.,.x.:.:.x.:.::::::::.:.::::::,:.:.> ..,:,,.,,, .-.:.:.:~::~:~.:~Ji:~~~::::::~::::.::::::::::::::,:,::::::::::: :.::.:,, “‘-‘.....A. . . . ...._.............................,.,.,,,~ .. . . . .. . .((.,./.. “.‘... . . . .. .. .. .... . . . . . .. . . .. .. . ii....: .,v... #::;:.:‘:“. Surface Science 279 (1992) 119-126 North-Holland .. .,.,., ,,,,,. . .. . . . . .. . ..../_. _, ,_ ..“:‘.:.:z:8 surface science .. .......‘.-“v.‘.‘.‘...,.(, ._, ./n.. .,.....,.... ,.(. z:.:.:::: .,., .,....... :.:.. >..:.:.:::::::g :,:.:::: .::::, ‘..“’ ‘.‘I:.: ‘.Y ..,.,........ ..v.....: .,.....,...... ““A” ,_:... “‘A”“‘. ‘.‘+5 .....,.,,. ..,,.,.,:,~.~,,,.,.,,,,,~~~,, ...~~.... ,i,,,.,,, ;::::::~ ‘-‘.:.:‘:‘::.::::::~~~~:~::~,~~!:~:~.~.:::: :.:,:, ;::::... X-ray photoelectron spectroscopic characterization of ultra-thin silicon oxide films on a Mo( 100) surface J.-W. He, X. Xu, J.S. Corneille Department of Chemistry, Texas A&M and D.W. Goodman University, College Station, * TX 77843-3255, USA Received 16 June 1992; accepted for publication 13 August 1992 Ultra-thin films of silicon oxides supported on a MoflOO) surface have been studied using X-ray photoelectron spectroscopy (XPS). The films were synthesized by evaporating Si onto the MO surface in oxygen ambient and were subsequently characterized using XPS with respect to the chemical states of silicon and the composition of the film. It has been found that the silicon oxide, prepared at room temperature with a silicon deposition rate of N 1.2 A/min and an oxygen pressure of 2 x lo-’ Torr, consisted of predominantly silicon dioxide with a small fraction of suboxides. Annealing to _ 1300 K yielded a stoichiometric film of SiO,. The subozides are believed to further react with oxygen forming SiO, at an elevated temperature. 1. Introduction Over the last decades, there have been numerous publications that have dealt with studies of silicon oxide thin films using surface science spectroscopies [l-18]. These previous studies have focused exclusively on the oxidation of silicon single crystal surfaces, addressing important issues such as the mechanism and kinetics of the thin film growth, structural and electronic properties of silicon dioxide, and the formation of silicon suboxides. These investigations have been mainly stimulated by important applications of silicon oxides in the fabrication of electronic devices, for example, metal/ oxide/ semiconductor transistors and SiO,/Si solar energy cells. Silicon dioxide is also extensively used as a catalyst support in the chemical industry. However, the surface chemistry of bulk silica has been studied far less with surface science spectroscopies compared to SiO,/Si interfaces. This is mainly because of the highly insulating and brittle properties of silica which often cause experimen* To whom all correspondence should be addressed. 0039-6028/92/$05.00 tal difficulties such as surface charging, sample mounting, sample heating and cooling. In order to circumvent these difficulties and to exploit microscopic processes on a silica surface using surface analytical techniques, experiments have been recently conducted to synthesize and characterize ultra-thin films of silicon oxide on a refractory metal surface [19,20]. Furthermore, thin films of SiO, prepared in this manner allow much greater flexibility with respect to thermal processing compared to SiO, films on silicon in that films of SiO, on molybdenum are stable up to 1500 K. Similar studies have been performed on other catalytically important oxides such as magnesium oxide [21] and iron oxides [22]. In previous studies of silicon oxide thin films on a MoQlO) surface using temperature programmed desorption (TPD), Auger electron spectroscopy (AES), electron energy loss spectroscopy (ELS) and infrared reflection absorption spectroscopy (IRAQ [19,20], it was found that a SiO, film can be synthesized by evaporating silicon in a low background pressure of oxygen at a sample temperature of N 300 K. The gas phase precursors for the SiO, film were reported to be SiO 0 1992 - Elsevier Science Publishers B.V. All rights reserved 120 J.