Analysis and characterization of surface oxides on intermetallic alloys of zirconium using auger electron spectroscopy by Rajesh G Mirpuri A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Chemical Engineering Montana State University © Copyright by Rajesh G Mirpuri (1991) Abstract: The surface composition of oxidized zirconium and nickel and their oxidized intermetallics, ZrNi3, ZrNi, ZrNi5 and Zr2Ni7 are evaluated. This was performed following the installation and set-up of an Auger electron spectroscope and development of relevant software for both digital process control and data analysis. Surface oxide layers formed on the samples under two different conditions, room temperature and at 300°C for I hour were analyzed. Depth profiles were performed using Auger electron spectroscopy and argon ion sputtering. The zirconium and nickel concentrations increased and the oxygen concentration decreased with increase in sputtering time. Longer sputter times were noticed in the case of the samples oxidized at 300°C indicating thicker oxide layers. The oxide layer formed at 300°C on zirconium was thicker than the oxide layer on nickel at 300°C since the former required 90 minutes of sputtering compared to 4 minutes of sputtering for the latter. The oxide layer formed on zirconium at 300°C is shown to have a ZrO2 stoichiometry. The sputter depth profiles on the intermetallics are consistent with earlier work reported in the literature, with a slight discrepancy in the steady state final intensities of the zirconium and nickel peaks noticed in the case of the intermetallics oxidized at 300°C. This can be attributed to a change in the primary Auger electron beam energy from 3 keV to 2 keV which diminished the peak intensities significantly. Surface cracks on the intermetallic surfaces which are laterally oxidized during high temperature oxygen exposure may have also resulted in the attenuation of the nickel and zirconium peak intensities and the increase in oxygen peak intensity. ANALYSIS AND CHARACTERIZATION OF SURFACE OXIDES ON INTERMETALLIC ALLOYS OF ZIRCONIUM USING AUGER ELECTRON SPECTROSCOPY by Rajesh G . Mirpuri A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Chemical Engineering MONTANA STATE UNIVERSITY Bo zeman, Montana May 1991 APPROVAL of a thesis submitted by Rajesh G. Mirpuri This thesis has been read by each member of the thesis committee and has been found to be satisfactory regarding content, English usage, format, citations, bibliographic style, and consistency, and is ready for submission to the College of Graduate Studies. i L m / Approved for the Major Department V>7 -C- ' Llll/ Dhte d, Major Department V Approved for the College of Graduate Studies /f?/ Date Graduate Dean iii STATEMENT OF PERMISSION TO USE In presenting this thesis in partial fulfillment of the requirements University, for a master's degree at Montana State I agree that the Library shall make it available to borrowers under rules of the Library. Brief quotations from this thesis are allowable without special permission, provided that accurate acknowledgement of source is made. Permission for extensive quotation from or reproduction of this thesis may be granted by my major professor, or in his/her absence, by the Dean of Libraries when, in the opinion of either, the proposed use of the material is for scholarly purposes. Any copying or use of the material in this thesis for financial gain shall not be allowed without my written permission. Signature Date ,UAjis I l ^ I cIaI I iv TABLE OF CONTENTS Page A P P R O V A L ........... ................................. . . .. ii STATEMENT OF PERMISSION TO U S E ..... , . . ................ iii TABLE OF CONTENTS ....................................... iv LIST vi LIST OF TABLES ................................... OF F I G U R E S ........................ A B S T R A C T ................................................. I .I N T R O D U C T I O N .......................... vii ix I 2 .B A C K G R O U N D ............................................. Research Objectives ................................ 6 10 3. OXIDATION OF METALS AND ALLOYS ...... ............ ;. . . Low Temperature O x i d a t i o n ......... Diffusion in Oxides ............................. '.. Lattice Defects ................................... Lattice Diffusion ................................ Diffusion Mechanisms ............................ High Temperature Oxidation o f Metals ............. Compact Oxide Scales ............................ Porous Oxide Scales ............................. High Temperature Oxidation of Metals & Alloys .... H 12 13 14 14 16 17 17 21 22 4. EXPERIMENTAL M E T H O D .............. '................... Auger Electron Spectroscopy ....................... Experimental S y s t e m ............ ................... ' Ultra-High Vacuum Systems ....................... Ion G u n ........................................... Sample Mount System ............................. Energy A n a l y z e r .................................. Sample Preparation ...'...... <...................... Surface P r e p a r a t i o n ............................... Sample Alignment .............. Elastic Peak Procedure ............................ ■ Acquiring AES D a t a .............................. Shut Down P r o c e d u r e ................................ 26 26 29 29 30 32 36 38 39 40 41 41 41 5. RESULTS .............. ................................. 42 6. INTERPRETATION 68 V TABLE OF CONTENTS-CONTINUED Page 7. SUMMARY AND C O N C L U S I O N S ............................. 80 8. RECOMMENDATIONS FOR FURTHER RESEARCH ................ 82 R E F E R E N C E S ............................................... 84 vi LIST OF TABLES Table 1. Steady State Intensity Profile Data of Zrl peak for the metal and intermetallie samples analyzed .......... Page 71 2. Steady State Intensity Profile of Nil and Ni2 peaks for the metal and intermetallie samples analyzed ........... 73 3. The sputter time required to remove the oxide layer for the metal and intermetal lie s a m p l e s ................ 78 vii LIST OF FIGURES Figure Page 1. Wagner Schematics for Oxidation of Alloys ........... 19 2. Wagner Schematics for Oxidation of Metal Alloys ...... 25 3. Energetics of the Auger p r o c e s s ...................... 27 4. AES Analytical E q u i p m e n t ............................. 31 5. Sample Holder for AES A n a l y s i s ....................... 33 6. Relative Orientation of Sample Mount with Ion Gun and Electron G u n ......................... 35 7. The Electron Gun and CMA A r r a n g e m e n t ................ 37 8. AES Survey of Zirconium Foil ......................... 43 9. AES Survey of Sputter Cleaned Zirconium 44 ............ 10. Expanded energy region of Sputter Cleaned Z i r c o n i u m .................................. 45 11. Multiplexed Zr2 Peak on Zirconium Foil .............. 47 12. Multiplexed Zr2 Peak on Sputter Cleaned Zirconium ... 48 13. Multiplexed Zrl Peak on Sputter Cleaned Zirconium ... 49 14. Multiplexed Oxygen Peak onZirconium ................. 51 15. Sputter Depth Profile for Z r ...................... . . . 52 15. 53 Sputter Depth Profile for Z r (ox) ................ 17. AES Survey of Nickel F o i l ....................... 54 18. AES Survey of Sputter Cleaned Nickel ........... 56 19. Multiplexed Nil Peak on Sputter Cleaned Nickel ..... 57 20. Multiplexed Ni2 Peak on Sputter Cleaned Nickel ..... 58 21. Sputter Depth Profile for N i .......................... 59 22. Sputter Depth Profile for Ni (ox) .......... 60 viii LIST OF FIGURES - CONTINUED Figure Page 23. Sputter Depth Profile for ZrNiS ...................... 61 24. Sputter Depth Profile for Zr2Ni7 .........•........... 63 25. Sputter Depth Profile for ZrNi3 ...................... 64 26. Sputter Depth Profile for Z r N i ....................... 65 27. Sputter Depth Profile for ZrNiS(ox) ................. 66 28. Sputter Depth Profile for ZrNi3(ox) ................. 67 29. Steady State Intensity Profile for Zr ............... 72 30. Steady State Intensity Profile for Ni ................ 74 31. An Optical Microscope Photograph of Polished ZrNi3 after Oxidation at 3 0 0 ° C ....................... 76 ix ABSTRACT The surface composition of oxidized zirconium and nickel and their oxidized intermetallics, ZrNi3, ZrNi, ZrNi5 and Zr2Ni7 are evaluated. This was performed following the installation and set-up of an Auger electron spectroscope and development of relevant software for both digital process control and data analysis. Surface oxide layers formed on the samples under two different conditions, room temperature and at 3OO0C for I hour were analyzed. Depth profiles were performed using Auger electron spectroscopy and argon ion sputtering. The zirconium and nickel concentrations increased and the oxygen concentration decreased with increase in sputtering time. Longer sputter times were noticed in the case of the samples oxidized at 300°C indicating thicker oxide layers. The oxide layer formed at 3OO0C on zirconium was thicker than the oxide layer on nickel at 3OO0C since the former required 90 minutes of sputtering compared to 4 minutes of sputtering for the latter. The oxide layer formed on zirconium at 300°C is shown to have a ZrO2 stoichiometry. The sputter depth profiles on the intermetallics are consistent with earlier work reported in the literature, with a slight discrepancy in the steady state final intensities of the zirconium and nickel peaks noticed in the case of the intermetallics oxidized at 300°C. This can be attributed to a change in the primary Auger electron beam energy from 3 keV to 2 keV which diminished the peak intensities significantly. Surface cracks on the intermetallic surfaces which are laterally oxidized during high temperature oxygen exposure may have also resulted in the attenuation of the nickel and zirconium peak intensities and the increase in oxygen peak intensity. I CHAPTER I INTRODUCTION The development of metal alloys resistance to surface oxidation, cost, durability and utility which have improved has a major impact on the of equipment and ,components utilized in high temperature and other corrosive environments. The useful structures conditions life and can of metallic electrical also be components systems incorporated operated significantly under extended into ambient through appropriate alloying to improve their resistance to oxidation. Thus a more fundamental in-depth knowledge of improved metal alloys and composites, resistance and high which demonstrate enhanced corrosion temperature stability, would greatly benefit modern industry. The reaction of oxygen with metal alloy surfaces is such that it can lead to the formation of a cohesive surface oxide layer, which protects the alloy from further significant oxidation. An in-depth study on this reaction would help in the development of metal alloys especially suited to a large range of future and current applications requiring oxidation resistance. Extensive literature[1,2,3] on the methods of relating surface oxidation mechanisms and oxide structures of pure metals provides the basis for the design and conduct of this investigation on the surface oxidation of metal alloys. 