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Shen 3/31/03
ERL & Coherent XERL & Coherent X--ray Applicationsray Applications
Qun ShenCornell High Energy Synchrotron Source (CHESS)
Cornell University
Talk OutlineTalk Outline
•• Introduction to xIntroduction to x--ray coherenceray coherence
•• Coherent xCoherent x--ray applications ray applications
•• Desired ERL propertiesDesired ERL properties
•• Options and improvements Options and improvements
•• Conclusions Conclusions
Shen 3/31/03
SourceSource EmittanceEmittance and Brillianceand Brilliance
xx’
Integrated total flux Fn
⇒ PhasePhase--space space EmittanceEmittance::
EM wave: E(r, t) = E0 ei(k·r−ωt)
t
E
στ
σE
ετ = στ σE / E
y
y’
σy
σy’
εy = σy σy’
x
x’
σx
σx’
εx = σx σx’
⇒ BrillianceBrilliance: photon flux density in phase: photon flux density in phase--spacespace
B =Fn
(2π)3 εx ·εy·ετ
^PeakB =Fn
(2π)2 εx ·εyAverage
Shen 3/31/03
Spatial (Transverse) CoherenceSpatial (Transverse) Coherence
2σ
θ2σ
2σ' ∆l = θ • 2σ = λ/2
=> 2θ • 2σ ~ λ
θ σ'
X-ray beam is spatially coherentif phase-space area 2πσ’σ < λ/2
=>
Diffraction limited source: 2πσ'σ = λ/2 or ε = λ/4π
Almost diffraction limited: 2πσ'σ ~ λ or ε ~ λ/2π
Shen 3/31/03
Temporal (Longitudinal) CoherenceTemporal (Longitudinal) Coherence
λ λ+∆λ Coherence length: lc = λ2/∆λ
Coherence time: ∆tc = lc/c
Temporally coherent source: pulse length FWHM τ ≤ ∆tclc = λ2/∆λ
⇒ uncertainty: τ ·∆ν ≤ 1τ ·∆Ε ≤ hFor λ = 1 Å, ∆λ/λ = 10-4 :
lc = 1 µm, ∆tc = 1 µm / 3x108 m/s = 3.3 fsDegeneracy Parameter δD
= Number of photons incoherent volume
= Number of photons within single quantum mode
X-ray optics can modify ∆λ/λ, but extinction length (~100µm) limits to ∆λ/λ = 10-6 => ∆tc= 330 fs
⇒ ERL with σt = 100 fs pulses coupled with 10 meV x-ray monochromator could mean temporal coherence at 10 keV.
Shen 3/31/03
Transverse Coherence from Transverse Coherence from UndulatorUndulator
θd Lθθ = = λλ/2d/2d
Example: APS, L =2.4m, λ =1.5Åσr' = 13.1 µrad
dy = 2.35x21µm, σy' = 6.9 µradθ = 1.5 µrad, Θ = 2.35x14.8 µrad
=> pc(vertical) = 4.3%
dx = 2.35x350µm, σx' = 23.1 µrad θ = 0.091 µrad, Θ = 2.35x26.6 µrad
=> pc(horizontal) = 0.15%
=> pc (overall) = 0.006%
Lr
r
2
'35.2
'
22'
λσ
σσ
=
+=Θ
⇒ A portion, θ/Θ in each direction, of undulator radiation is spatially coherent within central cone
⇒ Coherent fraction pc: depends only on total emittances
yxnn
cc F
BFF
pεεπ
λλ2
22
)4()2/(
=⋅
==ERL: pc ~ 20% (45% in x or y)
Shen 3/31/03
ERL Spatial CoherenceERL Spatial Coherence
Diffraction limited @ 8keV (0.123Å)ESRF emittance(4nm x 0.01nm) ERL emittance (0.015nm=0.15Å)
Diffraction limited source: 2πσ'σ = λ/2 or ε = λ/4π
Almost diffraction limited: 2πσ'σ ~ λ or ε ~ λ/2π
Phase II ERLPhase II ERL: diffraction: diffraction--limited source limited source E < 6.6 E < 6.6 keVkeValmostalmost diffractiondiffraction--limited tolimited to 13 13 keVkeV
Shen 3/31/03
XX--ray Coherence Workshop Programray Coherence Workshop Programhttp://www.chess.cornell.edu/Meetings
Friday, 22 August, 2003
8:30 Qun Shen (CHESS) Welcome
8:35 Sol Gruner (Cornell) Energy recovery linac source properties
8:55 Jerry Hastings (SLAC) XFEL source properties
9:15 Bruno Lengeler (Aachen) Tutorial on X-ray coherence
10:05 Coffee Break
10:30 Mark Sutton (McGill) X-ray photon correlation spectroscopy
