The low energy auger electron spectroscopy lines as an index of the Ba overlayer order on the Ni(110) surface.
Auger electron spectroscopy (AES) is one of the most fundamental techniques in surface science providing chemical, growth mode, and coverage information [1, 2]. Despite the emerging wealth of knowledge coming from this surface analytical technique, to the best of our knowledge, structural information seems to be very limited. Although there are reports for different structural phases of C and Si studied by AES [3-5], in the case of metals, analogous contributions are rare . It would be a useful application of AES if the lineshape can be correlated to surface structural changes, either to order-order or to order-disorder transitions. This is the main issue of this work.
The material system, which we use in order to investigate the potential use of AES as a structural tool, is Ba on the Ni(110) surface. This system has been extensively studied before [7, 8], and the present study is an extension of our previous work . That work shows that Ba develops in successive layers on the Ni(110) surface, with the first one strongly interacting with the substrate and comprising a mixture of random c(2x2) domains and disordered adatoms. On the other hand, the second layer is disordered and more weakly bound. Substrate annealing at ~500[degrees]C opens up a kinetic channel, where Ba atoms are transferring from the second layer to the first one, increasing the c(2 x 2) ordering of Ba. Depending on the initial coverage, desorption of Ba is also observed. Stronger annealing up to ~800[degrees]C ends up with a substantial remaining subsurface Ba quantity (~0.35ML), with an unclear symmetry. In this work, the remaining barium on the surface presents a newly observed (2 x 2) symmetry, which might be the previously unidentified one. More importantly, by studying the thermal stability of the Ba overlayer on the Ni(110) surface, we demonstrate the sensitivity of the low energy Auger electron spectrum to the overlayer order. Specifically, we correlate the lineshape of the double Ba(73 eV)[N.sub.45][O.sub.23][P.sub.1] core-core-valence Auger transition line with amorphous and ordered barium structures.
2. Materials and Methods
The experiments were carried out in a typical ultrahigh vacuum (UHV) system equipped with AES and low energy electron diffraction (LEED) techniques. The base pressure in the UHV chamber was of the order of [10.sup.-10] Torr, while as a substrate a Ni(110) single crystal was used. The specimen could be heated by a Ta tape firmly attached to the back side of the crystal and uniformly pressed between the crystal and a Ta metallic case. The temperature of the crystal could be measured by a NiCr-CrAl thermocouple, spot-welded onto the center of the Ta case, and calibrated by an infrared pyrometer. For the crystal cleaning process, an argon ion gun was used for sputtering at energy 2 keV, at partial pressure ~5 X [10.sup.-5] Torr, and at sputtering time ~20 min. After the sputtering process and a following annealing at 700 K, a sharp (1x1) LEED pattern could be observed. Barium deposition was carried out by using a commercial evaporation SAES Getters source. The AES measurements were performed with a primary electron beam of energy 2 keV and anode current 15 [micro]A, while the electrons were collected and analyzed by a Varian cylindrical mirror analyzer (CHA). The AES signal was recorded in the first derivative mode, dN(E)/dE, with modulation voltage 5 V, sensitivity in lock-in amplifier 10 [micro]V, and photomultiplier voltage 1.750 kV. The Ba deposition was done in steps of 2 min deposition time, with the evaporation source at constant current 6.5 A. Based on this and combining the previous AES, LEED, thermal desorption spectroscopy, and work function results , the barium coverage could be estimated in monolayers with a flux of ~0.1ML/2min. The quantity of 1 ML is defined as the atomic density of the Ba(110) plane equal to 0.57 x [10.sup.15] at/[cm.sup.2], which is the densest atomic array of barium on the Ni(110) surface.
