for a low-gain FEL is the derivative of the spontaneous emission spectrum. The small-signal gain is positive (amplification) at positive detuning, zero on resonance and negative (absorption) at negative detuning.

    ( )( )3

    3

    4 41 cos sin

    2w

    ss

    Ng

    pr æ öD ÷çD = - D- D÷ç ÷çè øD

    2.6 14 5w w

    EE N NpD

    = »

    Maximum gain is at = 2.6

    10 7.5 5 2.5 0 2.5 5 7.5 100.5

    0

    0.5

    g ( )

    gss()

    4 wEN

    E

    Maximum gain occurs at positive energy detuning (higher energy) than resonance, or at a fixed energy, longer wavelength.

    ( )3max 2 2 wssg Npr»

  • 11--8585LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Visualization of Madey’s TheoremOn resonance R No gain or loss

    12 wN

    Positive detuning R Amplification1

    5 wN

    Negative detuning R Absorption

    15 wN

    R

  • 11--8686LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Small-Signal Gain

    [ ]23

    2 wwss

    w A

    JJ aN Igk I

    pg s

    æ ö æ öæ ö ÷ ÷÷ ç çç ÷ ÷= ÷ ç çç ÷ ÷÷ ç çç ÷ ÷÷ ççè ø è øè ø

    where

    and IA (Alfven current) = 17 kA

    The small-signal gain for a planar wiggler at the peak of the gain curve, assuming the electron beam radius is smaller than the optical beam, is

    ( )1out ss inP g P= +

    Small-signal gain in a low-gain FEL is proportional to Nw

    3

    0 0.06 0.12 0.18 0.24 0.3 0.36 0.42 0.48 0.54 0.6

    1h

    Fundamental power

    z (m)

    Peak

    Pow

    er (W

    ) gssPin

    Pin

    Power versus z in a low-gain FEL

    gss scales with z3

    Pout

    Wiggler length (m)

    Pea

    k P

    ower

    (W)

    2w

    w

    k pl

    =

  • 11--8787LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Large-Signal Gain

    ( )1

    ss

    S

    gg III

    =æ ö÷ç ÷+ç ÷ç ÷çè ø

    Large-signal gain

    At high intensity, more electrons reside at the bottom of the bucket and FEL gain decreases. Saturation intensity is the intensity at which FEL gain reduces to one-half of gss.

    z (m)

    Peak

    Pow

    er (W

    )Pe

    ak In

    tens

    ity (W

    /cm

    2 )

    Wiggler Length (m)

    Large-signal gain

    Saturation Intensity

    Peak Intensity

    Small-signal gain

    [ ]

    2 431 18S w w w

    mcIJJ a N

    gp s l

    æ ö æ ö÷ç ÷ç÷ ÷= ç ç÷ ÷ç ç÷ ÷ç÷ç è øè ø

    FEL gain is reduced when optical intensity approaches the saturation intensity,

  • 11--8888LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Synchrotron Oscillation

    2

    2

    2

    sin

    2

    s w

    R R

    wR

    ka addz

    d dkdz dz

    Energy and phase equations

    22

    2 sin 0Sd Kdz

    2nd-order differential equation of phase evolution with z

    2 22 2

    1w s w s w

    S wR w

    k ka a a aK ka

    Synchrotron oscillation wavenumber

    212w w

    Ss w

    aa a

    Synchrotron period

    0 0.4 0.8 1.2 1.6 2 2.4 2.8 3.2 3.6 4

    z (m)

    Peak

    Pow

    er (W

    )

    Plot of power vs z showing synchrotron oscillations

    S

  • 11--8989LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Wiggler length ~ synchrotron period

    Extraction Efficiency

    2

    max

    max

    12

    2

    2

    w ww S

    s w

    ww

    w

    w

    aLa a

    L

    L

    At saturation, the wiggler length is about the same as a synchrotron oscillation period. The electrons rotate to the bottom of the “bucket.” The bucket half-height is inversely proportional to 2Nw.

    max1

    2 wN

    1

    2 wN

  • 11--9090LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    High-Gain FEL

    [ ] ( ) ( )0 1JJ J Jx x= -

    [ ]2 13 31

    2w

    w A

    JJ a Ik I

    rg s

    æ ö æ ö÷ ÷ç ç÷ ÷= ç ç÷ ÷ç ç ÷÷ çç è øè ø

    Dimensionless Pierce parameter as a function of kw (left) or w (right)

    34w

    GL

    High gain FEL is applicable in a long wiggler driven by a high-brightness electron beam (one with high peak current and small emittance). The wiggler length must be significantly longer than the power gain length, given by

    [ ]2 13 31

    4 2w w

    A

    JJ a II

    lr

    g ps

    æ ö æ ö÷ ÷ç ç÷ ÷= ç ç÷ ÷ç ç ÷÷ çç è øè ø

    Recall JJ is the difference between J0 and J1 Bessel functions of argument

    ( )2

    22 1w

    w

    aa

    x =+

    where[ ]

    2

    12 4

    JJ x x» - -

    Power gain length

    ( )2

    0 1 4J xx » - ( )1 2

    J xx »

  • 11--9191LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Power Growth in High-Gain FEL

    GLzexpP)z(P 09

    1

    Power grows exponentially with distance by one e-folding (2.7) every power gain length. Starting from noise, the FEL saturates in 20 power gain lengths. FEL saturation power, Psat, is approximately times the electron beam power.