11:00 Gerhard Gruebel (ESRF) Coherent SAXS
11:30 Jeroen Goedkoop (WZI) Magnetic speckle
12:00 Discussion on coherent scattering I: time correlation
12:15 Lunch
14:00 Ian Robinson (UIUC) Crytallography on nanocrystallites
14:30 John Spence (ASU) Ptychography and diffractive imaging: How it works, with electrons and x-rays
15:00 Coffee Break
15:20 Tetsuya Ishikawa (SPring8) Coherence preserving reflecting and crystal optics
15:50 Christian David (PSI) Diffractive optics and shearing interferometer
16:20 David Paterson (APS) X-ray coherence measurements
16:50 Discussion on coherent optics
Saturday, 23 August, 2003
8:30 Chris Jacobsen (SUNY-SB) Overview on coherent x-ray microscopy
9:00 Keith Nugent (Melbourne) Phase imaging and phase retrieval
9:30 Peter Cloetens (ESRF) 3D phase tomography
10:00 Discussion on phase contrast microscopy
10:15 Coffee Break
10:35 Enzo Di Fabrizio (Eletra) Wavefront shaping & lithography
11:05 Anatoly Snigirev (ESRF) Fourier transform holography
11:35 Makina Yabashi (SPring8) Two-photon interferometry
12:05 Discussion on holography and interferometry
12:20 Lunch
14:00 David Sayre (SUNY-SB) Crystallography applied to noncrystalline materials
14:30 John Miao (SSRL, SLAC) Imaging with single molecule diffraction
15:00 Malcolm Howells (LBNL) Holography by phase retrieval
15:30 Discussion on coherent scattering II: structure determination
Shen 3/31/03
XX--ray Microscopyray Microscopy
ESRF ID21: TXMTXM 3-6 keV
• Increasing number of SR imaging microscopes worldwide due to availability of => lens-like optics: zone plates, KB mirrors, CRLs=> high-brilliance & high-energy synchrotron sources
• All types of materials are studied, from biological to magnetic
• Two types: full field & scanning
⇒ transmission⇒ fluorescence⇒ XPEEMERL hi-coherence
ESRF ID21: SXM 2-10 keV & < 2keVSXM
Shen 3/31/03
Issues in Hard XIssues in Hard X--ray Microscopyray Microscopy
• Focusing opticsFocusing optics
• High coherence sourcesHigh coherence sources:
Coherence fraction ~ λ2/(εxεy). => Requires 100x smaller emittance product for
1keV => 10 keV
ERL would offer 102-103x better emittanceproduct than present-day hard x-ray sources
=> Better coherence @10 keV than @1 keV at ALS
• Absorption vs. phase contrastAbsorption vs. phase contrast
Only recently has Fresnel zone-plate (FZP) achieved <100nm resolution at 8keV (Yun, 1999)
Refraction index: n = 1 − δ − iβ
absorption contrast: µz = 4πβz/λ ∼ λ3
phase contrast: φ(z) = 2πδz/λ ∼ λz
C94H139N24O31S
1010
108
106
104
103102 104
Kirz (1995): 0.05µm protein in 10µm thick ice
X-ray Energy (eV)
Dos
e (G
r) absorption contrast
phase contrast
• In general, phase contrast requires:=> coherent hard x-ray beams
• Phase contrast is x104 higher than absorption contrast for protein in water @ 8keV
• Dose reduced to level comparable to using water-window in soft x-ray region
Shen 3/31/03
Phase Imaging &Phase Imaging & TomographyTomography
λ
Cloetens et al. (1999): ESRF, ID19, 18 keVPolystyrene foam 0.7x0.5x1mm3
1.4T wiggler, B~7x1014 ph/s/mr2/mm2/0.1% @100mA4x700 images at 25 sec/image
• A form of Gabor in-line holography• Coherence over 1st Fresnel zone (λR)1/2
• Image reconstruction (phase retrieval)• Spatial resolution limited by pixel size
• With ERL: it would be possible to reduce the exposure times by orders of magnitude.
