1. Introduction
The study of the inelastic scattering of electrons near a surface region and inside the bulk material has a long history. The inelastic scattering phenomenon is important to quantitative surface analysis based on electron spectroscopy techniques, such as x-ray photoelectron spectroscopy (XPS), Auger electron spectroscopy (AES), elastic peak electron spectroscopy (EPES) and reflection electron energy loss spectroscopy (REELS). During the last decades, measurements of the energy loss suffered by fast electrons have been used for determining optical constants. Typical kinetic energies of electrons are 50–300 keV when they are transmitted through thin (500–2000 Å) solid films. The probability of the energy loss is determined by the imaginary part of the dielectric response function ε (q, ω), which is a function of the frequency ω and the wavenumber
q of the electromagnetic disturbance. Raether [
1] pointed out that the dielectric properties determined by electron energy loss spectroscopy (EELS) agree well with those obtained by optical methods. At an energy loss above some tens of eV, however, multiple-scattering events become significant, and the measured properties are surface sensitive [
2], thereby complicating the extraction of ε (q, ω).
The excitation of surface plasmons of thin films by fast electrons was first theoretically investigated by Ritchie in 1957 [
3]. Two years later, it was observed experimentally by Powell and Swan [
4,
5]. Since the first observation of surface excitations, there has been a continued interest in developing a method or technique for the clear separation of surface and bulk properties. Even more, in the pioneering work of Ritchie [
3], the surface effects were split into two parts. The first one is the result of additional surface modes of the polarization field in the vicinity of the surface, which have a lowered resonance frequency. The second one is the coupling between surface modes and bulk modes near a boundary, which leads to a decrease of the intensity of bulk excitations. Such a depolarization effect is referred to as the Begrenzungs effect. For more details of plasmon theory, see [
6]. For the investigation of the surface and bulk contribution, we presented a Monte Carlo simulation of the reflected electron energy loss spectroscopy (REELS) spectra of silver [
7]. The simulation was based on the application of the dielectric function formalism [
3,
8,
9,
10], where both the individual elastic and the inelastic scattering events in the solid were taken into account. In our early Monte Carlo simulations, the simple form of the surface energy loss functions as well as the bulk ones were applied. We showed that for the proper description of the measured REELS spectra, the contribution of the surface losses are significant, especially at low incident energies.
Regarding the energy loss events, we can distinguish between soft and hard collisions. Heavy particles feature the advantage that for projectiles moving parallel to a planar surface, the stopping power resulting from the dielectric response of the surface can be probed without direct (“hard”) collisions. However, since the ion is always attracted towards the surface by its self-image potential, it will suffer a close collision upon impact on the surface. This problem can be avoided using a microcapillary target. This technique has been introduced as a tool to study above-surface processes [
11,
12,
13,
14]. As an interesting application, we showed that the trajectories that do not undergo charge exchange but come close enough to the walls to suffer a significant stopping power can probe the individual surface loss function of the capillary material.
In this work, the reflected electron energy loss spectra of aluminum are studied experimentally. The backscattered electron energy spectra were measured in reflected mode at an energy range between 250 eV and 2000 eV and at a wide range of incident angles, including the grazing geometry of an 88° incident angle compared to the surface normal. Many authors have studied the combination of surface and bulk losses in various models [
1,
2]. The absolute intensities of surface and bulk plasmons strongly depend on the primary energy and on the geometrical conditions, such as the angle of incidence of impacting and escaping electrons. Opposite to the bulk losses, the description of surface loss events has not been fully addressed; in particular, the grazing conditions have yet to be determined. We designed a special geometrical arrangement in which the grazing angle of the primary beam is reliably set up. We present and analyze a series of spectra measured by reflected electron energy loss spectroscopy on an aluminum sample using a cylindrical mirror analyzer. Our novel experimental condition makes possible the determination of the surface plasmon energies with an improved accuracy and that allowed the revealing of the energy shift of the surface plasmon.
2. Experimental
Loss spectra were measured on an aluminum layer target that was a 100 nm Al layer evaporated onto an Si wafer. The target was mounted in the UHV condition of 1.0 × 10−9 mbar and cleaned before the measurement by a widely scanned 1 keV Ar ion bombardment.