-W. He et al. / Characterization of ultra-thin silicon oxide films on Mo(100) which was produced by oxidative etching of the Si source. The as-deposited films mainly consist of SiO,, as indicated by the AES spectra. The SiO, film annealed to - 1400 K exhibited electronic and structural properties similar to those of vitreous silica. The thermal stability of the SiO, film was found to depend on the film ;hickness. Annealing a thin SiO, film (< 50 A) to 1500 K caused a reduction of the film by the MO substrate, forming the volatile products SiO and MOO,. Recently, we have further examined the silicon oxide thin films grown on a Mo(100) surface with X-ray photoelectron spectroscopy (XPS), addressing the effects that oxygen ambient pressure and annealing temperature have on the chemical states of Si and the composition of the films. The results are presented and discussed in this paper. 2. Experimental The experiments were carried out in an ultrahigh vacuum chamber equipped with XPS, TPD and low energy electron diffraction (LEED). A detailed description of this chamber has been given elsewhere (231. The Mo(100) crystal was spot-welded onto a 0.2 mm Ta wire that allowed cooling of the crystal to 90 K and resistive heating to 1400 K. In addition, the sample could be heated to 2300 K using e-beam heating. A W-5%Re/W-26%Re thermocouple was spot-welded onto the sample’s back face for temperature measurement. The Mo(100) surface was cleaned using the procedure described in ref. [24]. The silicon source used for deposition was a high purity Si block (- 1 x 1 X 3 mm3) wrapped by a tantalum heating wire. The Si source was degassed extensively prior to each dosage. The Si oxide films, synthesized in this work, showed no C, S or N impurities within the XPS and AES detection limit (< 1 at%>. The thickness of the films was zstimated using the electron mean free path (23 A) in SiO, films for Mo(3d) photoelectrons, which have a kinetic energy of 1020 eV with the Mg Ka X-ray source (1253.6 eV) [25,26]. The Si oxide deposition rate varies with both oxygen pressure and the Si source temperature, and owascontrolled at approximately either 0.6 or 1.2 A/min for this work. In the present study of the SiO,/Mo(lOO) surfaces, the core level binding energies were measured with reference to the Mo(3d,,,) binding energy at 277.7 eV [27]. The pass energy of the spectrometer was 40 eV for this work, and the substrate Mo(3d,,,) peak exhibited a full width at half maximum (FWHM) of 1.4 eV which can be taken as the instrumental resolution. The XPS spectra in this paper were acquired using Mg Ka X-rays (1253.6 eV>. 3. Results Fig. 1 shows the Si(2p) XPS spectra for silicon oxide thin films that were prepared at three different oxygen background pressures. The thicknesses of the films are estimated to be 36 A. At an oxygen ambient pressure of 1 X lop8 Torr, spectrum a exhibits a significant peak at 99.4 eV that corresponds to silicon. This value is 0.2 eV higher than the Si(2p) binding energy (99.2 eV) from a pure silicon crystal [27]. The peak at - 102.5 eV is broad, and is thus best decomposed into two peaks using mixed Gaussian-Lorentzian curve fitting. These two peaks at 103.2 and 101.7 eV correspond to oxidized silicon. As the oxygen pressure increases (spectra b and c), the 103.2 eV peak intensity increases along with a shift in its peak position to higher binding energy, the intensity of the 101.7 eV peak first increases and then decreases, and the intensity of the peak at 99.4 eV decreases considerably. In spectrum c, the 103.6 eV peak shows a binding energy similar to that for silicon dioxide (103.4 eV>, and the peak at 102.7 eV falls in the binding energy range of suboxides (SiO,, with x < 2) [2-8,271. Therefore, we assign these two peaks at 103.6 and 102.7 eV to correspond to SiO, and suboxides, respectively. Previous studies also indicated that the oxide films prepared at an oxygen pressure of 1,X 1O-5 Torr with a deposition rate of - 1 A/min consist predominantly of silicon dioxide, as evidenced by AES and ELS spectra [19,20]. This suboxide may contain several Si oxidative J.