• It offers great potential for flash imaging studies of biological specimens, at ID beam lines.
Shen 3/31/03
FarFar--Field Diffraction MicroscopyField Diffraction Microscopy
• Spatial resolution: essentially no limit.(only limited by ∆λ/λ and weak signals at large angles)
• Key development: oversampling phasing methodcoherent flux!!
• Coherent diffraction from noncrystalline specimen:=> continuous Fourier transform
• Diffraction microscopy is analogous to crystallography, but for noncrystalline materials
• Coherence requirement: coherent illumination of sample
Coherent X-rays
Miao et al. (1999) >>>soft x-rays, reconstruction to 75 nm
Shen 3/31/03
Diffraction MicroscopyDiffraction Microscopyrecent resultsrecent results
reconstructed image: to d~7nm resolution
Miao et al. PRL (2002) λ = 2 Å
Gold: 2.5µm x 2µm x 0.1µm
=> could achieve higher resolution,limited only by radiation damage
ERL high-coherence option:B=5x1022 ph/s/mr2/mm2/0.1% @10mAExposure time for Si & d~7nm: 0.6 min.
for C & d~7nm: 3.5 min.
SPring-8 BL29XU:standard undulator 140 periods λu=3.2 cmB=2x1019 ph/s/mr2/mm2/0.1% @100mAFor Au, exposure time 50 min, d~7nmbut: for Si, (ZSi/ZAu)2~1/32 => 26 hrs !
for C, (Zc/ZAu)2~1/173 => 6 days !!
Shen 3/31/03
Imaging Whole Escherichia Coli Bacteria Using Single Particle X-ray Diffraction
Jianwei Miao*†, Keith O. Hodgson*‡, Tetsuya Ishikawa§,
Carolyn A. Larabell¶?, Mark A. LeGros**, and Yoshinori Nishino§
Miao et al., Proc. Nat. Acad. Sci. (2003)
E. Coli bacteria ~ 0.5 µm by 2 µm
SPring-8, λ = 2 Å, pinhole 20 µm
Total dose to specimen ~ 8x106 Gray
Diffraction image to ~30nm resolution
Shen 3/31/03
XX--ray Photon Correlation Spectroscopyray Photon Correlation Spectroscopy
Dierker (2000), ERL Workshop
Shen 3/31/03
XX--ray Holography with Reference Waveray Holography with Reference Wave
Wilhein et al. (2001).Leitenberger & Snigirev (2001)
Howells et al. (2001); Szoke (2001).