The novelty of our experimental arrangement is that the specimen in oblique condition results in altering the angle of incidence by changing the azimuthal angle of the specimen. We show this uncommon arrangement in
Figure 1. As is visible, the target was mounted at a 45° slope to a sample holder with rotating ability around a vertical axis, as shown in
Figure 1. The electron beam of primary electrons was produced by an electron gun from a side position, and it reached the surface in a 150 micrometer spot. The rotation of the sample around its vertical axis provides an easy way of changing the angle of the primary beam relative to the surface plane. Describing this angle, we use the glancing angle (the angle measured from the surface plane) further in this paper, which is complementary to the usual angle of incidence (measured from the surface normal). The observed spectra cover the 1.3–73.7° range of glancing angles. This particular geometry enables us to provide very accurate angular conditions for small grazing cases (1–10°). Because at first a zero-grazing-angle (parallel to the surface) position was determined, the required grazing angle was adjusted by turning the sample away. This setup is less accurate, however, for high grazing angles (above 30°).
Electron spectra of backscattered electrons were detected by a vertically mounted cylindrical mirror analyzer (CMA), whose ring-shaped entrance slot is marked in yellow in
Figure 1. The axis of the sample rotation was adjusted to be identical to the symmetry axis of this cone-shaped detection. Thus, the angular relation to the detector slot did not change with sample rotation, though the cone defined a range of glancing angles for the escaping electrons.
The analyzer itself was a special retarding field CMA (type DESA 150 made by Staib Instrumente Gmbh, Langenbach, Germany), with a constant energy resolution over the whole energy range. The energy resolution of measured spectra was limited by the energy width of the primary beam. It was 1.0–1.2 eV, depending on the primary energy. Electron spectra were detected with 0.1 eV steps.
3. Results and Discussion
Aluminum spectra were detected varying excitation energy from 250 eV to 2000 eV and a changing excitation beam of the glancing angle from 1.3° to 73.7°. This resulted in a wide range of surface/bulk intensity ratios, according to the conditions.
To describe the electron backscattering, the events of electron transport that need to be taken into account concern both the primary electrons and the raised secondary electrons. After the primary electrons reach the target, several types of interactions with stochastic relevance start to influence the electron movement. The elastic scattering on the atomic potential produces high angle alteration of the electron path without energy loss (disregarding the tiny energy exchange with the recoil atom). Without elastic scattering, practically no backscattering could be observed, since other interaction events cannot provide enough momentum transfer to the primary electron to result in backscattering. Energy loss processes like ionization loss and plasmon loss are responsible for the alteration of electron energy, though they contribute to the path deviation as well. The multiple occurrences of these inelastic processes result in an energy distribution of electrons that is dependent on the penetrating distance from the surface. A special slice of this distribution that is present at the surface can be observed by external detector and yields the backscattered spectrum. In case of aluminum, the dominant energy loss process is plasmon excitation, including bulk and surface plasmon excitation. These plasmon loss peaks can easily be observed in the neighborhood of the elastic peak (the heap of electrons backscattered without energy loss). With a simple consideration of geometrical conditions, the lowering glancing angle results in
- -
higher surface plasmon peaks, because the longer path is traveled in the surface region where the surface plasmon is excited;
- -
lower bulk plasmon excitation, because primary electrons penetrate shallowly and the primary electron is able to lose energy without bulk plasmon excitation.
The strengthening of the surface feature should also reflect the standalone and overlapping multiple plasmon peaks.
For demonstration, two spectra are shown in
Figure 2, measured at 1 keV excitation energy with different angles of the excitation beam. The ratio of surface/bulk can be changed back and forth with altering the glancing angle of the excitation beam. The experimental setup allows the varying of the angle of the primary beam only while the escaping electrons traveled on the same paths with the same angles in all cases. This results in some equalization of the ratio. Obviously, an experimental condition where the geometry of escaping electrons can be adjusted too, would provide a more significant change of surface/bulk plasmon ratios.
On the other hand, using the same simple consideration, lowering the energy of primary beam results in
- -
lower bulk plasmon excitation (because of lower penetration of primary electrons);
- -
larger surface plasmon excitation (because of larger cross section of surface plasmon excitation.
The lower bulk and higher surface excitation has a consequence for single and multiple plasmons.
Figure 3 shows two spectra detected at a moderate glancing angle of 32.3° at different energies. The ratio of surface/bulk plasmon losses can be varied in a wide range by adjusting the excitation energy.
