Physicochemical Characterization: IR and UV-vis Spectroscopy

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Abteilung Anorganische Chemie Fritz-Haber-Institut der Max-Planck-Gesellschaft Faradayweg 4-6, 14195 Berlin Physicochemical Characterization: IR and UV-vis Spectroscopy Friederike C. Jentoft Mitteldeutscher Katalyseverbund Universität Leipzig October 30, 2006

Outline 1. Introduction When to use (UV-vis and IR) spectroscopy in heterogeneous catalysis research? 2. Measurement of solid materials Transmission and Diffuse Reflection 3. Examples Catalyst and catalyst surfaces Characterization of sites through adsorption of probe molecules Spectroscopy during catalysis

MIR - NIR vis UV Type of transition Molecular rotation Molecular vibrations Electronic excitation Spectral range Radio waves Micro waves Infrared F M N UV X-ray radiation Mid IR (MIR) Near IR (NIR) UV-vis Wavenumber 3300 to 250 12500 to 3300 50000 to 12500 / cm -1 Wavelength / nm 3000 to (25000-40000) electronic transitions, vibrations (rotations) (700-1000) to 3000 200 to 800 Energy /ev 6.2 to 1.5

A Catalyst Life When to Use Spectroscopy? 1. Preparation of a Solid (a Heterogeneous Catalyst) Formation of a solid from solution (e.g. precipitation, sol-gel method) Modification of solid (e.g. preparation of a supported catalyst) 2. Catalyst Characterization Catalyst structure, surface functionalities Surface sites: non-reactive interactions with probe molecules 3. During Catalytic Reaction Gas phase Liquid phase 4. Aged / Spent Catalyst Changes to structure & surface functionalities, deposits on surface Remaining surface sites

A Catalyst Life When to Use Spectroscopy? 1. Preparation of a Solid (a Heterogeneous Catalyst) Formation of a solid from solution (e.g. precipitation, sol-gel method) Modification of solid (e.g. preparation of a supported catalyst) 2. Catalyst Characterization Catalyst structure, surface functionalities Surface sites: non-reactive interactions with probe molecules 3. During Catalytic Reaction Gas phase Liquid phase 4. Aged / Spent Catalyst Changes to structure & surface functionalities, deposits on surface Remaining sites

From An Experimental Point of View Spectroscopy of a solid preparation steps, product, spent material Spectroscopy of solid and surrounding gas phase Probing sites on fresh/spent catalyst (RT or low T, p of probe small) During catalytic reaction: in situ (p usually atm or larger, T > RT) Spectroscopy of solid and surrounding liquid Preparation steps: formation / modification of solid During catalytic reaction: in situ (suspension or thin film phase boundary)

Spectroscopy of a Solid h υ DETECTOR place sample in sample holder/accessory in sample compartment of spectrometer

Spectroscopy of a Solid h υ DETECTOR if no special measures are taken, sample compartment + parts of the spectrometer are in air gas phase N 2, O 2 : no absorption bands in (UV)-vis-NIR-MIR gas phase CO 2, H 2 O: rotational vibrational bands in NIR and MIR

Spectroscopy of a Solid h υ DETECTOR can correct for air absorption through reference measurement provided there is no change in composition with time modern spectroscopy software can make a calculated correction

Spectroscopy of a Solid h υ DETECTOR can correct for air absorption through reference measurement provided there is no change in composition with time modern spectroscopy software can make a calculated correction

Spectroscopy of Solid in Controlled Gas Atmosphere h υ DETECTOR HEATER In beam: solid catalyst, windows, adsorbate, gas phase Usually interested in solid and adsorbate Evacuate / dose or flow gas Molecules that do not absorb (He, N 2 ) in gas phase: no problem

Spectroscopy of Solid in Controlled Gas Atmosphere h υ DETECTOR HEATER Absorbing gases: depends on partial pressure and length of beam path in gas phase Evacuate / dose or flow gas Absorbing gases, static conditions: can often be corrected

Spectroscopy of Solid in Controlled Gas Atmosphere h υ DETECTOR HEATER Evacuate / dose or flow gas Absorbing gases, dynamic conditions (catalysis): often problem

Spectroscopy of Solid and Liquid Surrounding h υ DETECTOR HEATER Liquid flow or flow Absorbing liquids, dynamic conditions: very difficult!