-W. He et al. / Characterization of ultra-thin silicon oxide films on Mo(100) B : oxidative states of Si. The spectral deconvolution yields two more peaks at 102.7 and 99.9 eV, which are characteristic of suboxides and silicon. The integrated areas indicate that this film has 82% SiO,, 13% SiO, and 5% Si. Annealing this film at 1023 K reduces the suboxide peak area to zero and results in a symmetric peak for SiO, with a small peak at 99.6 eV for Si. This clearly indicates that annealing has eliminated the suboxides from the film. The SiO, species may have been either oxidized to SiO,, desorbed into vacuum, or decomposed into Si and 0. The decomposition is unlikely because spectrum b shows no 101.9 rh I 103.1 A ’ - . g-* / /’ i ;?\: ,; - “F4 -I ‘,c ‘1 : I BINDING . . Y \ x0.3 99.4 F 106 121 i’ 102 98 ENERGY (eV) Fig. 1. The Si(2p) XPS spectra of silicon oxide films (36 A) on a Mo(100) surface. The films were prepared by evaporating Si in an 0s pressure of 1 X 10-8 Torr (a), 5 X 10W8Torr (b) and 2 X 10W5Torr (c). The substrate temperature during the film preparation was - 350 K. The oxide deposition rate was approximately 1.2 IQmin. states, as have been unambiguously observed in the studies of SiO,/Si interfaces using synchrotron XPS [2,6]. The present work is, however, unable to further distinguish between these states due to the resolution limitation of the XPS spectrometer. Figs. 2 and 3 show the effect that annealing temperature has on the silicon oxide films prepared at N 350 K. In fig. 2, the film deposited at room temperature with an oxygen pressure of 2 X lo-’ Torr (spectrum a> is composed predominantly of SiO,. The spectral tail at the low binding energy side indicates the existence of the low 106 BINDING 102 ENERGY 98 (eV) Fig. 2. The Si(2p) XPS spectra of silicon oxide films (36 & on a Md100) surface. The films were prepared by evaporating Si if an 0, pressure of 2~ lo-’ Torr with a dosing rate of - 1.2 A/min. The substrate temperature during the film preparation was - 350 K. The film was then annealed to 393 K (a), 1023 K (b) and 1373 K (c). J.-W. He et al. / Characterization of ultra-thin silicon oxide film on MoilOOi 122 sity has been significantly decreased when compared to that of spectrum a. Fig. 3 demonstrates that the film synthesized at relatively low oxygen pressure has a considerable amount of suboxides and Si. This is consistent with previous studies, which showed that the film prepared at an oxygen pressure less than 1 x 10m6 Torr contained silicon or silicon suboxides [19,201. Annealing the film to elevated temperatures was found to remove the suboxide spectral features [19]. We will discuss this SiO, in more detail in the following section. The OfIs) spectra for a silicon oxide film are shown in fig. 4. After the film preparation at 330 K, the O(ls) spectrum indicates a single peak with a binding energy of 533.0 eV. This peak exhibits a symmetric lineshape with a full width at half maximum (FWHM) of 2 eV, identical to that reported for a thick SiO, film grown on a silicon surface [IS]. Annealing this film to 1373 K causes a 0.3 eV shift in the peak maximum with no noticeable change in the peak width or peak shape. 105 BINDING 101 97 ENERGY (ev) Fig. 3. The Si(‘2pf XPS spectra of silicon oxide a Mo(100) i,” an 0, A/min. tion was surface. The films were prepared pressure of 5 X IO-’ The substrate - 350 films (36 A) on by evaporating Si Torr with a dosing rate of - 1.2 temperature during the film prepara- K. The film was then annealed to 373 K (a), 803 K (b) and 1198 K Cc). significant increase in the Si peak area. Further annealing to 1373 K eliminates the silicon peak with a highly symmetric peak of SiO, remaining. Fig. 3a is the XPS spectrum for a silicon oxide film that was dosed at relatively low OZ pressure (5 x lo-’ Torr). This film consists of 26% SiO,, 38% SiO, and 36% Si, as estimated from the areas of the deconvoluted peaks. Annealing to 803 K causes a significant increase in the SiOz peak intensity with a concurrent decrease in the intensities of SiO, and of Si. Spectrum c, collected after annealing the film to 1198 K, exhibits virtually no suboxide peak, and the Si peak inten- 540 526 533 BINDING ENERGY (eV) Fig. 4. The O(ls) XPS spectra of a silicon oxide film (100 ,&I. The film was prepared by evaporating Si at an oxygen pressure of 1 X lo-’ Torr with a dosing rate of - 0.6 .