2 By enhancing the protective surface oxide layer, which can be either porous or compact, improved oxidation resistance is usually realized in metals and alloys. Compact oxide layers offer the best protection against high temperature oxidation because they form a nonporous barrier between the unreacted metal and oxidizing environment. Thus oxidation resistance in alloys in which at least one of the components combine readily with which oxygen are b u l k [4]. can be effective generally barriers attributed to to further surface oxidation layers of the On oxidation of a metal alloy, where the base metal oxidizes rather rapidly, the base metal oxide forms on the outer scale and the oxide of the alloying element forms on the inner scale[2,3]. oxide layer can The ratio of the components in a surface be different from surface oxide thickness keeps that in the increasing until bulk. The it inhibits further growth. Cracking or flaking of these oxidized layers leads to the loss of their protective property. If the oxide layer cracks, then the metal alloy can return to its initial stage and the oxidation rate increases. On the contrary, if the resulting oxide layer remains intact and is cohesive, it will eventually permeability, any resist, further by virtue significant of reduced growth in the oxygen oxide layer thickness. The indicates layer Wagner oxidation model that the growth rate decreases with time for metal of a compact and increasing alloys[2,3] surface oxide oxide layer 3 thickness. When a clean metal alloy is exposed to an oxidizing atmosphere, initial reaction kinetics controls the extent of oxide formation of each of the metallic components. oxide layer forms on the surface of the alloy, Once a further oxidation is limited by the diffusion of the oxygen through the oxide layer. Concentration gradients develop in the metal near the metal/oxide interface. The rate of oxygen diffusion into the alloy will depend in part on the concentrations of the metal oxides resulting from the surface oxidation reaction and partly developing on the oxide dif fusivities layer and the of oxygen metallic in both elements in the the underlying reduced alloy. The surface oxidation characteristics of the intermetallic alloys of zirconium make an excellent choice as a subject for investigation because of zirconium's industrial importance and the fact that it has received little previous attention in this area. Zirconium is used extensively[5] in the nuclear power industry as a major constituent of various fuel cladding alloys that separate the fuel from coolant water in atomic reactors. The most widely used alloys, zircaloys, as they are commonly known, consist of zirconium, together with tin, chromium, better iron, nickel etc. which are added to promote corrosion resistance. An important property of zirconium is its low capture cross section for neutrons i.e., neutrons pass freely through the internal zirconium structure without an appreciable energy loss and a corresponding 4 temperature rise in the cladding material[6] . Zirconium based fuel cladding alloys are resistant to the corrosive environment inside the atomic reactors. The corrosive resistance of zirconium based alloys is due to the formation of thin, protective, cohesive surface oxide layers. Extensive w o r k [6] has been carried out on the kinetics of bulk oxidation temperatures of zirconium and under different its alloys environments at elevated including air, water, steam and oxygen. The primary method of analyzing the composition of oxide surface layers in this study is Auger Electron Spectroscopy (AES) which composition alloys[7]. lends itself of the surface One of the to investigating strata most of clean interesting the and atomic oxidized applications of quantitative AES analysis is the depth profiling technique, in which surface atoms are removed by ion bombardment with A E S [8] analysis of equipment surface used composition in AES depth at sequential profiling is depths. equivalent The to a standard Auger spectrometer in combination with an ion gun. The ion gun is used to bombard the surface atoms of the sample at a relatively slow rate, and remove surface atoms almost atomic a carried layer out by layer. during If quantitative ion bombardment, the AES analysis results yield is the composition of the sample at different depths. Single phase metals are a better choice for a surface study of the present type even though most important alloys 5 consist primarily of polyphase composites of solid solutions and intermetallic compounds( ! C s ) . The main drawback in using polyphase alloys is that spectroscopic information gathered after the oxidation of these alloys is difficult to interpret due to the probable presence of more than one surface phase[l]. This complication can be circumvented by utilizing alloy compositions corresponding to intermetallic compounds which are multi-element single phase metals. The information thus developed can then be used to model the oxidation resistance of composite alloys from an improved understanding of the surface oxidation properties of their individual solid phases. 6 CHAPTER 2 BACKGROUND Techniques of Electron Spectroscopy, Electron Spectroscopy, have been especially. employed to Auger study the interaction of oxygen with various metal surfaces. The types of metallic surfaces intermetallic analyzed compounds in include both pure single metals crystal and and polycrystalline form and composite alloys of intermetallics and solid solutions. These materials have been subjected to wide ranges of temperatures, pressures and exposures to various oxidizing atmospheres. durations of Several surface analytical methods have been used in combination with argon ion milling for depth profiles. The most extensively used methods are the Secondary Ion Mass Spectroscopy (SIMS) and the Electron Spectroscopy methods, in particular Auger Electron Spectroscopy(AES) and X-ray Photoelectron Spectroscopy (XPS). The oxidation behavior of both single and polycrystalline samples of zirconium have been investigated. It has been shown that a cohesive surface oxide layer, which stoichiometry is formed on bulk zirconium [4]. has a ZrO2 The initial exposure of zirconium to oxygen results in the.formation of a nuclei of surface completion at an O2 oxide which grow to coalescence exposure of 3 0 to 60 L(1 L = and IO"6 Torr.s) and has a thickness of approximately 2 nm at room temperature. 7 Since this oxidation proceeds slowly there is a transition region of intermediate oxides between the ZrO2 layer and the bulk Zr [I]. The formation protects the of the underlying thin metal ZrO2 surface from layer further on Zr significant oxidation at 300 K, since the diffusion of O2 through ZrO2 is very slow. However at higher temperatures, oxygen permeation into the bulk metal measurable rates from the surface oxide layer occurs at due to increased oxygen .diffusivity and solubility in Zr. J.S. Foord et a l ., studied the adsorption of D2, CO, N2, NO and O2 on Zr at 300 K [9]. Work function, electron impact, Auger, and adsorbed diffusion phases data leads indicated that to 'rapid surface heating to of these bulk oxygen diffusion and very little desorption. A related study [10] conducted by P.Sen et al., investigated the surface oxidation of three metglasses in the copper-zirconium system by employing X-ray Photoelectron Spectroscopy and Auger Electron Spectroscopy to compare their oxidation behavior with that of the corresponding crystalline states of the alloys. The study was conducted over a wide range of temperatures, oxidation pressures and alloy compositions. It was shown that both glassy and crystalline states of the Cu-Zr alloys exhibit preferential oxidation at intermediate oxygen exposures. 