Luc Patthey, leader of the research group of Spectroscopy on Novel Materials at the Synchrotron Radiation and Nanotechnology Laboratory at PSI, presents the Swiss Light Source and the future X-ray free electron laser, SwissFEL.
DevEX - reference for building teams, processes, and platforms
Light Sources - Paul Scherrer Institute
1. Research at Paul Scherrer Institute's Large
Scale Facilities
L. Patthey
June 22, 2010
San Francisco
SWISSNEX
L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
3. Paul Scherrer (1890 – 1969)
– Studied physics and
mathematics at
the Swiss Federal Institute of
Technology (ETH) Zurich, in
Königsberg and Göttingen in
Germany
– 1920: Director of The Institute
of Physics at the ETH Zurich.
Became well-known for the
clarity of his lectures
– Researched X-ray scattering
on crystals, liquids and gases.
Later research work was in
nuclear physics
– 1946: President of the Swiss
Study Commission on Atomic
Energy
– Involved in the founding of
CERN
L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
4. Political embedding
Swiss Federal Government
EDA EDI EJPD VBS EFD EVD UVEK
Board of the Swiss Federal
Institutes of Technology
ETHZ EPFL PSI Empa WSL Eawag
Swiss Federal Swiss Federal Paul Scherrer Swiss Federal Swiss Federal Swiss Federal
Institute of Institute of Institute Laboratories Research Institute for
Technology Technology for Materials Institute for Water Resour-
Zurich Lausanne Testing Forestry, Snow ces and Water
and Landscape Pollution
Control
Universities
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5. Research at PSI
Health Energy
Proton and
therapy Environment
Micro- Large
and scale
Nano- facilities
technology
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6. Our Mission
– To play a leading role at an interna/onal level in
– physics of condensed ma0er and materials sciences
– structural biology
– radiochemistry, radiopharmacy and proton radia8on therapy
– par8cle physics and accelerator developments
by using large‐scale facili/es
(SLS, SINQ, SµS, par8cle beams)
– To be a UserLab for external science community
– Energy research, primarily using complex facili/es, towards an efficient,
environmentally friendly and reliable energy supply
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7. Personalentwicklung in den Forschungsschwerpunkten
Development of PSI research activities des PSI
(ohne Drittmittelstellen)
1200
1000
Nuclear Energy
Personenjahre pro Jahr
Employees/year Particle Physics
800
Biology
600 General Energy
SLS
SLS (Light source)
400
Materials Research
200
SINQ SINQ (Neutrons)
0
Year
Budgetjahr
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8. Swiss Light Source
3rd+ Generation storage ring
• 400 mA, Top-up injection
• In operation since 2001
• 17 beamlines
• 1053 experiments in 2009 (PSI: 1734)
• 3145 users in 2009 (PSI: 4526)
Main activities
• Physics of condensed matter
• Materials sciences
• Structural biology
• Micro- and Nano- Technology
• Energy and Environment
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9. Synchrotron Analogy
Phone: SLS:
Wave length ~ 10 cm ~ 0.000’000’01 cm
Power ~ 2 Watt ~ 200’000 W
99,999’997 % Speed of light
-> directional radiation
Acceleration of charge -> Electromagnetic wave (light)
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10. X-ray and light sources
X-Ray Source Milestones
1895 Röntgen (Würzburg)
1953 Rotating-anode (Rigaku)
1947 Synchrotron radiation (GE)
1961 1st generation synchrotron (NBS) - parasitic
1981 2nd gen. (Daresbury) - dedicated to SR
1984 3rd gen. (Grenoble) - undulators
2001 3rd+ gen. (SLS, Villigen) - high-brightness
2009 4th gen. (Stanford) - X-ray Free Electron Laser
Bending magnet
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11. Synchrotron Radiation
Crab Nebula
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12. Micro-bunching and coherent emission
λ Micro‐bunches radiate coherently.
E = NE1
Ini8ally uniform e‐ distribu8on (blue) Pincoh = NP1
evolves into microbunches (red). Pcoh = N 2 E12 = NPincoh
N ≈ 10 9 !!
XFEL undulator
€
€
„Self‐amplifying spontaneous emission“ (SASE)
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13. X-Ray Source Brilliance
1024
XFEL
1021
rd
3 Generation
Average Brilliance
1018
Synchrotrons
nd
2 Generation
15
10
1012 st
1 Generation
109
X-ray tubes
106
1910 1930 1950 1970 1990 2010
Calendar Year
brilliance =
# photons / time / area / solid-angle / energy-bandwidth
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14. Time resolved (Motion and shutter speed)
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15. How fast can we go?
1/8’000 0.000’000’000’000’01 sec
10 Billion
time faster
10-4 sec 10-14 sec
1/10 msec 10 Femto sec.
