Abstract
The four dopants (Nd, Gd, Dy, and Er) substitutionally occupy the Li+ sites in lithium tetraborate (Li2B4O7: RE) glasses as determined by analysis of the extended X-ray absorption fine structure. The dopants are coordinated by 6-8 oxygen at a distance of 2.3 to 2.5 Å, depending on the rare earth. The inverse relationship between the RE-O coordination distance and rare earth (RE) atomic number is consistent with the expected lanthanide atomic radial contraction with increased atomic number. Through analysis of the X-ray absorption near edge structure, the rare earth dopants adopt the RE3+ valence state. There are indications of strong rare earth 5d hybridization with the trigonal and tetrahedral formations of BO3 and BO4 based on the determination of the rare earth substitutional Li+ site occupancy from the X-ray absorption near edge structure data. The local oxygen disorder around the RE3+ luminescence centers evident in the structural determination of the various glasses, and the hybridization of the RE3+ dopants with the host may contribute to the asymmetry evident in the luminescence emission spectral lines. The luminescence emission spectra are indeed characteristic of the expected f-to-f transitions; however, there is an observed asymmetry in some emission lines.
Introduction
Materials containing boron investigated for solid state neutron detection [] include semiconducting boron carbide [–], boron nitride [–], boron phosphide [–], Mg2B14 [] and lithium borates [–]. In particular, undoped lithium tetraborate (Li2B4O7) is capable of being enriched with 6Li up to 95% and 10B up to 97.3% [], well above the natural abundances (6Li–7.42%, 10B–19%), thereby increasing thermal neutron capture [, , ].
Many rare earth (RE) ions exhibit high luminescence efficiency in host borate crystals and glasses with various chemical compositions [–]. Consequently, combining rare earth dopants with the high thermal neutron capture cross-sections of 6Li and 10B may result in highly efficient neutron scintillators [, , , ]. In lithium tetraborate, this is particularly true as undoped Li2B4O7 has a wide band gap of ~9.8 eV, based on measurements of {100} and {110} oriented single crystals [, –] and is highly transparent in the visible spectrum. In general, the borates, including lithium tetraborate (Li2B4O7) single crystals, are characterized by high optical transmission from far infrared to vacuum ultraviolet [, ].
Obtaining single crystal Li2B4O7 is technologically challenging; thus, application to large area scintillation detectors will favor glasses over single crystals due to lower fabrication costs. The very low crystal growth velocity and high melt viscosity lead to difficulties with dopants, particularly rare earths [, ]. Therefore, from the technological viewpoint, the vitreous Li2B4O7 compounds are more advantageous when compared with their crystalline analogs.
Padlyak, Teslyuk and coworkers studied the luminescence properties of some rare earth doped lithium tetraborate (Li2B4O7:RE) glasses [, ]. They deduced from the optical characteristics that the rare earths generally occupy the Li+ site exclusively in the +3 valence state. Compared to other rare earth doped borates and crystalline counterparts, a broadening of the spectral lines was observed which was theorized to be a result of the dopant interaction with a varying O-coordination environment in the glassy material. Studying this varying O-coordination structure is not ideal [] with traditional bulk diffraction measurements (e.g., XRD) due to the lack of long range order. Instead, a more localized probe such as extended X-ray absorption fine structure (EXAFS) may be used.
In this research, lithium tetraborate glasses have been separately doped with four different rare earth elements: Nd, Gd, Dy, and Er. The local environment about the dopants was studied with EXAFS in order to determine the positional disorder of the varying O environment, an average coordination number and bond length, and to assist in validating the presumption that a varying O-environment is the source of the spectral line broadening. Further, the experimentally determined site has been used as a basis for density functional theory (DFT) calculations to investigate the electronic nature behind the spectral line broadening observed in the emission spectra.
Materials and methods
The doped Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy, and Li2B4O7:Er glasses were obtained in the air from corresponding polycrystalline compounds according to standard glass synthesis. For solid state synthesis of the doped materials, highly pure carbonate (Li2CO3) and boric acid (H3BO3) were used. Solid-state synthesis of the doped Li2B4O7:RE compounds was carried out using a multi-step heating process that follows the reaction sequence [, ]:
The Nd, Gd, Dy, and Er impurities were added as RE2O3 (RE= Nd, Gd, Dy, and Er) in amounts of 0.5 and 1.0 mol. %. Large doped glasses were obtained by fast cooling of the corresponding melt that was heated more than 100 K higher than the melting temperature for excluding the crystallization processes. Samples were cut for optical measurements and polished to a size of approximately 5 × 3 × 2 mm3.
Optical absorption spectra were recorded at room temperature with a Varian spectrophotometer (model 5E UV–VIS–NIR). Emission and luminescence excitation spectra were acquired with a Dongwoo (model DM711) scanning system consisting of an excitation monochromator with 150 mm focal length and emission monochromator having 750 mm focal length equipped with a photomultiplier and an InGaAs detector.
The Li2B4O7:RE extended X-ray absorption fine structure (EXAFS) spectra were measured using a double crystal monochromator of Lemonnier type [] at the DCM and WDCM beamlines located at the Center for Advanced Microstructures and Devices (CAMD) [–]. Due to the thickness of the glass samples and low dopant concentrations (nominally 1%), the absorption spectra were measured in fluorescence mode and the spectra analyzed without self-absorption corrections. For all samples, the L3 (2p3/2) edge fluorescence was measured corresponding to the M5-L3 (3d5/2–2p3/2) transition and was found to be in reasonable agreement with expectations [].
The EXAFS spectra were analyzed in two different ways. First, the spectra were analyzed using standard procedures with the IFEFFIT tool suite and FEFF 6 [–]. This consisted of isolating the EXAFS signal, converting to k-space, then using the Fourier transform to determine the average coordination number and element-type around the rare earth dopants, as detailed elsewhere for other doped Li2B4O7 crystals [] and glasses []. The second method of analysis employed the use of a Latin hyper-cube sampling (LHS) routine and the scattering code FEFF 9 for phase shifts and backscattering amplitudes. This code was developed as a bridge between a Monte Carlo modeling approach and traditional EXAFS fitting and is a more recent development. The power of this latter approach lies in the ability to cover a very large parameter space in modeling the experimental data and locating false minima in the fits to the data. The results of both analysis methods are generally in agreement, although the Latin hyper cube (LHS) approach is computationally faster.
Despite the glassy nature of the samples that may result in positional disorder around the RE dopant, the model used for fitting the EXAFS was based on the known crystal structure (Figure 1) of Li2B4O7 [; , –]. This was an appropriate starting point for analyzing EXAFS spectra that will on average reflect the coordinating environment, including an average distance to the first shell and an average coordination number. As it is hypothesized that the rare earth dopants will substitutionally dope for the Li+ atoms, starting with the crystalline model and then adjusting the O environment to reflect the average coordinating environment makes the most sense. Furthermore, due to the low Z nature of the glassy matrix, it is expected that the photoelectric backscattering signal will be very weak beyond the first shell, unless there is significant dopant clustering in the material, which would result in a detectable RE-RE scattering shell.
Figure 1
Optical absorption and luminescence
High-quality scintillation is dependent upon significant quantum efficiency while retaining optical transparency [
Figure 2