8 The surface oxidation of pure zirconium and its dilute binary alloys investigated by with tin, XPS. In chromium this and study iron Lalit has Kumar et been a l ., compared the oxidation behavior of zirconium and its alloys at room temperature [11]. It was observed that mostly suboxides of Zr are formed during the initial stages of oxidation at oxygen exposures less than 10 L, while at higher exposures, ZrO2 is the dominant oxide suboxides are present. species formed, although two Pure Zr as well as its dilute alloys exhibit a decreasing rate of oxidation with increasing oxygen exposure. Bertolini et al. , analyzed the surface metallic properties of Ni63 7Zr36 2 alloy by Auger electron spectroscopy and photoelectron spectroscopy in combination with argon ion bombardment [12]. The elemental composition as a function of depth below the surface was analyzed. A thin ZrO2 oxide layer was observed to extend up to 15-35 A below the outer surface beyond which an abrupt interface with the Ni63 7Zr36 2 alloy- existed. Several studies of the surface oxidation behavior of nickel-zirconium intermetallic compounds have been conducted. Wright, Cocke and Owens conducted a detailed study [13] on five Ni-Zr intermetallic compounds, Zr2Ni, ZrNi, ZrNi3, Zr2Ni7 and ZrNi5. The analysis included sputter cleaning of the metal alloys by argon ion milling followed by exposure to sequential treatments of hydrogen, oxygen, and hydrogen a second time. 9 These experiments were carried out at room temperatures and at 4OO0C. The depth concentration profiles were then analyzed using high resolution AES. The results showed that the surface was covered by ZrO2 after exposure to air at room temperature and covered by NiO after high temperature oxidation at 4 OO0C . The ratio at the surface of Ni to Zr was always greater after oxidation than after reduction. This indicates a preferential oxidation of Zr over Ni when both are present in a reduced form and the outward diffusion of Ni cations through the oxide strata at 4OO0C during oxidation. Deibert and Wright investigated [14] two of the above mentioned intermetallics, ZrNi3 and Zr2Ni7, by high resolution Auger Spectroscopy and Ar ion sputtering. The intermetallics were subjected to sequential hydrogen, oxygen and hydrogen treatments. The results indicate an essentially pure reduced Ni surface on a layer of oxidized zirconium, which in turn is supported on constituted a the unaltered highly active alloy. The catalyst reduced surface for nickel various reactions of possible industrial relevance. The thickness of the reduced Ni layer is estimated to be between 10 and 20 nm. In another series of experiments by Deibert and Wright [15], the initial surface oxidation of sputter cleaned nickelzirconium intermetallics (ZrNi5, Zr2Ni7, ZrNi3, ZrNi, ZrNi3) at room temperature analysis and surfaces of was argon the investigated ion alloys by sputtering. were shown quantitative The to be Auger sputter-cleaned enriched in Zr 10 relative to their bulk, relatively dilute especially for the alloys which are in Zr. The experimental results indicate that the ratio of the sputtering rate of Ni to that of Zr is dependent on the composition of the alloy. Research Objectives * Installation Spectroscope and set-up of the PHI Auger Electron and development of relevant software for both digital process control and data analysis. * Study intermetallic of the surface compounds of compositions zirconium and of the nickel oxidized including ZrNi3, ZrNi, ZrNi5 and Zr2Ni7 and oxidized zirconium and nickel metal foils. * Develop an improved understanding of the surface oxidation of the zirconium alloys at 3OO0C. * Compare the results of this study with recent studies of Zr-Ni intermetallics, with particular emphasis on oxidation of the intermetallics. 11 CHAPTER 3 OXIDATION OF METALS AND ALLOYS The total chemical equation for the reaction between a metal and oxygen gas is: aMe+^ Though this appears to be a simple equation, the reaction path and the oxidation behavior of a metal depends on a variety of factors. The metal oxidation reaction mechanisms, as a result, are complex. The initial step in the metal-oxygen reaction involves the adsorption of gas on the metal surface. As the reaction proceeds, oxygen may dissolve in the metal; then oxide is formed on the surface as an oxide layer. Both the adsorption and the initial orientation, preparation, oxide crystal and formation defects impurities are at functions the of .surface surface, in both the metal surface and the gas [16] . The surface oxide separates the metal and the gas. When a compact film covers the surface, the reaction proceeds through a solid-state diffusion of the reactants through the film. For thin films the driving force for this transport of reactants is mainly due to electric fields (migration of charged imperfections) in or across the film. For thick films 12 or scales it is determined by the chemical potential gradient across the scale [17]. Metals may also form porous oxide scales which as such do not serve as a reactants. In solid-state such cases diffusion the barrier reaction may between be the limited by processes occurring at phase boundaries. At high temperatures, oxides may also be liquid or volatile. The overall driving force of metal-oxygen reactions is the free energy change associated with the formation of the oxide from the reactants. Thermodynamically the oxide will be formed only if the ambient oxygen pressure is larger than the dissociation pressure of the oxide metal in equilibrium with its [16]. Low-Temperature Oxidation The initial step in the reaction between a metal oxygen is the adsorption of gas on the metal surface. and Then isolated oxide nuclei form at random positions on the surface. After formation of the random oxide nuclei the oxidation proceeds through a growth of the individual crystallites until the whole surface is covered with oxide. The rate of reaction during the initial stage increases with time; sticking coefficients of oxygen increases that is, as oxygen the is consumed. This increased activity is due to an initial oxide nucleation at through lateral a preferred sites surface and growth the reaction of the proceeds nuclei [16]. 13 Dislocations, surface defects, impurities, etc., serve as nucleation sites. The adsorbed oxygen diffuses on the surface to the growing nuclei, causing an oxygen depletion in a zone around each nucleus in which no other nuclei form. The size of these zones is governed by the supply of adsorbed oxygen and the rate of surface migration [18]. Diffusion in Oxides When a dense, compact oxide film or scale has been formed on a metal surface, the oxide separates the reactants. Thus, reaction can only proceed through a solid-state diffusion of reactants through the oxide [19]. Diffusion in solids takes place because of the occurrence of imperfections or defects in solids [16] . Imperfections in solids can be broadly divided into point or lattice defects. Vacancies, interstitial misplaced atoms come under point defects. atoms, and Line and surface defects include dislocations, grain boundaries and inner and outer surfaces. Point or lattice defects are responsible for lattice diffusion, also called volume or bulk diffusion [16]. In polycrystalline material's the relative contributions of the different types of diffusion are a function of temperature, partial pressure of the components, grain size, porosity, activation etc. Grain energy than boundary volume diffusion diffusion has and as a smaller a result becomes increasingly important at lower temperatures [20]. 14 Lattice Defects In a perfect crystal both the entropy and internal energy of the system increases with the creation of point defects. The equilibrium concentration of the defects will be reached when the free energy of the system is at a minimum. given crystal all types of defects, in principle, In any will be formed although the free energies of formation of different types and systems of defects will have widely different values. Correspondingly one type of defect structure commonly predominates in a particular solid at equilibrium. The relative concentrations of the different types of defects is a function of temperature and other variables which influence the state and the composition of the compound. Thus, defect equilibria with a large positive enthalpy of formation which are not favored at low temperatures, may become important at high temperatures. Lattice defects may be neutral or Lattice diffusion takes place through the movement of charged. Lattice Diffusion point defects. The presence of 7 different types of defects gives rise to different mechanisms of diffusion. Pick's laws of diffusion give the mathematical relationship between the concentration gradient and the diffusion coefficient [18] . The rate of diffusion is expressed in terms of the diffusion coefficient D, which is defined by Pick's first law, 15 where J is the instantaneous flow rate per unit area of the diffusing species across a plane, the diffusing concentration diffusion species at gradient constant D the normal is the c is the concentration of plane, to and the flow dc/dx plane. rate/unit is the Thus, the area at unit concentration gradient normal to the plane. Pick's second law relates the concentration gradient to the change in concentration with time. For the case in which the diffusion coefficient is independent of concentration: dt These equations can be Qx 2 solved under certain boundary conditions which may be closely approximated experimentally. For homogenous diffusion in a solid the concentration of the diffusing species normal to the plane is given by: exp (-■ 2\JitDt ADt where c represents the concentration at a distance x from the surface, cQ is the concentration of the species present on the surface, originally and t the time of diffusion anneal. The typical experiment used to establish the constants in this relationship involves deposition of a very thin film of radioactive isotopes on a plane surface of a sample and, after subsequent diffusion anneal, determination of the & 16 concentration of diffusing species as a function of distance from the plane surface [16]. If diffusion is nonhomogenous, different relationships between concentration and penetration distance may result. The temperature dependence of the diffusion coefficient is given by: D-Z^exp(--^L) where Q is the activation energy, and the pre-exponential factor D0, the frequency factor [20]. Diffusion Mechanisms Diffusion is said to take place by a vacancy mechanism if an atom on a normal lattice site jumps into an adjacent unoccupied lattice site. If an atom moves from an interstitial site to one of diffusion occurs movement, or its by jump, neighboring an of interstitial interstitial the atom sites, mechanism. involves a Such the a considerable distortion of the lattice, and this mechanism is probable only when the interstitial atom is smaller than the atoms on the normal lattice position [20]. jump becomes too probable, an interstitial neighbors If the distortion during the large to make on normal the interstitial atom .pushes lattice site one of into another mechanism its nearest interstitial position and itself occupies the lattice site of the displaced atom. 17 A variant of the interstitialcy mechanism is the crowdion[20] . In this case an extra atom is crowded •into a line of atoms and thereby displaces several atoms along the line from their equilibrium positions. High Temperature Oxidation of Metals High-temperature oxidation usually results in the formation of an oxide film. The mechanism of oxidation depends