LCLS-PPT-03-3
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Transcript LCLS-PPT-03-3
Approaches for the generation
of femtosecond x-ray pulses
Zhirong Huang (SLAC)
The Promise of X-ray FELs
Ultra-bright
Ultra-fast
Single Molecule Imaging with Intense fs X-ray
R. Neutze et al. Nature, 2000
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 100~200 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!
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
Temporal Characteristics of a SASE FEL
E(t)=j E1(t-tj), tj is the random arrival time of jth eE1: wave packet of a single e- after Nu undulator period
Nu
Coherence time coh determined by gain bandwidth
Sum of all e- E(t)
coh
bunch length Tb
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)
• LCLS near saturation (80 m)
bunch length 230 fs
coherence time 0.3 fs
number of modes ~ 700
statistical fluctuation
w/W ~ 4 %
Shortest possible XFEL
pulse length is only 300
as!
1 % of X-Ray Pulse Length
Optical manipulations of
a frequency-chirped SASE
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
X-ray Pulse Slicing
Instead of compression, use a monochromator to select
a slice of the chirped SASE
ω
monochromator
short x-ray slice
t
compression
Single-stage approach
SASE FEL
Monochromator
Two-stage Pulse Slicing
C. Schroeder et al., NIMA, 2002
Chicane
SASE FEL
FEL Amplifier
Monochromator
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
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 m passes MF
modes
Minimum Pulse Duration
The rms pulse duration t after the monochromator
ω
/ u
u
t
Minimum pulse duration is limited to
for either compression or slicing
/u
Slightly increased by optical elements (~ fs)
One-stage Approach
SASE bandwidth reaches minimum (~r~10-3) at saturation
minimum rms pulse duration ( ) min / u ~ r / u = 6 fs
(15 fs fwhm) for 1% energy chirp
t minimum for broad m choose m ~ to increase MF
(decrease energy fluctuation) and increase photon numbers
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
Electron Bunch Manipulations
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
1.0 m
E = 4.5 GeV,
z = 200 mm,
V0 = 5 MV
+2y
0
-2y
y vs. z at start of undulator
?
• No additional hardware for LCLS
• RF deflector before BC2 less jitter
• Beam size < 0.5 mm in linac
FWHM x-ray pulse ~ 30 fs
Courtesy S. Reiche
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
Where else can we access fs time?
Large x-z correlation inside a bunch compressor chicane
2.6 mm rms
LCLS BC2
Easy access to
time coordinate
along bunch
0.1 mm rms
Slotted-spoiler Scheme
1 mm emittance
5 mm emittance
1 mm emittance
P. Emma et al. submitted to PRL, 2003 (Mo-P-51)
Parmela Elegant Genesis Simulation, including foil-wake, scattering and CSR
fs and sub-fs x-ray pulses
• A full slit of 250 mm unspoiled electrons of 8 fs (fwhm)
2~3 fs x-rays at saturation (gain narrowing of a
Gaussian electron pulse)
2 fsec fwhm
• stronger compression + narrower slit (50 mm) 1 fs e sub-fs x-rays (close to a single coherence spike!)
Statistical Single-Spike Selection
Unseeded single-bunch HGHG (8 4 2 1 Å )
8Å
I 8 / I 18
Saldin et al., Opt. Commun., 2002
1Å
sub-fs spike
Selection Process
Set energy threshold to reject multi-spike events (a sc linac helps)
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