Illumination of two objects, one as reference, e.g. pin-hole arrays
• X-ray holography is exciting but not ready for applications
• ERL is an ideal source for further research in this area
Shen 3/31/03
Coherent XCoherent X--ray Patterning & Lithographyray Patterning & Lithography
DOEDOE: diffractive : diffractive optics elementoptics element
Coherent XCoherent X--raysrays
SHAPING X-RAYS BY DIFFRACTIVE CODED NANO-OPTICS
Enzo Di Fabrizio TASC-NNL-INFM (National Institute for the Physics of Matter) Elettra Synchrotron Light Source
(invited talk X-ray Coherence 2003)
Lithography Lithography XX--ray CVD ray CVD
MasklessMaskless patternpattern
Shen 3/31/03
Desired ERL PropertiesDesired ERL Properties
X-ray photon correlation spectroscopyPhase-contrast imaging & microscopy
Coherent far-field diffractionCoherent crystallography
X-ray holographyCoherent x-ray lithography
full transverse coherencehigh coherent flux / coh. fractionhigh ∆λ/λ for high resolutionsmall beam (some cases)large coherent area (some cases)CW operation: long pulses okay
D1 D2
Basic Requirement:Basic Requirement:
⇒⇒ low transverse low transverse emittancesemittances
⇒⇒ long long undulators undulators (large (large NNuu))
⇒⇒ low machine energy spreadlow machine energy spread⇒ X-ray optical slope error
δθ << σx/D1 ~ 4µm/40m ~ 0.1µrad ⇒⇒ coherence preserving xcoherence preserving x--ray opticsray optics
Shen 3/31/03
Phase II ERL Coherent FluxPhase II ERL Coherent Flux
3 4 5 6 7 8 910 20 30 40 50
109
1010
1011
1012
1013
1014
1015LCLS SASE
APS 2.4m
ESRF U35
APS 4.8m
Sp8 5m
Sp8 25m
0.15nm 100mA
ERL 25m0.015nm 10mA
Coh
eren
t Flu
x (p
hoto
ns/s
/0.1
%)
Photon Energy (keV)
• Time-averaged coherent flux comparable to LCLS XFEL
• Coherent fraction ~100x greater than 3rd SR sources
• Peak coherent flux (coherent flux per pulse) ~1000x greater than 3rd SR sources
???
Shen 3/31/03
CHESS Tech Memo 01CHESS Tech Memo 01--002: 3/8/01002: 3/8/01http://erl.chess.cornell.edu/papers
Ave. flux Fn (p/s/0.1%) 1.5· 1016 1.5· 1015 7.0· 1014 4.2· 1015 1.3· 1015 2.4· 1015 9.0· 1015 3.3· 1010 2.4· 1014 6.4· 1012 4· 1017 Ave. brilliance B
(p/s/0.1%/mm2/mr2) 1.3· 1022 5.2· 1022 1.5· 1019 1.5· 1021 3.1· 1020 5.0· 1020 2.2· 1021 1.6· 1017 4.2· 1022 3.6· 1019 8· 1025
Coh flux Fc (p/s/0.1%) 8.1· 1013 3.1· 1014 0.9· 1011 9.0· 1012 1.8· 1012 3.0· 1012 1.3· 1013 9.0· 108 2.4· 1014 1.4· 1011 4· 1017
DC
exp
erim
ents
Coh. fraction pc (%) 0.52 20 0.013 0.22 0.14 0.13 0.14 2.7 100 2.1 100
Photons / bunch 1.2· 107 1.2· 106 9.6· 107 1.9· 108 5.7· 106 7.1· 106 2.7· 107 2.8· 108 2· 1012 1.1· 108 7· 1012 Peak brilliance
(p/s/0.1%/mm2/mr2) 3.0· 1025 1.2· 1026 2.5· 1022 8.3· 1023 3.3· 1022 3.6· 1022 1.6· 1023 4.8· 1027 1.2· 1033 3.4· 1027 7· 1033
Peak flux (p/s/0.1%) 3.9· 1019 3.9· 1018 1.3· 1018 2.6· 1018 1.6· 1017 1.9· 1017 7.4· 1017 1.2· 1021 7.2· 1024 6.0· 1020 3· 1025
Pk coh. flux (p/s/0.1%) 2.1· 1017 7.9· 1017 1.7· 1014 5.6· 1015 2.2· 1014 2.5· 1014 1.1· 1015 2.7· 1019 7.2· 1024 1.4· 1019 3· 1025 Puls
ed e
xpts
.
Peak degen. par. δD 95 368 0.078 2.6 0.103 0.113 0.49 1.3· 104 3.3· 109 4.7· 103 8· 109
Assuming high duty-cycle operations
ERL hi-flux
ERL hi-coh.
APS und. A
APS upgrade
ESRF U35
Spring8 5m
Spring8 25m
LCLS spont.
LCLS SASE
TESLA spont.