The optical absorption spectrum of Nd3+ centers in Li2B4O7:Nd glass.
Although the luminescence emission spectra are characteristic of the f to f transitions of the +3 rare earth ions, the effect of the host matrix plays a role. In the case of the Nd3+ centers, where four characteristic f to f transition bands due to the 4F3/2 → 4I9/2, 4F3/2 → 4I11/2, 4F3/2 → 4I13/2, and the 4F3/2 → 4I15/2 dipole transitions (some shown in Figure 3) combine to provide a net quantum efficiency of 24%, inhomogeneous broadening of spectral lines does occur [
Figure 3

The luminescence emission spectrum of Nd3+ in Li2B4O7:Nd glass.
Extended X-ray absorption fine structure
In Figure 4, the normalized experimental XAFS signal is plotted for Li2B4O7:Nd. All the rare earth doped samples of this study, Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy, and Li2B4O7:Er, have very similar XAFS spectra (Figure 4 inset), including the presence of the sharp white line: a strong feature just above the absorption edge. The measured L3 edge for the Li2B4O7:Nd was determined to be 6212 eV by identifying the inflection point on the rising photoelectric edge, or about 4 eV greater than the expected 6208 eV [
Figure 4

X-ray absorption fine structure spectrum of Li2B4O7:Nd. The absorption coefficient was measured for the L3 edge from 100 eV below the edge to approximately 500 eV above the edge. In addition to the X-ray absorption fine structure, a vertical line is shown at 6208 eV, which is at a smaller value than the experimental edge found to be 6212 eV. In the inset, the X-ray absorption fine structure spectra for all four samples (Nd, Gd, Dy, and Er) are plotted, shifted by their absorption edge energies so that they are centered at 0 eV to compare them directly.
In Figure 5, the experimental EXAFS spectra have been extracted from the data in Figure 4, taken above the rare earth dopant L3 edge, have been replotted as a function of wave vector k for the Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy, and Li2B4O7:Er glass samples. In all cases, the EXAFS is evident up to approximately 6 Å−1 and is similar for the rare earth doped lithium tetraborate samples studied, with only small shifts. The signal-to-noise in the EXAFS spectra deteriorate with wave vectors greater than about 7.5 Å−1 as is expected for glassy samples when the host matrix about the dopant consists primarily of low Z material [
Figure 5