The evaluation of the measured spectra took place by determining the contributions of elastic peak, single surface excitation, and single bulk excitation. Multiple excitations were also determined, however, they are not presented here because their intensity could be calculated with less certainty. The spectrum was decomposed by fitting these components with a Gaussian-Lorantzian shape. As a result, the fit included an optimized peak position, intensity, width, and asymmetry. The intensity of a peak is defined by the area of the peak. For characterizing the surface excitation, the surface plasmon peak/elastic peak ratio as well as the surface plasmon peak/bulk plasmon peak ratio were calculated. These ratios are shown in
Figure 4a,b, respectively, for the entire observed ranges.
According to our measurements, at low energies and grazing incident angles, the surface plasmon intensity can be larger than the elastic peak intensity. The measurement of the energy loss spectra of Al revealed a barely studied feature. The energy of the surface plasmon slightly shifted with the variation of the incident angle. The loss spectra measured with 250 eV excitation energy at different glancing angles are shown in
Figure 5a. It clearly shows the shift of the surface plasmon peak, that is, the change of the surface plasmon energy, as the larger glancing angle beam generates surface loss with larger energy.
Because this is a new experimental finding for a well-studied topic, further explanation is necessary regarding our findings. Though the energy shift is a relatively small change (a few 100 meV) of a wide (4 eV) peak, it is more significant at low grazing angles. Plasmon measurements are mostly carried out at higher grazing angles, where the energy shift is small (below 100 meV). Detection is difficult because the surface plasmon peak overlaps with the bulk plasmon peak. We introduced, however, an experimental novelty that made possible the determination of the energy shift with reasonable accuracy. The measurement at low grazing angles improved the accuracy by twofold:
- -
the low grazing angle resulted in higher energy shift (over 300 meV) of the surface plasmon peak, which was easier to identify;
- -
the low grazing angle resulted in larger surface plasmon and smaller bulk plasmon peaks, and thus the influence of bulk to the surface plasmon is less disturbing (see black and purple lines in
Figure 5).
Obviously, the actual energy of the surface plasmon is not identical to the position of the visible peak in the loss spectrum. The correct surface plasmon energies are calculated from the measured spectra and are shown in
Figure 5b. The energy values are derived from the decomposition of loss spectra by peak fitting, which is much more precise (see details below) than reading the peak position.
Figure 5b shows that the energy of the surface plasmon changes almost 0.4 eV, while the excitation angle changes from 1.4° to 73.7°.
To conduct analyses of the possible errors made in this decomposition, one needs to consider that the visible spectrum is a sum of several loss processes that also provide contributions at the position of the surface plasmon. If these other losses have a slope at the location of the surface plasmon, it may shift the position of the visible peak. The most significant effect is the bulk plasmon loss, which indeed provides some slope at the surface plasmon. Consequently, the larger the glancing angle, the larger the contribution of the bulk plasmon, which provides a larger shift of surface plasmon toward higher energies. The evaluation of the measured spectra showed that this bulk plasmon–induced shift of the visible peak is far less than the detected shifts. The largest bulk plasmon–induced shift of the visible peak is obtained at the highest glancing angle (73.7°), when the bulk contribution is the largest. In this case, the bulk plasmon–induced shift of the visible peak is 0.11 eV, that is, the position of visible peak is shifted from 10.72 eV to 10.83 eV due to the presence of bulk plasmon. This 0.1 eV is much smaller than the observed 0.5 eV difference for the changing glancing angle. For lower glancing angles, the bulk plasmon –induced shift of the visible peak quickly diminishes and thus becomes less disturbing. Thus, we can state that the shift of the visible surface plasmon peak cannot be explained by the increasing bulk contribution; instead, it basically results from the changing energy of the surface plasmon.
It must be noted here that the experimentally observed surface plasmon is a sum of all the surface losses generated in the actual geometrical condition. The exciting beam had a definite glancing angle and was controlled by sample rotation, according to the graph of
Figure 1. The escaping electrons had identical paths toward the detector, disregarding the excitation condition and covering a range of glancing angles. The detector has a ring-shaped slot with an axis of 45° glancing angle and about +/−22° cone width. Thus, the detected surface plasmon heap has contributions from the controlled angle incoming electrons and the fixed-ranged escaping electrons. These contributions have slightly different plasmon energy, however, and cannot be separated because of their great overlapping. This may explain our finding that the shape of the surface plasmon obtained by decomposition is not an ideal Lorentzian, but still has a weak asymmetry (see
Figure 6). For better visibility, the ideal (symmetrical) shape of the surface plasmon is drawn by a dotted line. The asymmetry is the most significant for the single surface plasmon shape, though the multiple losses are also influenced (not shown in
Figure 6).