Focused X-Ray Beams : Generation and Applications Advances in Science, Engineering and Technology Colloquium lodha@rrcat.gov.in X-ray Interaction with Matter source: Spring-8 web site Focused X-ray Beams W.C. Roentgen : Refractive index of all materials ≈ unity Difficult to make an x-ray lens. With the recent availability of extremely bright x-ray sources (synchrotron storage rings, x-ray free electron lasers, …), R&D efforts towards focusing x-rays to smaller and smaller size have become intense. At present it is possible to generate focused x-ray beam of <30 nm, using the reflection, diffraction and refraction phenomena in the x-ray region. Optics for X-ray (~10 keV) Complex refractive index: n=1-δ+iβ Refraction is small: Re(n)=1-δ with δ=10-6 ….10-5 Focal length: f=R/2 (n-1) = R/2δ Absorption is high: absorption lengths 1μm … 10μm Figure of merit: β/δ = 10-5 (Li,Be) …10-3 (C,Al,Si) …10-1 (Au,Pt,W) Dilemma smaller f smaller R more flux larger aperture larger R Why focus x-ray to sub micron size? X-ray microscopy: Most materials are heterogeneous at length scale of micron to nm (transmission microscopy, scanning microscopy…). Increased flux: Higher sensitivity due to reduced background. Small samples or samples in different environment (pressure, temperature, magnetic field …) General Terminology in X-Ray Optics Magnification Numerical Aperture Resolution Depth of focus Astigmatism Chromatic Aberration Ideal focusing lens: Converts plane wave to a spherical wave, with the conservation of the coherence In-coherent source Geometric Optics Refraction 1/F = (n-1) (1/Do + 1/Di) Coherent source Wave Optics Refraction Phase shift along the optical path Magnification: M=Di/Do For generating x-ray micro/ nano focused beam M~10-2 to 10-4 in synchrotron beamline. Numerical Aperture • Measure of light collection power NA= n Sin θmax NA ~ 0.5 (D/f) NA is very closely related to performance of the optics (e.g. depth of focus, diffraction limited resolution, flux etc.). Low NA is one of the major constraint for x-ray optics. For high photon flux at the focus: High brightness and large numerical aperture Focusing increases the angular spread. Brightness: B= P/ (ΔAs . ΔΩs) P : radiated power; ΔAs :source area ; ΔΩs : source divergence The photon flux at the focus is ~ B. 2 . NA2. η is spot size and η is the efficiency of the optics. Thus the high photon flux at the focus requires high source brightness and large numerical aperture optics. Rayleigh’s Criterion: Resolution Limit Point sources are spatially coherent Mutally incoherent Intensities add Rayleigh criterion (26.5% dip) Conclusion : With spatially coherent illumination, objects are “just resolavable” when source: D. Attwood Resolution improves with smaller λ Depth of focus Where is a spot size source: Xradia Astigmatism Horizontal and vertical focusing are separated at grazing incidence. fm = (R Sin θ)/2 fs = R/(2Sinθ) Source Reflection Crossed mirror pair (Kirkpatrick-Baez system) Focus Synchrotron radiation sources or or Chromatic aberration Reflective Optics: Can focus pink beams using grazing incidence optics. Grazing angles can be higher by using x-ray multilayer reflector, but at the cost of limited energy Diffractive Optics : f ~ E , small NA Refractive Optics : f ~ E2 X-ray Micro focussing optics Reflective optics Diffractive optics Refractive optics X-ray Reflectivity: Single and Multilayer Single Layer Multilayer Total external reflection when θ<θc (a few mrad) Large θ leads to larger acceptance or shorter mirror length. c = √2 = λ√Z Spectral bandwidth ~ a few % X-ray Multilayer Optics Advantages Layer Can thicknesses can be tailored be deposited on figured surfaces Reflective optics Schwarzschild objective Wolter microscope Capillary optics Kirkpatrick-Baez mirrors Schwarzschild objective Near normal incidence with multilayer coating (126 eV) N.A. > 0.1 Imaging microscope source: F. Cerrina (UW-Madison), J. Underwood (LBNL) Wolter microscope Use 2 coaxial conical mirrors with hyperbolic and elliptical profile Imaging microscope Difficult to polish for the right figures and roughness Capillary optics One-bounce