Introduction to X-Ray Diffraction Structure Molecular, Extended, Quasi, etc 10-10m Angstrom (Å) H Visible Light 4x10-7-9x10-7m 4000-9000 Å Leptons X-rays 0.1 to 14 Å Fermions Neutrons Electrons Interaction between X-ray and Matter • incoherent scattering λ C (Compton-Scattering) • coherent scattering (XRD) wavelength λο λο (Bragg´s-scattering) • Absorption (XANSE etc) intensity Io Beer´s law I = Io*e-µd • Fluorescence (XRF) λ> λo • Photoelectrons (XPS) Part 1. The X-ray Diffractometer Primitive Crystallographers Laue’s Experiment in 1912 Single Crystal X-ray Diffraction Tube Tube Crystal Collimator Film Von Laue’s Camera X-ray Source Pin-hole Optic Specimen Film Rosalind Franklin Powder X-ray Diffraction Film Tube Powder Max Theodor Felix von Laue Max von Laue put forward the conditions for scattering maxima, the Laue equations: a(cosα-cosα0)=hλ b(cosβ-cosβ0)=kλ c(cosγ-cosγ0)=lλ W. H. Bragg and W. Lawrence Bragg W.H. Bragg (father) and William Lawrence.Bragg (son) developed a simple relation for scattering angles, now call Bragg’s law. n⋅λ d= 2 ⋅ sin θ Bragg’s Description The incident beam will be scattered at all scattering centers, which lay on lattice planes. The beam scattered at different lattice planes must be scattered coherent, to give an maximum in intensity. The angle between incident beam and the lattice planes is called θ. The angle between incident and scattered beam is 2θ . The angle 2θ of maximum intensity is called the Bragg angle. Bragg’s Law A powder sample results in cones with high intensity of scattered beam. Above conditions result in the Bragg equation n ⋅ λ = 2 ⋅ d ⋅ sin θ or d = n ⋅λ 2 ⋅ sin θ Essential Parts of the X-ray Diffractometer 1. X-ray Tube: the source of X Rays 2. Incident-beam optics: condition the X-ray beam before it hits the sample 3. The goniometer: the platform that holds and moves the sample, optics, detector, and/or tube 4. The sample & sample holder 5. (Receiving-side optics: condition the X-ray beam after it has encountered the sample) powder 6. Detector: count the number of X Rays scattered by the sample The Generating of X-rays Emission Spectrum of a Molybdenum X-Ray Tube 0.040 amps Vacuum e- 50,000 Volts 2000 watts Chilled water characteristic radiation = line spectra (direct collisions) M e- L K Kα1 Kα2 Kβ1 Kβ2 Bremsstrahlung = continuous spectra (near misses, bending radiation) Monochromator Type 1. Filter Ni foil will filter Cu Y foil will filter Mo (high flux) Type 2. Crystal Graphite (cheap) Ge (better, expensive) (lower flux) Type 3. X-ray Mirrors Thin layers (~10A) of Heavy Metals (very expensive) (high flux) Detectors CCD/Phosphor – Fast, High DQE, Inexpensive – High Background, Hot Spots – Resolution inverse of phosphor thickness IMAGE PLATE – Wide Area, Adaptable – High Background, Slow – Resolution based on grain size MWPC/Micro Gap (VANTEC-2000) – No Detector Background, Fast – Limited Area, Expensive – Resolution limited to wire separation Pixel Area Detector (PAD) – Silicon Strip Technology, very adaptable – Background, very expensive – Resolution based on individual “chips” The X-ray Diffractometer monochromator specimen Detector collimator shutter goniometer X-ray Tube Three-Circle Single-Crystal Diffractometer ⎛ 2⎞ ⎟ χ = 54.73561 = sin ⎜⎜ ⎟ ⎝ 3⎠ o -1 Part 2. The crystal. To view an atom (structure)with X-rays you must find a way to hold it in place! The Crystal A crystal is a solid material whose constituent atoms (molecules and ions) are arranged in an orderly repeating pattern extending in all three spatial dimensions. The Unit Cell c a α β γ b Crystal Systems Crystal systems Axes system cubic a = b = c , α = β = γ = 90° Tetragonal a = b ≠ c , α = β = γ = 90° Hexagonal a = b ≠ c , α = β = 90°, γ = 120° Rhomboedric a = b = c , α = β = γ ≠ 90° Orthorhombic a ≠ b ≠ c , α = β = γ = 90° Monoclinic a ≠ b ≠ c , α = γ = 90° , β ≠ 90° Triclinic a ≠ b ≠ c , α ≠ γ ≠ β° Reflection Planes in a 2D Lattice (3,1) Miller Indices (1/a 1/b) (1,2) b (1.0) (1,1) a Three Dimensions The (200) planes of atoms in NaCl The (220) planes of atoms in NaCl Parallel planes of atoms intersecting the unit cell are used to define directions and distances in the crystal. These crystallographic planes are identified by Miller indices (hkl). Relationship