TESLA SASE
Energy EG (GeV) 5.3 5.3 7 7 6 8 8 15 15 25 25
Current I (mA) 100 10 100 300 200 100 100 72· 10-6 72· 10-6 0.063 0.063
Charge q (nC/bunch) 0.077 0.008 14 14 0.85 0.29 0.29 1 1 1 1
εx (nm-rad) 0.15 0.015 8 3.5 4 6 6 0.05 0.05 0.02 0.02
εy (nm-rad) 0.15 0.015 0.08 0.0035 0.01 0.003 0.003 0.05 0.05 0.02 0.02
Bunch fwhm τ (ps) 0.3 0.3 73 73 35 36 36 0.23 0.23 0.188 0.090
Mac
hine
des
ign
# of bunches f (Hz) 1.3· 109 1.3· 109 7.3· 106 22· 106 2.3· 108 3.4· 108 3.4· 108 120 120 56575 56575
Undulator L (m) 25 25 2.4 4.8 5 4.5 25 100 100 30 87
Period λu (cm) 1.7 1.7 3.3 3.3 3.5 2.4 3.2 3 3 3.81 5
Inse
rtion
de
vice
# of period Nu 1470 1470 72 145 142 187 781 3300 3300 787 1740
Shen 3/31/03
Desired Changes to MemoDesired Changes to Memo
•• Inclusion of effects of machine energy spread Inclusion of effects of machine energy spread σσEE
0 1 2 3 4 50.0
0.2
0.4
0.6
0.8
1.0
Decrease due to Energy Spread σE
Rel
ativ
e Fl
ux G
ain
Undulator Length Nu / N0
Relative Gain in Undulator Flux]cm[)2/1(
]GeV[95.0]keV[ 2
2
1u
G
KEE
λ+
⋅=
EG
G
EE
EE
σ35.2221
1 ×=
∆=
∆
01
1 1NE
E=
∆
uNEE 1
=∆
transverse transverse εεxxεεyyscale with scale with qq
•• Performance numbers for microPerformance numbers for micro--beam beam undulator undulator
•• Separate ultraSeparate ultra--fast mode: less frequent fat bunch fast mode: less frequent fat bunch qq
Shen 3/31/03
Phase II ERL PropertiesPhase II ERL Properties
Type of experiments Hi-flux Hi-coh I Hi-coh II µ-beam Ultra fast I Ultra fast II
Machine energy E (GeV) 5.3 5.3 5.3 5.3 5.3 5.3Charge per bunch q (nC) 0.077 0.0077 0.0077 0.0077 0.4 1.2
Repetition rate f (MHz) 1300 1300 1300 1300 0.01 0.01Machine current I (mA) 100 10 10 10 0.004 0.012
Horizontal emittance εx (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Vertical emittance εy (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Rms bunch length σt (ps) 2.0 2.0 2.0 2.0 0.1 0.1
Energy spread σE/E 0.0002 0.0002 0.0002 0.0002 0.0027 0.0027Limit on number of periods N0 1064 1064 1064 1064 79 79
Diffraction-limited to Ed (keV) 0.658 6.578 6.578 6.578 0.913 0.527Undulator length L (m) 25 25 30 3.4 2.2 2.2Undulator period λu (cm) 1.7 1.7 1.5 1.4 1.4 1.4
Number of periods Nu 1470 1470 2000 240 160 160Effective number of periods Ne ff 861.8 861.8 939.2 234.1 70.7 70.7
Horizontal beta βx (m) 12.5 4.0 4.8 0.5 1.0 1.0Vertical beta βy (m) 12.5 4.0 4.8 0.5 1.0 1.0
Deflection parameter K 1.34 1.34 1.52 1.6 1.9 1.9Magnetic field B (T) 0.84 0.84 1.08 1.22 1.45 1.45
Fundamental energy E1 (keV) 8.27 8.27 8.25 8.36 6.80 6.80Fundamental wavelength λ1 (A) 1.50 1.50 1.50 1.48 1.82 1.82
