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Enhanced Self-Amplified Spontaneous Emission

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Presentation on theme: "Enhanced Self-Amplified Spontaneous Emission"— Presentation transcript:

1 Enhanced Self-Amplified Spontaneous Emission
P. Emmaa, W. Fawleyb, Z. Huanga, S. Reichec, G. Stupakova, A. Zholentsb a) SLAC, b) LBNL, c) UCLA

2 ESASE: “nuts and bolts”
Modulation Acceleration Bunching Energy modulation in the wiggler at ~ 4 GeV 20-25 kA 50 fs laser pulse lL= 2 microns Peak current, I/I0 z /lL Only one optical cycle is shown Electron beam after bunching at optical wavelength Laser peak power ~ 10 GW Wiggler with ~ 10 periods

3 Zoom-in on a single spike
Electron beam phase space after bunching B=Dg/sg Peak current Energy spread z /Dz0 Peak current and energy distribution within one micro-bunch *) Dz0 should be > slippage ~ 8 MGlx= 240 nm

4 Shaping x-ray pulse Peak power, P/P0 z /lL
The x-ray radiation output from the entire electron bunch Radiation from electrons interacted with laser dominate, thus Absolute synchronization to the pump laser source for ultra-fast experiments with x-rays

5 The output x-ray radiation from a single micro-bunch
-200 -100 100 200 Each spike is nearly temporally coherent and Fourier transform limited Carrier phase for an x-ray wave is random from spike to spike Pulses less than 100 attoseconds may be possible with 800 nm laser

6 Coherent off-axis radiation in the undulator
sz c bz y z lu Off-axis radiation field in the undulator catches up the beam by one l ~ 2psz in one undulator period lu 1D “wake” (E. Saldin et al., NIM A 417, ) For Ipeak = 23 kA, and z = 30 nm, we get:  / = 0.15% at Lu ~ 30 m

7 Suppression of off-axis coherent radiation due to finite beam size
angle y<<1 2 = 4p/(lu k) Bunch form factor : Dg per meter of undulator z/lL 1D 2D Dg per meter of undulator A consideration for a choice of focusing ! z/lL Energy loss distribution along the spike

8 Coherent synchrotron radiation in the chicane
Does not look bad at all ! A finite horizontal beam extend prevents the micro-bunching until almost the very end of the chicane. ex ey Slice emittance after chicane at various locations along the e-beam

9 Resistive wall wake field
2b e-beam lL= nm 2a a) Transient wake field effect Single bunch catch-up distance c 2a bz ~30 m

10 Resistive wall wake field cont’d
b) Steady state wake 800 nm 2a=5 mm We calculate the electron Coulomb field at the wall of the vacuum chamber: . and compare it with the field produced by continuous electron beam: The field from a modulated beam is only a factor ~ 1.3 larger

11 A schematic of the LCLS with ESASE
Linac-0 L 6 m Linac-1 L  9 m rf -25° Linac-2 L  330 m rf  -41° Linac-3 L  550 m rf  -10° BC1 R5639 mm BC2 R5625 mm DL2 R560 DL1 R56-6 mm undulator L 130 m …existing linac new rf gun X Laser Heater SC Wiggler SLAC linac tunnel undulator hall 14.1 GeV 4.54 GeV z  0.02 mm Wiggler Laser Heater Laser New elements

12 Beta and dispersion functions in the LCLS
3-m wiggler existing buncher

13 Peak current, emittance and energy spread after linac
gex gey

14 Beta and dispersion functions in the DL2 buncher
two 5% quadrupole gradient changes, plus one new ‘tweaker’ quad E = 14.1 GeV R56 = 0.19 mm (nom. is 0.11 mm)

15 At undulator entrance: E = 14.1 GeV

16 X-ray radiation Average power vs z 2200 nm

17 Pump-probe experiment concept
Laser excitation pulse X-ray probe pulse ∆t X-ray detector sample ion or e- detector Requires control/measure of Dt with a resolution better than x-ray pulse duration (possibly as small as 100 attoseconds)

18 Pump-probe cont’d One can hope to get a required synchronization if all sources are linked to a common origin Master laser source Near IR pump controlled delay XUV pump Courtesy H. Kapteyn laser - e-beam energy modulation X-ray probe pulse

19 Second Harmonic correlator
Pump-probe cont’d Jitter control by cross-correlation of wiggler radiation with seed laser pulse Near IR pump Second Harmonic correlator one period wiggler isochronous bend LCLS wiggler radiation, ~0.5 GW x-rays

20 Potential of ESASE Saturation length Saturation length B=Dg/sg
Shorter gain length Larger emittance 1.2 mm-mrad, Std. b=28 m 2.4 mm-mrad, B=8 Saturation length Saturation length b=14 m b=7 m B=Dg/sg Beta-function, m Smaller wavelength 1.5Å, Std. 0.75Å, B=8 Saturation length Beta-function, m

21 Summary ESASE offers: 1) Short gain length, high peak power, comparable average power. 2) Easy tunability for a duration of x-ray pulse by laser pulse shaping. 3) Nearly temporally coherent and Fourier transform limited radiation within the spike with random carrier phase between spikes. A solitary attosecond x-ray pulse. 4) Absolute synchronization between laser pulse and x-ray pulse. 5) Relaxing emittance requirement. 6) Shorter x-ray wavelengths


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