between d-value and the Lattice Constants λ = 2 d s in θ Bragg´s law The wavelength is known Theta is the half value of the peak position d will be calculated 2 2 2 2 2 1/d = (h + k )/a + l /c 2 Equation for the determination of the d-value of a tetragonal unit cell h,k and l are the Miller indices of the peaks a and c are lattice parameter of the elementary cell if a and c are known it is possible to calculate the peak position if the peak position is known it is possible to calculate the lattice parameter The Bragg-Brentano Geometry Detector Tube q focusingcircle Sample measurement circle 2q Powder Pattern and Structure The d-spacings of lattice planes depend on the size of the elementary cell and determine the position of the peaks. The intensity of each peak is caused by the crystallographic structure, the position of the atoms within the elementary cell and their thermal vibration. The line width and shape of the peaks may be derived from conditions of measuring and properties - like particle size - of the sample material. D8 ADVANCE Bragg-Brentano Diffractometer A scintillation counter may be used as detector instead of film to yield exact intensity data. Using automated goniometers step by step scattered intensity may be measured and stored digitally. The digitised intensity may be very detailed discussed by programs. More powerful methods may be used to determine lots of information about the specimen. The atoms in a crystal are a periodic array of coherent scatterers and thus can diffract X-rays. Diffraction occurs when each object in a periodic array scatters radiation coherently, producing concerted constructive interference at specific angles. The electrons in an atom coherently scatter X-rays. The electrons interact with the oscillating electric field of the X-ray. Atoms in a crystal form a periodic array of coherent scatterers. The wavelength of X rays are similar to the distance between atoms. Diffraction from different planes of atoms produces a diffraction pattern, which contains information about the atomic arrangement within the crystal X-Rays are also reflected, scattered incoherently, absorbed, refracted, and transmitted when they interact with matter. From Signal to Intensity Integration Signal Lp correction ABS correction Raw hkl Scale Absorption Correction Intensity and hkl • I (hkl) == Reflections (hkl file = *.hkl) – hkl => where the atoms are • hkl ~ d = Position in reciprocal space –I => what the atoms are • Intensity ~ number of scattering electrons Calculated I(hkl) = K|F(hkl)|2 F (hkl ) = ∑ f i exp[2π (hxi + kyi + lzi )] i observed Fourier Transform Electron density = ρ(xyz) Reciprocal Space to Real Space and Back Fourier Transform ( Phase angle 1 ∞ ∞ ∞ ' ρ ( xyz) = ∑ ∑∑ Fhkl cos 2π hx + ky + lz − α hkl V h k =−∞ l ) Model building employing known Intensities Structure Solution Phase Refinement Fourier ρ ( xyz) = ( Guess? 1 ∞ ∞ ∞ ∑ ∑∑ Fhkl cos 2π hx + ky + lz − α hkl' V h k =−∞ l ) atom (i) Calc. structure factor for atom (i) I (hkl ) = K F (hkl ) obs F (hkl ) cal = ∑ f i exp[2π (hxi + kyi + lzi )] 2 i ρ ( xyz) = D = ∑w hkl (F 2 obs hkl ( 2 ⎛ − kFcalc w F ⎜∑ obs hkl wR 2 = ⎜ 2 2 ⎜ w F ∑ obs ⎜ hkl ⎝ ( ) ) 2 2 1/ 2 ⎞ ⎟ ⎟ ⎟ ⎟ ⎠ − kF calc ) 2 2 Minimize D (modify x,y,z + Thermal p’s) ( 1 ∞ ∞ ∞ ∑ ∑∑ Fhkl cos 2π hx + ky + lz − α hkl' V h k =−∞ l L.S./Fourier ∂D ΔD ~ ∂p Δp ) Summary • Crystal – periodicity – Reduce N X 1020 → N problem • Lattice/Symmetry describes the periodicity – Visual and Mathematical • Scattered X‐rays describe the atomicity – Intensity ~ e‐ density [ρ(xyz)] F ( hkl ) ~ I ( hkl ) • A Model is fit (L.S.) to the ρ(xyz) map. – Minimize the difference between the observed F(hkl) and the calculated F(hkl). • Report the Model The Model • Unit Cell/Symmetry/Coordinates _symmetry_cell_setting _symmetry_space_group_name_H‐M _cell_length_a _cell_length_b _cell_length_c _cell_angle_alpha _cell_angle_beta _cell_angle_gamma ATOM Element X Y Monoclinic P2(1)/c 11.379(11) 39.43(3) 9.824(8) 90.00 109.87(3) 90.00 Z Thermal P. F1A F F2A F O1A O O2A O …. 1.2353(7) 0.6898(7) 1.1028(9) 1.2981(8) 0.084(2) 0.072(2) 0.067(3) 0.057(2) ‐0.4863(6) 0.4873(6) 0.3271(8) ‐0.0537(7) 0.09196(14) 0.07626(13) 0.03134(15) 0.03345(15)
© Copyright 2026 Paperzz