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Faustlin, R.R.     [Fäustlin, R.R.]

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FROB01 Achieving Microfocus of the 13.5-nm FLASH Beam for Exploring Matter Under Extreme Conditions 784
 
  • A.J. Nelson, R.W. Lee
    LLNL, Livermore, California
  • J. Andreasson, J. Hajdu, N. Timneanu
    Uppsala University, Biomedical Centre, Uppsala
  • S. Bajt, H. Chapman, R.R. Fäustlin, S. Toleikis
    DESY, Hamburg
  • J. Chalupsky, V. Hajkova, L. Juha
    Czech Republic Academy of Sciences, Institute of Physics, Prague
  • T. Dzelzainis, D. Riley
    Queen's University of Belfast, Belfast, Northern Ireland
  • M. Fajardo
    GoLP, Lisbon
  • M. Jurek, R. Sobierajski
    IP PAS, Warsaw
  • A.R. Khorsand
    FOM Rijnhuizen, Nieuwegein
  • J. Krzywinski
    SLAC, Menlo Park, California
  • B. Nagler
    STFC/RAL, Chilton, Didcot, Oxon
  • K. Saksl
    IMR SAS, Kosice
  • T. Tschentscher
    European X-ray Free Electron Laser Project Team, c/o DESY, Hamburg
  • S.M. Vinko, J.S. Wark, T.J. Whitcher
    University of Oxford, Clarendon Laboratory, Oxford
 
 

We have focused a beam (BL3) of FLASH (Free-electron LASer in Hamburg: 13.5 nm, 15fs, 10μJ, 5Hz) using a fine polished off-axis parabola having a focal length of 270 mm and coated with a Mo/Si-ML giving a reflectivity of 67% at 13.5 nm. The OAP was mounted and aligned with a picomotor control six-axis gimbel. Beam imprints on PMMA were used to measure focus and the focused beam was used to create isochoric heating of various slab targets. Results show the focal spot has a diameter of <1μm producing intensities greater than 1016 Wcm−2. Observations were correlated with simulations of best focus to provide further relevant information. This focused XUV laser beam now allows us to begin exploring matter under extreme conditions. Future experimental efforts at ’4th generation’ light sources will be outlined.

 

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FROB04 Saturable Absorption with VUV FEL Radiation  
 
  • S.M. Vinko, G. Gregori, W.J. Murphy, B. Nagler, J.S. Wark, T.J. Whitcher
    University of Oxford, Clarendon Laboratory, Oxford
  • S. Bajt, H. Chapman, S. Düsterer, R.R. Fäustlin, T. Laarmann, S. Toleikis
    DESY, Hamburg
  • T. Bornath
    Rostock University, Faculty of Computer Science and Electrical Engineering, Rostock
  • T. Burian, J. Chalupsky, J. Cihelka, V. Hajkova, L. Juha
    Czech Republic Academy of Sciences, Institute of Physics, Prague
  • T. Doeppner, S.H. Glenzer, R.W. Lee, A.J. Nelson, H.J. Vollmer
    LLNL, Livermore, California
  • T. Dzelzainis, D. Riley
    Queen's University of Belfast, Belfast, Northern Ireland
  • M. Fajardo, M. Kozlova
    GoLP, Lisbon
  • E. Foerster, I. Uschmann
    IOQ, Jena
  • C. Fortmann, S. Goede, K.H. Meiwes-Broer, A. Przystawik, R. Redmer, H. Reinholz, G. Roepke, R. Thiele, J. Tiggesbaumker
    Rostock University, Rostock
  • E. Galtier, F. Rosmej, R. Schott
    UPMC, Paris
  • P.A. Heimann
    LBNL, Berkeley, California
  • M. Jurek, D. Klinger, R. Sobierajski
    IP PAS, Warsaw
  • F.Y. Khattak
    Kohat University of Science and Technology, Kohat
  • A.R. Khorsand
    FOM Rijnhuizen, Nieuwegein
  • J. Krzywinski
    SLAC, Menlo Park, California
  • H.J. Lee
    UCB, Berkeley, California
  • P. Mercère
    SOLEIL, Gif-sur-Yvette
  • T. Tschentscher
    European X-ray Free Electron Laser Project Team, c/o DESY, Hamburg
  • U. Zastrau
    FSU Jena, Jena
 
 

We report for the first time saturable absorption in the soft x-ray regime: by photoionizing L-shell core electrons we observed on a 15fs timescale a multifold increase of transmission through an aluminium foil. While saturable absorption is a phenomenon readily seen in the optical and infrared wavelengths, it has never been observed in a core electron transition due to the short lifetimes of the created excited states and the high intensities of the soft x-rays that are needed. The experiments were performed at the XUV Free Electron Laser FLASH and used record high intensities. After the FEL pulse has passed, the aluminum sample is in an exotic state where all the aluminum atoms have a L-shell hole, and the conduction band has a 9eV temperature, while the atoms are still on their crystallographic positions. Subsequently, Auger decay heats the material to Warm Dense Matter condition, at 20eV temperatures. The saturable absorption allows for a very homogeneous and efficient heating. Therefore the method is an ideal candidate to study homogeneous Warm Dense Matter, highly relevant to planetary science, astrophysics and inertial confinement fusion.

 

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