capillary Multi- bounce condensing capillary Large working distance (cm) Easy to make with small opening (submicron) Compact: may fit into space too small for K-B Nearly 100% transmission Short working distance (100 μm) Low transmission N.A. ~ 2-4 mrad (¡Ü 2θc) Difficult to make submicron spot source: D. Bilderback (Cornell) Kirkpatrick-Baez mirrors A horizontal and a vertical mirror arranged to have a common focus Achromatic: can focus pink beam (but not with multilayer coating) Can be used to produce ~ round focal spot Very popular for focusing in the 1-10 μm APS 85x90 nm2 ESRF 45 nm, Spring8 25x30 nm2 (diffraction limit ~ 17 nm) Diffractive optics Fresnel zone plates (FZP) Multilayer Laue Lens (MLL) Fresnel zone plates (Phase ZP and Amplitude ZP) Efficiency of an amplitude ZP with opaque zones ~ 10% Efficiency of a phase ZP with π-phase shift ~ 40% Phase For a phase shift of Fabrication Fresnel zone plates E Anderson, A Liddle, W Chao, D Olynick and B Harteneck (LBNL) Hard X-ray ZP: recently available W. Yun (Xradia) Δr = 24 nm, 300 nm thick, Aspect Ratio = 12.5 (Xradia) Aspect ratio > 100 is probably difficult to achieve with lithographic zone plates! Multilayer Laue Lens (MLL) For high aspect ratio Aspect ratio > 1000 (Δr = 5-10 nm, 10 μm thick) demonstrated Source : A. Macrander (APS) Refractive optics Compound refractive lens (CRL) Small aperture Small focusing strength Strong absorption E>20keV f = R/2N R radius (~200 m) N number of lenses (10 …300) real part of refractive index (10-5 to 10-6) 2R0 800 m -1000 m d 10 m -50 m Parabolic profile : No spherical aberration Source : Achen Univ., APL 74, 3924 (1999) What is Synchrotron Radiation? Synchrotron radiation is emitted from an electron traveling at almost the speed of light (0.99999999C) and its path is bent by a magnetic field. It was first observed in a synchrotron in 1947. Thus the name "synchrotron radiation". Generation of Synchrotron Radiation Synchrotron radiation is emitted at a bending magnet or at an insertion device. Corresponding to the weak and strong magnetic field, there are two types of insertion devices: an undulator and a wiggler. General Properties of Synchrotron Radiation Ultra-bright Highly directional Spectrally continuous (Bending Magnet /Wiggler) or quasi-monochromatic (Undulator) Linearly or circularly polarized Pulsed with controlled intervals Temporally and spatially stable Synchrotron Radiation Spectrum Brightness of synchrotron sources X-ray Sources: Peak Brilliance Synchrotron Radiation(SR) Sources… America: Asia: Europe: Oceania: 18 25 22 1 IV generation light sources under construction/ planning stage. A Typical Synchrotron Facility Creating SR light (3) Then they pass into the booster ring accelerated to c (4) And are finally transferred into the storage ring (1) Electrons are generated here (2) Initially accelerated in the LINAC A typical Synchrotron source With BM and ID Building a Synchrotron Source… Magnets Beam physics Survey and alignment Controls LCW UHV Power supplies Synchrotron Health physics Beam diagnostics RF systems Chemical Cleaning Cryogenics etc. Fabrication and metrology shop Utilization of the properties of the SR beam: A few examples Microbeam: Diffractometry, microscopy Pulsed Structure : Time-resolved experiments Energy Tunability: Crystal structure analysis, anomalous dispersion High collimation: Various types of imaging techniques with high spatial resolution Linear / circular polarizion : Magnetic properties of materials. High energy X-ray: High-Q experiments, Compton scattering, Excitation of high-Z atoms High spatial coherence: X-ray phase optics and X-ray interferometry Application of SR Life Science Atomic structure analysis of protein macromolecules Elucidation of biological functions Materials Science Precise electron distribution in inorganic crystals Structural phase transition Atomic and electronic structure of advanced materials superconductors, highly correlated electron systems and magnetic substances Local atomic structure of amorphous solids, liquids and melts Chemical Science Dynamic behaviors of catalytic reactions X-ray photochemical