3. Results and Discussion
First we deposited 20 min (~1 ML) of Ba on the clean Ni(110) surface, and we performed annealing for ~2min increasing the substrate temperature in steps of 50 K each time. The AES measurements were performed when the substrate was cooled down to ~320 K. Figure 1 presents the low energy AES curves of the Ba(1ML)/Ni(110) surface after annealing at different temperatures. Next to each curve the observed symmetry by LEED is noticed. In these spectra we basically record the Ni(61 eV)[M.sub.23][M.sub.45][M.sub.45], a core-valence-valence Auger transition line (ATL), and the Ba(73 eV)[N.sub.45][O.sub.23][P.sub.1], a core-core-valence ATL. We also record the intense Ba(57 eV)MMN line, but this is strongly overlapping with the Ni(61 eV) line and it cannot be analyzed properly. This overlapping, in combination with the small electron mean free path of the Ni(61 eV), may be the main reason why this intense ATL almost vanishes after only 1 ML of Ba deposition. Based on the LEED observations, within the 300-650 K range, the Ba overlayer was amorphous. On further annealing, however, between 650 and 850 K, the Ba overlayer exhibits a c(2x2) pattern. This phase ofBais known from a previous work . For annealing from 850to950Kthe c(2 x 2) order deteriorated, while from 950 to 1050 K a new (2 X 2) pattern appears. While the c(2 x 2) structure was seen before , the (2 x 2) one is observed for the first time.
Figure 2 shows the LEED patterns of (a) (1 x 1) clean Ni(110) at energy 147 eV, (b) Ba-c(2 x 2) at 124 eV after annealing at 650 K, and (c) Ba-(2x2) at 124 eV after annealing at 1000 K, for Ba(1ML) deposition on the Ni(110) surface at room temperature. By taking into account the metallic diameters of Ba and Ni atoms (4.34 and 2.48 [Angstrom], resp.), structural models of the amorphous as well as the ordered barium structures are illustrated in Figure 3. The c(2 x 2) structure in Figure 3(b) represents the complete monolayer of Ba (1ML) on the nickel surface, since it is the densest atomic array of Ba adatoms on the Ni(110) surface in one layer. On the other hand, the (2 x 2) structure represents half of the monolayer (0.5 ML) of Ba. The transition from c(2 x 2) to (2 x 2) occurs at the same time with Ba desorption from the nickel surface.
Going back to Figure 1, attention is drawn to the change of the Ba(73 eV) lineshape as the substrate is annealed and the ordering of the Ba overlayer is established. Specifically, as long as the Ba overlayer is amorphous and at room temperature, the Ba(73 eV) ATL appears to be a single and rather sharp line. A weak peak at ~68 eV is due to the oxidation of a small portion of the barium overlayer, owing to the high reactivity of barium to chemisorbed oxygen from the environment [9,10]. This peak disappears at temperatures >500 K indicating a dissociation of BaO on the surface. As the c(2 x 2) symmetry develops, the Ba(73 eV) ATL becomes flatter consisting of two contributions. The following (2 x 2) structure at higher temperatures sustains the same lineshape. We need to point out that the O(510 eV) ATL was negligible with the appearance of the c(2 x 2) structure and absent with the (2 X 2) one.
We repeated the annealing experiments for higher Ba coverage at the 2.25 ML, and as Figure 4 illustrates, the amorphous layer of Ba at 600 K gives a rather flat Ba(73 eV) ATL, while both the c(2 x 2) and (2 x 2) structures cause a split of the line into another two with energy distance ~2.5 eV. A similar low energy Ba Auger double line has been recorded for a c(2 x 2) barium structure on the W(110) surface ; however, its origin was not commented upon. Thus, out of the comparison between the amorphous and the ordered Ba overlayers, it is obvious that the overlayer order affects drastically the Ba(73 eV) lineshape. To the best of our knowledge, no similar effect has been observed before.
Let us try to explain why this effect happens. The Ba(73 eV)[N.sub.45][O.sub.23][P.sub.1] Auger transition line is a core-corevalence transition, which involves the 4d, 5p, and 6s atomic orbitals. As previous photoemission measurements have shown, both the 4d and 5p orbitals are split into two states each one due to the spin-orbit coupling . Thus the first orbital participates in the Auger transition with the [4d.sub.3/2] and [4d.sub.5/2] states, while the second one participates with the [5p.sub.1/2] and [5p.sub.3/2] states. In this manner, the emitted Auger electrons from the 6s orbital should appear with four different kinetic energies, which are listed in Table 1 . In our AES spectra the split of the Ba(73 eV)[N.sub.45] [O.sub.23] [P.sub.1] line seems to fit well with the [N.sub.5][O.sub.2][P.sub.1] and [N.sub.5][O.sub.3][P.sub.1] Auger transitions. The contribution of both of these lines is expected to be dominant compared to that of the other two ([N.sub.4][O.sub.2][P.sub.1] and [N.sub.4][O.sub.3][P.sub.1]).
