1. X - Rays & Crystals Characterizing Mineral Chemistry & Structure J.D. Price Characterizing Mineral Chemistry & Structure J.D. Price

2. Wave behavior vs. particle behavior If atoms are on the 10 -10 m scale, we need to use sufficiently small wavelengths to explore this realm if we want to learn something about atoms and lattices. Light - electromagnetic spectrum

3. Diffraction E.B. Watson

4. wave property Diffraction of light

5. Where intersections of the diffracted wave fronts occur, there is constructive interference E.B. Watson

6. The difference is only of scale. We can use optical wavelengths for the grid on the left, because they are appropriately spaced for those wavelengths. With small wavelengths, lattices diffract. Scale - grating and

7. Crystalline structure diffracts x-rays (XRD) Bragg equation:  = 2d sin  Crystal with unknown d spacing X-ray source with known Crystal diffractometry

8. Modern diffractometer

9. Diffraction lines are generated by any plane within the crystal geometry. That of course means the root planes to the unit cell, but it also includes all of the possible diagonals. Miller indices are used to label to the lines resulting from the planes (you know all about indexing). In a powdered sample, grains typically orient in a myriad of directions*, such that many diffraction lines are simultaneously generated *exception - sheet silicates

10. The resulting information is structural! (100) 4.1341 Å (011) =3.259 Å (110) 2.3868 Å This is the diffraction patter for quartz (mindat.org). Peaks correspond to specific lattice planes. Their relative intensity is diagnostic. Powder diffraction plot

11. This is great for polymorphs. Calcite (top) and aragonite (bottom) have the same composition, but different structures as evidenced from their diffraction patterns. Polymorphs

12. Most minerals are sized between 0.1 - 100’s of mm. The rather ordinary rock slab on the left is composed of small (1- 5mm) grains of quartz and feldspar. The feldspar below is large (15 mm) but is concentrically zoned. Chemical analysis

13. Feldspars are solid-solutions and exhibit a range of compositions. How might we determine the composition of the minerals in our rocks? What is unique about each element? M T T

14. E photon = E H - E L = h f = h c / 1. To obtain composition, we need a measurable characteristic for each element. Electron structure is element specific. In other words, E photon is the result of a specific jump in a specific element. Fluorescence: electromagnetic radiation results from moving electrons closer to the nucleus Photoelectric characteristic

15. Photo by Elizabeth Frank Fluorescence Visible light is produced by energies in U.V. light.

16. Examples of transition levels in Barium K 37.44 keV L I 5.99 keV L II 5.63 keV L III 5.25 keV So L II to K (K  1 ) is… 31.81 keV Heavier atoms have many energy levels Energy levels

17. So L II to K is 31.81 keV or 31,810 eV The wavelength of the photon produced by this jump is  h c / E h = 6.626 × 10 -34 m 2 kg/s c = 3 × 10 8 m/s E = 31,810 eV × 1.602 × 10 -19 J/ eV = 5.096 × 10 -15 J So  = 3.900 × 10 -11 m Calculating the wavelength

18. 2. To get analysis at micron scale, we need high energies (keV) focused on small area Electrons are charged particles that can be focused and redirected using a magnets Lower energy example: the CRT Raymond Castaing formulated the technique for microanalysis and built the first working unit by 1951. Focus!

19. 3. Fluoresced x-rays need to be collected and counted. Recall that crystalline structure diffracts x-rays (XRD) Bragg equation: = 2d sin  Crystal with unknown d spacing X-ray source with known Count

20. Castaing’s machine: focused electron beam that produces x-rays in an unknown, that may be counted at known diffraction angles. Wavelength dispersive spectrometry (WDS) Bragg equation: = 2d sin 

21. The intensity of x-rays is much smaller relative to those generated from a tube (as in XRD) The EMP wavelength spectrometer uses crystals with curved lattices and ground curvature to reduce lost x-rays The Rowland Circle Crystal Detector Inbound X-rays Maximizing counts

22. Example of a modern EM probe Locate the following: Cathode and anode Beam Magnets Sample Crystal Detector

23. The Cameca SX100 Five spectrometers Each with 2-4 crystals The new RPI facility Cameca SX 100 EMP Rontec EDS detection Gatan mono CL

24. Electron forces jump Char. photon produced Glancing background ph n Produced photon adsorbed - may produce Auger e - Electron bounces off atom (high E): backscattered Electron knocks out another e - (low E): secondary Electron-sample interactions

25. EMPA does not analyze surfaces (thin film), but penetrates a small volume of the sample. The collectable products of electron collision origin originate from specific volumes under the surface. Analysis volume

26. Secondary electrons emitted from the first 50 nm Images surface topography Backscattered electron intensity are a function of atomic density Images relative composition Useful interactions

27. Ti Characteristic x-ray emission

28. The x-ray volume changes as a function of a number variables. A sample with higher average atomic density will have a shallower but wider volume than one with a lower density. A beam with higher energy (keV) will produce a larger volume than one with a lower E 0. Nonunique nature of emission volume

29. From the excitation volume behavior, it is clear atomic density (Z) makes a difference in the emitted intensities. Some of the x-rays are absorbed into atoms within and adjacent to the excitation volume. Some of the x-rays promote electron jumps in atoms within and adjacent to the excitation volume. Z A F Raw data are corrected for ZAF influences. The total correction produces a rather long equation that may be satisfied only through iteration. The microprobe advanced as a tool because of the microprocessor Sample effects

30. The number of x-rays counted at the appropriate diffraction angle is proportional to the concentration of the fluorescing element. But the excitation volume is not unique. Quantification requires comparison to a well-characterized standard. Standard analyzed by other means Your sample with unknown composition Standardization

31. Castaing’s micro WDS machine was a breakthrough. By 1960, advances in semiconduction permitted the construction of a new detector that could collect all of the emitted x-ray energies (pulses and background) within a few seconds. Energy Dispersive Spectrometry (EDS) Measures charges in semiconductor [Si(Li)] Makes histogram of measured charges Extremely fast Very inexpensive Lower accuracy relative to WDS EDS

32. EDS spectrum for a 15kV beam on a gemmy crystal from the Adirondacks (M. Lupulescu, NYSM). Al K  &  Si K  &  KKKK K K  Energy spectrum

34. EMPA traverses of spinel using WDS Formula for the spinel Nom: Mg Al 2 O 4 Act: Mg 1-3x Al 2+2x O 4

36. EMPA is a powerful tool for compositional analysis at the micrometer scale High voltage electron beam can be focused on one micrometer area Composition is determined by characteristic x-rays from excited atoms WDS Characteristic x-rays are focused through diffraction Permits better resolution EDS All x-rays are counted simultaneously Permits faster analysis / identification

37. Limitations Good standards are essential Quantification is dependant on accurate correction for ZAF effects User needs to be aware of excitation volume Results Accurate assessment of mineral stoichiometry WDS provides trace element compositions May assess inhomogeneity at small scales