    Power vs distance

    bsat

    IEPe

    Saturation power0 0.4 0.7 1.1 1.4 1.8 2.2 2.5 2.9 3.2 3.6

    1h

    Fundamental power

    z (m)

    Log

    Pow

    er

    Natural log of FEL power vs z (wiggler length)

    Exponential growth

    SynchrotronOscillation

    Psat

    P0

    0

    9ln satsat GPL LP

    Saturation length

    Lsat

  • 11--9292LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Slowly Varying Envelope ApproximationSo far, we’ve considered only the electron phase-space motion. To be complete, we must write self-consistent FEL equations for N electrons and the optical field. We’ll treat the optical field as a slowly varying phasor (ignoring the optical frequency oscillation). The phasor’s amplitude is the usual dimensionless optical field as. This is known as the Slowly Varying Envelope Approximation (SVEA).

    ( ) [ ]341 12

    i

    wb A

    JJ I ea a iaz c t k I

    qpg g

    -é ùæ öé ù¶ ¶ ÷ç ê ú÷ê ú+ = -ç ÷ê úç ÷çê ú¶ ¶ S è øë û ë ûThe electron bunch is assumed to be many wavelengths long, so the beam current density is assumed to be independent of z over many wavelengths.

    Wave equation without the fast time scale terms (e.g. 2nd order derivatives)

    0( ) exp ( )E t E i kz t Optical electric field with fast oscillations

    e sisa af-=

    SVEA phasor

  • 11--9393LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Self-Consistent FEL Equations

    The term corresponds to the real part of the e-beam’s susceptibility (refractive index) and term corresponds to the imaginary part (gain).

    22 1 2 cos2

    sin

    jw w w s j

    j

    j w sj

    j

    d kk a a a JJdz

    d ka a JJdz

    Evolution of the jth electron’s phase and energy

    ( ) [ ]

    ( ) [ ]

    3

    3

    4 cos 12

    4 sin2

    ws

    b A s

    ws

    b A

    a JJd Idz k I a

    a JJda Idz k I

    pf qg g

    p qg

    é ùæ ö÷ç ê ú÷= -ç ÷ç ê ú÷çS è ø ë ûæ ö÷ç ÷= ç ÷ç ÷çS è ø

    Evolution of optical phasor’s phase and amplitude

  • 11--9494LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Scaled Variables

    • Scaled axial position

    • Dimensionless current density

    • Scaled phasor equation

    ( )32 4 wj Np r=

    ( ) '0' ' '02

    i

    i

    da j edda j a e dd

    q

    tn t

    t

    t t t tt

    -

    -

    =-

    = -ò

    w

    zL

    t =

  • 11--9595LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Take the derivative of the last equation successively

    Assuming solutions are of the form ei and at resonance condition, we obtain the characteristic cubic dispersion relation

    Note: are roots of the cubic equation, not wavelength

    Solutions of the cubic equation are of the form

    Cubic Equation

    ( ) ( )33 2

    d a jad

    t tt

    =-

    3 02j

    l + =

    ( ) 0 ia a e ltt =

  • 11--9696LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Solutions to Cubic Equation

    11 13 13 3 32 2

    2 22 2 2 2

    3 3 30( )

    3

    jj j j

    iiE eE e e e

    Complex root

    13

    11 3

    2 2 2j i

    Complex root

    13

    3 2j

    Real root

    Three roots of the cubic equation

    Solutions in electric field

    13

    21 3

    2 2 2j i

    growingmode

    decayingmode

    oscillatorymode

    Im

    Re-1½

    32

  • 11--9797LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    Exponential GrowthIn the limit of large z, only the growing mode needs to be considered. The optical field vs scaled length is given by

    Multiplying the electric field by its complex conjugate yields the FEL intensity versus the scaled length

    1232 0( ) exp 3

    9 2E jE

    0 4 3( ) exp9 w

    I zI z

    1 13 3

    23

    2 2 2103( )

    j ji

    E E e e

    Plug in the expressions for and j, we arrive at the expression for intensity vs. distance in the wiggler. This equation gives the exponential growth with wiggler length and the initial 1/9 reduction in signal intensity.

  • 11--9898LA-UR 09-01205US Particle Accelerator School 2009US Particle Accelerator School 2009

    University of New Mexico University of New Mexico -- Albuquerque NMAlbuquerque NM

    References

    Free-Electron Lasers C.A. Brau

    Particle Accelerator Physics I & II H. Wiedmann

    Physics of Free Electron Lasers E.L. Saldin, E.A. Schneidmillerand M.V. Yurkov

    “Free Electron Lasers” S. Khan (2008) J. of Modern Optics, 55:21,3469 – 3512

    “Development of X-ray Free-Electron Lasers” C. Pellegrini and S. Reiche (2004)J. Quantum Electronics, 10(6) 1393-1404

    Books and Articles

    URLUC Santa Barbara WWW FEL http://sbfel3.ucsb.edu/www/vl_fel.html

    Linac Coherent Light Source http://www-ssrl.slac.stanford.edu/lcls/

    European XFEL http://xfel.desy.de/