X-ray Powder Diffraction
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1 X-ray Powder Diffraction Chemistry 754 Solid State Chemistry Lecture #8 April 15, 2004 Single Crystal Diffraction Diffracted Beam Incident Beam Powder Diffraction Diffracted Beam Incident Beam In powder diffraction only a small fraction of the crystals (shown in blue) are correctly oriented to diffract. 1
2 Single Crystal Diffraction (3D) Powder Diffraction (1D) Intensity Theta (Degrees) Single Crystal Diffractometer (4 circles) Powder Diffractometer (2 circles) 2
3 Powder Diffraction Methods Qualitative Analysis Phase Identification Quantitative Analysis Lattice Parameter Determination Phase Fraction Analysis Structure Refinement Rietveld Methods Structure Solution Reciprocal Space Methods Real Space Methods Peak Shape Analysis Crystallite Size Distribution Microstrain Analysis Extended Defect Concentration Information in a Diffraction Pattern Peak Positions Unit Cell Dimensions Crystal System Translational Symmetry Qualitative Phase Identification Peak Intensities Unit Cell Contents Point Symmetry Quantitative Phase Fractions Peak Shapes & Widths Crystallite Size (2-200 nm) Non-uniform microstrain Extended Defects (stacking faults, antiphase boundaries, etc.) 3
4 Debye-Scherrer Camera & Cones of Diffraction λ = 2d hkl sin θ hkl Measuring Diffraction Rings Area Detector Film Strip 4
5 Measuring Diffraction Rings U U = 4θ hkl R θ hkl = Bragg Angle R = Diffractometer Radius Preferred Orientation/Texture Area Detector Film Strip 5
6 Bragg-Brentano Brentano Parafocusing Diffractometer Horizontal Diffraction Circle Antiscatter Slit Sample (Vertical Flat Plate) 2θ θ Divergence Slit Divergent X-ray Source Horizontal Soller Slits Receiving Slit Detector Peak Positions Bragg s Law: λ = 2d hkl sin θ hkl The interplanar spacing, d, for a given hkl reflection is given by the unit cell dimensions Cubic: 1/d 2 = (h 2 + k 2 + l 2 )/a 2 Tetragonal: 1/d 2 = {(h 2 + k 2 )/a 2 } + (l 2 /c 2 ) Orthorhombic: 1/d 2 = (h 2 /a 2 ) + (k 2 /b 2 ) + (l 2 /c 2 ) Hexagonal: 1/d 2 = (4/3){(h 2 +hk+ k 2 )/a 2 } + (l 2 /c 2 ) Monoclinic: 1/d 2 = (1/sin 2 β){(h 2 /a 2 ) + (k 2 sin 2 β/b 2 ) + (l 2 /c 2 ) (2hlcos β/ac)} 6
7 Example: SrTiO 3 The crystal structure of SrTiO 3 is cubic, space group Pm3m with a unit cell edge a = 3.90 Å. Calculate the expected 2θ positions of the first three peaks in the diffraction pattern, if the radiation is Cu Kα (λ = 1.54 Å). 1. Recognize the hkl values for the first few peaks: 100, 110, 111, 200, 210, 211, 220, etc. 2. Calculate the interplanar spacing, d, for each peak: 1/d 2 = (h 2 + k 2 + l 2 )/a 2 3. Use Bragg s Law to determine the 2θ value: λ = 2d hkl sin θ hkl Example: SrTiO 3 hkl = 100 1/d 2 = ( )/(3.90 Å) 2 d = 3.90 Å sin θ 100 = 1.54 Å/{2(3.90 Å)} θ= 11.4 (2θ = 22.8 ) hkl = 110 1/d 2 = ( )/(3.90 Å) 2 d = 2.76 Å sin θ 100 = 1.54 Å/{2(2.76 Å)} θ= 16.2 (2θ = 32.4 ) hkl = 111 1/d 2 = ( )/(3.90 Å) 2 d = 2.25 Å sin θ 100 = 1.54 Å/{2(2.25 Å)} θ= 20.0 (2θ = 40.0 ) 7
8 Effect of Sample Height Displacement 2θ (in radians) = (2s cos θ)/r S = sample height displacement R = Diffractometer radius Examples S = 0.1 mm 2θ ~ 0.05 (2θ ~ 20 a=12.00 A A) 2θ ~ 0.05 (2θ ~ 62 a=12.00 A A) S = 1.0 mm 2θ ~ 0.5 (2θ ~ 20 a=12.00 A A) 2θ ~ 0.5 (2θ ~ 62 a=12.00 A A) Diffraction Intensities We are mainly interested in the elastic scattering that gives rise to coherent diffraction lines. The intensity of each diffraction line depends upon the following factors: I(hkl) = LP(θ) p A(hkl) F(hkl) 2 F(hkl) = Structure Factor p = Multiplicity LP(θ) = Lorentz & Polarization Factors A(hkl) = Absorption Temperature (Displacement) Factors Preferred Orientation & Extinction 8
9 Qualitative Analysis Searching with the ICDD Once you have a powder pattern you can use it like a fingerprint to see if it matches the powder pattern of an already known compound. Nowadays this is usually done with the help of a computer. The International Centre for Diffraction Data (ICDD) maintains a database of known powder diffraction patterns ( 115,000 patterns (not all unique) 95,000 Inorganic compounds 20,000 Organic compounds Sample ICDD Card 9
10 Indexing Indexing is the process of determining the unit cell dimensions from the peak positions. Assign Miller indices, hkl, to each peak Inductive and not reversible First step in Rietveld refinement and structure solution Autoindexing Using a computer to index the powder pattern Indexing a Cubic Pattern λ = 2d hkl sin θ hkl 1/d 2 = 4 sin 2 θ/ λ 2 1/d 2 = (h 2 + k 2 + l 2 )/a 2 sin 2 θ /(h 2 + k 2 + l 2 ) = λ 2 /4a 2 Need to find values of h,k,l for each sin 2 θ that is a constant. 10
11 Cubic Example 2-Theta 1000 sin 2 θ 1000 sin 2 θ /CF hkl CF = Theta 1000 sin 2 θ 1000 sin 2 θ /CF hkl
12 CF = (37.1/1000) = λ 2 /4a 2 (a = 4.00 A) 2-Theta 1000 sin 2 θ 1000 sin 2 θ /CF hkl / Indexing & Systematic Absences Typically there will be some systematic absences. Consider the following example. Assume Cu radiation, λ = A. 2-theta d 1000/d