&/min at a sample temperature of 300 K. The film was then annealed to the indicated temperatures. J.-W He et al. / Characterization of ultra-thin silicon oxide jilms on Mo(100) z !z nealing temperature of N 1300 K, we assign the ratio corresponding to the spectra at 1480 K to be two, the atomic ratio of 0 to Si in SiO,. In the calculation of the ratios, the contribution of oxygen from the MO substrate has been subtracted. The O(1.s) binding energies are 533.0 eV for SiO, and 530.7 eV for 0 chemisorbed on Mo(lOO), and thus are easily discernable at a low coverage of SiO,. Finally, we present the Mo(3d) XPS spectra for a SiO,/Mo(lOO) surface at several annealing temperatures. The Mo(3dgJ peak has a FWHM of 1.3 eV and a binding energy of 227.7 eV for all the spectra. These values remain unchanged in the 1023-1473 K annealing temperature range. Deposition of SiO, and subsequent annealing cause no measurable change in the MO substrate. The intensity increase in the 1473 K spectrum is due to the desorption of SiO, [20]. SiPp E-l 103.9 0% zal E- 103.7- ifi CL .; 103.5 G :: 533.4 - - 533.2 - 533.0 - : 01s 3 2 s E501 z s m i; 400 123 600 ANNEAL 600 1000 1200 TEMPERATURE 1400 ! 1600 (K) Fig. 5. The change of Si(2p) and O(k) binding energies and the ratio of the Si(2p) integrated intensity to that of O(k) for a SiO, film (100 A) on a Mo(100) surface. The SiO, film was prepared by evaporating Si at an ?xygen pressure of 1 X lo-’ Torr with a dosing rate of - 0.6 A/min. The sample temperature during the SiO, deposition was - 300 K. Fig. 5 shows the plots of the Si(2p) and O(1.s) binding energies and the ratio of the integrated intensity of 0 to that of Si as a function of annealing temperature. The silicon oxide film was synthesized in an oxygen pressyre of 1 X lo-’ Torr with a dosing rate of 0.6 A/min at room temperature. Upon annealing to 800-1300 K, the O(ls) binding energy shifts 0.3 eV and the Si(2p) shifts 0.4 eV toward a higher binding energy. The integrated intensity ratio of 0 to Si shows an increase in the 1100-1350 K annealing temperature range. Since all the experimental evidence, including the XPS spectra in fig. 2 and the TPD, AES and ELS spectra in previous work [19,20], have indicated that both suboxides and Si have been totally eliminated from the film at an an- 4. Discussion One of the primary goals of synthesizing silicon oxide on a MO surface is to prepare a stoichiometric silica film that can be used for model catalyst studies. Figs. l-3 indicate that such a silica film can be obtained by evaporation of Si with an oxygen pressure ,of 2 X lo-’ Torr at a deposition rate of N 1.2 A/min, followed by annealing the film to 1300 K. At a relatively low oxygen pressure ( < 5 X lo-* Torr), the film has a significant amount of suboxides and silicon in coexistence with SiO,. Fig. 1 further indicates that the film synthesized at room temperature contains more than 10% of suboxides even with an oxygen pressure of 2 X 1O-5 Torr. A further increase in oxygen pressure produces little improvement in the film composition. Annealing to 1300 K, however, eliminates the suboxides and silicon and results in a film consisting of only SiO,. The silica film has been suggested to assume a vitreous SiO, structure in which the basic [SiO,] blocks are networked via bridging oxygen atoms [19,20]. This film showed no LEED pattern and thus lacks long range order. The suboxide species formed during oxidation of silicon surfaces have been extensively studied 124 J.