Possible Transitions Heterogeneous Catalysts = Solids Inorganic materials: salts, oxides, carbon, metals Resins (functionalized polymers) Characterization Vibrations Electronic transitions Catalyst bulk Lattice, structural units Band gap energy of semiconductors Catalyst surface Stretching and deformation vibrations of functional groups, vibrations of supported species: metal complexes Charge transfer and d-d transitions of metal complexes, metal particles Adsorbates Functional groups Must have chromophores

Spectral Interpretation - Analoga Catalyst Catalyst surface functional groups (-OH, -COOH, -SO 3 H, - NH 2 ) Supported metal complexes Adsorbed inorganic or organic molecules Reference compounds in Organic and Inorganic Chemistry Functional group fingerprints Metal complexes in solution Gas or liquid phase spectra of free molecules

Example 1.2 Absorbance 1.0 0.8 0.6 0.4 Absorbance 0.2 0.1 0.2 0.0 450 500 550 600 650 700 750 800 Wavelength / nm 0.0 450 500 550 600 650 700 750 800 Wavelength / nm Methylene blue in aqueous solution Methylene blue adsorbed on TiO 2

Example 0.6 2965 2955 VSIR 27 FeSZ 0.418 mbar neopentane gas phase A 10, difference spectra 0.4 0.2 2897 2866 2817 0.0 3100 3000 2900 2800 2700 Wavenumber / cm -1 CH 3 H 3 C CH 3 2,2-Dimethylpropan (Neopentan) CH 3

Spectroscopy with Powder Samples how to measure spectra of a powderous solid? absorption as a function of wavelength, qualitatively and quantitatively

Interaction of Light with Sample scattered light incident light transmitted light reflection at phase boundaries absorption of light (luminescence) how to extract absorption properties from transmitted light? how to deal with reflection and scattering?

How to Deal with Reflection (1) incident light transmitted light reflection at phase boundaries fraction of reflected light can be eliminated through reference measurement with same materials (cuvette+ solvent)

Transmittance τ = I I 0 I 0 Sample if luminescence and scattering are negligible: 1 = α + τ + ρ α τ(t) ρ if we manage to eliminate reflection: 1 = α + τ I absorptance, absorption factor, Absorptionsgrad transmittance, transmission factor, Transmissionsgrad reflectance, reflection factor, Reflexionsgrad in this case, the absorption properties of the sample can be calculated from the transmitted light

Transmitted Light and Sample Absorption Properties τ = I I 0 di I 0 = I k dl I = I κ c dl decrease of I in an infinitesimally thin layer I di I I0 I ln I = 0 l 0 κ c = κ c l dl c: molar concentration of absorbing species [mol/m -3 ] κ: the molar napierian extinction coefficient [m 2 /mol] separation of variables and integration sample thickness: l

Transmitted Light and Sample Absorption Properties τ = A e I I 0 = e κ c l = 1 α = B = κ c l = ln(τ ) Lambert-Beer Law napierian absorbance Napier-Absorbanz A10 = ε c l = log( τ ) extinction E (means absorbed + scattered light) absorbance A (A 10 or A e ) optical density O.D. all these quantities are DIMENSIONLESS!!!! (decadic) absorbance dekadische Absorbanz standard spectroscopy software uses A 10!

Self-Supporting Wafers 50 40 H 4 PVMo 11 O 40 Cs 2 H 2 PVMo 11 O 40 Cs 3 HPVMo 11 O 40 Cs 4 PVMo 11 O 40 Transmission (%) 30 20 10 2118 2036 2119 2040 1934 1625 1379 1257 CaF 2 - Fenster- Absorption 0 1632 1612 4000 3500 3000 2500 2000 1500 1000 Catalysts may absorb strongly! Wellenzahl (cm -1 )

Limitations of Transmission Spectroscopy 0.07 0.06 sulfated ZrO 2 after activiton at 723 K Transmittance 0.05 0.04 0.03 0.02 0.01 0.00 5000 4000 3000 2000 1000 Wavenumber / cm -1 Catalysts are fine powders (high surface area) and may scatter strongly

Scattering scattering is negligible in molecular disperse media (solutions) scattering is considerable for colloids and solids when the wavelength is in the order of magnitude of the particle size Wavenumber Wavelength Mid-IR (MIR) 3300 to 250 cm -1 3 to (25-40) µm Near-IR (NIR) 12500 to 3300 cm -1 (700-1000) to 3000 nm UV-vis 50000 to 12500 cm -1 200 to 800 nm scattering is reduced through embedding of the particles in media with similar refractive index: KBr wafer (clear!) technique, immersion in Nujol

But.Reaction with Material Used for Embedding Transmittance (%) 60 40 20 1083 H 4 PVMo 11 O 40 (NaCl) (KBr) (CsCl) 0 1073 1059 983 960 896 862 788 1100 1000 900 800 700 Wavenumbers (cm -1 ) reaction with diluent possible dilution usually not suitable for experiments at high T/ with reactive gases

Can We Use the Reflected Light? instead of measuring the transmitted light, we could measure the reflected light can we extract the absorption properties of our sample from the reflected light? Detector

Reflection of Radiation mirror-type (polished) surfaces mat (dull, scattering) surfaces mirror-type reflection mirror reflection surface reflection equally intense in all directions (isotropic)

Diffuse Reflection intensity of diffusely reflected light independent of angle of incidence (isotropic) due to multiple reflection, refraction, and diffraction (scattering) inside the sample ca. 20 µm need theory that treats light transfer in an absorbing and scattering medium want to extract absorption properties! scanning electron microscopy image

A Simplified Derivation of the Schuster-Kubelka-Munk (or Remission) Function J R = J I I di = I K dl I S dl + J S dl dj = J K dl J S dl + I S dl with K, S: absorption and scattering coefficient [cm -1 ] Divide equations by I or J, respectively, separate variables, introduce R=J/I R R R 2 2dR 2R(1 + K S ) + 1 = 0 0 S l dl Integrate via partial-fraction expansion

A Simplified Derivation of the SKM Function assume black background, so that R 0 = 0 make sample infinitely thick, i.e. no transmitted light (typical sample thickness in experiment ca. 3 mm) R = K + S + S K( K + 2S) 2 constants are needed to describe the reflectance: absorption coefficient K scattering coefficient S (1 R ) F ( R ) = = 2R 2 K S Kubelka-Munk function remission function for K 0 (no absorption) R 1, i.e. all light reflected for S 0 (no scattering) R 0, i.e. all light transmitted or absorbed

Kubelka-Munk Function mostly we measure R, i.e. not the absolute reflectance R but the reflectance relative to a standard depends on wavelength F(R ) λ corresponds to extinction in transmission spectroscopy in case of a dilute species is proportional to the concentration of the species (similar to the Lambert-Beer law): F( R ) ε c s

Spectroscopy in Transmission Catalyst Light Source Detector reference nothing = void, empty cell, cuvette with solvent in IR transmission is widely applied for solids in UV-vis transmission is rarely used for solids (zeolites!) spectrum: transmission of catalyst vs. transmission of reference

Diffuse Reflectance Spectroscopy Light Source Catalyst Detector reference white standard spectrum: reflectance of sample (catalyst) vs. reflectance of standard need element that collects diffusely reflected light need to avoid specularly reflected light need reference standard (white standard)

