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Free Electron Lasers Lecture IV Brian M c Neil, University of Strathclyde, Glasgow, Scotland.

Free Electron Lasers Lecture IV - Cockcroft

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Page 1: Free Electron Lasers Lecture IV - Cockcroft

Free Electron Lasers

Lecture IVBrian McNeil,University of Strathclyde, Glasgow, Scotland.

Page 2: Free Electron Lasers Lecture IV - Cockcroft

Spoiling effects

Page 3: Free Electron Lasers Lecture IV - Cockcroft

Energy spread

( ) ( )00 r j

j jr

zp z

γ γδ

ρ γ− =

= = ≡

The effects of energy spread can be investigated by introducing a spread in the initial values of pj :

The steady state dispersion relation becomes:

with solutions for the imaginary part of lambda, determining the high gain case, shown opposite. Energy spread effects become less important when:

1 γγ

σσ ρ

γ< ⇒ <

( )f δ

γσγσ−

2 γσ

Page 4: Free Electron Lasers Lecture IV - Cockcroft

Emittance*

http://www.fieldp.com/cpb.htmlCharged Particle Beams:*Stanley Humphries,

The beam emittance introduces two main effects:

1) The electron beam radius in a matched focussing channel** is determined by the emittance via:

2) The emittance introduces an energy spread in the resonant electron energy***. This can be added in quadrature with the real energy spread to estimate emittance effects in a 1D model:

β – betafunction of focussing lattice.

effσρ

γ⇒ <

**See H. Owen course***

Page 5: Free Electron Lasers Lecture IV - Cockcroft

Diffraction

The Rayleigh length lZR is that in which a beam diffracts to twice its transverse mode area. In an FEL amplifier, if the gain length of the FEL interaction is greater than the Rayleigh length then diffraction can cause reduced coupling and longer saturation lengths.

lZR

Good coupling

Reduced coupling

Gain length, lg

Page 6: Free Electron Lasers Lecture IV - Cockcroft

http://www.4gls.ac.uk/documents.htm*4GLS Conceptual Design Report, Chapter 8:

*

Page 7: Free Electron Lasers Lecture IV - Cockcroft

Real FEL designsas taken from the 4GLS design*

http://www.4gls.ac.uk/documents.htm*4GLS Conceptual Design Report, Chapter 8:

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4GLS CDR – April 2006

750-950MeV

600MeV

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XUV-FEL (~10-100nm)

Page 12: Free Electron Lasers Lecture IV - Cockcroft

HHG seed sources

These sources result from the high harmonic emission from a gas jet of noble gas driven by a high power laser:

Page 13: Free Electron Lasers Lecture IV - Cockcroft

The Undulators

Tuning the FEL is achieved by varying the undulator gap and by changing the electron beam energy between 750-950MeV. For the planar undulators above a period of 45mm was chosen to enable tuning over the photon energy range 10-100eV.

The resonant photon energy (eV)

Page 14: Free Electron Lasers Lecture IV - Cockcroft

Undulator lattice

The undulator is split into many modules of length ~2m each (PU - planar undulator; VU - variable polarisation undulator). Between each module are phase-matching magnets, quadrupole focussing units for electron transport (a FODO lattice is used) and beam positioning monitors. Note the use of the variable polarisation units in the last few undulator sections to give variably polarised radiation output.

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Gain length Saturation power

Optimising the focussing lattice

The beta-function was chosen to be ~5m. This was to stop ‘sausaging’ of the electron beam due to the variation in the beta-function of a FODO lattice:

⇒ oscillates.

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Beam quality

The gain length and the saturated power for 100eV operation

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VUV-FEL 3-10eV

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IR-FEL 2.5-200μm

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Some advanced schemes

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2-undulator conceptAn electron beam bunched at a fundmental wavelength also has a stron bunching component at harmonics of the fundamental.

Page 34: Free Electron Lasers Lecture IV - Cockcroft

HGHG concept

D

56D k Rρ=

Page 35: Free Electron Lasers Lecture IV - Cockcroft

e-

Seed field – λ1 resonant with γ1λn resonant with γn

2-beam FEL amplifier

γ1γn

The coherence properties of the seed field will be transferred to the higher energy interaction via the coupled harmonic interaction.

1γγ nn =By choosing the fundamental resonant wavelength ofbeam γn is the nth resonant harmonic of beam γ1.

Page 36: Free Electron Lasers Lecture IV - Cockcroft
Page 37: Free Electron Lasers Lecture IV - Cockcroft

Harmonic Amplifier FEL

Normal planar FEL amplifier including the 3rd & 5th

harmonics (Undulator aw=3)

Harmonic Amplifier FEL demonstrating dominance of 3rd

harmonic over fundamental & 5th

harmonic

Seeding

Page 38: Free Electron Lasers Lecture IV - Cockcroft

Attosecond pulse generation

Page 39: Free Electron Lasers Lecture IV - Cockcroft

Mode-Locked SASE FEL

Spike FWHM ~ 23 as

Chicanes introduce identical shifts in relative electron/light pulse positions

Page 40: Free Electron Lasers Lecture IV - Cockcroft

Mode-Locked Afterburner*

*DJ Dunning, BWJ McNeil & NR Thompson, Phys. Rev. Lett. 110, 104801 (2013)

Can generate few-cycle pulses – this takes x-ray FELs into the zeptosecond regime (10-21s)

Page 41: Free Electron Lasers Lecture IV - Cockcroft

High-Brightness SASE*

*BWJ McNeil, NR Thompson & DJ Dunning, Phys. Rev. Lett. 110, 134802 (2013)

Chicanes introduce increasing shifts in relative electron/light pulse positions

Greatly improved temporal coherence over SASE to give close to transform limited pulses in the hard x-ray

Page 42: Free Electron Lasers Lecture IV - Cockcroft

Some advantages of FELsTuneable by varying electron energy or

undulator parameters Bu and/or λuSpectral reach – THz, VUV to x-rayCannot damage lasing medium (e--beam)High peak powers (>GW’s)Very bright (>~1030 ph/(s mm2 mrad2 0.1% B.W.))

High average powers – 10kW at JeffersonShort pulses (<100fs 100’s zs (10-21s) )

The next generation of FELs will ensure that these sources are at the fore of light source provision for many years to come. Other sources are unable to meet all of the qualities of FELs by orders of magnitude in at least one respect.

Page 43: Free Electron Lasers Lecture IV - Cockcroft

Thank you!