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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
Paul Scherrer Institute




                  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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
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 

                                                                        L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Research at PSI



  Health             Energy
  Proton               and
 therapy           Environment




   Micro-               Large
    and                 scale
   Nano-              facilities
technology




                                   L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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 



                                                 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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




                                                                        L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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
                                         L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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)


                                         L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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
                                                       L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Synchrotron Radiation




                         Crab Nebula


              L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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) 

                                                                L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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

                                                                                            L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Time resolved (Motion and shutter speed)




                      L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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.
                              L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Space and Time
 Space




         mm        µm                                        nm
         ns        ps                                         fs




Time
                          L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Light as probe




Resolution:
   Space→ λ
   Time→ τ

                            λ




                       cτ
                            L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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


                                                   L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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

                                            L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
SwissFEL Tunnel & Building




                 •  Accelerator, beamlines and experiment
                 underground
                 •  Linac HF and other facilities
                 above ground


                       L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
SwissFEL: Villigen or Würenlingen




10.11.2009 


                              L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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 


                                                                                  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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




                                           L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Our Sisters...




  1 km
                               Europe
                               EU-XFEL–DESY 2014


                               Japan
                               SCSS–SPring8
                               2011

         USA
         LCLS-SLAC
         2009
                     L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Scientific Challenges




                L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Correlated electrons



                weak and strong
                interacting electron
                systems




               L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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




                                                                      L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Averaging in time (slow shutter speed)




                      L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Time resolved (fast shutter speed)




Dynamics in correlated electron:
new aspect and new physics!

                                   L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Lattice, Charge, Spin and Orbital orders
Lattice                Charge




   Orbital               Spin




                      L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Resonant X-ray Scattering

Resonant X-ray (emission):                Scattering (diffraction):
   Chemical information                    Structural information

   Photon       Photon
     In          Out                           Back scattering angle




                                     L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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




                                   L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
Time-resolved Resonant X-ray Scattering

Goal: 
•  Pump: Melt charge/spin order with 
op8cally phase transi8on   
•  Probe: Study the dynamics which 
govern charge reorganiza8on 




                                        L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
• 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)
                                                    L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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)




                  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
end‐sta8on at SLS, PSI  
      Em                       hv`  



    hv 

                  ΔE
            E f 
       Ei 
             Energy transfer:                  Momentum transfer: 
              ΔE = hv – hv` 
                                                  q = kin ‐ kout 


RIXS Spectrometer: 




                                        L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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  

                                                                  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
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

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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
  • 2. Paul Scherrer Institute 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  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 5. Research at PSI Health Energy Proton and therapy Environment Micro- Large and scale Nano- facilities technology L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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) L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 11. Synchrotron Radiation Crab Nebula L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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)  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 14. Time resolved (Motion and shutter speed) L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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. L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 16. Space and Time Space mm µm nm ns ps fs Time L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 17. Light as probe Resolution: Space→ λ Time→ τ λ cτ L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 20. SwissFEL Tunnel & Building •  Accelerator, beamlines and experiment underground •  Linac HF and other facilities above ground L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 21. SwissFEL: Villigen or Würenlingen 10.11.2009  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 24. Our Sisters... 1 km Europe EU-XFEL–DESY 2014 Japan SCSS–SPring8 2011 USA LCLS-SLAC 2009 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 25. Scientific Challenges L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 26. Correlated electrons weak and strong interacting electron systems L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 28. Averaging in time (slow shutter speed) L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 29. Time resolved (fast shutter speed) Dynamics in correlated electron: new aspect and new physics! L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 30. Lattice, Charge, Spin and Orbital orders Lattice Charge Orbital Spin L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 31. Resonant X-ray Scattering Resonant X-ray (emission): Scattering (diffraction): Chemical information Structural information Photon Photon In Out Back scattering angle L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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 L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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) L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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) L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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:  L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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   L. Patthey, June 22, 2010, San Francisco, swissnex San Francisco
  • 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