on the nature of the scale, that is, whether the oxide is solid or liquid or if it also partially evaporates. If solid scales are formed, the oxidation behavior also depends on whether the scales are compact or porous. Compact Oxide Scales A compact scale acts as a barrier separating the metal and the oxygen gas. The rate of oxidation at high temperatures is limited by diffusion through the compact scale, provided there is sufficient oxygen available at the oxide surface. The oxide grows in thickness leading to an increase in diffusion distance. This results in a decrease in the rate of reaction with time. Compact scales offer the best protective properties. Improving the protective properties of the oxide scale leads directly to an improvement in the oxidation resistance of metals and alloys [16]. Wagner [2,3] has provided a fundamental understanding of the essential features of high temperature oxidation of pure metals in his theory of high temperature parabolic oxidation. * 18 Figure I shows the Wagner schematics of concentration gradient of oxygen and metal ion vacancies and the transport processes occurring in an oxide scale containing such vacancies = The legend for Figure I is as follows: VHP" Vgq+ e e" M MqOp P represents metal ion vacancies represents oxygen ion vacancies represents electron holes represents electrons represents electrons represents the hypothetical metal oxide represents the functional dependence of V mP- on P0(d) g represents the functional dependence of V0q" on Pp(s) pQ<d) represents dissociation pressure of oxide P0^9) represents ambient oxygen partial pressure Wagner's theory applies to compact products. Volume corresponding point diffusion of defects) or the a scales of reaction reacting transport ions of (or electrons across the growing scale is assumed to be the rate-determining process of considered the to total migrate reaction. Electrons independently of and each ions other. are Since diffusion through the scale is rate-determining, reactions at phase boundaries are considered rapid, and it is assumed that thermodynamic equilibrium is established between the oxide and the oxygen gas at the M0/02 interface and between the metal and the oxide at the M/MO phase boundary [16]. The driving force of the reaction is the free-energy change associated with the formation of the oxide MO from the metal M and the oxygen gas. The partial pressure of oxygen at the M/MO interface is equal to the equilibrium dissociation 19 M 0? IyITl*•const fptojtf#* i» IyITI “ «n$t (pgp Metal Ion Vacancies [Va11+I - const f p $ -SPTi -[V0^+I= Censtfpa^ r Oxygen Ion Vacancies F i g u r e I, W a g n e r S c h e m a t i c s for O x i d a t i o n of Alloys 20 pressure of the oxide in contact with its met a l , p0(d), while at the oxide/oxygen interface it is equal to the oxygen pressure in the gas phase, P0^95• For an oxide scale with metal ion vacancies, the metal ions diffuse outward from the M/MO to the M/M02 interface. direction, The vacancies migrate in the opposite and their equilibrium concentrations at the gas phase interface are given by the defect equilibrium: When p0_ <9) > p0^d), the metal ion vacancies are continuously produced at interface. the MO/O2 interface Oxygen ion and vacancies opposite to the metal consumed migrate ion vacancies, in at the the M/MO direction and their equilibrium concentration at the M/MO and MO/O2 interfaces is given by: +?e-+-^-Og Oxygen ion vacancies are correspondingly created continuously at the M/MO interface and consumed at the M0/02 phase boundary. The rate of growth is, in these terms, determined by the gradients and the rate of diffusion of the components. These mechanisms lead to parabolic oxidation behavior. The Wagner theory permits an evaluation of the rate constant of high-temperature parabolic oxidation provided the diffusion coefficient is known. In evaluating experimental results the parabolic rate constant is expressed as 21 -AE=A dt x Here kp is the parabolic rate constant and x, the oxide thickness. On rearranging and integrating, JL X=Cfc 2 Porous Oxide Scales During compact oxide scale formation the rate of reaction is governed by the solid-state diffusion of the reactants through the scale, as long as sufficient oxygen is available at the oxide surface. Deviations from ideal behavior, i.e. compact and pore-free oxides, occur when porous scales form. If the transport occurs by an outward migration of metal ions by the vacancy mechanism, vacancies may collect to form cavities and pores at the metal/oxide interface and produce appreciable porosity in the oxide scale after extended reaction. The cavities then act as barriers to the solid-state diffusion process. These oxide scales can rupture and breakup becoming non-barriers to gaseous oxygen. Also when phase boundary processes become rate-determining instead of solidstate diffusion through the scale, then porous scales may be formed. When porous scales are formed, the kinetics of the reaction is commonly found to be linear with time. The rate of initial oxidation indicating the is often observed to decrease with formation of a protective phase before time the oxidation transforms to a linear rate. Phase boundary process 22 limitations occur when the linear oxidation for porous scales is faster than the protective oxidation rate. Cracks can form which rupture leading to the formation of porous scales. Thus porous scales are non—protective. These scales usually occur during later stages of the reaction because of rupture and fragmentation of the oxide scale after it has reached a critical thickness [16]. High Temperature Oxidation of Metal Alloys Oxidation mechanisms for alloys are more complex than for pure metals. The alloyed metal atoms do not diffuse at the same rates either in the oxide or alloy phase and the components of alloys have different affinities for oxygen. As a result, relative oxide amounts scales of on alloys the alloy do not contain constituents as the does same the metallic phase. As the oxidation proceeds, the composition and structure of oxide scales often change. kinetics Thus the oxidation often markedly deviate from ideal and simple rate equations. Also, if oxygen dissolves in the alloy phase, the least noble alloy component can form oxide inside the alloy. Since more than one oxide is formed, Wagner classified alloy oxidation in terms of different types of behavior. 1. S e l e c t i v e o x i d a t i o n in w h i c h t h e least n o b l e c o n s t i t u e n t is s e l e c t i v e l y or p r e f e r e n t i a l l y oxidized. 2. Formation of composite scales. 3. Formation of scales with complex oxides. 23 Under1 any set of conditions selective oxidation takes place only above a critical concentration of the active alloy component. Wagner [2,3] analyzed the conditions necessary for oxidation in expression extended to binary alloys this critical for the case of and derived a mathematical concentration. composite scales This and can scales be with complex oxides. Wagner considered an alloy A-B in which B is the less noble metal and A and B do not react to form a double oxide or spinel. Making the assumption that compact oxides are formed, three main cases for the oxidation of the alloy A-B may be considered. 1. At low concentrations of B, only the A oxide will be formed and B will diffuse into the alloy from the alloy/oxide interface. 2. For sufficiently high concentrations of B in the alloy only the B oxide will be formed and A will diffuse into the alloy from the alloy/oxide interface. 3. At B concentrations ranging from the low concentrations in case I to the high concentration in case 2, A oxide and the B oxide will simultaneously be formed (composite scale). Figure 2 shows the schematics for the three different oxidation cases. Assuming the formation of a compact, free oxide scale, Wagner showed that the pore- critical concentration N b (above which only the B oxide is formed) given by : is 24 U k r. V i T D whsire V is the molar- volume of the alloy t Zg is the valence of the B atoms, M0 is the atomic weight of oxygen, diffusion coefficient of B in the alloy, and D is the kp is the parabolic rate constant for the exclusive formation of the B oxide. The same type of assumptions can be made for composite scales that are practically insoluble in each other. For the case of formation of scales with complex oxides, diffusion rates are often appreciably smaller than in single oxides„ The protective scales on high-temperature oxidation-resistant alloys often consist of complex oxides (double oxides, spinels etc.) [16]. 25 A-B alloy A-B alloy A (A) DO "E B A A oxide B oxide 0,* (B) Diffusion Processes During Oxidation of A-B Alloys (A) Exclusive Formation of A Oxide (B) Selective Oxidation of B Oxide (C) Simultaneous Formation of A-Oxide (AO) and B Oxide (BO) B Oxide Grows According to the Displacement Reaction AO + B2+ = A2 + BO F i g u r e 2. W a g n e r S c h e m a t i c s f o r O x i d a t i o n o f M e t a l A l l o y s 26 CHAPTER 4 EXPERIMENTAL METHOD Auger Electron Spectroscopy Auger-electron spectroscopy(AES) is based on the Auger radiationless process, is [21] . The process shown in Figure energetics' 3. This of process the Auger involves an electron excitation, which leaves a hole in a core level of an atom. This preliminary excitation process can be stimulated by absorption of energy excitation process, from the recombination process. the core hole is a core primary hole electron. is filled by After an the Auger In the Auger recombination processes filled by an electron occupying a higher energy level, that is, either a shallower core electron or a valence electron. transferred to The another energy lost electron. by This this last receive enough energy to leave the system, electron electron is may thus becoming an Auger electron. The whole process, excitation plus Auger recombination, is usually notations labeled for the using initial the conventional states of the spectroscopic three electrons involved [22]. If the excitation involves a hole in a Is state and this hole is filled by an electron in the 2s state that transfers its energy to another electron in the 2s state, then the entire process