-W. He et al. / Characterization of ultra-thin &cm with a variety of spectroscopies including XPS [Z-9], ELS 13,10-121 and IRAS [13-151. It is generally believed that the SiO, species are located at the SiO,/Si interface with a thickness of a few angstroms. In studies of oxygen adsorption on Si surfaces, suboxide species were also observed for a monolayer surface oxide [8,11]. An iuvesti~ation of silicon oxidation by means of ion implantation at room temperature has indicated the formation of a thin layer inside a Si crystal which contains a mixture of SiO,, SiO, and Si [4]. The SiO, species, investigated by both high resolution XPS spectra [7,83 and theoretical calculations [S], consist of all four of the Si oxidative states, Si’+, Si2+, Si”+ and Si” with the Si(2p) core level shifts of 0.6, l&2.8 and 4.5 eV, respectively. Therefore, we believe that the suboxide film prepared at room temperature in this work may contain all four oxidative states. The shift in the maxima of the oxide peaks towards a higher binding energy (fig. I), as the oxygen pressure increases, reflects the increase in the relative population of the higher oxidative states. At an annealing temperature of 1300 IS, the film is present as pure SiO,. The peak in fig. 2c indicates a chemical shift of 4.4 eV relative to the binding energy of Si (99.2 eV). This value is in good agreement with those (4.3-4.5 eV> of SiO, reported in previous pubIicati~ns [4,7,8,27]. The XPS peaks corresponding to silicon in figs. t-3 exhibit binding energies of 99.4-99.9 eV, a few tenths of an eV higher than that of single crystal Si (99.2 eVl [27]. This difference may be due to the fact that the silicon atoms are ~nt~rrn~ed with the silicon oxides and thus are electronically perturbed with respect to bulk Si. It is also possible that the Si peaks are a convolution of Si and Si’ +. This would also shift the maximum of the resultant peak to a higher binding energy. The binding energy and symmetric lineshape of spectrum c in fig. 2 indicate that the film consists of only SiO,. The stoichiometry was calcufated using the integrated intensities of Si and 0, normalized by the atomic sensitivity factors [27]. This calculation yielded an 0 to Si atomic ratia of 2 : 1, further confirm@ the existence of a singIe phase of SiO, in the film. The stoichiome- oxide films on Mo(100) try of the film prepared at room temperature without annealing is estimated to be 1.7: 1, consistent with a film which has a composition of 82% SiO,, 13% suboxide and 5% silicon as shown in the fig, 2a. The disappearance of the SiO, species from the film upon annealing is 1ikeIy via reaction with oxygen within the film to form SiO,. This reaction is apparent by the increase in the SiO, peak intensity and a concurrent decrease in the SiO, peak intensity (figs. 2 and 31, while the stoichiometry of the film remains unchanged in the 4001000 K annealing temperature range (fig. 5). The interaction between SiO, and 0 upon annealing has also been observed in previous studies of the oxidation of Si crystals [4,61. The oxygen involved in the post-reaction in the present work was likely trapped in the film during SiO, synthesis I.51or was contributed by the decomposition of [SiO,] moieties [19,20]. The increase in the film stoichiometry at 1100-1400 K is associated with the disappearance of the Si peak in fig. 2. The Si appears to have interacted with SiO, to form volatile SiO that immediately desorbed [20]. The Oils) spectra of the silicon oxide film show a single peak with a binding energy of 533.0 eV and a FWHM of 2 eV, both identical to the values reported for bulk SiO, [18]. It seems that the oxygen involved in the SiO, post-oxidation has a binding energy similar to that of 0 in SiO, and thus is not discernable in the present XPS spectra. Annealing the film to 1373 K causes a 0.3 eV shift toward a higher binding energy (figs. 4 and 5). The Si(2p) peak also shifts 0.4 eV upwards (fig. 5). The variation of O(ls) and Si(2p) binding energies has been measured in detail as a function of the thickness of the SiO, films on Si [183. The present study also found that the Si(2p) and O&s) binding energies change with the fifm thickness. These shifts can be attributed to several physical processes such as extra-atomic reIaxation due to a high defect concentration [18], band bending in the SiO, film that causes a static surface potential change [28,29], or a local charging effect as the small islands of SiO, nucleate into large clusters. Fig. 6 shows that upon film deposition and subsequent annealing of the sample, the Mo(3d) J.