process at surface Atomic and molecular spectroscopy Analysis of ultra-trace elements and their chemical states Archeological studies Earth and Planetary Science In situ X-ray observation of phase transformation of earth materials at high pressure and high temperature Mechanism of earthquakes Structure of meteorites and interplanetary dusts Environmental Science Analysis of toxic heavy atoms contained in biomaterials Development of novel catalysts for purifying pollutants in exhaust gases Development of high quality batteries and hydrogen storage alloys Industrial Application Characterization of microelectronic devices and nanometer-scale quantum devices Analysis of chemical composition and chemical state of trace elements X-ray imaging of materials Residual stress analysis of industrial products Pharmaceutical drug design Medical Application Application of high spatial resolution imaging techniques to medical diagnosis of cancers SR Based Research Methods X-ray Diffraction and Scattering Spectroscopy and Spectrochemical Analysis X-ray Imaging Radiation Effects Indus building complex Synchrotron Complex at RRCAT housing Indus-1 and Indus-2 Schematic View of Indus Complex Booster Synchrotron (700 MeV) TL-1 (Started in 1995) Microtron (20 MeV) (Started in 1992) TL-2 TL-3 Indus-1 (450 MeV, 100 mA) (Working since 1999) Indus-2, 2.5 GeV SR Trials to store the beam began in December 2005 Indus-1 Storage Ring Schematic representation of experimental hall Five beamlines have been operational. Several publications (~50) have resulted from utilization of these beamlines. Beamlines operational on Indus-1 λ/Δλ Experimental station 1.4 m TGM with three gratings ~400 Reflectometer and time of flight mass spectrometer Pt coated Toroidal 2.6 m TGM with three gratings ~600 Hemi-spherical analyzer (HSA) 4-100 Pt coated Toroidal 1.4 m TGM with three gratings ~400 Angle resolved HSA electron analyzer Photo Physics (BARC) 50-250 Au coated Toroidal 1 m Seya-Nomioka ~1000 Absorption cell , sample manipulator High resolution VUV (BARC) 70-200 Au coated cylindrical 6.65 m off plane Eagle mount spectrometer ~70000 High temperature furnace, absorption cell Beamline Range (nm) Beamline Optics Pre and Post mirror Reflectivity (RRCAT) 4-100 Au coated Toroidal Angle Integrated PES (UGC-DAECSR) 6-160 Angle Resolved PES (BARC) Monochromator Recent studies using Indus -1 Reflectivity near absorption edge energies Hydrogen bond braking near absorption edge energies Interface studies Photo dissociation spectroscopy X-ray multilayer optics and optical response in soft x-ray region X-ray Telescope Calibration Indus-2 beamlines BM Beamlines ADXRD (commissioned) BL# Groups BL-12 RRCAT EDXRD (commissioned) BL-11 BARC EXAFS (commissioned) BL- 8 BARC GIMS ( being installed) Bl-13 SINP PES (being installed) BL-14 BARC BM MCD/PES BL-1 UGC-DAE-CSR Imaging BL-4 BARC + UGC-DAE-CSR ARPES/PEEM BL-6 BARC White-beam lithography BL-7 RRCAT Scanning EXAFS BL-9 BARC XRF-microprobe BL-16 RRCAT SWAXS BL-18 BARC Protein Crystallography BL-21 BARC X-ray diagnostics BL-23 RRCAT Visible diagnostics BL-24 RRCAT Soft X-ray BL-26 RRCAT Under Construction being installed/ under construction Installed X-ray Multilayer Deposition Laboratory Reflectivity Beamline Indus-1 Normal incidence soft x-ray reflector: Mo/Si multilayer 0.8 Reflectivity 10 0.6 Reflectivity 10 0 -1 0.4 0.2 0.0 100 110 120 130 140 150 160 Wavelength A 10 -2 10 -3 0 20 40 60 Incidence angle deg 80 100 X-ray calibration: Soft X-ray Telescope ASTROSAT :One of the most ambitious space astronomy programme initiated by Space Science Community in India. Payload of soft x-ray imaging telescope (SXT) sensitive to 0.3 to 8 keV is planned. Performance of SXT grazing incidence foil mirrors evaluated using Indus-1 soft x-ray reflectivity beamline Archana et al Experimental Astronomy (2010) 28:11-23 Soft & Deep X-ray Lithography (SDXRL) beamline -BL7 SDXRL beamline - Applications MEMS (Micro-Gears, …) Zone Plate Fabrication of Hard x-rays optics Small periodicity gratings Micro Electro Mechanical Systems (MEMS) Photonic band gap crystals (for visible radiation) Quantum