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Approaches for the generation of femtosecond x-ray pulses

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Title: Approaches for the generation of femtosecond x-ray pulses


1
Approaches for the generation of femtosecond
x-ray pulses
Zhirong Huang (SLAC)
2
The Promise of X-ray FELs
Ultra-bright
Ultra-fast
3
Single Molecule Imaging with Intense fs X-ray
R. Neutze et al. Nature, 2000
4
Introduction
  • Femtosecond (fs) x-ray pulses are keys to
    exploring ultra-fast science at a future light
    source facility
  • In typical XFEL designs based on SASE the photon
    pulse is similar in duration to the electron
    bunch, limited to 100200 fs due to short-bunch
    collective effects
  • Great interests to push SASE pulse length down
    to 10 fs and even below 1 fs
  • A recent LCLS task force studied upgrade
    possibilities, including short-pulse approaches
  • I will discuss and analyze several approaches

in the next 1800000000000000000 fs!
5
Outline of the Talk
  • Temporal characteristics of a SASE FEL
  • Optical manipulation of a frequency-chirped SASE
  • Compression
  • Slicing single-stage and two-stage
  • Statistical analysis
  • Electron bunch manipulation
  • Spatial chirp
  • Enhancing undulator wakefield
  • Selective emittance spoiling (slotted spoiler)
  • Sub-femtosecond possibilities

6
Temporal Characteristics of a SASE FEL
E(t)?j E1(t-tj), tj is the random arrival time
of jth e-
E1 wave packet of a single e- after Nu undulator
period
Nu ?
Coherence time ?coh determined by gain bandwidth
??
7
?coh
  • Sum of all e- ? E(t)
  • SASE has M temporal (spectral) modes with
    relative intensity fluctuation M-1/2
  • Its longitudinal phase space is M larger than
    Fourier transform limit
  • Narrower bandwidth for better temporal coherence
  • shorter x-ray pulse (shortest is coherence time)

8
  • LCLS near saturation (80 m)
  • bunch length 230 fs
  • coherence time 0.3 fs
  • number of modes 700
  • statistical fluctuation
  • sw/W 4

Shortest possible XFEL pulse length is only 300
as!
9
  • Optical manipulations of
  • a frequency-chirped SASE

10
X-ray Pulse Compression
  • Energy-chirped e-beam produces a
    frequency-chirped radiation
  • Pair of gratings to compress the radiation pulse

C. Pelligrini, NIMA, 2000
  • No CSR in the compressor, demanding optics
  • Pulse length controlled by SASE bandwidth and
    chirp

11
X-ray Pulse Slicing
  • Instead of compression, use a monochromator to
    select a slice of the chirped SASE

?
monochromator
short x-ray slice
t
compression
  • Single-stage approach

12
Two-stage Pulse Slicing
C. Schroeder et al., NIMA, 2002
  • Slicing after the first undulator before
    saturation reduces power load on monochromator
  • Second stage seeded with sliced pulse
    (microbunching removed by bypass chicane), which
    is then amplified to saturation
  • Allows narrow bandwidth for unchirped bunches

13
Analysis of Frequency-chirped SASE
  • Statistical analysis (S. Krinsky Z. Huang,
    PRST-AB, 2003)
  • Frequency-chirp
  • coherence time is indep. of chirp u
  • frequency span and frequency spike width ?coh u
  • A monochromator with rms bandwidth sm passes MF
    modes

14
Minimum Pulse Duration
  • The rms pulse duration st after the
    monochromator

?
u
t
  • Minimum pulse duration is limited to
  • for either compression or slicing
  • Slightly increased by optical elements ( fs)

15
One-stage Approach
  • SASE bandwidth reaches minimum (r10-3) at
    saturation
  • ? minimum rms pulse duration
    6 fs (15 fs fwhm) for 1 energy
    chirp
  • st minimum for broad sm ? choose sm sw to
    increase MF (decrease energy fluctuation) and
    increase photon numbers

16
Two-stage Approach
  • Slicing before saturation at a larger SASE
    bandwidth leads to a longer pulse

Ginger LCLS run
  • Synchronization between sliced pulse and the
    resoant part of chirped electrons in 2nd
    undulator 10 fs

17
Electron Bunch Manipulations
18
Spatially Chirped Bunch
P. Emma Z. Huang, 2003 (Mo-P-52)
200-fs e- bunch
30-fs x-ray
Undulator Channel
  • FEL power vs. y offset for LCLS
  • Gain is suppressed for most parts of
  • the bunch except the on-axis portion

19
E 4.5 GeV, sz 200 mm, V0 5 MV
1.0 m
2sy?
0
-2sy?
y? vs. z at start of undulator
?
  • No additional hardware for LCLS
  • RF deflector before BC2 less jitter
  • Beam size lt 0.5 mm in linac

? FWHM x-ray pulse 30 fs
20
Courtesy S. Reiche
21
Using Enhanced Wakefield
  • Ideal case (step profile) with various materials
    for the vacuum chamber to control wakefield
    amplitude

4 fs (FWHM)
  • Change of vacuum chamber to high resistivity
    materials (graphite) is permanent, no long pulse
    operation

S. Reiche et al., NIMA, 2003
22
Where else can we access fs time?
Large x-z correlation inside a bunch compressor
chicane
LCLS BC2
Easy access to time coordinate along bunch
2.6 mm rms
0.1 mm rms
23
Slotted-spoiler Scheme
1 mm emittance
5 mm emittance
1 mm emittance
P. Emma et al. submitted to PRL, 2003 (Mo-P-51)
24
Parmela ? Elegant ? Genesis Simulation, including
foil-wake, scattering and CSR
25
fs and sub-fs x-ray pulses
  • A full slit of 250 mm ? unspoiled electrons of 8
    fs (fwhm)
  • ? 23 fs x-rays at saturation (gain narrowing of
    a Gaussian electron pulse)
  • stronger compression narrower slit (50 mm) ? 1
    fs e-
  • ? sub-fs x-rays (close to a single coherence
    spike!)

26
Statistical Single-Spike Selection
Unseeded single-bunch HGHG (8 ? 4 ? 2 ? 1 Å )
I8 / I18
8 Å
1 Å
sub-fs spike
Saldin et al., Opt. Commun., 2002
27
Selection Process
Set energy threshold to reject multi-spike events
(a sc linac helps)
28
Conclusions
  • XFEL can open both ultra-small and ultra-fast
    worlds
  • Many good ideas to reduces SASE pulse lengths
    from 100 fs to 10 fs level
  • Optical manipulations are limited by SASE
    bandwidth, available electron energy chirp, and
    optical elements
  • Electron bunch manipulations and SASE
    statistical properties may allow selection of a
    single coherent spike at sub-fs level
  • Time for experimental investigations
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