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16. Space and Time
Space
mm µm nm
ns ps fs
Time
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17. Light as probe
Resolution:
Space→ λ
Time→ τ
λ
cτ
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18. Light sources
Optical Laser
„Fast“ : τ = 2 fs … (0.4 fs)
„ Low res. “ : λ = 200 nm…(14 nm)
Synchrotron light
„ High res.“ : λ = 0.1 nm
„Slow“ : τ = 100.000 fs
XFEL: High res. and Fast λ = 0.1 nm, τ = 10 fs
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19. The SwissFEL
• hν:Mg L-edge (50 eV) - 57Fe Mössbauer resonance (14.4 keV)
• Soft X-rays: circular polarization, transform-limited (seeding)
• Hard X-rays: 5-20 fs (low-charge mode)
• Synchronized THz pump source
• 100 Hz repetition rate ⇒ condensed matter applications
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20. SwissFEL Tunnel & Building
• Accelerator, beamlines and experiment
underground
• Linac HF and other facilities
above ground
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21. SwissFEL: Villigen or Würenlingen
10.11.2009
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22. SwissFEL Milestones
Gun laser 0.25 GeV
2010 Commissioning 250 MeV Injector
Ende 2014
Realisation main building
Gun laser
2.1 GeV 3.4 GeV 5.8 GeV ARAMIS FEL 1-7 Å
Exp2
Beginning 2016, SwissFEL Phase I Laser pump
Commissioning Linear Accelerator und ARAMIS FEL
Gun laser
2.1 GeV 3.4 GeV 5.8 GeV ARAMIS FEL 1-7 Å
Exp2
2018, SwissFEL Phase II ATHOS FEL 7‐70 Å
Commissioning ATHOS FEL Seed laser Exp2 Laser pump
THz pump
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23. SwissFEL: Cost
Target: Installation cost
Expected cost distribu/on
without manpower:
275.5 MCHF
+ pre-investment
≈ 20 MCHF
without the XFEL preparation
phase
(250 MeV Injector)
-> = 38 CHF (34 USD) / Citizen
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24. Our Sisters...
1 km
Europe
EU-XFEL–DESY 2014
Japan
SCSS–SPring8
2011
USA
LCLS-SLAC
2009
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25. Scientific Challenges
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26. Correlated electrons
weak and strong
interacting electron
systems
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27. Modern electronic properties of condense mater
Colossal magnetoresistance effect (CMR) High temperature Superconductivity
Large drop of resistivity upon relatively small magnetic No resistivity at liquid nitrogen temperature
fields
Electron energy
Emission angle
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28. Averaging in time (slow shutter speed)
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29. Time resolved (fast shutter speed)
Dynamics in correlated electron:
new aspect and new physics!
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30. Lattice, Charge, Spin and Orbital orders
Lattice Charge
Orbital Spin
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31. Resonant X-ray Scattering
Resonant X-ray (emission): Scattering (diffraction):
Chemical information Structural information
Photon Photon
In Out Back scattering angle
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32. Time-resolved Resonant X-ray Scattering
Pump and Probe
Optical pulse from Laser
X-ray from X-FEL
ΔT
Optical Pump Pulse X-ray Probe Pulse
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33. Time-resolved Resonant X-ray Scattering
Goal:
• Pump: Melt charge/spin order with
op8cally phase transi8on
• Probe: Study the dynamics which
govern charge reorganiza8on
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34. • May 2010
Tested at ALS
• June 2010
Installation at SLAC
• July 2010
1st experiment with
LCLS (X-FEL)
W.-S. Lee, Z.X. Shen (SIMES, Stanford), Y.D. Chuang, Z. Hussain (LBL, ALS)
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35. Fast 2-D CCD detector
• Developed by LBNL.
• 200 frames per sec. ->Pulse-by-
pluse data collection.
• 480 by 480 array of 30 mm square
pixels
• 8o acceptance, 0.017o per pixel
• Successfully tested at the ALS
(May 2010)
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36. end‐sta8on at SLS, PSI
Em hv`
hv
ΔE
E f
Ei
Energy transfer: Momentum transfer:
ΔE = hv – hv`
q = kin ‐ kout
RIXS Spectrometer:
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37. Conclusion
Learn from experience accumulated at LCLS trough collaboration and joint projects
-New physics Resonant X‐ray Sca0ering end‐sta8on for LCSL (ALS, Stanford)
-Problems and difficulties
-Share expertise
Resonant Inelas8c X‐ray Sca0ering end‐sta8on at SLS, PSI
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38. Acknowledgment
Stanford National Accelerator Laboratory (SLAC), LCLS
W. Schlotter, All LCLS team
Advanced Light Source (ALS), Lawrence Berkeley National Laboratory (LBNL)
Y.-D. Chuang, K. Chow, Z. Hussain
Lawrence Berkeley National Laboratory (LBNL)
R. Schoenlein and R. Kaindl
Lawrence Berkeley National Laboratory (LBNL)
P. Denas, D. Doering, N. Andresen
Stanford Institute for Materials and Energy Science (SIMES)
Stanford University and National Accelerator Laboratory (SLAC)
W.‐S. Lee, Z. X. Shen, T. P. Devereaux
University of Illinois
P. Abbamonte
Swiss Light Source (SLS), Paul Scherrer Institut (PSI)
S. L. Johnson, U. Staub, R. De Souza, P. Beaud, G. Ingold
Spectroscopy group, Swiss Light Source (SLS), Paul Scherrer Institut (PSI)
T. Schmitt, K. Zhou, V. Strocov
SwissFEL, Paul Scherrer Institut (PSI)
B. Patterson, R. Abela
L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco