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    MOLECULARSPECTROSCOPYOF OXIDE CATALYSTSURFACES

    Anatoli DavydovUniversity of Alberta, Edmonton, Canada

    Syntroleum Corporation, Tulsa, Oklahoma, USA

    Edited by N. T. Sheppard

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    Copyright 2003 John Wiley & Sons Ltd, The Atrium, Southern Gate, Chichester,

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    Library of Congress Cataloging-in-Publication Data

    Davydov A. A. (Anatoli Aleksandrovich)Molecular spectroscopy of oxide catalyst surfaces / Anatoli Davydov ; edited by N.T. Sheppard.

    p. cm.Includes bibliographical references and index.ISBN 0-471-98731-X (cloth : alk.paper)

    1. Metallic oxides Surfaces Analysis. 2. Molecular spectroscopy. I. Sheppard, N. T. II.Title.

    QD509.M46 .D38 2003

    541.33 dc212002191080

    British Library Cataloguing in Publication Data

    A catalogue record for this book is available from the British Library

    ISBN 0-471-98731-X

    Typeset in 9.5/11.5pt Times by Laserwords Private Limited, Chennai, IndiaPrinted and bound in Great Britain by TJ International, Padstow, Cornwall

    This book is printed on acid-free paper responsibly manufactured from sustainable forestryin which at least two trees are planted for each one used for paper production.

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    Dedicated to my wife Marina

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    CONTENTS

    Preface xi

    Symbols and Abbreviations xiii

    Introduction xv

    1 Theoretical fundamentals and experimental considerations of thespectroscopic methods used in surface chemistry 1

    1.1 Electronic spectroscopy 1

    1.1.1 Transmission spectra 4

    1.1.2 Diffuse reflection spectra 5

    1.2 Vibrational spectroscopy 5

    1.2.1 Infrared spectroscopy 11

    1.2.2 Photoacoustic spectroscopy 18

    1.2.3 Raman spectroscopy 19

    1.3 Electron energy loss spectroscopy 21

    1.4 Inelastic electron tunneling spectroscopy 221.5 Inelastic neutron scattering spectroscopy 23

    1.6 Other vibrational spectroscopies 23

    1.6.1 Infrared ellipsometric spectroscopy 23

    1.6.2 Surface electromagnetic wave spectroscopy 23

    1.7 In situ measurements 24

    1.8 Quantitative measurements 25

    2 The nature of oxide surface centers 27

    2.1 Systems investigated 27

    2.1.1 Solid structures 27

    2.1.2 Surfaces 28

    2.1.3 Active sites 29

    2.2 Spectra of oxide surfaces 31

    2.2.1 Vibrations of metal oxygen bonds on oxide surfaces 32

    2.2.2 Molecular forms of adsorbed oxygen 44

    2.2.3 Surface hydroxyl groups 56

    2.3 Determination of the nature of surface sites and their chemical properties

    using the adsorption of simple molecules 77

    2.3.1 Adsorption of ammonia and pyridine 78

    2.3.2 Adsorption of carbon monoxide 95

    2.3.3 Adsorption of hydrogen and nitrogen 114

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    viii CONTENTS

    2.3.4 Adsorption of water 120

    2.3.5 Adsorption of nitrogen oxide and nitrogen dioxide 123

    2.3.6 Adsorption of carbon dioxide 133

    2.3.7 Adsorption of hydrogen sulfide 139

    2.3.8 Adsorption of sulfur dioxide 146

    2.3.9 Surface isocyanate complexes 157

    2.4 Determination of acidic surface properties 161

    2.4.1 Protic acid sites 162

    2.4.2 Lewis acid sites 166

    2.5 Determination of basic surface properties 171

    2.6 Surface defects 177

    3 Study of cation states by DRES and FTIR spectroscopies of the probe

    molecules 181

    3.1 Copper-containing systems 1823.1.1 Zeolites 182

    3.1.2 Oxides 200

    3.2 Nickel-containing systems 207

    3.2.1 Zeolites 207

    3.2.2 Oxides 215

    3.3 Co-containing systems 217

    3.3.1 Zeolites 217

    3.3.2 Oxides 218

    3.4 Iron-containing systems 220

    3.4.1 Zeolites 2203.4.2 Oxides 222

    3.5 Silver-containing systems 223

    3.6 Palladium-containing systems 228

    3.6.1 Zeolites 228

    3.6.2 Oxides 235

    3.7 Rhenium-, ruthenium-, and rhodium-containing systems 237

    3.8 Platinum-containing systems 238

    3.8.1 IR-Spectra of CO adsorbed on supported metals 238

    3.8.2 Cationic states of platinum 248

    3.9 Molybdenum-containing systems 252

    3.9.1 Molybdenum aluminum oxide compounds 252

    3.9.2 Molybdenum silicon oxide compounds 253

    3.9.3 Molybdenum titanium oxide compounds 255

    3.10 Vanadium-containing systems 257

    3.10.1 Vanadium titanium oxide compounds 259

    3.10.2 Vanadium silicon oxide compounds 263

    3.10.3 Vanadium aluminum oxide compounds 266

    3.11 Chromium-containing systems 269

    3.12 Effects of the states of adsorption sites on the stretching frequencies of

    adsorbed carbon monoxide and nitrous oxide and the problem of detecting

    the states of cations in oxide catalyst surfaces 2713.12.1 M2+CO, Mn+CO (n >2) 272

    3.12.2 M+CO and M0 CO 274

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    CONTENTS ix

    4 Interactions of inorganic compounds with oxide surface

    active sites 277

    4.1 Organometallic complexes 281

    4.2 Metal carbonyls and nitrosyls 282

    4.3 Interactions with simple acids and bases 284

    4.3.1 F- and Cl-modified oxide systems 285

    4.3.2 SO42-modified oxide systems 286

    4.3.3 BO32-modified oxide systems 291

    4.4 Heteropoly compound systems 294

    4.4.1 Effects of the supports 295

    4.4.2 Acidic properties of molybdenum heteropoly compounds 300

    4.5 Thermal stabilities of molybdenum compounds, decomposition mechanisms

    and the role of modifiers 303

    4.5.1 Bulk and supported heteropoly acids 303

    4.5.2 Modified molybdates 305

    4.6 Cationic modification 308

    5 Formation of surface complexes of organic molecules 309

    5.1 Complexation of alkenes 310

    5.1.1 Complexation with OH groups 310

    5.1.2 Carbenium ions and alkoxy compounds 313

    5.1.3 Interaction with cations 327

    5.1.4 Interaction with cation anion pairs 342

    5.1.5 The complexation of alkenes with surface oxygen 351

    5.2 Complexation of aryls and aryl halides 355

    5.2.1 Hydrogen-bonding 3555.2.2 Alkylaromatic carbenium ions 358

    5.2.3 -complexes 366

    5.2.4 Interaction with ionic pairs 373

    5.2.5 Complexation with surface oxygen 376

    5.2.6 Formation of aryl halide complexes 378

    5.3 Complexation of alkynes 381

    5.3.1 Silicon dioxide zeolites 381

    5.3.2 Aluminum oxide 385

    5.3.3 Zinc oxide 386

    5.3.4 Titanium oxide 387

    5.4 Complexation of alkanes 389

    5.4.1 Interactions with OH groups, carbenium-like ions 389

    5.4.2 Interaction with cations 392

    5.4.3 The activation of C H bonds in alkane molecules 395

    5.5 Complexation of chlorofluorocarbons 407

    5.6 Complexation of nitriles 411

    5.6.1 Acetonitrile 411

    5.6.2 Benzonitrile 415

    5.7 Complexation of alcohols 416

    5.7.1 Saturated alcohols 416

    5.7.2 Phenol 4275.8 Complexation of aldehydes and ketones 430

    5.8.1 Formaldehyde and acetaldehyde 430

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    x CONTENTS

    5.8.2 Acrolein 435

    5.8.3 Benzaldehyde 439

    5.8.4 Maleic anhydride 440

    5.8.5 Acetone 442

    5.9 Complexation of acids 445

    5.9.1 Formic acid 445

    5.9.2 Acetic acid 453

    5.9.3 Acrylic acid 453

    5.9.4 Benzoic acid 455

    5.10 Deactivation catalysts due to carbonaceous depositions as a result of

    catalyst interactions with hydrocarbons and their derivatives 456

    6 The mechanisms of heterogeneous catalytic reactions 459

    6.1 Reactions involving carbon monoxide 461

    6.1.1 The oxidation of carbon monoxide 461

    6.1.2 The water-gas shift reaction 4666.1.3 Carbonization and hydroformylation 473

    6.1.4 The synthesis and decomposition of alcohols 475

    6.2 Reactions with the participation of hydrocarbons 479

    6.2.1 Complete oxidation of hydrocarbons and their derivatives 479

    6.2.2 Selective transformations of alkenes 483

    6.2.3 Partial oxidation 499

    6.2.4 Ammoxidation of hydrocarbons and their derivatives 518

    6.3 Transformations of aldehydes and ketones 526

    6.3.1 Oxidation of acrolein 526

    6.3.2 Oxidation of formaldehyde 5316.3.3 Transformation of acetone 531

    6.3.4 Hydrogenation of aldehydes and ketones 532

    6.4 Transformations of alcohols 532

    6.4.1 Dehydration of alcohols 532

    6.4.2 Dehydrogenation of alcohols 536

    6.4.3 Methanol oxidation to formaldehyde 538

    6.5 Transformations of nitrogen-containing compounds 545

    6.5.1 Decomposition of nitric oxide 545

    6.5.2 The reduction of nitrogen oxides 552

    6.5.3 Reactions of NOx and NH3 Mixtures 556

    References 559

    Index 643

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    PREFACE

    Molecular spectroscopic methods, together with X-ray diffraction, have played key roles in estab-

    lishing the concepts of coordination chemistry, as originally developed in the study of individual

    transition-metal complexes in aqueous solutions or the solid state. This present book is concerned

    with the even greater importance of molecular spectroscopic methods in developing similar under-

    standings of the coordination chemistry of oxide surfaces where application of diffraction methods

    is much more difficult. The adsorption of molecules on the surfaces gives rise to ligands attached

    to free sites on the surface cations.The book commences with an account of the basic theoretical principles and experimental

    techniques of the various molecular spectroscopic methods as applied to surfaces, namely the

    electronic (UV Vis), vibrational (transmission IR, diffuse reflection, reflection absorption IR

    and Raman), electron energy loss, inelastic electron tunneling, and inelastic neutron scattering

    spectroscopies. Special attention is devoted to in situ measurements where the oxide or catalyst

    sample is in contact with the adsorbate or reactant. The local approach has been chosen as the

    basis of the spectroscopic analysis of adsorption on the active sites of the oxide surfaces, while

    the collective properties of the solid adsorbents, based on analysis of their crystal structures, is

    used to describe the sites themselves. This approach is applied to pure oxides and also to oxide

    systems such as cation-substituted zeolites, heteropoly compounds of molybdenum, or supported

    catalysts prepared by ionic exchange or the interaction of the support with various complexes.

    In some cases, the crystallographic positions of both cations and anions can be unambiguously

    determined by means of molecular spectroscopic (ESR, UVVis, Mossbauer, etc.) or diffraction

    (for zeolites, etc.) methods.

    An attempt has been made to cover all of the spectroscopic literature on oxide adsorption

    studies, covering many different oxide adsorbate systems in a comparative manner. Because

    the number of such publications is now very large (numbered in thousands), it is impossible to

    analyze all of them individually in one single book. A particular goal is to provide a critical

    analysis of the literature on the interpretation of the spectra of surface compounds on oxides

    going back to the earliest days of the 1950s. A comparative analysis of the changes in the IR

    spectra of adsorbed molecules, based on an improved knowledge of the bonding between the

    adsorbed molecule and the surface site, has allowed this present author to improve the reliability

    of interpretation of many of the spectra. Special emphasis is placed on the spectral characteristics

    of active sites on oxide surfaceshydroxyl groups, or coordinatively unsaturated surface cations

    and oxygen anions. The concept of the decisive role played by surface sites in surfacemolecule

    adsorption is used to systematize and classify the spectral data relating to the interaction of

    numerous organic and inorganic molecules, and their transformation products, with the types of

    surfaces referred to above. The structures of many surface species have been identified from the

    spectroscopic data.

    A detailed account is presented of methods for spectroscopically characterizing the oxida-

    tion state and degree of coordination of surface cations and oxygen anions by the adsorption ofprobe molecules such as NH3, pyridine (Py), CO, CO2, H2, N2, H2O, NO, NO2, H2S and SO2(Chapter 2). Special attention is paid to the critical investigation of protic and aprotic acidic and

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    xii PREFACE

    basic surface centers, including specific correlations for comparing the strengths and concentra-

    tions of surface centers on different oxides, zeolites, supported oxides, etc. by using the UVVis,

    ESR and IR spectral characteristics of the adsorbed probe molecules, particularly CO and NO.

    This includes the testing of cation states during the process of stationary-state heterogeneous

    catalytic reactions. Systems containing Cu, Ni, Co, Fe, Ag, Pd, Re, Ru, Rh, Pt, Mo, V and Cr

    are examined in detail. The vibrational frequency ranges of the CO and NO probes characteristicof different surface states are presented.

    Attention is also paid to the interactions of organometallic (allylic and other types) and inorganic

    compounds (such as metal carbonyls), simple acids and heteropoly compounds with various

    supports (Al2O3, SiO2, TiO2 and MgO), i.e. to the problems that occur during the preparation or

    modification of supported catalysts. The dependence of the structure and properties of the surface

    complexes formed and the properties of the catalytic systems are also shown.

    The complexation of many organic molecules alkenes, alkene halides, alkynes, aryls, aryl

    halides, alkanes, nitriles, alcohols, aldehydes, ketones and acids (saturated and unsaturated, aro-

    matic and non-aromatic) with different oxide systems are critically examined. The surface

    compounds formed are classified in relation to the nature and properties of the available surfacecenters (H+, OH, O2, Mn+, Mn+O2, etc.).

    The final chapter is devoted to discussions of possible mechanisms of catalytic reactions as

    deduced from spectroscopic identification of the reaction intermediates. The latter identifica-

    tions are based on the comparison of the rates of reaction with those of the transformations

    of surface compounds. The catalytic reactions discussed include carbon oxide oxidation, the

    water gas shift (WGS) reaction, the synthesis and decomposition of alcohols, carbonization,

    hydroformylation, full and partial transformations of alkenes (including isomerization, hydro-

    genation, oligomerization, polymerization, cracking and metathesis), partial oxidation of alkanes,

    alkenes and aryls, ammoxidation of hydrocarbons, alcohols and aldehydes, conversion of alco-

    hols, transformations of aldehydes and ketones, NO decomposition, NO+ CO, NO/hydrocarbons,

    and reactions between NO and NH3.

    Taking into account common understandings and the results of the analysis of detailed schemes,

    the mechanisms of heterogeneous catalytic reactions can be classified as stepwise (when sequen-

    tial interactions of the reaction components occur) or associative (where the stages of product

    separation and interaction of the reaction mixture components with the catalyst occur in parallel)

    with the help of spectroscopic analyses.

    This book is intended for specialists working in the fields of surface physical chemistry, surface

    science, adsorption phenomena and heterogeneous catalysts.

    Special thanks are due to Professor N.T. Sheppard for his attention, interest, valuable correc-

    tions and useful advice, to Professor J.T. Yates Jr for important comments, and also to my wife,

    Dr M. Shepotko, and son, Davydov, A.A. Jr, for their help in the preparation and design ofthis book.

    Anatoli Davydov

    Tulsa, OK, USA

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    SYMBOLS AND ABBREVIATIONS

    AES Auger electron spectroscopy

    AFS atomic fluorescence spectroscopy

    AO atomic orbital

    BAS Brnsted acid site

    BS basic site

    CTB charge-transfer band

    DRES diffuse reflection electron (UV Vis) spectroscopyDRIRS diffuse reflection infrared spectroscopy

    EELS electron energy loss spectroscopy

    EHM extended Huckel Method (quantum-chemical calculations)

    EPR electron proton resonance (spectroscopy)

    ES electron spectroscopy

    ESR electron spin resonance (spectroscopy)

    FTIR Fourier-transform infrared (spectroscopy)

    GC gas chromatography

    HFB high-frequency band

    HM Huckel Method (quantum-chemical calculations)

    HOMO highest-occupied molecular orbital

    HPA heteropoly acid

    HPC heteropoly compound

    HREELS high-resolution electron energy loss spectroscopy

    IETS inelastic electron tunneling spectroscopy

    INSS inelastic neutron scattering spectroscopy

    IP ionization potential

    IRAS infrared absorption spectroscopy

    IRES infrared ellipsometric spectroscopy

    IRS infrared spectroscopy

    LAS Lewis acid siteLFB low-frequency band

    LOMO lowest-occupied molecular orbital

    M metal

    Mn+cuo coordinatively unsaturated octahedral site (on a metal)

    Mn+cus coordinatively unsaturated site (on a metal)

    Mn+cut coordinatively unsaturated tetrahedral site (on a metal)

    MO molecular orbital

    MS mass spectrometry

    MY-A faujasite-type zeolite containing preferably strong

    associated cationsMY-I faujasite-type zeolite containing preferably isolated cations

    NMR nuclear magnetic resonance (spectroscopy)

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    xiv SYMBOLS AND ABBREVIATIONS

    NRS nuclear-resonance spectroscopy (Mossbauer spectroscopy)

    PAS photoacoustic spectroscopy

    R hydrocarbon fragment

    RAIRS reflection absorption infrared spectroscopy

    RS Raman spectroscopy

    SAPO silicoaluminophosphateSCR selective catalytic reduction

    SERS surface-enhanced Raman spectroscopy

    SEWS surface electromagnetic wave spectroscopy

    SIC surface isocyanate complex

    SIMS selected-ion mass spectrometry

    SMSI strong metalsupport interaction

    TPD temperature-programmed desorption

    UEP unshared electron pair

    UHV ultra-high vacuum

    UV Vis spectroscopy in the ultraviolet and visible regionVAPO vanadiumsilicophosphate

    WGS water gas shift

    XPS X-ray photoelectron spectroscopy

    XRD X-ray diffraction

    A absorbance

    A0 absorption coefficiente electron charge

    E activation energy

    g parameter of level split in ESR spectrumK reaction rate constant

    N number of active sites

    PA proton affinity

    q charge (on a dipole)

    Q heat of absorption

    r interatomic distance (A)

    deformation vibration

    extinction coefficient(cm2 molecule1)

    surface coverage

    vibration wavenumber (reciprocal wavelength, 1/) (cm1)

    out-of-plane deformation vibration

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    INTRODUCTION

    Numerous technological processes are dependent on the nature of the molecular and chemical

    interactions which occur on contact of various media with solid surfaces. These include, for

    example, the separation of mixtures by adsorption, heterogeneous catalysis, the chromatographic

    separation of pure substances, the production of polymer and lubricant fillers, materials for micro-

    electronics and the manufacture of controlled-property semiconductors, pigments and catalysts.

    It is therefore an important objective to gain a better understanding of the nature of the processes

    which occur at the surfaces of solids.This book is concerned with the development of the principles of the coordination chemistry

    of oxide surfaces as brought about by the use of analyses of experimental data obtained by

    means of molecular spectroscopy methods which are the most widely used in chemistry [135a].

    The concepts of coordination chemistry, originally established for transition-metal complexes

    in aqueous solutions [35b e], can frequently be usefully extended to heterogeneous systems

    consisting of transition-metal ions dispersed on the surfaces (or incorporated within a solid matrix)

    of oxides despite the differences in behavior of transition-metal ions at gassolid or liquidsolid

    interfaces [30, 35f h]. The phenomena occurring at the latter interfaces can be described in

    terms of the coordination chemistry concept of coordination number of the transition-metal ion

    (the number of atoms donated by ligands) which can vary over a wide range. At the solid surface,

    a transition-metal ion has necessarily a lower coordination number than in the bulk of the solid

    and so it can complete its coordination sphere by bond formation through adsorption from the

    gas or liquid phase. The first coordination sphere predominantly determines the reactivity and

    properties of the central transition-metal ion in both homogeneous and heterogeneous systems,

    although the influence of the addition of ligands to the coordination spheres is much greater in

    heterogeneous systems. This can lead in the latter case to the existence of a number of transition-

    metal ion complexes and, moreover, this is the cause of the creation and stabilization of species

    with unusual oxidation states or coordination numbers at solid surfaces which are different from

    those in the bulk of the oxide. Compared with homogeneous coordination chemistry, such species

    show new types of reactivity. Thus, these peculiar features of heterogeneous coordination systems

    containing transition-metal ions open up new, special and unique potentialities in adsorption and

    catalysis [30, 35fh].

    The principles of coordination chemistry, established essentially by Grinberg, Jorgensen and

    Werner, were based on results obtained for solution complexes with the single transition-metal

    ion surrounded by ligands [35be]. The properties of these complexes were the main subjects

    of study, for example, reactivity, structure, the nature of the different chemical bonds involved,

    the presence of optical and/or geometric isomers, the number of isomers, optical and magnetic

    properties, chemical reactivities, etc. Different theoretical treatments, such as crystal field, molec-

    ular orbital, valence bond, etc., improved the understanding of the transition-metal complexes in

    solution or in the solid state.

    Attempts to apply these theories to catalytic processes have been more successful for homoge-neous than for heterogeneous systems. The main results are that (i) the properties of the partially

    filled d-orbitals of oxide surfaces can be studied at a molecular level by using probes with

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    xvi INTRODUCTION

    characteristic optical properties, (ii) oxide surfaces may act as either s-donor or p-donor ligands

    and hence be classified within the spectrochemical series of ligands, (iii) an oxide support can

    play a role in reactivity similar to that of a solvent, and (iv) the distinctions and similarities

    between interfacial coordination chemistry and surface organometallic chemistry can be made in

    a similar fashion as for complexes in solution [30, 35fh].

    Molecular interactions at solid surfaces are very complicated because of a number of factors.The most important of these are the nature and properties of the adsorption centers, which deter-

    mine the types of surface complexes formed. Hence, the main tasks in surface chemistry are the

    identification of these surface centers, the determination of their concentrations and characteristic

    chemical properties (for instance, via investigations of the interaction between a given center and

    adsorbed molecules with different chemical properties) and the establishment of the relationships

    between bulk crystal structures and the nature of the surface centers.

    Morrisons term surface center [35i] will be applied in this book to describe the microscopic

    group of atoms which exhibits a particular chemical activity on the surface. This term applies

    to a surface atom of the lattice with a free bond, the free bonding orbital with a low ionization

    potential, etc.; such centers can be situated on a uniform surface or can occur in nonhomogeneousareas, where their activity is often highest. It has been shown that surface heterogeneity has a

    great effect on the chemical properties of surfaces as it leads to a wide range of different types

    of adsorption centers. These centers may be related to defects, e.g. sites where a crystal defect

    meets the surface. It should be noted that the surface itself, in both the microscopic and the

    electronic senses, is a major defect of a three-dimensional crystal structure. Hence, any real

    surface is in principle nonhomogeneous. Additional nonhomogeneity is caused by a variety of

    possible microscopic defects (steps, cracks, dislocations, corners, etc.) or point defects (vacancies,

    interstitial atoms, substitution or insertion atom sites). Defect concentrations on real surfaces

    increase with diminishing crystal size. In highly dispersed systems, they may reach, or at times

    exceed, the concentrations of normal surface sites.In addition, any real surface may have chemical nonhomogeneities formed during its prepa-

    ration or from adsorption in the form of surface chemical compounds which modify the surface

    properties. It is therefore evident that all properties of a surface must be taken into account when

    considering its further interactions. Cause and effect can be difficult to distinguish here. Although

    the surface itself determines the nature of the adsorption of molecules from its surroundings, those

    adsorbed molecules often modify the surface properties.

    Classifications of surface centers, plus a knowledge of the chemistry of surface complexes (the

    chemical properties governing the interaction of molecules with each type of center), make it

    possible to characterize the various possible types of surface compounds formed after adsorption.

    The facility for surface-compound formation is more diverse than, and qualitatively different

    from, that of individual molecular complexes since the surface may incorporate cationic states of

    various coordinations and valencies, sometimes unusual ones. Location on a surface can change

    the oxidative reductive properties of a ligand site; adsorption is dependent on the collective

    properties of the solid and multi-centered adsorption can occur [30].

    The study of the nature and properties of a surface entails great experimental difficulties. As

    the traditional methods of defect analysis (electro-physical methods and radioactive labeling)

    practically cannot be applied to polydispersed materials, it is clear that the development of

    concepts of the mechanisms of molecular processes on solids (which require information about the

    nature of bonds formed, surface structure, molecular mobility, etc.) is impossible without spectral

    analysis, which yields direct data on interactions at the molecular level. A particularly versatile

    role is played by vibrational spectroscopy. ESR (EPR) and NMR spectroscopies are limited toselected elements; the former requires paramagnetic ions or radical forms of adsorption, while

    the latter requires nuclei with a magnetic moment. In addition, changes resulting from adsorption

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    INTRODUCTION xvii

    can be detected by UV or visible spectroscopy only for the limited proportion of species that

    give well-defined electronic absorption spectra. The vibrational spectroscopic methods (especially

    Fourier-transform infrared (FTIR), Raman and high-resolution electron energy loss spectroscopy

    (HREELS)) are by far the most versatile techniques for the analysis of surface layers on solids.

    Vibrational spectroscopy provides data on the composition and structure of surface compounds,

    the nature of the bonds formed between adsorbed molecules and the surface, and the existenceof different types of surface compounds and active surface centers. As the vibrational spectrum

    reflects both the properties of the molecule as a whole and the characteristic features of separate

    chemical bonds, this method offers the fullest possible information on the perturbation experienced

    by a molecule on contact with the solid surface, and often determines the structure and properties

    of adsorption complexes and of surface compounds.

    Terenin [17, 35j] first pioneered the successful study of adsorption using molecular spec-

    troscopy in the near-infrared region. Today, the literature contains much generalized experimental

    material on the character of interactions of various molecules with surfaces of silica gels, alumina

    gels, aluminosilica gels and zeolites as determined by infrared spectroscopy in the fundamental

    region. The principles of the study of surface compounds and adsorbed molecules by molecularspectroscopy have been described in several books [1835a]. New experimental developments

    have been reviewed pertaining to studies (for example, by IR spectroscopy) of solids at high

    pressures and/or temperatures in various chemical media, to the determination of kinetic param-

    eters for individual stages of surface reactions, and to the use of computers to process spectral

    data in order to improve the volume of information.

    This book does not repeat a consideration of these problems but instead concentrates on the

    analysis of surface properties, the interaction of relevant simple molecules with the surface of the

    solid, and the reactions which occur on the surface of oxides of the transition-metals. This latter

    choice has been made for two reasons: first, transition-metal oxide systems were not extensively

    studied by molecular spectroscopy in the earlier days and the more recent results have not beensubjected to detailed analysis and comparison, and secondly, such oxides and their surfaces are

    important because of their wide use as heterogeneous catalysts. The main objective of this work

    is to systemize scientific approaches to spectral studies in this area of surface chemistry. The

    entire volume of data obtained for each individual system cannot be examined in detail. Bearing

    in mind that catalysis is of central importance in a conceptual chemistry of the surface, and

    that it provides a means for achieving chemical transformations in the laboratory and in nature,

    this author considers it important to discuss the currently considered concepts by using catalytic

    systems and processes as examples.

    As the main objects of early molecular spectroscopy studies were systems involving silica

    gels, alumino gels and aluminosilica gels, and as it proved fairly easy to obtain their spectra in

    the OH-stretching region, the greatest attention was at first focused on establishing the existence

    and significance of surface hydroxyl groups in adsorptive interactions. At that time, there were

    practically no methods accurate enough for the qualitative, let alone quantitative, differentiation of

    coordinatively unsaturated cations and anions on the surface of oxides. The difficulties involved in

    the analysis of the nature and surface properties of the latter oxides also proved a major obstacle

    to determining the character of the interactions between such centers and adsorbed molecules. In

    fact, until recently no data have become available on some aspects of the interaction between,

    say, alkenes and Lewis centers, even in such well-studied systems as alumina and crystalline or

    amorphous aluminosilicates, which are widely used as catalysts in hydrocarbon transformations.

    The specificity of the material discussed here required novel approaches to the properties of

    the surface. It is known that in the important stage of initial complex formation, mechanisms ofcatalytic reactions involve interactions with transition-metal ions and/or oxygen on the surface

    of the catalyst. Evidently, both the nature and valency/coordination state of the cations, together

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    xviii INTRODUCTION

    with the properties of the surface oxygen ions, exert a considerable influence on the character of

    activation and, possibly, on the directions of transformation of the adsorbed molecules. Hence,

    there is a need to find methods for the identification of such centers on the surface and to establish

    their concentrations and their differences in chemical properties.

    The use of probe molecules, based on the analysis of their spectral changes as a result of

    donor or acceptor molecules interacting with their opposites on the surface, have been widelyused for investigating these centers. This book contains a preliminary description of the authors

    approach to the analysis of surface properties, which includes the isolation of specific interactions

    of elementary simple molecules so-called probe molecules with every possible type of center

    on the solid.

    This authors views on the main goals of molecular spectroscopy in surface chemistry can be

    described as the analysis of the important relationships between the nature of the surface centers

    on oxides, and the forms and directions of transformation of molecules adsorbed on them; these

    considerations account for the manner in which the material is presented. Information about the

    surface states of solids (particularly oxides), about their active sites, and also about the structures

    of surface compounds formed upon adsorption of the various types of molecules, is very important.Such information can be obtained by means of different physico-chemical methods, among which

    those of molecular spectroscopy [116] are the most widely used in chemical applications. In

    the past few decades, these have been very effectively used to investigate the surface chemistry

    of oxide systems [1735].

    Taking into account the large amount of literature covering these fields, the methods of IR and

    UVVis spectroscopies have been the principal means of investigating the surface chemistry of

    such solids. A short introduction to the development and analysis of the data obtained by means

    of these techniques, and the theory of such methods, is given in Chapter 1 of this book. For

    the EPR method, the strong reasons for its use as a tool for the investigation of transition-metal

    chemistry on oxide surface have been described in reference [35h], while the theoretical basis ofsuch applications has been reviewed in various references [25, 31, 33]. Therefore, in this present

    book I will only use the results of this informative method.

    The various molecular spectroscopic methods play even more of a key role in the development

    of the concepts of the surface coordination chemistry originally established for transition-metal

    complexes in aqueous solutions. The local approach has been chosen as the basis of the inter-

    pretation of the absorption bands which characterize the active sites on oxide surfaces and the

    interaction of these sites with adsorbing molecules. The collective properties of the solid adsor-

    bents are also used, based on the analysis of the crystal structures of the oxides or of systems

    such as cation-substituted zeolites, heteropoly compounds of molybdenum, precisely prepared

    (for example, by ionic exchange or interactions of supports with complexes) supported systems

    in which the crystallographic positions of both cations and anions can be well and unambiguously

    determined by means of ESR, UVVis or Mossbauer spectroscopic methods. In the middle of

    the 1980s, a first attempt was made to develop the principles of surface coordination chemistry of

    transition-metal oxides based on the analysis of principally my own spectroscopic investigations

    of oxides surfaces and the compounds formed upon them through adsorption (of a limited number

    of molecules) [30]. In this present book, practically all of the international literature has been

    analyzed for the developing concepts and experimental data over a very wide range of molecular

    reactants and oxide systems. A correct comparative approach limits the number of published

    works that have to be considered individually, such as those which take into account results for

    only one molecule or another. The total number of such publications is so large (in thousands)

    that it is impossible to analyze all of them in detail in one single book.A dramatic increase in the number of recent studies concerning applications of molecular spec-

    troscopic methods to studies of the surface states, and to the structures of adsorbed species, has

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    INTRODUCTION xix

    led to the writing of this present book. More sensitive methods, such as FTIR, laser Raman spec-

    troscopy and Surface-enhanced Raman Scattering (SERS), the sensitivities of which are order of

    magnitude greater then those of earlier vibrational spectroscopic methods, and especially the cre-

    ation of new methods for obtaining vibrational spectra (diffuse reflection, high-resolution electron

    energy loss spectroscopy, electron tunneling spectroscopy and the spectroscopy of electromagnetic

    waves), as well as the wide use of computers to process the spectral information (for instance,to subtract spectra and to separate complex spectral contours into those of separate components),

    have stimulated progress in the study of the physico-chemical properties of heterogeneous sys-

    tems and processes proceeding at the gassolid, gasliquid and solidliquid interfaces, at

    the molecular level [1766]. Due to these advances, it is now possible to obtain practically any

    spectra which reflect the interaction of a surface with molecules in the gaseous or liquid states.

    It is reasonable to affirm that these developments in spectral methods have caused a renaissance

    in interest in the surface chemistry and catalytic applications [67108] of oxides and metals.

    The appearance of more sensitive methods and new techniques has become a reason for a

    reassessment of a significant part of the spectral information obtained ten and more years ago,

    based on the use of more modern techniques. New spectral effects and characteristics, which couldnot be observed in earlier studies because of very low concentrations of the corresponding surface

    species, or because of low values of extinction coefficients, can now be detected. Unfortunately,

    authors of such new studies do not always cite the related previous work, although they use

    the main ideas and conclusions as a basis for interpretation. This is why, in this book, the

    data obtained in the 1970s and 1980s or earlier are reexamined, along with those from studies

    published during the past decade.

    A significant contribution to the development of spectroscopic investigations of surface com-

    pounds has been made by the evolution of cryoscopic methods [109, 110], which allow the

    registration of the spectra of individual molecules, their fragments, ions and radicals, both in

    free states and in interaction with clusters of metal particles of different sizes (from monatomicupwards) or with cations (anions) frozen in a matrix. Since these interactions have similari-

    ties with such structures formed on solid surfaces, the use of this cryoscopic data helps in the

    interpretation of the spectra of reactive surface compounds.

    The development of the catalytic systems based on the organometallic compounds supported

    on different supports (so-called precise catalysts) [111115] became another way in catalytic

    chemistry that contributed a lot to the identification of the surface compounds.

    It should be particularly pointed out that, in spite of the now relative ease of obtaining spectral

    information (including spectra registration), the interpretation of the spectra obtained and asso-

    ciated phenomena (which are investigated by means of spectral methods) is extremely difficult.

    In order to solve these problems, it is necessary to have knowledge in at least three areas: spec-

    troscopy itself, the surface chemistry and heterogeneous catalysis. It cannot be assumed that the

    presence of an absorption band, close in position to that expected in the spectrum of a possi-

    ble fragment, provides a sufficient reason to draw such a conclusion about the structure of the

    complex (and all the more about its subsequent participation in different interactions). Such a

    simplified approach to the use of spectral information to explain, for example, catalytic phenom-

    ena, has often led to wrong conclusions which in turn have caused further mistaken studies. As

    will be shown below, doubtful surface compounds are often postulated as intermediates in cer-

    tain reaction mechanistic schemes. This is why this author, who has devoted more than 30 years

    to the application of spectroscopic methods in surface chemistry, and particularly heterogeneous

    catalysis, has undertaken the difficult task of summarizing and analyzing the voluminous related

    literature and data on the investigation of surface centers and the interactions of these centerswith a large number of molecules of both inorganic and organic types. Principal attention is paid

    to the spectral identification of surface compounds (especially to evidence for their formation)

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    xx INTRODUCTION

    formed upon the interaction of different molecules with solid surfaces. The development of spec-

    tral criteria to identify such compounds is the second subject of this book, since at present the

    main problem in using physical methods in surface chemistry is to obtain reliable proof that the

    suggested surface compounds are really present.

    Chapter 1 summarizes the fundamentals of the different vibrational spectroscopy methods, and

    their main strengths and weaknesses with respect to each other, as well as their different fieldsof application in studies of surface chemical problems. Several substantial books and reviews

    devoted to such subjects, and analysis of the applications of different spectroscopic methods in

    adsorption and catalysis, have already been published [27, 43, 44, 52, 6366]. Among them, the

    books devoted to particular spectroscopic methods [24, 25, 31, 32, 34, 34a] have been written

    by leading scientists in their fields. Readers who are interested in the possibilities of some

    particular spectral method can find the answers in the appropriate text. The main question of in

    situ studies, including kinetic and spectral measurements, have also been described in reasonable

    detail [35a, 6365].

    It should be pointed out that such numerous data have been obtained by different spectral

    methods during investigations of surface phenomena and that it is impossible to describe andanalyze all such data in a single book. In general, studies can be divided into two groups,

    (i) those devoted to spectroscopic investigations, and (ii) works in which spectroscopic methods

    are used to check on the information obtained by nonspectroscopic methods. The second group

    is widely represented in the literature, and is used for the study of adsorption and catalysis.

    However, the spectral information obtained in a large number of such works is not sufficiently

    reliable and the formation of one or another type of a postulated surface compound is not always

    proven. For these reasons, the conclusions of such studies are not always discussed in detail in

    this book, although appropriate ones will be mentioned. Studies of the other group, which form

    the basis of this book, are as a rule carried out by highly qualified spectroscopists and are based

    on a detailed analysis of the spectral information obtained. These studies contain very importantdata about solids and the surface compounds formed during interaction with different molecules.

    Chapter 2 is devoted to the examination of spectral images of both simple oxides and binary

    oxide surface systems in the various regions where they occur, and includes discussions of

    the following: (i) the fundamental frequencies of the lattices, (ii) surface cationanion bonds,

    (iii) molecular states of adsorbed oxygen, and (iv) surface hydroxyl group vibrations. Particular

    attention is given to the study of electron-donating centers, oxygen ions, electron-accepting centers

    and coordinatively unsaturated cations. The principles of crystal structures of oxides are used to

    interpret the spectra, because it has been shown earlier that the homogeneity or otherwise of

    an oxide surface, as well as the properties of different surface centers, depends on the degree

    of dispersion and is related to the exposure of different crystal faces. The reactivity of surface

    centers to different adsorbed molecules is analyzed for numerous oxide systems. The different

    types of surface centers observed on oxide systems are classified, and the procedures used for

    their investigation by means of molecular spectroscopy are analyzed.

    Probe molecules with spectral parameters sensitive to the state of different adsorption centers

    are described. Particular attention is paid to data on the identification of both Brnsted and Lewis

    acidic sites on the surfaces of different oxide systems through the IR spectra of adsorbed ammonia

    and pyridine. Practically all of the data in the literature on spectral patterns from ammonia bonded

    to coordinatively unsaturated surface cations are considered in this chapter. Correlations revealed

    between the changes in the frequencies of the symmetric deformational vibration of the ammonia

    molecule due to adsorption ammonia and the acceptor abilities of coordinatively unsaturated

    surface cations show the relative strengths of different cation acceptor centers on the oxidesurfaces (the established influence of the nature of the cations on their acceptor ability). It is

    shown that ammonia adsorption opens the way to the identification of surface acidbase pairs

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    INTRODUCTION xxi

    (both surface cations and anions) which lead to ammonia dissociation and the formation of NH 2and OH species. For a number of systems involving acid-forming oxides, the presence of protic

    acid centers is demonstrated, in which a proton compensates for a charge on several surface

    anions through mobility.

    Analysis of the different spectral methods of determination of both the acidic and basic proper-

    ties of an oxide surface is represented in this chapter. Sections where these questions are examinedcontain (i) equations to calculate the strengths of both protic and aprotic surface centers in simple

    and complex oxide systems, (ii) quantitative data on the different nature of active surface centers,

    and (iii) extinction coefficients and values of integral intensities for a number of the most com-

    monly used probes (NH3, Py and CO). In several cases an analysis of the correlations between

    the quantitative characteristics of different types of surface centers and the pre-treatment and/or

    preparative conditions of the surfaces is carried out. Spectral characteristics of both regular and

    defective surface centers are also examined in this chapter.

    In Chapter 3, the states of different cations in zeolites, oxides, supported oxides and heteropoly

    acid systems, which depend on preparation methods and other experimental conditions are ana-

    lyzed on the basis of detailed examinations of diffuse reflection electronic and ESR spectra.Special attention is paid to the cations of copper, nickel, cobalt, palladium, silver and platinum,

    and to their changes upon modification by supports or other active components. Spectral char-

    acteristics of metal particles are dependent on their sizes, types of support (including strong

    metalsupport interaction (SMSIs)) and upon lateral interactions between adsorbed molecules.

    Analysis of the spectra of adsorbed species on a number of metals, as well as the spectral

    manifestations of the complexes formed at the active-component support interface, are also

    considered.

    The data covered in Chapter 3 illustrate the special roles of CO and NO molecules as probes.

    Use of these molecules, coupled with the direct study of cationic states (by diffuse reflectance

    electron spectroscopy (DRES), ESR, etc.), enables the establishment of correlations betweenCO (NO) and both the charge and coordination states of the cations. A number of model

    examples of real oxide surfaces, created on the basis of oxide crystal structures, are examined.

    These models describe sufficiently the experimental data obtained about interactions of the probes

    with both active and inactive surface centers and surface structures. Sections are devoted to the

    detailed examination of the spectral data in this field available from the literature concerning the

    interactions of different types of oxide surfaces with other simple molecules such as H 2, N2, NO,

    H2S, SO2, NO2 and CO2. Such data establish the direct interrelationships between the nature

    of the activation and properties of the surface sites and the activation of these molecules. For

    each molecule, the analysis of its electronic structure is carried out and changes observed upon

    complexation are explained in terms of the changes in the vibrational spectra. It is shown that the

    N2 molecule is a good probe for investigating electron-acceptor centers, whereas the H2 molecule

    is a unique one for describing the properties of acidbase pairs. This chapter concludes with data

    about the limits of spectral ranges characteristic for the complexes of CO (NO) with the variable

    valence and coordination states of different cations, and also with metal clusters of different sizes.

    The potentialities of spectral methods to investigate the interactions of inorganic or organometal-

    lic compounds with oxide surfaces are briefly summarized in Chapter 4. Principal attention is

    given to data representing the analysis of spectral changes resulting from the interactions between

    molybdenum heteropoly acids (HPAs) and the surfaces of different supports, and also the changes

    in properties of such unsupported systems themselves. It is shown that the examined spectra enable

    us to determine whether or not such interactions occur, and can also detect the interactions of

    different types of organometallic systems such as metal- allylic and carbonyl compounds of dif-ferent cations or metals. The results of the modification of oxide surfaces by anions, in particular

    SO42, occupy a significant part of the data discussed in this chapter.

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    xxii INTRODUCTION

    Interactions between oxide surfaces and organic molecules of different types, such as alkanes,

    alkenes, alkynes, aryls (including their halide derivatives), nitriles, alcohols, aldehydes, ketones

    and acids, are presented in Chapter 5. Wherever possible, the complexation with each type of

    surface center is differentiated and analyzed separately. Spectral images of the complexes formed,

    their features and spectral parameters, which depend on the type and particularities of the surface

    center, are examined in detail.Using the spectral data, general correlations are demonstrated between the character of the

    nature and reactivity of the complex being formed from a particular adsorbate and its dependence

    upon the nature of the surface center. The formation of new types of surface species (such as

    unsaturated compounds interacting with coordinatively unsaturated surface cations), first revealed

    by spectral features, is described for a number of systems. This chapter also contains numerous

    energy and spectral characteristics of the surface compounds, such as the - and -allylic com-

    plexes of unsaturated hydrocarbons, formed upon dissociative interactions of organic molecules

    with oxide surfaces.

    Special attention is paid to the estimation of the character of CH bond activation in alkanes.

    Analysis of recently obtained data on methane activation allows the representation of a schemewhich establishes and provides a correlation between the active surface centers and the particular

    intermediate species formed upon them. The latter provide a possibility for understanding the

    pathway by which hydrocarbons are converted to other products on the different surfaces. As

    a result of the spectral classification of the different adsorption species, new types of surface

    compounds have been shown to be formed on oxide surfaces, which are otherwise absent or

    extremely unstable under normal conditions.

    Finally, in Chapter 6 a discussion is given of the mechanisms of a number of catalytic reactions

    which have been investigated by means of vibrational spectroscopy.

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    1 THEORETICAL FUNDAMENTALSAND EXPERIMENTALCONSIDERATIONS OF THESPECTROSCOPIC METHODSUSED IN SURFACE CHEMISTRY

    Three principal types of problems may be distinguished in the application of molecular spec-

    troscopic techniques in surface chemistry, namely (i) the characterization of the surface, (ii) the

    estimation of the type and structures of surface compounds, and (iii) the obtaining of information

    required to understand the mechanisms of the processes proceeding on the surface of a solid. The

    first problem requires the determination of the types and properties of surface centers, which are

    dependent on the structure and morphology of the solid. The second and third problems concernadsorption processes and involve the study of the following: (i) the structures and properties of the

    surface compounds forming at different surface centers, (ii) reaction intermediates, and (iii) the

    directions of their transformations to the products. During recent years, the situation in this areahas greatly improved, and different spectroscopic methods are now available for these studies.

    The general principles of all of the techniques is the interaction between the incident radiation

    or particle beam and the specimen and the following analysis of both the nature and energy of

    the beam after such interaction. The energy regions involved in the different spectral methods

    involving electromagnetic radiation are represented in Figure 1.1, while Table 1.1 summarizes

    some of the essential characteristics of the various techniques.It is clear today that any progress in the field of surface chemistry is impossible without

    the application of such modern methods of molecular spectroscopy as UVVis spectroscopy,

    Fourier-transform infrared (FTIR) spectroscopy, Raman spectroscopy, electron energy loss spec-

    troscopy, (EELS) including high-resolution electron energy loss spectroscopy (HREELS), and

    neutron spectroscopy.

    The main feature of these methods is that they are nondestructive analytical methods, because

    the electromagnetic (radiation) or particle beams which are used, disturb the investigated systeminsignificantly. This is why such vibration techniques in different electromagnetic variants, such

    as transmission, reflectance and emission, or the low-energy electron loss spectroscopies, are very

    widely used nowadays.

    1.1 Electronic spectroscopy

    Electronic spectroscopy (ES) is normally concerned with the valence electronic transitions

    between molecular orbitals. The transmissions between the electronic levels (Figure 1.2) are

    Molecular Spectroscopy of Oxide Catalyst Surfaces. Anatoli Davydov 2003 John Wiley & Sons, Ltd ISBN: 0-471-98731-X

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    2 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    103

    105 107 109 1011 1013 1015 1017 1019

    101 101 103 105 107 109 1011

    (m)

    (Hz)

    Region

    Process NMR ESR

    Molecular

    rotations

    Molecular

    vibrations

    Electronic

    transitions

    Imer-electronic

    transitions

    Nuclear

    excitations

    Radiofrequency Microwave IR UV X-Rays

    Large Medium Short VHF Far ConventionalNear Near Far

    Visible

    Figure 1.1. The regions of the electromagnetic spectrum, classified according to the experimental techniquesemployed and the molecular information that can be obtained.

    E2

    E1

    E0

    ~1 eV

    ~0.1 eV~0.01 eV

    vn

    v1 rnr1

    Figure 1.2. Scheme of energy levels: E, electronic; v, vibrational; r, rotational.

    located in the range of the electromagnetic spectrum (50 000 3000 cm1) this is the basis ofUVVis spectroscopy. The energies associated with the electronic jumps are large enough to

    provokevibrations of the molecule, and the transitions are thereby broadened [6, 810, 33, 116].

    Light in the UV Vis region of the electromagnetic spectrum can be used to study the

    electronic transitions of the substrates. According to the nature of the electronic jumps,

    the electronic transitions found in organic and inorganic chemistry can be classified into

    several groups: (i) d d transitions (Figure 1.3(a)), (ii) charge transfers, (iii) transitions(Figure 1.3(b)), and (iv) n (Figure 1.3(b)). In the far-UV range are found other transitions,e.g. (n ) and ( ) (Figure 1.3(b)). Charge transfers occur due to electron transfersfrom an occupied orbital localized on a donor to an unoccupied orbital of an acceptor. In organic

    systems, these transitions are between electron acceptors and electron donors and produce theabsorption bands in the UV and visible regions of the spectra with 103 106 (see below).In inorganic systems, the charge-transfer phenomena are of two types, involving an electron

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    3

    Table1.1.C

    omparativecharacteristicsofthe

    differentspectralmethodsusedinsurfacechemistry.

    Characteristic

    Technique

    Molecularspectroscopy

    R

    esonancespectroscopy

    Surfacestudies

    IR,PAS

    Raman

    UVVis

    EPR

    NMR

    Mossbauer

    Neutron

    EELS

    XPS

    AFS

    SIMS

    spectroscopy

    Thicknessa

    nalyzed

    mm

    mm

    mm

    mm

    mm

    100m

    0.1mm

    m

    2050A

    1020A

    23A

    Areaanalyzed

    cm2

    m2

    cm2

    cm2

    cm2

    cm2

    mm2

    cm2

    cm2

    cm2

    cm2

    Sampledeg

    radation

    No

    Possible

    No

    No

    No

    No

    Possible

    Verysmall

    Possible

    Possible

    No

    Samplepreparation

    Easy

    Easy

    Easy

    Easy

    Easy

    Easy

    Difficult

    Difficult

    Easy

    Easy

    Easy

    Quantitative

    measurem

    ents

    Possible

    difficult

    Possible

    Yes

    Yes

    Yes

    Yes

    Yes

    Possible

    Possible

    Gaseous

    atmosphe

    re

    Yes

    Yes

    Yes

    Yes

    Yes

    Yes

    Yes

    No

    Difficult

    Difficult

    No

    Temperaturerange

    (C)

    196to500

    196to500

    196to500

    269to1000

    196to200

    269to400

    269to800

    Ambient

    180to600

    180to6

    00

    Ambient

    Information

    obtained

    Functional

    groups;

    adsorbing

    species

    Functional

    groups;

    adsorbing

    species

    Degreeof

    oxidation;ion

    symmetry;

    adsorbing

    species

    Paramagnetic

    species;

    degreeof

    oxidation;

    symmetry

    Func

    tional

    groups

    Degreeof

    oxidation;

    symmetryof

    environment

    Adsorbing

    species;

    atomic

    structure

    Metalligand

    bonds

    Degreeof

    oxidation;

    surface

    composition

    Surface

    composition

    Surface

    composition

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    4 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    eg

    6Dq

    4Dq

    10Dq

    l2g

    Octahedralfield, Voh

    Sphericallysymmetrical

    repulsiond

    Free ion

    (a)

    (b)

    s*

    s

    p*

    p

    p p* n p n s* s s*

    n

    Figure 1.3. Schemes of electron transfers: (a) d d electron transitions in an octahedral field; (b) relativeenergies of electronic transitions between different types of orbitals typical of organic molecules (,

    and n).

    transfer in different directions: (i) from an orbital mainly localized on the metal to that mainly

    localized on the ligand (M L), and (ii) in the opposite direction (L M). The energies ofthese transitions is higher than that for d d transitions, and accordingly the absorption bandsare in the UV region of the spectra ( 103 106). Optical spectra can be directly obtained byeither internal or external reflectionabsorption techniques (reflectance spectroscopy).

    1.1.1 TRANSMISSION SPECTRA

    The transmitted light of intensity I is related to the incident light intensity I0 by the transmit-

    tance, T, given by I /I0 (0< T < 1). For thin samples, the transmittance can be related to the

    concentration of the absorber (c) and the thickness of the sample (l) by the LambertBeer law,

    as follows:

    T () = exp(lc) (1.1)

    where is known as the molar absorption coefficient (cm2 mol1). The optical density orabsorbance, A(= log(I/I0) is also used frequently. It is often preferable to use this parameter inthe integral form (A), as follows:

    A = 2

    1

    A() d= 2

    1

    ln[I0()/I()] d (1.2)

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    VIBRATIONAL SPECTROSCOPY 5

    UVVis spectroscopy is distinguished by a fairly high sensitivity. In particular, the intensity of

    the absorption for allowed one-electron d d transitions is characterized by a molar absorptioncoefficient of the order of1 100. The value is significantly lower for complexes with a highsymmetry and is much greater in the case of the bands characteristic of the charge transfer in

    the complex.

    1.1.2 DIFFUSE REFLECTION SPECTRA

    In surface chemistry, the UV Vis spectroscopic method is usually used in its diffuse reflec-

    tion modification. The radiation reflected from a powdered crystalline surface consists of two

    components, i.e. (i) that reflected from the surface without any transmission (mirror or specular

    reflection), and (ii) that absorbed into the material and which then reappears at the surface after

    multiple scattering. Modern spectrometers minimize the first component, and the term reflectance

    is thus used for diffusely reflected radiation [25, 117].

    Since only a part of the diffuse radiation is returned to the detector, measurement of the diffused

    intensity is difficult. For this purpose, a special integrative sphere (Table 1.2), coated inside witha highly reflecting layer, such as MgO or BaSO4, is used. Such a sphere increases the part of

    the diffused intensity that reaches the detector (3050 %). Spectra are recorded in ratio with a

    sample which has similar diffusion characteristics to the sample under investigation, but without

    any absorption losses.

    The evaluation of the intensities of diffuse reflectance spectra is based on the theory of Kubelka

    and Munk. The reflectance is given by R= I /I0 (0< R

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    6

    Table1.2.Basicexperime

    ntalprinciplesandapplicationsofthedifferentspectralmethodsusedforsurfacechemistryanalysis.

    Method

    Commonscheme

    Thickness

    analyzed

    Quantitative

    measurements

    Information

    obtained

    UVVis

    Source

    Integratingsphere

    Detector

    Standard

    Sample

    mm

    Possible

    Ionsymmetry;

    ad

    sorbing

    sp

    ecies;degree

    ofoxidation

    Transmission

    IR

    Source

    Scatteredlight

    Scatteredlight

    Transmittedlight

    Detector

    KBr

    KBr

    Sample

    disk

    mm

    Possible

    Adsorbedspecies;

    su

    rfaceactive

    sites;functional

    groups

    Reflectio

    nIR

    (RAIR

    S)

    Source

    Detector

    Reflectingsam

    ple

    mm

    Possible

    Adsorbedspecies;

    su

    rfaceactive

    sites;functional

    groups

    ATR

    Sample

    Crystal

    IRradiation

    mm

    Possible

    Adsorbedspecies;

    su

    rfaceactive

    sites;functional

    groups

    Diffuse

    reflection

    (DRIR

    S)

    Source

    Collectingmirror

    Samplepowd

    er

    Detector

    Diffusively

    reflectedlight

    mm

    Possible

    Adsorbedspecies;

    su

    rfaceactive

    sites;functional

    groups

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    7

    .

    EmissionIR

    Furnace

    Detector

    KBr

    Sample

    mm

    Possible

    Adsorbedspecies;

    su

    rfaceactive

    sites;functional

    groups

    Raman

    UVVISorNIRbeam

    Detector

    90

    back-scatteredbeam

    mm

    Possible,butwith

    difficulties

    Functionalgroups;

    ad

    sorbedsites;

    su

    rfacestructure;

    bulkstructure;

    structureof

    ad

    sorbedspecies

    EELS

    Ultra-high-

    vacuumchamber

    Electronbeam

    Impact-scatteredbeam

    Dipole-scatteredbeam

    Sample

    m

    Metalligand

    bonds;phase

    transitions;

    ch

    emical

    structure

    IETS

    Metal

    Metal

    Elec

    tronflow

    Adsorbate

    Oxidelayer

    m

    Possible,butwith

    difficulties

    Vibr

    ationalspectra

    ofminute

    quantitiesof

    m

    aterials

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    8 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    frequencies of atoms within the molecules, but allows us to explain the existence of rotational

    frequencies only if the electronic motions occur at the same frequencies.

    The vibration of a diatomic molecule can be reduced to the motion of a single particle of

    reduced mass m. In this model, the problems are simplified by considering that the diatomic

    molecule can be analogous to the harmonic oscillator (Figure 1.4), in which two masses ( m1 and

    m2) are joined by a perfect spring of length r0. A restoring force fis directly proportional to thedistance r , as follows:

    f= kr= m(d2r/dt2) (1.4)

    where k is known as the harmonic force constant, and is a function of the potential energy U in

    accordance with Hookes law:

    f= dU/dr= kr (1.5)

    Integration of this equation leads to the following parabolic relationship see (Figure 1.4(a)):

    U= 1/2kr 2 (1.6)

    For diatomic molecules AB, r represents the displacement of the atoms from the equilibrium

    separation r0. A small displacement of one of the masses relative to the other will cause the

    system to vibrate as a simple harmonic oscillator with a frequency given by the following:

    0= (1/2 )

    k/m (1.7)

    where m is the reduced mass of the system. At the assignment of the frequencies observed

    in the infrared spectra, this relationship is often used in conjunction with isotopic exchange, in

    particular deutero exchange, as follows:

    X H/X D=

    2 = 2mx/(2 + mx) (1.8)

    where mx is the mass of the X atom. This ratio is 1.37 for OHOD and NHND, and 1.36 for

    CHCD (i.e. ca.

    2).

    According to quantum theory, the energy of the molecule is given in terms of a series of discrete

    energy levels, E0, Ev1 , E

    v2 , etc. (see Figure 1.2), and each discrete molecule must exist at one

    or other of these levels. The frequency of absorption or emission of radiation for a transmission

    between the levels with energies E0 and E1 is given by the following:

    = (E1 E0)/ h (1.9)where h is the Planck constant.

    From the Schrodinger wave equation, the total energy of vibration is as follows:

    Evib= h(v + 1/2) (1.10)

    where is the frequency of vibration of the oscillator and v is the vibrational quantum number.

    For any transition between quantized levels in which v v= 1.

    E= h (1.11)

    The differences between two levels arise directly as a result of the quantum-mechanical deriva-tion of Equation (1.10). For the simple quantum-mechanical model, the presence of combination

    bands and overtones in the spectrum is forbidden, because such bands involve jumps between

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    VIBRATIONAL SPECTROSCOPY 9

    Potentialenergy

    (b)

    DeD

    r0

    V=0V=1V =2

    Internuclear separation

    r

    f= kr

    U= 1 kr22

    Potentialenergy

    Equilibriumposition

    (a)

    Separation

    Figure 1.4. Potential-energy functions for (a) a mass and spring system obeying Hookes law, and (b) a

    real diatomic molecule with a dissociation energy De and equilibrium bond length re (where r0 represents

    the first energy level).

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    10 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    several different quantum levels. There are no such stringent rules in the case of an anharmonic

    oscillator, where overtone and combination bands can appear, often weakly in the spectra, accord-

    ing to the following:

    Evib

    =h(v

    +1/2)

    xe(v

    +1/2)2 (1.12)

    wherexe is the anharmonicity constant. Introduction of this parameter leads to the potential curve

    shown in Figure 1.4(b).

    The movements of the atoms in a molecule during vibration can be approximately classified

    into two groups, i.e. (i) bond stretching, and (ii) angle deformations. For an N-atomic molecule,

    the number of fundamental vibrations is 3N 6 for a nonlinear and 3N 5 for a linear molecule.There are four types of vibrations, i.e. , , , and (Figure 1.5). Generally, the frequencies of

    these vibrations decrease in the order > > > .

    All molecules can be classified into a limited number of symmetry groups, which obey the rules

    of group theory. A knowledge of the symmetry group of a molecule allows the determination

    of the symmetry classes of the 3N 6 normal modes of vibration and their activities in IR andRaman spectroscopies.Assignment of the bands in the spectrum to particular types of vibrations is an important stage

    and is based, as a rule, on group-characteristic (of limited dependence on the nearest molec-

    ular environment) modes. Calculations based on vibrational theory are used for more accurate

    assignment [4, 1416]. These calculations show that there are no strictly characteristic vibrational

    modes; frequencies of many group vibrations are coupled and make certain contributions to each

    other. A vibration with a minimum contribution from other vibrations is known as a group char-

    acteristic. Usually, interpretations of the spectra of adsorbateadsorbent systems are made by the

    stretching

    symmetricstretching

    symmetricstretching

    asymmetricstretching

    asymmetricstretching

    bending

    bendingin-plane

    bendingout-of-plane

    bending

    bending

    + +

    rocking twisting wagging

    +

    ++

    +

    (a) Linear molecules (b) Non-linear molecules

    Figure 1.5. Fundamental modes of vibration of (a) linear, and (b) nonlinear molecules.

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    VIBRATIONAL SPECTROSCOPY 11

    comparison with the spectra of bulk compounds or fragments isolated in a matrix. However, in

    this way only certain types of compound can be identified. Calculations of the vibrational spectra

    of individual surface species based on the modeling of the potential function of the molecule

    (vibrations in the force constants of the potential function) are useful for interpreting changes in

    vibrational frequencies and their reactions to changes in the force field of molecules subjected to

    the influence of a highly nonuniform field at an adsorbent surface [19, 118].Several forms of vibrational spectroscopy are now in routine use, i.e. (i) transmission infrared,

    (ii) Raman, (iii) diffuse reflection, (iv) reflectionabsorption infrared, and (v) electron energy

    loss, but in the study of surfaces none has found wider application than infrared spectroscopy.

    1.2.1 INFRARED SPECTROSCOPY

    The infrared (IR) region corresponds to the energies of the vibrations and rotations of molecules.

    If a molecule is subjected to IR radiation whose frequency is equal to that of one of its oscillators,

    this oscillator will resonate and absorb part of the radiation. The absorption (emission) intensity

    is given by the transition probability between the ground and excited states. Not all vibrations are

    observedonly those transitions corresponding to vibrations with variation of the dipole momentare active in IRS. The intensity of the infrared band is proportional to the square of the change

    in dipole moment. The principles of this method have been presented in numerous books and

    reviews [15, 1116, 119123] and are summarized in Table 1.2.

    In the study of processes occurring on surfaces, transmission, reflectance, emission and diffuse

    reflection infrared spectroscopies are used.

    Transmission spectroscopy

    A common infrared transmission spectrum is obtained as a result of the direct transmission of an

    infrared beam through a sample when the following conditions apply: = +1 (/Q)0 = 0,where is the dipole moment, and Q is a normal coordinate. As in UVVis spectroscopy,the spectrometer records the transmission, T (= I /I0= exp(kl)), the intensity of which can befound from the LambertBeer law (Equation (1.1)). The sensitivity of this method is determined

    by both the characteristics of the radiation detector and by the absorption coefficient of the

    medium. Approximately a 10-fold gain in sensitivity can be achieved by the use of the Fourier

    transform (FT) technique [1, 120].

    To study the spectra of bulk oxides, dilution in either KBr (down to 400 cm1) or CsI (downto 200 cm1), or polyethylene disks are used. If the sample is stable in air and does not reactwith KBr or CsI, these are the methods most often used. However, if any interactions take place,

    then the techniques of attenuated total (internal) reflection (ATR) or emission spectroscopies have

    to be used.

    For both cases, in order to obtain a typical transmission IR spectrum from oxides in the

    region of surface vibrations (in this case, the thickness of the corresponding sample is ten times

    more, as a minimum, than that of the corresponding samples prepared in an immersion media),

    the sample has to allow at least a partial transmission, preferably 10 % or more, of the IR

    beam. Scattering of the radiation by the particles can be another factor which leads to low

    transmission. The transparency is improved when the oxide particle sizes are small relative to

    the radiation wavelength. Scattering may be significantly reduced by the use of pressed disks

    or highly dispersed samples (particles size less than 1 m). The latter can be prepared in two

    different ways, i.e. (i) sedimentation of the dissolved sample from an inert solvent or from air

    onto a transparent window, or (ii) by using an electrical field [42]. When a material is pressed into

    a thin flat self-supported disk, the scattering, which takes place during the transmission of the IRradiation through the sample, can be substantially reduced. In general, such a disk should be from

    one to a few tenths of a millimeter in thickness and have a density between 10 and 100 mg cm2

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    12 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    Figure 1.6. A typical mold used for compressing self-supported pellets of adsorbent in infrared studies.

    in order to give good transmission in the infrared and also to have good mechanical properties.

    It is better to press the samples in a demountable mold (Figure 1.6) [19, 42], which then allows

    adjustment of the lateral pressure on the compressed sample by means of a number of screws

    and plates, in order to prevent cracking of the thin disk and to facilitate its removal from the

    mold. Preparation of such thin samples, especially from transition-metal oxides or zeolites, istruly an art. If the solids are not transparent or cannot be molded as disks and hence have

    to be handled as powders, the following methods can be useful: (i) the use of a grating; (ii) a

    (powder) technique in which the powder is finely pulverized, sifted, and then spread out on an

    IR-transparent disk (such as KBr, CaF2 or a silicon single crystal) and, if this covering is stable,

    then covered by a second disk; (iii) dilution of the sample in a compound that is transparent

    and inert to the reaction being studied (e.g. SiO2 and Al2O3); (iv) the use of special cells. The

    problem of sample preparation is minimized in the case of diffuse reflection spectroscopy [25,

    61, 122124].

    To record the infrared spectra of adsorbed molecules, special vacuum cells are used these

    are available in many different and widely variable types, depending on the system being studied[1821, 2326, 2835, 42, 4446, 63, 64]. Ideally, these cells should be designed so that the

    sample can be heated up to 1273 K, and cooled to liquid nitrogen temperature, to adsorb/desorb

    both gases and vapors at different temperatures, be able to maintain a high vacuum, and to record

    the spectra of adsorbed molecules without exposing the pellet (disk) to the air. The main problem

    here is achieving an hermetic sealing of the windows (plates) which are transparent in the

    IR (Table 1.3 [42, 119, 125127]). Frequently, such a sealing is made by the use of different

    cements and glues with low vapor pressures, or alternatively by using O-rings and flanges.

    There are two types of cells used for recording infrared spectra under high vacuum over a wide

    temperature range: (i) a cell, large in length, which gives the possibility of separating a heater

    from the region of the sealed windows, i.e. where the recording of spectra and the heating of the

    sample are carried out in different parts of the cell or if a static sample is heated, a cooling of

    the windows is required (see, for example, a cell design resulting from the work of this present

    author (Figure 1.7) [42, 128]); (ii) a cell with a very short optical pass (

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    VIBRATIONAL SPECTROSCOPY 13

    Table 1.3. Various optical materials used for lenses and windows in infrared studies.

    Material Low-energy cutoff

    (cm1)Comments

    Sapphire >1600 High mechanical strength; inert;

    connected with metal; hard; expensiveQuartz >2500 Good for high-temperature work and in

    the overtone region; insoluble; easy to

    work in fused form

    LiF >1200 Good dispersion in the near-IR region;

    easily scratches

    MgF2 1400 Strong; chemically durable

    CaF2 1200 Inert to most chemicals; tends to be

    costly; slightly soluble; good from

    73373 K

    MgO >1200 Hard and costly; can be sealed to a

    high-expansion glass

    Silicon 1100 Inert; insoluble; connected with glass; not

    transparent at high temperatures

    NaF 1000 Slightly hydroscopic

    BaF2 900 Hard; expensive

    ZnS 714 Good up to 1073 K; strong; chemically

    durable

    NaCl 600 Slightly hydroscopic; cheap; easily

    worked

    KCl 550 Slightly hydroscopic; cheap

    AgCl 500 Photosensitive; can corrode metals

    ZnSe 500 Good up to 573 K; soluble in acids

    KBr 350 Hydroscopic; easily scratched; used aspowder for pressed-disk technique

    CsBr 250 Very hard; expensive

    KRS-5 250 Very soluble; expensive; toxic; deforms

    under pressure

    CsI 180 Very hard; expensive

    been reviewed by Little [18], Kiselev and Lygin [19], Delgass et al. [25], Shchekochikhin and

    Davydov [42], Bell [119, 127], and Basu, Ballinger, Yates et al. [128a], as well as in numerous

    original studies.

    The best materials for windows directly connected to glass are silicon, MgO and AgCl, while

    sapphire is the best material for connection to metals (see Table 1.3). Quartz cells, which are

    usually routinely used in the visible and UV regions of the spectrum, can also be employed in

    the infrared region, but only above 2000 cm1. A very convenient cell is one with silicon singlecrystal windows (Figure 1.8(a)) but, unfortunately, this cannot be used at temperature higher than

    473 K because of the reduced transparency of the silicon single crystal as a result of internal

    electron transfer mechanisms.

    There are several types of cells of minimized volume, used in order to record spectra under

    dynamic conditions (e.g. at high temperatures during catalytic transformations so-called in

    situ conditions see, for example, Figures 1.7(b) and 1.10). A simple flow-cell-reactor made

    from metal [42] or quartz [64, 65] practically without any free volume, has been proposed(Figures 1.7(b) and 1.11). The main part of such a cell is a reactor made from metal or quartz.

    Both the reactor and windows (CaF2, BaF2, ZnS or ZnSe) are polished and clamped to each

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    14 SPECTROSCOPIC METHODS IN SURFACE CHEMISTRY

    Furnace

    Thermocouplepocket

    Pyrex

    Catalyst disk

    NaCl window

    Quartz sampleholder

    Quartz retainingring

    10

    10/1

    19

    11

    13

    2

    4

    56 7

    812

    (a) (b)

    9

    Figure 1.7. Schematics of cell-reactors used for studying the spectra of adsorbed molecules at (a) room,and (b) high temperatures: 1, cell body; 2, sample holder; 3, evacuation port; 4, case for thermocouple;

    5, container for heater; 6, 10, cooling channels; 7, 11, flanged connectors; 8, windows; 9, connectors; 12,

    sample pocket.

    Tovacuum

    10 mmSi window

    NaClwindow

    Liquid N2

    Siliconwindow

    (a) (b)

    Figure 1.8. Schematics of vacuum cells with silicon windows: (a) for low-temperature investigations;

    (b) with a short optical path.

    other [64, 65]. Connections between the cell body and the windows is achieved by using iridium

    or gold foils, or with Teflon [42]. The Graseby Specac company now produces standard in situ

    high-temperature cells for temperature ranges up to 773 K, as well as high temperature and

    pressure cells.

    Emission spectroscopy

    Methodological difficulties in the study of surface species caused by strong scattering or absorp-

    tion of infrared light by the adsorbing sample can be eliminated if emission spectra are recorded

    [1, 25, 35]. This method, however, is less frequently used since the intensities of the emissionbands are quite low, except at higher temperatures. Emission spectra are usually produced by

    heating the sample above 473 K (Figure 1.12) [129] and are the most appropriate in cases where

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    VIBRATIONAL SPECTROSCOPY 15

    Figure 1.9. Schematics of types of sample holder.

    reactions proceed on surfaces at high temperatures (see Table 1.2). The spectrum is obtained bymeasuring the ratio of the emitted radiation at any wavelength to that emitted by a perfect black

    body at the same wavelength and temperature. According to the Kirchoff law, = a , wherea is the absorbance (fra