is labeled KL1L2. In this notation the 27 Ee = Auger energy FL = Fermi Level F i g u r e 3. E n e r g e t i c s o f t h e A u g e r P r o c e s s 28 L valence states are denoted by the letter V. Thus the final energy of the Auger electrons is linked to the energies of the three electron states. Therefore the emission of Auger electrons at a given energy reveals the presence of certain energy levels characteristic in of the a system. given Since element, those levels are also reveals the it presence of that element in the system. This provides for the analytical capability of AES. The exact link between the kinetic energy of the emitted Auger electrons and the corelevel energies is complicated by factors such as electronic relaxation on formation of a core hole and final-state multiplet interactions. Nevertheless, the uncorrected binding energies of the three electrons are the most important factor in determining the Auger-electron kinetic energy. Neglecting all energies, factors except the uncorrected binding and calling these energies E1, E2 and E*3, for the first excited electron, the electron that fills the core hole, and the Auger electron, respectively, the kinetic energy of the latter can be written as: Ek = E*3 + E2 - E 1 This equation is derived by estimating the energy of the two-hole final states in two subsequent steps, one creating a hole in state 2 and the other creating a hole in state 3. The energies in this equation are measured from the zero of the kinetic-energy scale, that is, from the vacuum level. The asterisk in the binding energy term E*3 means that this is not 29 the unperturbed binding energy but rather the binding energy in the presence of another core hole. The Auger electrons [7] thus have unique energies for each atom and if the energy spectrum from about 0 to 2 keV is analyzed, the energies of the Auger electron peaks allow for I the identification of the surface elements present, hydrogen and helium. The reason that AES is a except surface- sensitive technique lies in the intense inelastic scattering that occurs for electrons in this energy range. Only Auger electrons from the top few atomic layers of a solid survive to be ejected and measured. An Auger electron spectroscopy ultra-high vacuum test system, excitation and an energy system consists of an an electron gun for specimen analyzer for detection of Auger electron peaks in the total secondary electron energy spectrum [2 1 ] . Experimental System Ultra-High Vacuum Systems A UHV system is required for AES for two reasons. First and foremost, meet as the electrons emitted from a specimen should few gas molecules on their way to the analyzer as possible so that they are not scattered [23] . More importantly the reduction of contamination on the surfaces under analysis by the residual gases in the vacuum establishes a necessary base pressure of about I x io"9 torr (I torr= I mm. Hg 30 pressure). Such a pressure falls into the regime of ultra-high vacuum (UHV). This greatly restricts the use of materials in AES. For the system used in the present AES study most materials used in fabrication are stainless steel with copper gaskets used as a sealing material between conflat flanges [7] . The system assembly including the two turbomolecular pumps, the electron gun, the ion gun and the vacuum chamber is shown in Figure sections, 4. a main The vacuum chamber is divided section and a differential into two section. The turbomolecular pumps differentially pump the ion gun as well as differentially pump a vacuum seal on the sample manipulator in the main chamber. Pumping speed is increased by using separate pumps on the two chambers. The two pumping systems each include a roughing pump and a turbomolecular pump. They reduce the main chamber and differential pressures of about 1.5 x IO'9 and I x after bakeout. The bakeout involves io ‘9 chamber to base torr, respectively, increasing the system temperature to about ISO0C for a few hours in order to remove most of the volatile contaminants. Ion Gun Argon ion bombardment is a method of producing a clean surface and can be used in conjunction with surface analysis to measure compositional information as a function of depth [24]. Depth simultaneous profiling ion is a bombardment and technique analysis which involves (AES analysis in 31 1. Sample Probe 2. Sample Mount 3. Main Chamber 4. Ion Gun 5. CMA & Electron Gun 6. CMA Control Hookup 7. Turbo Pump (Main Chamber) 8. Roughing line (Main Chamber) 9. Turbo Pump (Differential Chamber) 10. Roughing line (Differential Chamber) 11. Argon Supply line 12. Leak Valve 13. Butterfly Valve 14. Differential Pumping line 15. Vacuum Seal Pumping line F i g u r e 4. A E S A n a l y t i c a l E q u i p m e n t 32 this case) to develop a continuous compositional profile. This technique involves the use of an argon ion gun. The ion gun is a V.G. Scientific electron devices impact source. dual Ion excitation with which positive are emitted ion guns in which the inert gas collisional energy FAB61 atom are ions gun simple which has an electrostatic (Ar+) are generated by electrons of typically 100 eV from a hot tungsten filament. The ions are accelerated, focused and rastered on the sample, creating a sputtered area [7]. The primary Ar+ ions are produced from 99.9995% minimum purity argon gas introduced in the differential pumping line. These ions electronic negotiate fields energy beam. an array of static and leave the gun. in a The primary beam and oscillating columated, is rastored to high scan an area larger than the cross sectional area of the primary ion beam. The FAB61 ion gun is controlled by a V.G. Scientific 400A power supply. A Leybold-Heraeus 867 916 raster power supply controls restoring of the primary ion beam. The energy of the primary ion beam used is generally 3.0 keV with a ion gun target current of about 950 nanoamps. The target current is controlled by manually adjusting the ion gun emission current. Sample Mount System Samples, both thin foil metals and thick intermetallics, are mounted on a sample holder, mounted on the end of a stainless steel rod in the vacuum chamber. A diagram of the sample holder is shown in Figure 5. It has provision for 1. SCREWS TO HOLD SAMPLES 2. SCREWS TO HOLD MOUNT ON CLAMPS 3. CLEARENCE FOR SCREWS 4. TOP VIEW 5. SIDE VIEW F i g u r e 5, S a m p l e H o l d e r f o r A E S A n a l y s i s 34 holding five samples of about I cm x I cm dimensions each including a LiF sample which is used for system alignment. Two micrometers connected to the support rod establish its forward-backward and side-to-side position. Provision is also made for rotational and z-directional motion. holder is grounded through a current meter. The sample This is done to prevent sample charging during the argon ion etching process the Auger analysis and also to monitor the target current. The relative spatial orientation of the samples and analytical equipment is critical. Figure 6 shows the relative orientation of the sample mount, electron gun and ion gun. The plane of the test sample surfaces is generally at an angle of about 45° to longitudinal axis of both the Ar+ ion beam and the electron gun, which have a 9O0 angle relative to one another. During analysis the sample surface is about 10 mm from the front end of the ion gun and about 8 mm from the end of the electron gun. A lithium fluoride foil is mounted on the sample holder to facilitate alignment of the samples in the primary Auger electron beam and the ion beam. This foil emits a brilliant red glow when sputtered. The lithium fluoride target foil is aligned relative to the ion gun by adjusting the probe position while observing the brilliant red spot at the point of impact of the ion beam. For this step the primary ion beam is static rather than rastored. 35 8mm 10 mm 1. Ion Gun 2. CMA 3. Rotatable Sample Probe 4. Sample Mount F i g u r e 6. R e l a t i v e O r i e n t a t i o n o f S a m p l e M o u n t w i t h Ion Gun an d E l e c t r o n Gun 36 The spot size of the primary ion beam, and the dimensions of the area sputtered are adjusted with the controls on the gun power supply and raster power supply while observing the sputter induced phosphorescence on the lithium fluoride coated target foil. The sputter area is adjusted to about 4mm x 4mm. The primary ion beam spot size is between 0.5 and Imm in dia. Energy Analyzer The energy analyzer used for the present study is the PHI Model 10-155 designed to excited by Cylindrical-Mirror detect an Auger Analyzer electrons electron beam. (CMA) ejected The primary which from is specimens electron beam is generated by an electrostatic electron gun mounted coaxially inside the analyzer. The analyzer also contains an electron multiplier which amplifies the detected secondary electron signals. The electron gun is controlled by the PHI Model 11-010 Electron Gun calibrated Control. steps of 500 Beam V voltages from 0 to are available 5 keV. The in filament current and emission voltage of the electron gun and the focus of the electron gun are adjustable. The electron gun is operated with a primary beam voltage of 3 keV for most of the tests, with a filament current of and 2 keV for other tests, about I milliamp. The target current on the sample is normally about 4000 nanoamps. The electron gun and CMA arrangement are shown in Figure 7. The electron gun has one electrostatic lens. Beam current --- OUTER \CYLINDER ELECTRON MULTIPLIER 0-4 kV !