Parameter K2/4/(1+K2/2) 0.2365 0.2365 0.2680 0.2807 0.3217 0.3217Parameter Qn (n=1) 0.7139 0.7139 0.7733 0.7949 0.8559 0.8559
Total source size x σx (µm) 43.85 10.35 11.34 3.79 10.64 13.87Total source divergence x σx' (µrad) 3.87 2.60 2.38 7.08 12.20 15.10
Total source size y σy (µm) 43.85 10.35 11.34 3.79 10.64 13.87Total source divergence y σy' (µrad) 3.87 2.60 2.38 7.08 12.20 15.10
Average flux Fn (p/s/0.1%) 8.81E+15 8.81E+14 1.04E+15 2.67E+14 3.46E+10 1.04E+11Average brilliance Bn (std units) 7.74E+21 3.08E+22 3.63E+22 9.40E+21 5.20E+16 6.00E+16
Average flux density @ 1:1 (p/s/0.1%/µm2) 7.30E+11 1.31E+12 1.29E+12 2.96E+12 4.87E+07 8.59E+07Peak flux Fp (p/s/0.1%) 1.27E+18 1.27E+17 7.49E+16 3.84E+16 1.30E+19 3.89E+19
Peak brilliance Bp (std units) 1.11E+24 4.43E+24 2.61E+24 1.35E+24 1.95E+25 2.25E+25Photons per pulse np (p/0.1%) 6.78E+06 6.78E+05 8.00E+05 2.05E+05 3.46E+06 1.04E+07
Coherent flux Fc (p/s/0.1%) 4.35E+13 1.73E+14 2.05E+14 5.17E+13 4.33E+08 4.99E+08
Shen 3/31/03
Options for ImprovementsOptions for Improvements
•• Injector Injector emittance emittance ? 0.015 nm? 0.015 nm--rad rad ????
•• Separate running modes for hiSeparate running modes for hi--coherence & ultracoherence & ultra--fast ? fast ?
•• Bunch decompression Bunch decompression longer pulse but smaller longer pulse but smaller σσEE/γ /γ ????
No Compression σσtt ~ 2 ~ 2 pspsσσEE/γ/γ ~ 2x10~ 2x10--44
onon--crestcrest∆φ ∆φ = 0= 0
σσtt ~ 0.1 ~ 0.1 pspsσσEE/γ/γ ~ 2.7x10~ 2.7x10--33
offoff--crestcrest∆φ ∆φ > 0> 0
σσtt ~ ?? ~ ?? pspsσσEE/γ/γ ~ 1x10~ 1x10--4 4 ??
offoff--crestcrest∆φ ∆φ < 0< 0
Shen 3/31/03
Improved Coherence PropertiesImproved Coherence Propertiesby reducing machine energy spreadby reducing machine energy spread
Type of experiments Hi-flux Hi-coh I Hi-coh II µ-beam Ultra fast I Ultra fast II
Machine energy E (GeV) 5.3 5.3 5.3 5.3 5.3 5.3Charge per bunch q (nC) 0.077 0.0077 0.0077 0.0077 0.4 1.2
Repetition rate f (MHz) 1300 1300 1300 1300 0.01 0.01Machine current I (mA) 100 10 10 10 0.004 0.012
Horizontal emittance εx (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Vertical emittance εy (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Rms bunch length σt (ps) 2.0 2.0 4.0 2.0 0.1 0.1
Energy spread σE/E 0.0002 0.0002 0.0001 0.0002 0.0027 0.0027Limit on number of periods N0 1064 1064 2128 1064 79 79
Diffraction-limited to Ed (keV) 0.658 6.578 6.578 6.578 0.913 0.527Undulator length L (m) 25 25 25 3.4 2.2 2.2Undulator period λu (cm) 1.7 1.7 1.7 1.4 1.4 1.4
Number of periods Nu 1470 1470 1470 240 160 160Effective number of periods Ne ff 861.8 861.8 1209.4 234.1 70.7 70.7
Operation Mode: Operation Mode: offoff--crestcrest∆φ∆φ<0 ?<0 ?