In general, the energetic position of an Auger electron peak is a characteristic of the element (i.e., the binding energies of the three electronic states involved) and its chemical state. The width of the peak including fine structure, on the other hand, depends on the local electron density of the valence states adjacent to the adsorption site and the localization of the final state holes. Particularly the width is strongly related to the lifetime of the three electronic states involved. In principle the energy width [DELTA]E of an Auger electron peak is given as
[DELTA]E = [([DELTA][E.sup.2.sub.XYZ] + [DELTA][E.sup.2.sub.a]).sup.1/2], (1)
where [DELTA][E.sub.XYZ] is the natural or inherent width of the Auger transition and [DELTA][E.sub.a] is the analyzer resolution all expressed in FWHM . Equation (1) assumes that all the energy widths have a Gaussian lineshape. In our experiments the CMA used was always operating under the same settings (modulation voltage, sweep time, sensitivity, etc.). Thus the only term that could possibly change the width of the recorded Auger Ba [N.sub.45][O.sub.23][P.sub.1] line should be the [DELTA][E.sub.XYZ] term. However, the natural width is not expected to change with the structure. Yet, the phase transition from amorphous to ordered barium can induce the following effect: in the amorphous phase the Auger electron emitting atoms have a range of different coordination numbers resulting in slightly shifted and overlapping Auger peaks, causing an effective broadening of the measured spectrum. The ordered structure, on the other hand, is characterized by a constant coordination number resulting in well-defined, in energy, peaks. In other words, the more ordered the atomic environment around the probe atom is, the narrower the measured FWHM is. From the discussion above, we conclude that the recorded splitting of the Ba [N.sub.45][O.sub.23][P.sub.1] line for both the c(2 x 2) and (2 x 2) structures can be assigned to the smaller observed width of the Auger electron transition. In that sense, the lineshape of the Auger Ba [N.sub.45][O.sub.23][P.sub.1] line may reflect the order of the barium overlayer.
In this work we studied the effects of the annealing temperature on the stabilization of different superstructures for Ba overlayer on the Ni(110) surface. A correlation between the overlayer order and the corresponding Ba AES lineshape was investigated. It was found that the lineshape of the low energy Ba [N.sub.45][O.sub.23][P.sub.1] Auger transition line is strongly influenced by the disorder-order transition of the barium adsorbate. Therefore, it appears that, under certain conditions, AES can differentiate ordered from amorphous overlayers.
Conflict of Interests
The authors declare that there is no conflict of interests regarding the publication of this paper.
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Correspondence should be addressed to D. Vlachos; firstname.lastname@example.org
Received 31 October 2013; Revised 3 February 2014; Accepted 18 February 2014; Published 26 March 2014
Academic Editor: Hakan Arslan
D. Vlachos, M. Kamaratos, and S. D. Foulias
Department of Physics, University of Ioannina, P.O. Box 1186, 45110 Ioannina, Epirus, Greece
TABLE 1: The atomic configurations of the Ba(N45O23P1) Auger transition line. The kinetic energies take into account the core-hole effect . Auger transition Atomic orbitals Kinetic energy (eV) [N.sub.4][O.sub.2][P.sub.1] [4d.sub.3/2]-[5p.sub.1/2]-6s 74.5 [N.sub.4][O.sub.3][P.sub.1] [4d.sub.3/2]-[5p.sub.3/2]-6s 76.5 [N.sub.5][O.sub.2][P.sub.1] [4d.sub.5/2]-[5p.sub.1/2]-6s 71.5 [N.sub.5][O.sub.3][P.sub.1] [4d.sub.5/2]-[5p.sub.3/2]-6s 73.5
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|Title Annotation:||Research Article|
|Author:||Vlachos, D.; Kamaratos, M.; Foulias, S.D.|
|Publication:||International Journal of Spectroscopy|
|Date:||Jan 1, 2014|
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