— MAGNETIC s h ie l d MODULATION CONTROL Figure 7 The E l e c t r o n Gun and CMA A r r a n g e m e n t 38 is varied by adjusting extraction voltage the filament temperature (V1 - beam voltage)„ A focused and beam the of primary electrons is obtained from the gun when the ratio of focus voltage (V2 - beam voltage) to the beam voltage is nominally 0.25. Secondary electrons electron beam are strikes generated the at specimen. ^-nc-*-u<^es an inner cylinder that is grounded, the point The the analyzer plus an outer cylinder that is biased through terminal Vm. Negative voltages applied to the outer cylinder repel the secondary electrons approaching the cylinder through openings in the side of the inner cylinder, forcing these electrons back through other openings in the inner cylinder so that they are collected by the electron- multiplier. The number of resulting electrons is multiplied, prior to striking the collector plate, by applying a voltage bias of a few kiloelectron volts to the multiplier. The energy analysis of the secondary electrdns is controlled digitally through a PHI 32-150 Digital AES Control and a 96 V/f Preamplifier. The signal from the analyzer passes through the preamplifier and the Digital AES Control which is connected to an IBM PC AT. Sample Preparation The intermetallie test samples used in this study were prepared by the argon arc melting of the appropriate amounts of the pure metal powders at the Idaho National Laboratory 39 Facility at EG&G,Inc. The samples are cut and polished to a final finish of 0.05 microns. The pure metal samples are cut from research grade foils. The pure zirconium metal samples are cut from 99.99% pure, 25 mm thick foil purchased from Johnson Mathey Inc. The pure Ni samples are cut from high purity nickel obtained from the Physics Department, Montana State University. Surface Preparation Prior to oxidation the intermetal^ic samples are polished to a high lustre. This is accomplished using a motor driven polishing wheel with the abrasive being a 0.05 micron gamma alumina number 3 suspended in distilled water. The samples are mounted on small aluminum blocks with a hot melt adhesive for convenience following during each polishing. oxidation Polishing and analysis to a cycle high lustre is assumed to remove the prior oxide scale to expose fresh bulk material. Before oxidation the intermetallics are rinsed in bulk grade acetone to dissolve the hot melt adhesive. The samples are then cleaned with bulk grade methanol. The pure zirconium and pure nickel samples are acid etched prior to oxidation with a 5% hydrofluoric acid solution to produce a clean and reproducible surfaces. The reason for this is their thickness and lack of flatness makes polishing impractical. The acid solution is prepared fresh for each etching. The samples are immersed in the acid solution for 15 40 seconds and are then rinsed in distilled water. This produces a high metallic lustre on the samples. Each sample is oxidized in air at SOO0C for I hour. The oxidation is accomplished in a small metallurgical oven. The temperature control and display of the oven were calibrated prior to its use. For each run the oven is brought up to the required temperature before introducing the samples. The temperature drop caused by opening the oven door to introduce the samples was observed to be negligible. Sample Alignment A sample is loaded into the system and the system is pumped down to a pressure of at least 2 x lb"9 torr prior to aligning the samples. The current meter is activated, before the electron or ion gun are operated, to ensure the sample mount is grounded. The electron beam target current is set as desired. The LiF sample is used to adjust the sample position. The electron beam and the ion beam impact location are brought close to each other by observing their characteristic spots, while adjusting the probe position. The elastic peak procedure is run on the LiF sample to ensure that the elastic peak is at 2000 eV. The other samples are aligned by adjusting the probe position to ensure the elastic peak is at 2000 eV. 41 Elastic Peak Procedure The electron gun control is activated and the voltage adjusted to 2 k e V . The electron beam current is set as desired. The multiplier supply is adjusted to obtain an energy trace of the secondary electrons on a CRT display, case a IBM PC AT. manipulator electron until gun The x, y and z-axis the peak focus is is aligned adjusted to in this is adjusted on the at 2 keV. maximize The n ■ the the signal intensity at 2000 volts. Acquiring AES Data The AES data is acquired by setting the energy sweep range, time per sweep and number of sweeps. The counts and the multiplier voltage for each survey as well as time between surveys are recorded. The data is then acquired and stored in a .DAT file on the IBM PC AT for further mathematical manipulation such as smoothing, differentiation, multiplexing at a later time. Shut Down Procedure Once the desired number of surveys have been taken, the ion gun power supply is shut do w n . This is followed by switching off the Electron Gun Control, Digital AES Control, and the Electron Multiplier Supply. 42 CHAPTER 5 RESULTS The Auger zirconium spectrum foil which from had 50 been to 550 exposed eV of to unsputtered air at room temperature is shown in Figure 8. The ordinate in the spectrum is the count rate, a measure of the intensity of the secondary electrons, in k counts/sec. The count rate at each energy is the sum of the offset value shown plus the multiple of the ordinate value times the scale factor specified on the figure. Thus an absolute value of 2 on the ordinate in Figure 8 represents 19.860 kcts/sec (2 x 2.800 + 14.260), for example. The survey shows oxygen and carbon auger peaks at about 505 eV and 270 eV, respectively. Small zirconium peaks are observed in the energy range from 80 to 180 eV. Figure 9 shows an Auger survey of the same zirconium foil after 40 minutes of argon ion sputtering. This survey shows strong zirconium peaks and significantly diminished carbon and oxygen peaks. The energy range between 80 and 180 eV from the survey shown in Figure 9 is expanded and displayed in Figure 10. The most important peaks for elemental Zr are the MNN peaks at 90 eV and 115 eV, MNV peaks at 123 eV and 145 eV and an M W at 172 eV. The Auger peaks used to establish Zr peak surface abundance and oxidation state in the present study are those at 90 eV and 145 eV which are designated as the Zrl and Zr2 2.800 K cts/sec Offset= 14.260 K cts/sec Count Rate, arbitrary units Scale factor= 50.0 100.0 150.0 Figure 200.0 250.0 300.0 Kinetic Energy, eV 8. 350.0 AES Sur v ey o f Z i r c o n i u m F o i l 400.0 450.0 500.0 550.0 Count Rate, arbitrary units 250 F i g u r e 9. AES Sur v e y o f S p u t t e r HOO .0 Cl eaned Z i r c o n i u m 450.0 500.0 550 . Count Rate, arbitrary units 80 .0 90.0 100.0 Figure 130.0 Kinetic Energy, eV 110.0 10. 120.0 140.0 iso.o iso .0 170.0 Expanded Ener gy Regi on o f S p u t t e r Cl eaned Z i r c o n i u m 180.0 46 peaks, respectively. The Auger surveys shown in Figures 8 and 9 have too broad an energy range of display to be used accurately in the determination of Zr Auger peak intensities. The Auger spectra are therefore expanded to smaller energy regions to provide a better resolution of the elemental Zr surface abundance from the peak intensities measured by the procedure described below. Figures 11 and 12 show the multiplexed surveys of the Zr2 peak on oxidized respectively. and sputter cleaned zirconium foil, On sputtering away the oxide layer a shift in the Zr2 peak position from 140 eV to 145 eV is noticed. This energy shift of the peak results from a change in the chemical state of the metal. The Zr2 peak is useful in indicating the oxidation state of zirconium and cannot be conveniently used in quantitative Auger analysis of Zr surface abundance. The MNN Zrl peak does not shift significantly when the zirconium is oxidized and therefore it can be reliably used for peak intensity measurements, which are proportional to Zr surface abundance. A display of the multiplexed Zrl peak from 70 to H O eV on sputter cleaned Zr foil (from Figure 9) is shown in Figure 13. The Zrl peak for this survey is at 90 eV. The count rate measured at the peak energy is 1901.200/sec and the base count rate, which is the count at the high energy base of the peak at 99 eV is 1693.629/sec. The peak height, the difference of the two, is 207.571/sec. This difference is divided into the 0.202 K cts/sec Count Rate, arbitrary units Scale factor = 120.0 128.0 Figure 132.0 136.0 ItO .0 Kinetic Energy, eV 11. Multiplexed 148.0 152.0 Zr2 Peak on Z i r c o n i u m F o i l 156.0 160 . actor = Count Rate, arbitrary units Scale 120.0 124.0 128.0 Figure 12. 132.0 140.0 Kinetic Energy, eV M ultiplexed 144.0 152.0 Zr2 Peak on S p u t t e r Cl eaned Z i r c o n i u m 160 . Count Rate, arbitrary units 70.0 78.0 Figure 13. 82.0 86.0 Kinetic Energy Multiplexed Zrl 90.0 98.0 102.0 106 .0 Peak on S p u t t e r Cl eaned Z i r c o n i u m 110.0 50 base count of 1693.629 to give a relative intensity of 0.1226 foT the Zrl peak in this spectrum. Using the same procedure the relative intensity for the Zrl peak for zirconium foil exposed to air from Figure 8 is 0.0311. A display of the oxygen Auger peak at 506 eV on oxidized zirconium foil is shown in Figure 14. The relative intensity for the oxygen peak at 506 eV is 0.1456. The relative intensities of the oxygen peak and Zrl peak at different sputter times for oxidized Zr foil are shown in Figure 15 as a function of sputter time. This constitutes the sputter depth temperature. profile The for zirconium oxidized at Zrl peak intensity increases with time while that of oxygen decreases. room sputter This indicates a slow sputtering of the oxide layer. The sputter depth profile of zirconium foil oxidized at 3OO0C for I hour is shown in Figure 16. The oxide layer in this case takes longer to sputter in comparison to Zr foil exposed to air. similar trends The to oxygen those of and Zrl peak the room intensities temperature show oxidized zirconium foil in Figure 15. The Auger spectrum from 3 0 to 930 eV for nickel foil which had been exposed to air at room temperature is shown in Figure 17. The survey shows carbon and oxygen peaks at about 270 eV and 5 05 eV, respectively. Weak nickel peaks are displayed at about 55 eV, 708 ev,. 775 eV and 840 eV. The 55 eV and 840 eV peaks are designated in this report as Nil and N i 2 , Scale factor Offset 4*6.0 510.0 Kinetic Energy Figure 14. 516.0 522.0 M u l t i p l e x e d Oxygen Peak on Z i r c o n i u m 534.0 Zr 1 int. Relative Intensity Ox int. 0.00 5.00 10.00 Figure 15. 15.00 20.00 25.00 30.00 35.00 Sputter Time (minutes) Sputter Depth P r o f i l e for Zr 40.00 Zr 1 int. Relative Intensity Ox int. 20.00 40.00 60.00 80.00 100.00 Sputter Time (minutes) Figure 16. S p u t t e r Depth P r o f i l e f o r Zr(ox) 120.00 Count Rate, arbitrary units 30 .O 120 .0 300.0 390.0 Kinetic Energy 210.0 Figure 17. 