White Standards KBr: IR (43500-400 cm -1 ) BaSO 4 : UV-vis MgO: UV-vis Spectralon: UV-vis-NIR Spectralon thermoplastic resin, excellent reflectance in UV-vis region

Methods and Collecting Elements Methods diffuse reflectance UV-vis spectroscopy (DR-UV-vis spectroscopy or DRS) diffuse reflectance Fourier-transform infrared spectroscopy (DRIFTS) Collecting Elements integrating spheres (IR and UV-vis-NIR) fiber optics (UV-vis-NIR) mirror optics (IR and UV-vis-NIR)

Diffuse Reflection & Macroscopic Surface Properties randomly oriented crystals in a powder: light diffusely reflected flattening of the surface or pressing of a pellet can cause orientation of the crystals, which are elementary mirrors causes glossy peaks if angle of observation corresponds to angle of incidence solution: roughen surface with (sand)paper or press between rough paper, or use different observation angle!

Specular Reflection: Angular Distribution incident beam azimuth 180 azimuth <180 reflected beam surface TOP VIEW the intensity of the specularly reflected light is largest at an azimuth of 180

Integrating Sphere Source Gloss trap Detector Screen 8 /d Sample the larger the sphere the smaller errors from the ports the larger the sphere the lower the intensity onto the detector typically 60-150 mm diameter coatings: BaSO 4, Spectralon (for UV-vis)

How to Avoid Specular Reflection SIDE VIEW TOP VIEW 120 90 sample surface sample surface specular reflection is strongest in forward direction collect light in off-axis configuration

Praying Mantis Optical Accessory (Harrick) can be placed into the normal sample chamber (in line with beam), no rearrangement necessary Detector Source first ellipsoidal mirror focuses beam on sample second ellipsoidal mirror collects reflected light 20% of the diffusely reflected light is collected http://www.harricksci.com/

Fiber Optics for UV-vis light conducted through total reflectance fiber bundle with 6 around 1 configuration: illumination through 6 (45 ), signal through 1 avoids collection of specularly reflected light Bilder: Hellma (http://www.hellma-worldwide.de) and CICP (http://www.cicp.com/home.html)

Catalyst Bulk & Catalyst Surface Support with functional groups Support + dispersed species OH OH SO 2- OH 4 M x+ SO 2- M M x+ 4 M M M M M x O y (e.g. M=Ti, Zr, Al, Si, Fe) OH M OH M x O y (e.g. M=Ti, Zr, Al, Si) OH

Comparison Transmission - Diffuse Reflectance (IR) 0.07 0.06 sulfated ZrO 2 after activation at 723 K Transmission: self-supporting 1.2 wafer Reflectance: powder bed 1.0 Transmittance 0.05 0.8 0.04 0.6 0.03 0.4 0.02 Reflectance 0.01 0.00 5000 4000 3000 2000 1000 Wavenumber / cm -1 0.2 0.0 spectra can have completely different appearance transmission decreases, reflectance increases with increasing wavenumber

Comparison Transmission - Diffuse Reflectance Absorbance A Napier 5.0 4.8 4.6 4.4 4.2 4.0 3.8 3.6 3.4 3.2 sulfated ZrO 2 after activation at 723 K 3.0 5000 4000 3000 2000 Wavenumber / cm -1 OH vibrations SO vibrations Transmission: self-supporting wafer 1.0 Reflectance: powder bed 0.8 0.6 0.4 0.2 0.0 Kubelka-Munk Function vibrations of surface species may be more evident in DR spectra

Dispersed V x O y Species (DR-UV-vis) 0.5 wt% VO x /Al 2 O 3 9.5 wt% VO x / Al 2 O 3 + CT bands at 359 and 376 nm: isolated octahedrally co-ordinated V 5+ species CT bands at 468 and 535 nm: octahedraly co-ordinated V 5+ species in V 2 O 5 clusters (XRD shows crystalline form of V 2 O 5 ) Kondratenko and Baerns, Appl. Catal. 2001