offoff--crestcrest∆φ∆φ>0>0
onon--crestcrest∆φ∆φ=0=0
Average brilliance Bn (std units) 7.74E+21 3.08E+22 4.32E+22 9.40E+21 5.20E+16 6.00E+16Average flux density @ 1:1 (p/s/0.1%/µm2) 7.30E+11 1.31E+12 1.84E+12 2.96E+12 4.87E+07 8.59E+07
Peak flux Fp (p/s/0.1%) 1.27E+18 1.27E+17 8.91E+16 3.84E+16 1.30E+19 3.89E+19Peak brilliance Bp (std units) 1.11E+24 4.43E+24 3.11E+24 1.35E+24 1.95E+25 2.25E+25
Coherent flux Fc (p/s/0.1%) 4.35E+13 1.73E+14 2.43E+14 5.17E+13 4.33E+08 4.99E+08
Shen 3/31/03
Other PropertiesOther Properties
Bandpass for pink beam ∆λ/λ (%) 0.116 0.116 0.083 0.427 1.415 1.415Coherent flux in pink beam Fc (p/s) 5.05E+13 2.01E+14 2.01E+14 2.21E+14 6.12E+09 7.06E+09Average flux in pink beam Fn (p/s) 1.02E+16 1.02E+15 1.02E+15 1.14E+15 4.90E+11 1.47E+12
Peak flux in pink beam Fp (p/s) 1.47E+18 1.47E+17 7.36E+16 1.64E+17 1.83E+20 5.50E+20Photons per pulse in pink beam np (photons) 7.87E+06 7.87E+05 7.87E+05 8.76E+05 4.90E+07 1.47E+08
Coherent flux fraction pc (%) 0.49 19.62 19.62 19.39 1.25 0.48Coherent ∆Ω fraction in ctr cone pc (%) 0.56 22.32 22.32 22.06 1.42 0.55
Coherence width fwhm @100m wc (mm) 0.074 0.413 0.413 1.114 0.373 0.284Coherence length for pink beam lc (µm) 0.129 0.129 0.181 0.035 0.013 0.013
Photons per coherent volume δD 3 12 9 4 99 114
Average total power P0 (W) 31,679 3,168 3,168 895 0.336 1.009On-axis power density @20m dP/dA (W/mm2) 2655 266 266 62.9 0.0199 0.0597
Peak total power Pp (MW) 4.563 0.456 0.228 0.129 126.0 377.9Peak electric field @ exit E0 (V/m) 5.34E+08 7.15E+08 5.06E+08 1.04E+09 1.16E+10 1.54E+10
Type of experiments Hi-flux Hi-coh I Hi-coh II µ-beam Ultra fast I Ultra fast II
Machine energy E (GeV) 5.3 5.3 5.3 5.3 5.3 5.3Charge per bunch q (nC) 0.077 0.0077 0.0077 0.0077 0.4 1.2
Repetition rate f (MHz) 1300 1300 1300 1300 0.01 0.01Machine current I (mA) 100 10 10 10 0.004 0.012
Horizontal emittance εx (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Vertical emittance εy (nm-rad) 0.15 0.015 0.015 0.015 0.108 0.187Rms bunch length σt (ps) 2.0 2.0 4.0 2.0 0.1 0.1
Energy spread σE/E 0.0002 0.0002 0.0001 0.0002 0.0027 0.0027
Shen 3/31/03
ShortShort--Pulse Source ComparisonPulse Source Comparison
fat bunch
Shen 3/31/03
ConclusionsConclusions
• Phase II ERL would offer 100x more coherent flux and coherence fraction for hard x-rays than present-day sources, comparable to prototype XFEL source
• Many scientific applications benefit substantially, e.g. in coherent scattering & diffraction, and in x-ray holography and coherent patterning, possibly opening up new research areas
• Improvements in ERL coherent flux require long undulator, which in turn requires reducing machine energy spread by bunch decompression or by some other means
• Further improvements in coherence are possible only ifinjector emittance can be further reduced
• Ultra-fast mode of ERL can still be a leader in peak brilliancefor short-pulses. Further improvement is determined by how much charge in a single bunch and by energy spread from bunch compressor