-W He et al. / Characterization of ultra-thin silicon oxide films on Mo(IO0) 125 stoichiometric SiO, film can0 be obtained with a Si deposition rate of N 1.2 A/min at an oxygen pressure of 2 X 10e5 Torr at 300 K, followed by an annealing of the film to N 1300 K. The film prepared at room temperature without annealing was found to contain a small fraction of suboxides and silicon which undergo post-oxidation at an elevated temperature, forming either SiO, or volatile SiO. MoJd Acknowledgement 236 229 222 BINDING ENERGY (eV) Fig. 6. The Md3d) XPS spectra of a Mo(100) surface covered with a silicon oxide film (36 A). The film was prepared by evaporating Si in an 0.z pressure of 2 x 10m5 Torr with a dosing rate of - 1.2 A/min at a sample temperature of - 350 K. The sample was then annealed to the indicated substrate temperatures. XPS spectra show no measurable change either in the peak binding energy or in the peak FWHM. This rules out any significant interaction between the MO substrate with the SiO, film at a substrate temperature below 1100 K. Previous TPD studies have indicated that the SiO, was reduced into volatile SiO by the substrate MO in the 1400-1700 K temperature range, and the products SiO and MOO, desorbed promptly [20]. The present XPS spectra detected no significant molybdenum oxide remaining after annealing the film to 1473 K and thus are consistent with the reduction mechanism previously proposed [20]. 5. Summary We have reported the experimental results regarding the synthesis and characterization of ultra-thin silicon oxide films on a Mo(100) surface using XPS. It was shown that the composition of the film, prepared by evaporating Si in an oxygen ambient with a substrate temperature of * 300 K, varies strongly with the oxygen pressure. A We acknowledge with pleasure the partial support of this work by the Department of Energy, Office of Basic Energy Science, Division of Chemical Sciences. References [ll N.F. Mott, S. Rigo, F. Rochet and A.M. Stoneham, Philos. Mag. 60 (1989) 189. 121M. Niwano, H. Katakura, Y. Takeda, Y. Takakuwa, N. Miyamoto and M. Maki, J. Vat. Sci. Technol. A 10 (19921 339. [31 N. Aoto, E. Ikawa, N. Endo and Y. Kurogi, Surf. Sci. 234 (1990) 121. [41 V.A. Labunov and P.V. Protasevich, Nucl. Instrum. Methods B 39 (1989) 466. 151A. Feldman, Y.N. Sun and E.N. Farabaugh, J. Appl. Phys. 63 (1988) 2149. 161W. Braun and H. Kuhlenbeck, Surf. Sci. 180 (1987) 279. [71 F.J. Grunthaner, P.J. Grunthaner, R.P. Vasquez, B.F. Lewis and J. Masetjian and A. Madhukar, Phys. Rev. Lett. 43 (1979) 1683. 181 G. Hollinger and F.J. Himpsel, Phys. Rev. B 28 (1983) 3651. 191A. Bianconi and R.S. Bauer, Surf. Sci. 99 (1980) 76. [lOI T. Adachi and C.R. Helms, Appl. Phys. L&t. 35 (1979) 15. [ill H. Ibach and J.E. Rowe, Phys. Rev. B 9 (1974) 1951. [12] J. Derrien and M. Commandre, Surf. Sci. 118 (19821 32. [13] W.C.M. Claassen, R.W.A.H. Schmitz and J. Dieleman, Appl. Surf. Sci. 36 (19891 240. [14] M. Nadamura, Y. Mochizuki, K. Usami, Y. Itoh and T. Nozaki, Solid State Commun. 50 (1984) 1079. [15] P.G. Pai, S.S. Chao, Y. Takagi and G. Lucovsky, J. Vat. Sci. Technol. A 4 (1986) 689. [16] S.H. Garofalini, J. Chem. Phys. 78 (1983) 2069. [17] V.M. Bermudez, Surf. Sci. Lett. 230 (1990) L155. [18] J. Finster, D. Schulze, F. Bechstedt and A. Meisel, Surf. Sci. 152/153 (1985) 1063. 126 J.-W. He et al. / Characterization of rdtra-thin silicon oxidefilms [19] X. Xu and D.W. Goodman, Appl. Phys. Lett., in press. [20] X. Xu and D.W. Goodman, to be published. 1211 M.-C. Wu, J.S. Corneille, S.A. Cesar, J.-W. He and D.W. Goodman, Chem. Phys. Lctt. 182 1199if 472. [22] J.S. Corneille, J.-W. He and D.W. Goodman, to be published. 1231 R.A. Campbell and D.W. Goodman, Rev. Sci. &strum. 63 f1992) 172. 1241 M. Grunze, H. Ruppender and 0. Eishazly, J. Vat. Sci. Technol. A 6 (1988) 1266. f25] R. Flits& and S.I. Raider, J. Vat. Sci. Technoi. 12 (1975) 305. on Mo(lOOl [26] M.F. Hochella and AH. Carim, Surf. Sci. 197 (1988) L260. I271 CD. Wagner, W.M. Riggs, L.E. Davis, J.F. Moulder. G.E. Muilenberg, Eds. Handbook of X-ray Photoelectron Spectroscopy (Perkin-Elmer, Eden Prairie, MN, 1979). [28] R.W. Grant, S.P. Kowalczyk, J.R. Waldrop and WA. Hill, in: The Physics of MOS Insulators, Eds. G. Lucovsky, S.T. Pantelides and F.L. Galeener (Pergamon, New York, 1980) p. 202. [29j W.F. Egelhoff, Surf. Sci. Rep. 6 (1987) 253.
© Copyright 2026 Paperzz