wires and quantum dots devices (high density pattering over large areas) Fabrication of high density hetrostructures for nano devices High aspect ratio micro-structures SDXRL beamline – Present Status Installed beamline inside hutch X-ray mirrors with manipulators Primary slits X-ray BL16 Beamline Front End Beamline optics DCM Beam transport pipes and vacuum components KB mirror Front end exit Pre-DCM section X-ray Microprobe beamline Beamline optics Post-DCM section DC M Beam transport pipes and vacuum components Road Ahead…. • A modest start has been done at RRCAT with the availability of synchrotron radiation sources Indus1 and Indus-2. These sources are being operated on a round the clock basis, week after week. • Few x-ray beamlines have become operational, with many more in implementation stage. • These are national science facilities. Users from various fields are welcome to plan research using these facilities, which will significantly help us to improve the performance further. It will be our endeavor to support all users of this national facility. All are welcome to Indus SR Facility 67 Acknowledgements: X-ray Diffraction and Scattering Research Methods Typical Examples of Research Subjects Macromolecular crystallography ( I-2) Atomic structure and function of proteins. X-ray diffraction under extreme conditions (I-2) Structural phase transition at high pressure / high or low temperature X-ray powder diffraction (I-2) Precise electron distribution in inorganic crystals Surface diffraction (I-2) Atomic structure of surfaces and interfaces. Phase transition, melting, roughening, morphology and catalytic reactions on surfaces Small angle scattering (I-2) Shape of protein molecules and biopolymers. Dynamics of muscle fibers X-ray magnetic scattering Magnetic structure. Bulk and surface magnetic properties X-ray Optics X-ray interferometry. Coherent X-ray optics. Xray quantum optics Spectroscopy and Spectrochemical Analysis Research Methods Typical Examples of Research Subjects Photoelectron spectroscopy (I-1) Electronic structure of advanced materials such as superconductors, magnetic substances, and highly correlated electron systems. Atomic and molecular spectroscopy (I-1) Photoionization spectra, photoabsorption spectra and photoelectron spectra of neutral , atoms and simple molecules. Spectra of multicharged ions. X-ray fluorescence spectroscopy (I-2) Ultra-trace element analysis. Chemical states of trace elements. Archeological and geological studies. X-ray absorption fine structure (I-2) Atomic structure and electronic state around a specific atom in amorphous materials, thin films, catalysts, metal proteins and liquids. X-ray magnetic circular dichroism (I-2) Magnetic properties of solids, thin films and surfaces. Orbital and spin magnetic moments. Infrared spectroscopy (I-2) Infrared microspectroscopy. Infrared reflection and absorption spectroscopy. X-ray inelastic scattering Electronic excitation. Electron correlations in the ground state. Phonon excitation. X-ray Imaging Research Methods Typical Examples of Research Subjects Refraction-contrast imaging (I-2) lmaging of low absorbing specimens. X-ray fluorescence microscopy (I-2) Imaging of trace elemental distribution with a scanning X-ray microprobe. X-ray microscopy (I-2) Imaging of materials by magnifying with microfocusing elements. X-ray topography (I-2) Static and dynamic processes of crystal growth, phase transition and plastic deformation in crystals. Crystal lattice imperfections. Photoelectron emission microscopy (I-2) Element-specific surface morphology. Chemical reaction at surface. Magnetic domains. Radiation Effects Research Methods Typical Examples of Research Subjects Material processing (I-2) Soft X-ray CVD. Microfabrication. Radiation biology (I-2) Radiation damage of biological substances. Mo/Si soft x-ray Polarizer multilayer 1 N=120 layers Top SiO2 20.7A: 6.7A: 2.78e-2 Si 72.0A; 7.1; 4.22e-3; 1.94e-3 Mo 31.0A; 7.0 ; 7.99e-2; 8.66e-3; SubS 5.0A Beam polarization 80% Reflectivity 0.1 wavelength 138A 0.01 1E-3 Measured Fit 1E-4 -10 0 10 20 30 40 50 Incidence angle deg 60 70 80