480.0 AES Sur v ey o f N i c k e l 570.0 Foil 750.0 840.0 930.0 55 respectively. The Auger spectrum of the same nickel foil after 10 minutes of argon ion sputtering is shown in Figure 18. The carbon peak is significantly diminished with an increase in the intensity of the nickel peaks. The Nil peak from Figure 18 is expanded between 45 and 75 eV and displayed in Figure 19. The relative intensity for this peak is 0.3770 from the peak intensity at 56 eV and the background intensity at 74 eV. The Ni2 peak on sputter cleaned Ni foil is shown in Figure 20 in the energy range between 825 and 870 e V . The relative intensity for this peak is 0.1099 based on the peak intensity at 840 eV and the background intensity at 867 eV. The relative peak intensities for the Nil, Ni2 and oxygen peaks for the room temperature exposed nickel foil at different sputter times are shown in Figure 21. This sputter depth profile shows an increase in nickel peak intensities and a decrease in the oxygen peak intensity with increase in sputter time. The sputter depth profile for the nickel foil oxidized at 300°C for I hour is shown in Figure 22. The profile shows a similar trend of peak intensities with sputter time. The decrease in the oxygen peak intensity is not clearly shown on the scale of these figures. The sputter depth profile for the oxygen, Zrl, Nil and Ni2 peaks for the intermetallic ZrNi5 after exposure to air is shown in Figure 23. With increase in sputter time, in the Nil, Ni2 and Zrl increases peak intensities are observed. The Count Rate, arbitrary units Scale factor= 30.0 120.0 210.0 300.0 480.0 570.0 Kinetic Energy, eV Figure 13. AES Sur v ey o f S p u t t e r Cl eaned N i c k e l 750.0 9 3 0 .0 Offset = 30.373 K cts/sec Count Rate, arbitrary units Scale factor = HS.O H S .0 S I .0 S H .0 57.0 60.0 63.0 66.0 63.0 Kinetic Energy, eV Figure 19. M u l t i p l e x e d Ni I Peak on S p u t t e r Cl eaned N i c k e l 72.0 75 Count Rate, arbitrary units 825.0 843.0 847.5 Kinetic Energy, eV F i g u r e 20. M u l t i p l e x e d N i 2 Peak on S p u t t e r Cl eaned N i c k e l 870.0 Ox int. Relative Iiitensity Nil int. Ni2 int. 0.00 1.00 2.00 3.00 4.00 5.00 6.00 7.00 8.00 9.00 10.00 Sputter Time (minutes) F i g u r e 21. Sputter Depth P r o f i l e f o r Ni Ox int. Relative Intensity Nil int. Ni2 int. 0.00 2.00 4.00 6.00 8.00 10.00 12.00 Sputter Time (minutes) F i g u r e 22. Sputter Depth P r o f i l e 14.00 f o r N i (ox) 16.00 Zr 1 int. Relative Intensity Ox int. Nil int. Ni2 int. 10.00 15.00 20.00 25.00 Sputter Time (minutes) F i g u r e 23. Sputter Depth P r o f i l e for Zr Ni S 30.00 62 sputter depth profiles for air exposed Zr2Ni7, ZrNi3 and ZrNi are shown in Figures 24, 25 and 26, respectively. These exhibit a similar trend to ZrNi5 in Figure 23. The intermetallies ZrNi5 and ZrNi3 were oxidized at 3OO0C for I hour. oxidized The sputter intermetallics depth is profiles shown in for these Figures 27 surface and 28, respectively. The peak intensities after removal of the oxide layers are different than those of the respective sputter cleaned room temperature oxidized intermetallics. The steady state Zrl peak intensity is almost halved, while an almost order of magnitude difference is observed in the case of Nil and Ni2 peak intensities. used for Auger spectrum The primary electron beam energy of the intermetallics oxidized at 300°C is 2 keV while that used for the other samples analyzed is 3 keV. Zr 1 int. Relative Intensity Ox int. Nil int. Ni2 int. 0.00 1.00 2.00 3.00 4.00 5.00 6.00 7.00 8.00 9.00 10.00 Sputter Time (minutes) F i g u r e 24. Sputter Depth P r o f i l e for ZrZNi7 Zrl int. Relative Intensity Ox ini. Nil int. Ni2 int. 0.00 5.00 10.00 15.00 20.00 25.00 30.00 Sputter Time (minutes) F i g u r e 25. Sputter Depth P r o f i l e f o r Zr Ni S 35.00 Zr 1 int. Relative Intensity Ox inf. Nil int. Ni2 int. 0.00 5.00 10.00 15.00 20.00 25.00 30.00 Sputter Time (minutes) F i g u r e 26. Sputter Depth P r o f i l e for Zr Ni 35.00 LLUib Zr 1 ini. Relative Intensity Ox ini. 0.025 Nil ini. Ni2 ini. 0.015 0.005 10.00 F i g u r e 27. 20.00 30.00 40.00 Sputter Time (minutes) Sputter Depth P r o f i l e 50.00 f o r Zr Ni 5 ( o x ) 60.00 0.045 Zr 1 inf. Relative Intensity 0.035 Ox inf. Nil inf. 0.025 Ni2 inf. 0.015 0.005 0.00 10.00 20.00 30.00 40.00 50.00 60.00 Sputter Time (minutes) F i g u r e 28. Sputter Depth P r o f i l e for Z r N i 3( o x ) 70.00 68 CHAPTER 6 INTERPRETATION The sputter depth profiles shown in chapter 5 indicate the time required to sputter the surface oxide layers. The oxide layers are formed at two different temperatures a) room temperature and b) heating at SOO0C for I hour. The sputter depth profile for room, temperature oxidized zirconium is shown in Figure 15. The total sputter time to remove the oxide layer is between thirty and forty minutes. The first three minutes of sputtering is characterized by a steady removal of surface carbon. The carbon is either deposited on the surface due to handling prior to insertion in the analysis system or as a result of outgassing from the chamber walls during the bakeout of the vacuum system. The Zrl peak intensity increases rapidly at the start of sputtering attaining a steady state value of about 0.12 after 3 minutes. The oxygen peak intensity starts decreasing steadily after three minutes of sputtering reaching a minimum of about 0.04 after 30 to 40 minutes of sputtering. This indicates the presence of some residual oxygen on the surface even after long sputter times. The sputter depth profile for zirconium foil oxidized at 300°C is shown consistent Zrl in Figure relative 16. The intensity profile of shows about 0.06 an almost after 85 minutes of sputtering. The oxygen intensity up to this point 69 steadily decreases. There is a increase ' in the Zrl peak intensity between 85 and 95 minutes of sputtering, indicating the change from an oxidized zirconium surface to a sputter cleaned surface. The longer sputter times observed in Figure 16 indicate a thicker surface oxide layer in comparison to that in Figure temperatures, in 15. This this case shows . that 3 OO0C, higher induce the oxidation formation of thicker oxide layers. In previous studies [11] it has been shown that lower temperatures of oxidation leads to dissociative chemisorption of oxygen on zirconium and formation of various suboxides. The suboxides formed are converted to ZrO2 at higher temperatures of oxygen exposure. oxidized at The longer sputter times 3OO0C can be attributed to the for zirconium formation of a thick ZrO2 layer on the zirconium surface. The sputter depth profile for room temperature oxidized nickel is shown in intensity profiles Figure 21. The for the Nil, figure shows relative Ni2. and oxygen peaks. The sputter time required for the three profiles to attain steady state intensities is about 3 minutes. The Nil and Ni2 peaks increase with sputter time with a decrease in the oxygen peak intensity. The sputter depth profile for nickel oxidized at 3OO0C is shown in Figure 22. The sputter time for the three profiles to attain steady state intensity values is about 10 to 14 minutes indicating temperature oxidation. thicker oxide layer due to high 70 Earlier studies the Nil Auger [15] on oxidized nickel signal attenuates more during the depth profiling of the indicated that than the surfaces Ni2 signal of both single metal foils and intermetallics. The sampling depth of the Ni2 Auger signal is about three times that of the Nil signal [25], rendering the latter much more sensitive to changes in surface Ni atomic Figures abundance. 21 and 22 The sputter indicate depth that the profiles Nil and shown Ni2 in signal intensities increase with increase in sputter depths, but the Nil peak intensity increases by a greater factor. The sputter oxidized Zr-Ni depth profiles intermetallics, for the room temperature ZrNi5, Zr2Ni7, ZrNi3 and ZrNi are shown in Figures 23, 24, 25 and 26, respectively. The Nil, Ni2 and Zrl peak intensities increase with sputter time in all four cases. There is a transition from an oxide layer on the intermetallics to a sputter cleaned surface for sputter times of between 7 and 20 minutes for ZrNi3, 8 and 15 minutes for ZrNi5, 12 and 25 minutes Zr2Ni7. Prior to this for ZrNi the and 3 and 6 minutes surface of the for intermetallics contains oxides of nickel and zirconium. Argon ion sputtering leads to the removal of the oxide layers and a transition to higher relative intensities for the Nil, Ni2 and Zrl peaks and a diminishing of the oxygen peak intensity. The different intensity room profile data temperature of the exposed Zrl metal peak for foils the and intermetallics after sputtering to steady state intensities 71 are as shown in Table I. The Zrl peak intensity increases with increase in atomic fraction of Zr. The Zrl peak intensity decreases from 0.1226 for pure Zr to 0.0549 for ZrNi with an atomic fraction of 0.5 Zr and to 0.0259 for ZrNi5 with an atomic fraction of 0.167 Zr. Thus a reduction in the atomic fraction of Zr in the sample reduces the Zrl peak intensity proportionally. Though this correlation is not followed as closely in the case of ZrNi3 and Zr2Ni7, within experimental tolerance limits this provides a rough indication of the change in the relative Zrl peak intensity with atomic fraction of Zr. This intensity profile for the Zrl peak intensity is shown in Figure 29. Table I. Steady State Intensity Profile Data of Zrl peak for the metal and intermetallic samples analyzed. NAME OF SAMPLE ATOMIC FRACTION OF ZIRCONIUM STEADY STATE INTENSITY OF ZRl PEAK Ni 0 0 ZrNis 0.167 0.0259 Zr2Ni7 0.222 0.0389 ZrNi7 0.25 0.0403 ZrNi 0.5 0.0549 Zr 1.0 0.1226 The intensity profile data of Nil and Ni2 peaks for the room temperature exposed metal foil and intermetallic samples after sputtering to steady state intensities are shown in Table 2. A correlation of the type discussed for the Zrl peak intensity is not as clear for the Nil and Ni2 peak intensities. A t o m i c fraction of Zirconium. Zr 1 ini. Zr2Ni7 ZrNiS 0 0.02 0.04 0.06 0.08 0.1 0.12 0.14 Relative Intensity F i g u r e 29. St e a d y S t a t e Intensity P rofile f o