13 It s immediately clear that 99.2 is not a common factor here. Though we can see that =33 might be a common factor. So we ll give it a try. 2-theta d 1000/d 2 hkl /33= /33= /33= /33= /33= /33= /33= /33= From the absences we see that the compound is F-centered, a = [1000/33] 1/2 = 5.50 Angstroms Autoindexing Manual indexing of cubic unit cells is a reasonably straightforward process. Tetragonal, trigonal and hexagonal cells can also be indexed manually with some experience, but it is not a trivial exercise. Generally indexing is done using a computer program. This process is called autoindexing. The input for an autoindexing program is typically: The peak positions (ideally lines) The wavelength The uncertainty in the peak positions The maximum allowable unit cell volume 13
14 Autoindexing Software A number of the most useful autoindexing programs have been gathered together by Robin Shirley into a single package called Crysfire. You can download Crysfire from the web and find tutorials on its use at To go index a powder diffraction pattern try the following steps: Fit the peaks using a program such as X-Fit ( Take the X-fit output file and convert to a Crysfire input file, as described on the web. Run Crysfire to look for the best solutions. Evaluate the systematic absences and refine the cell parameters. This can be done using the material in the front of the international tables for crystallography or using a program like Chekcell ( Autoindexing - Pitfalls Inaccurate data Analytically fit the peaks Either correct for or avoid sample displacement error (internal standard if necessary) Impurities Try different programs Drop out various weak peaks Try different sample preps Complimentary analysis Psuedosymmetry Unit cell dimensions are close to a more symmetric crystal system Inadequate number of peaks You really need peaks, particularly if the symmetry is low 14
15 How do I know when I m finished? Evaluate output based on figure of merit, when the following conditions are met the solution warrants close consideration M 20 > 10 All of the peaks are indexed Solutions with figures of merit above 20 or so almost always have some degree of the truth in them, but closely related solutions and partially correct solutions are common. Favor high symmetry solutions over low symmetry ones. Autoindexing is a way to get your foot in the door. Solutions always have to be checked further. Structure Solution Once you have prepared a crystalline, single phase sample there are three basic steps to complete in order to derive an accurate crystal structure Indexing the Pattern and assigning the space group symmetry Provides unit cell dimensions and space group symmetry Structure Solution Provides approximate identities and locations of the atoms within the unit cell Structure (Rietveld) Refinement Provides most accurate values of the atomic positions, occupancies and displacement parameters We ve already covered Indexing and Rietveld refinements, now lets look at structure solution more closely. 15
16 Reciprocal Space Methods Extract peak intensities from the powder data (using whole pattern fitting) and then use single crystal methods to analyze these intensities. Patterson Methods Direct Methods Maximum Entropy Methods Difference Fourier Mapping Single crystal techniques are not nearly as reliable and powerful when applied to powder data due to the problem of peak overlap. High resolution data is essential High angle data is often important, but not useful when peak overlap is severe. Real (Direct) Space Methods Real space techniques make use of computer power to try and find the structure that best fits the data. Input a random guess at the crystal structure Calculating a powder pattern and compare it with the observed pattern Modify the structure and compare again Repeat the process numerous times until the best match to the experimental pattern is found. Often used for molecular solids where atomic connectivity and bond distances may be known Define a molecular unit Vary torsion angles, location and orientation of molecule 16
17 Rietveld Refinements What is the goal of a Rietveld refinement? To obtain an accurate crystal structure What is the basic idea of a Rietveld refinement? To fit the entire diffraction pattern at once, optimizing the agreement between calculated and observed patterns What input is needed to carry out a Rietveld refinement? Correct space group symmetry Reasonably accurate unit cell dimensions Approximate starting positions for the atoms (correct Wyckoff sites) Structural Complexity How complex of a crystal structure can one accurately refine with the Rietveld method? Depends upon several factors Quality of the sample (sharp peaks or broad, diffracts out to what value of d) Quality of the instrument (the more peak intensities the better, so we want high resolution and large coverage of Q space) Pseudosymmetry gives heavy peak overlap that can severely limit your accuracy. Soft Constraints, rigid bodies, etc. are ways to get information where full unconstrained refinement is not accurate. In the best cases people have accurately refined structures with atomic parameters. 17
18 Intensity (Arb. Units) 70 K Blue = Observed Green = Calculated Red = Difference Black = Expected peak positions Theta (Degrees) 18
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