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James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

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Earth & Planetary Science Applications of X-Ray Diffraction: Advances Available for Research with our New Systems. James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico. 401/501 Colloquium November 11, 2011. Outline. What can you do with X-ray Diffraction? - PowerPoint PPT Presentation
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Earth & Planetary Science Applications of X-Ray Diffraction: Advances Available for Research with our New Systems James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico 401/501 Colloquium November 11, 2011
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Page 1: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Earth & Planetary Science Applications of X-Ray Diffraction: Advances Available

for Research with our New Systems

James R. ConnollyDept. of Earth & Planetary Sciences

University of New Mexico

401/501 ColloquiumNovember 11, 2011

Page 2: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Outline

• What can you do with X-ray Diffraction?• X-Ray Powder Diffraction – Introduction to the method• Advances in X-ray detectors• Our Current Scintag system – strengths and weakness• Our New systems (arriving January) – new capabilities• Details of our New Systems (as time allows at end)

Acknowledgements: Thanks to Aya Takase, Al Larsen, and Sean Bird from Rigaku, USA, for help with technical graphics, Maarten DeMoor for use of his sample data, the NationalScience Foundation for funding our new instruments, and CoPIsAdrian Brearley, Abhaya Datye and Darren Dunphy for making it all happen.

Page 3: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

• Identify crystalline materials in powdered samples• Determine of amounts of major and minor phases in multi-phase

samples +• Obtain precise crystal structure data for phases in powders +• Analyze most materials totally non-destructively • Identify crystalline materials in thin coatings on natural or

engineered materials *• Obtain good quality crystallographic data on extremely small

amounts of material *• Analyze materials in controlled environments (oxygen-free,

controlled gas, controlled temperature) *• Perform real-time experiments with materials under controlled

conditions *• Identify phases in a non-destructive manner in intact small samples *

What can you do with X-ray Diffraction?

* Indicates capabilities to be added with our new systems+ Indicates capability greatly enhanced with our new systems

Page 4: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

• Identify trace amounts of phases in a multi-phase sample – though new instruments can detect smaller amounts of material, trace amounts are difficult to impossible to detect

• Quantitatively determine amounts of amorphous material in a sample – this can be done by “difference” with an internal standard but does not leave original material unaltered

• Do single-crystal diffraction analysis (though this capability can be added to one of our new systems as an option)

• Do direct chemical analysis of samples – XRD can do crystallographic analysis NOT chemical analysis

What can’t you do with X-ray Diffraction?

Page 5: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Diffraction patterns contains two “components”:

• Peak position provides information about crystal structure or “d-spacings” in a crystalline phase

• Peak intensity provides information about the scattering power of those “d-spacings”; this is in turn related to the arrangements of constituent atoms in the structure and abundance of phases in a mixture

• Lots of other information may be obtained from peak shape and symmetry

Page 6: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

The Bragg Equation

where n is an integer

is the wavelength of the x-rays

d is the interplanar spacing in the specimen

is the diffraction angle

sin2dn

•The Bragg equation is the fundamental diffraction equation• It is used to calculate interplanar spacings in crystal structures• It is valid only for monochromatic X-rays.

Page 7: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

An XRD Data Plot: 2 (x-axis) vs. intensity (y-axis)

Inte

nsity

Sca

le

2 Angular Scale

Page 8: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Adding Peak Intensity Information to Positions

• Different diffraction peaks show differing intensities

• Scattering occurs at the atomic level• Intensities are related to how all of the scattered

X-rays from atoms in a particular diffracting “d-spacing” add as a vector sum

• The combination of position and intensity is used to “fingerprint” particular crystalline structures (and often but not always unique phases)

Page 9: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Source

Specimen

Monochromator

Detector

Page 10: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 11: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 12: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

An XRD Data Plot: 2 (x-axis) vs. intensity (y-axis)

Page 13: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Search/Match: Results Display

Page 14: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Search/Match: Printout of Results

Page 15: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

GasLiquid /

amorphousPowder /

polycrystalline Single crystal

X-ray Diffraction Patterns

Page 16: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Extracting Information from a diffraction pattern

Background

Amorphous scatteringDiffraction

Peak position Lattice parameters

Whole pattern Phase identification, quantitative analysis

Peak width Crystallite size & strain

%Crystallinity

Page 17: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Phase identification

Page 18: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 19: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Differing Intensity from strong preferred orientation

“Hump” in background indicatespresence of amorphous material

Page 20: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Our Existing Scintag Pad V System

• Sturdy, solid, reliable, good quality data• Point detector collects data in 0.01° to 0.05° steps – avg.

data collection times 1-2 hours per sample; overnight for high resolution (quantitative-capable) data