r Zr 73 although the Nil and Ni2 peak intensities increase with atomic fraction of Figure 30. Figures 27 and 28 show the sputter depth profiles for ZrNi5 and Ni. These ZrNi3 oxidized results at are plotted 300°C, in respectively. The total sputter time for the Zrl, Nil and Ni2 peaks to attain steady state intensities is about 45 minutes in both cases. Table 2. Steady State Intensity Profile of Nil and Ni2 peaks _________ for the metal and intermetallic samples analyzed. NAME OF SAMPLE ATOMIC FRACTION OF NICKEL Nil PEAK INTENSITY Ni2 PEAK INTENSITY Zr 0 0 0 ZrNi 0.5 0.0769 0.0485 ZrNi7 0.75 0.2988 0.0929 Zr7Ni7 0.777 0.3237 0.0989 ZrNi7 0.833 0.3521 0.0998 Ni 1.0 0.385 0.1136 On comparing temperature the oxidized sputter ZrNi3 to depth that profiles for high for room temperature oxidized ZrNi3, the final steady state Zrl, Nil and Ni2 peak intensities are reduced from about 0.046, 0.3 and 0.09 to about 0.024, 0.035 and 0.0195, respectively. The primary beam energy used for the metal foils and intermetallics oxidized at room temperature and the pure metal foils oxidized at 300°C was 3 keV. Excessive background noise in the Auger spectrums while operating the electron gun at this energy prompted a change in beam energy to 2 keV for the intermetallics oxidized at 3 00 °C . This change in operating conditions resulted in A t o m i c Fraction of Ni Ni I int. Ni2 int. 0.833 Zr2Ni7 0.777 0.05 0.1 0.15 0.2 0.25 0.3 0.35 Relative Intensity Figure 30. S t ea dy S t a t e Intensity P rofile f o r Ni 0.4 75 a significant reduction in the background noise and background intensities. The software adopted for determining the peak intensities was not normalized for changes in the operating conditions which resulted in a significant drop in the observed peak intensities and hence the reduction in the Z r l , Nil and Ni2 peak intensitiy values, as noted above. This reduction in the peak intensities may also be partially attributed to cracks developed on the intermetallic surfaces which are laterally oxidized during high temperature oxygen exposure. An optical microscope photograph of the ZrNi3 surface after oxidation at 3OO0C and polishing Figure 31. The photograph shows surface. The darker portions a lateral removed oxide of layer extending is shown in a crack running along the the photograph indicates from a crack which is not after long polishing or sputtering times. The steady state relative peak intensities for oxygen for ZrNi3 exposed 0.0101, to air and respectively. oxidized at 3OO0C are 0.0031 and The relative degree of oxidation of a metal alloy can be estimated from the ratio of the oxygen peak intensity to the intensity of the major metal peaks. Since Ni is the major metallic component in the high temperature oxidized intermetallics, the Nil peak intensity is used here for the oxygen to metal peak intensity ratio analysis. This ratio of the oxygen and Nil steady state peak intensities, for ZrNi3 at the oxidizing conditions listed above are 0.0104 and 0.2837, respectively. There is thus an increase in the degree F i g u r e 31. A n O p t i c a l M i c r o s c o p e P h o t o g r a p h o f P o l i s h e d Z r N i 3 a f t e r O x i d a t i o n at S O O 0 C 77 of oxidation after high temperature oxidation and extensive sP^ttering, probably due to oxidized surface cracks. Regardless of the length of sputtering the presence of oxygen in the oxidized crack surface diminishes the Z rl, Nil and Ni2 peak intensities and increases the oxygen peak intensity. Under high temperature conditions, it is known that bulk Zr can dissolve interstitial Zr/Ni up to 28 atomic percent solute in its hep lattice alloys also, therefore, oxygen [14]. as an The untreated probably have absorbed some oxygen in the process of their being prepared, which can lead to an attenuation of the Zrl, Nil and Ni2 peak intensities. Surface roughness before oxidation may have varied because of slight differences in the way the samples were polished. Contaminants may have found their way to the surface before oxidation and affected the development of the surface oxide layer. The surface contaminants could also cause a diminished peak intensity after high temperature oxidation. The sputter time required to remove the oxide layers, formed at both room temperature and at 3OO0C, for all the samples analyzed is shown in Table 3. Except in the case of the Zr foil, this value of sputter time was evaluated as the time taken to attain 8 0% of the steady state intensity. The Nil profiles are used because cases they show a sharp transition Nil peak in almost all from a surface with an absorbed oxide layer to a sputter cleaned surface. For the room temperature oxidized ZrNi3 the Nil steady state peak 78 intensity is 0.2988, 80% of which is about 0.24. This indicates a sputter time of about 7 minutes from the sputter depth profile in Figure 25. Since pure Zr does not contain any Ni, the time taken to attain 80% of the final Zrl peak intensity is chosen as the sputter time. In the case of room temperature oxidized zirconium foil the sputter time is about 3 minutes. Table 3. The sputter time required to remove the oxide layer __________for the metal and intermetallic samples. SAMPLE NAME SAMPLE TYPE/TYPE OF OXIDATION1" TIME FOR SPUTTERING THE OXIDE LAYER Zr METAL FOIL/R.T. 3 Zr,0 METAL FOIL/H.T. 90 MINUTES Ni METAL FOIL/R.T. 2 MINUTES NiO METAL FOIL/H.T. 6 MINUTES ZrNis INTERMETALLIC/R.T . 6 MINUTES ZrNis(ox) * INTERMETALLIC/H.T . 39 MINUTES ZrpNi7 INTERMETALLIC/R.T . 2 MINUTES ZrNix INTERMETALLIC/R.T . 7 MINUTES ZrNix (ox) * INTERMETALLIC/H.T . 25 MINUTES MINUTES ZrNi INTERMETALLIC/R.T . 9 MINUTES " R.T. = ROOM TEMPERATURE ;H .T . = HIGH TEMPERATURE (300°C/lhr.) t BEAM ENERGY = 2 keV The sputter depth profiles for the pure metal Zr and Ni foils shown in Figures 15 and 22, respectively indicate the relative depth of the high temperature oxide layers formed. Since the sputtering conditions were consistent for these surfaces, and since the oxides should sputter at approximately the same rate [27], this indicates a thicker ZrO2 layer (90 79 Iflirvute sputter time) nickel relative to the oxide layer formed on (4 minute sputter time)„ 80 CHAPTER 7 SUMMARY AND CONCLUSIONS The objectives of this research included the installation and set-up of development of control data and the PHI relevant Auger electron software analysis spectroscope for both together with digital the study and process of the surface compositions of the oxidized intermetallic compounds of zirconium and nickel including ZrNi3, ZrNi, ZrNi5 and Zr2Ni7 and oxidized zirconium and nickel foils. The significant findings of this investigation are as follows: 1) Since the operating conditions were maintained constant during the sputtering of the' oxide layers formed on the metal foils at 3OO0C, this indicates a thicker oxide layer on Zr layer than the oxide layer on nickel. 2) The nickel and zirconium concentrations in both metal foils and intermetallics increased with sputter time, regardless of the oxidation temperature, with a subsequent decrease in the oxygen concentration. 3) The sputter depth profiles of the intermetallics are consistent with those of similar investigations in literature [14,15]. There is a discrepancy in the sputter depth profiles of the oxidized intermetallics (3OO0C) with recent findings. As reported in chapter 7 this could be due to a variety of reasons such as differences in operating conditions, oxidized 81 surface cracks and also surface contamination during polishing. 4) The Nil peak intensity diminished by almost an order of magnitude on oxidizing the intermetallics at SOO0C in comparison to the room temperature oxidized intermetallics„ This is a direct result of changing the operating conditions from 3 keV to 2 keV which caused a change in the background intensity. The software developed to calculate the relative peak intensities is not equipped to normalize for such large changes in operating conditions. 5) Since the temperature, surface outlined. samples i.e. oxidation SOO0C, were an oxidized improved characteristics only at one understanding cannot be of high the accurately 82 CHAPTER 8 RECOMMENDATIONS FOR FURTHER RESEARCH Based on the results of this experimental work the following recommendations are made: 1) Develop information zirconium and nickel work using method Seat's relates on the concentrations of from the results of this experimental quantitative the depth surface Auger region method mole [26]. fractions Seat's of two components to their Auger signal strength. This can be used to evaluate the surface atomic ratios of the two components which provides a measure of the surface concentrations of the two components. 2) Maintain constant operating conditions during an investigation of this nature so that the results of different depth profiles are directly comparable. This would require the elimination of the background noise developed in the system. The background noise can be eliminated by ensuring that the electronics in the power supplies connected to the Cylindrical-Mirror Analyzer is performing satisfactorily. This was beyond the scope of the present investigation but maintaining constant operating conditions would require the rectification of this problem before further research is undertaken. 3) Perform Auger analysis of the intermetallics of zirconium 83 with t i n , chromium, and iron to develop the basis for an improved understanding of the zircaloys over a wide range of compositions, temperatures and extents of oxygen exposures. 4) Estimate the thickness of the oxide layers which can be related to the rate of formation of these layers to give a better understanding of the kinetics of the development of the surface strata during oxygen exposure. 84 REFERENCES 1) Deibert, M.C., "A study of Surface Oxidation Reactions on the Intermetallic Compounds of Zirconium", Proposal submitted to the N S F , 1988. 2) Wagner, Carl, "Theoretical Analysis of Processes Determining the Oxidation Rate Electrochem S o c .. 99 (10) (1952) 369 - 380. the Diffusion of Alloys",j. 3) Wagner, Carl, "Formation of Composite Scales Consisting of Oxides of Different Metals".J. 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