• One sample at a time (no sample changer)• Cannot change parts easily – limited to Cu X-ray source,

single sample stage, point detector, -2 “Bragg-Brentano” scans

• Alignment is a several-day affair• Analytical Software (DataScan4 & Jade+) good but not

well integrated with instrument• State-of-the-art system in 1985; upgraded but limited by

its age

Page 21: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Laboratory Needs• EPS XRD Lab is a service center used by multiple departments

on campus including: E&PS, Various Engineering Departments and Institutes including CE, ChNE, CMEM, CHTM, Chemistry, Anthropology, Pharmacy, Biology, Water Resources Program

• New System requirements:– Easily reconfigurable for different analytical needs– Operable by non-experts in XRD– Easy, automated alignment after exchange of components– Add new research capabilities including:

• High throughput for standard powder analyses• Microdiffraction (phase identification from very small areas)• Non-ambient (atmosphere, controlled temperature & pressure) experiments• High-speed data collection (for real-time experiments)• Data collection from wet or damp materials• Low-angle data from films and coatings • Small angle scattering (SAXS) analysis for nano-materials

Page 22: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

New Systems to Arrive January 2012• Funded by NSF MRI Grant to CMEM (ChNE) and E&PS• To best meet diverse needs of investigators, we opted for two

new instruments:– Rigaku SmartLab Multi-purpose diffractometer capable of:

• Automated, multi-sample analysis w. sample spinning option• 0D (Point) or 1D High Speed detector• Non-ambient (elevated T, controlled environment) experiments• Focused (parallel) X-ray beam or divergent beam geometry• Horizontal sample orientation (low-volume and wet samples ok)• Glancing Incidence, SAXS, GISAXS, HiRes XRD capabilities and

more– Rigaku Rapid II

• Small area-micro-diffraction w. large 2D detector• Work with very small amounts of powder or intact samples• Obtain diffraction data with highly oriented crystalline material• Standard powder diffraction (when other systems busy)

Page 23: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Rigaku SmartLab

Page 24: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 25: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Rigaku D-Max Rapid II

Page 26: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 27: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Powder Sample

3-Dimensional Diffraction Space

Page 28: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Advances in X-Ray Detectors

• Point or “0d” detectors have a limited “view” of diffraction space – one point at a time, usually 0.2 to 0.5°

• Data collection is by fixed time at each point, usually ½ to severalseconds, thus slow

• If lines are “spotty” because of preferred orientation, diffractions will be missed

• Most common 0d detector is the Scintillation counter -- still widelyused for many applications

• Most efficient if used with a samplechanger in unattended mode

Page 29: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Advances in X-Ray Detectors• Linear or 1d Detectors sample a larger angular slice of diffraction space,

usually 1-3° (but to 120° with specialized detectors)• Moves through a range of diffraction

space as a “sliding window” collecting data throughout its angular range

• Results in greatly increased speed ofdata collection (typically 50x to 100xthat of a scintillation counter)

• Most modern 1d detectors are someform of Silicon strip technology andare very durable and robust devices

Page 30: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Rigaku D/teX Ultra 1d Detector

Linear range of diffraction space (up to 1.5°) measured simultaneously = 50-100x faster data collection

Page 31: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

D/teX Ultra

Zeolite sample measured in 60 seconds

Page 32: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Variable temperature XRD experiment with D/teX Ultra Detector

Page 33: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Advances in X-Ray Detectors

• Area or 2d detectors view a substantial “slice” of diffraction space in two dimensions

• Smaller 2d detectors can be moved through diffraction space and imagescombined to produce large map of 2d space

• Larger 2d detectors can remain fixedrecording a “snapshot” of 2d space

• 2d detectors enable collection of diffraction data from samples withextreme preferred orientation – in some cases collecting useful datafrom single crystals

Page 34: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 35: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Rigaku Rapid II Microdiffraction Advantages

• Extremely large detector (25.6 x 46.6 cm)• Image plate records all X-ray energies – different

sources (Cu, Co, and Mo) may be used.• Sources are easily changed• 3-axis sample stage allows many different sample

types to be mounted and analyzed• Beam collimators cover range from 800 µm to 30 µm• Image recording times can be from 5 to 60 minutes

(or more if needed)• Image is digitally read, data recorded and plate ready

for reuse within a couple of minutes

Page 36: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 37: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Meteorite ALH 84033 – Microdiffraction Data from Rigaku Rapid II

“Black” area

Page 38: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Meteorite ALH 84033 – Microdiffraction Data from Rigaku Rapid II

“Brown” area

Page 39: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Meteorite ALH 84033 – Microdiffraction Data from Rigaku Rapid II

“White” area

Page 40: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 41: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 42: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 43: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 44: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico
Page 45: James R. Connolly Dept. of Earth & Planetary Sciences University of New Mexico

Using the XRD Lab

• XRD lab is open to any faculty, students or staff wanting to incorporate XRD in their research

• Radiation safety training and exam must be completed by all users

• Training for equipment operation will be available• The lab is a service center so fees are charged for use• Fee schedules for analyses will be similar to that for the

current instrument with additional schedules for use of new experimental equipment

• Anyone wanting to incorporate XRD into research proposals should connect with me about how best to do that


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