The k2 weighted extended X-ray absorption fine structure taken above the L3 rare earth dopant edge for Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy and Li2B4O7:Er.
The rare earth doped lithium tetraborates are very similar in structure, as is evident from the EXAFS spectra in Figure 5. The similarity in the EXAFS features for all the samples is an indication that the rare earths dope the Li2B4O7 lattice in a similar fashion. This is expected, as nearly all lanthanides adopt the +3 valence state [
The reliability of the structural information from our EXAFS data is limited in scope to the first coordination shell due to the signal-to-noise deterioration. Furthermore, the structural information is an indication of the average environment due to the glassy nature of the lithium tetraborate host. The Fourier transformed EXAFS spectrum for Li2B4O7:Nd is plotted in Figure 6. The Fourier transformed EXAFS is typical for all the rare earth doped glass samples studied: Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy, and Li2B4O7:Er. The out-of-phase real and imaginary components of the R-space signal (plotted in Figure 6) demonstrate the high level of confidence that may be placed in the Fourier transform.
Figure 6

The Fourier transformed extended X-ray absorption fine structure signal (solid) for Li2B4O7:Nd plotted in Figure 5. The real (long dash) and imaginary (small dash) components are plotted to show Fourier transform contributions. In the inset, the Fourier transform imaginary components for Nd, Gd, Dy, and Er are shown. There is a trend from left to right in the inset, with the left most (small dash) line resulting from the Er doped sample and then as the atomic number decreases the peak position moves to longer bond length (Er → Dy → Gd → Nd) with Nd as the right most (solid) line.
In the inset of Figure 6, the imaginary component for the Fourier transforms of the data of Figure 5 are plotted for all the doped samples. Traditionally, peaks in the imaginary spectra for EXAFS transforms have been correlated to physical distance in the radial distributions. Figure 7 is provided to show the quality of the EXAFS fit results and is indicative of the RE located substitutionally in a Li+ site. Although all the fits are not exact, this and the extracted coordination numbers are an indication of multiple interactions being measured coherently. If each interaction was known exactly, then a multiple-FEFF calculation could be made and different weights applied to each in order to determine an exact fit. Figure 7, nonetheless, demonstrates that the fits, despite deficiencies, are acceptable for all of the studied doped glass samples. The bond length contraction is noticeable with increasing Z, matching with the inset of Figure 6. The fit quality may be determined from the fitting parameters given in Table 1 for both the standard fitting method and using the LHS routine. For this result of the rare earth dopant substituting in a Li+ site, the greater charge of the RE3+ dopant may be easily compensated by anion vacancies, (VLi)− and (VB)3−, elsewhere in the glassy matrix.
Figure 7

Plotted are the R-space Fourier transformed extended X-ray absorption fine structure signals for Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy and Li2B4O7:Er. The vertical dotted lines indicate the fitting window used for the backward Fourier transform range (1.3–4 Å). The primary peak is the first coordination shell, comprised of O atoms.
Table 1
| Coord. Shell | N (atoms) | Eo (eV) | R (Å) | σ2 (Å) | Procedure |
|---|---|---|---|---|---|
| Nd-O | 8.32 ± 0.58 | 3.14 ± 1.90 | 2.47 ± 0.03 | 0.014 ± 0.007 | Standard |
| 8.61 ± 0.01 | 0.42 ± 0.20 | 2.48 ± 0.03 | 0.010 ± 0.001 | LHS | |
| Gd-O | 7.26 ± 0.56 | −1.98 ± 2.06 | 2.37 ± 0.03 | 0.011 ± 0.002 | Standard |
| 8.03 ± 0.26 | −2.55 ± 0.62 | 2.36 ± 0.01 | 0.009 ± 0.001 | LHS | |
| Dy-O | 7.56 ± 0.66 | 1.24 ± 1.98 | 2.34 ± 0.03 | 0.012 ± 0.002 | Standard |
| 7.90 ± 0.12 | 0.25 ± 0.19 | 2.35 ± 0.00 | 0.010 ± 0.001 | LHS | |
| Er-O | 7.00 ± 0.42 | 2.54 ± 1.40 | 2.32 ± 0.02 | 0.009 ± 0.003 | Standard |
| 7.94 ± 0.04 | 0.96 ± 0.17 | 2.31 ± 0.00 | 0.008 ± 0.000 | LHS | |
| Nd-O (BO3 model) | 3 | 30.9 ± 0.05 | 1.92 ± 0.03 | 0.003 ± 0.005 | Standard |
Tabulated are the final fit parameters for the four rare earths analyzed including coordination number N, extracted photoelectric edge shift Eo, the first shell bond length R(Å) and σ2 which is the mean squared displacement in the rare earth to oxygen bond length, often referred to as the EXAFS Debye-Waller factor.
The analysis procedures used are indicated: application of the FEFF 6 scattering codes [
Due to the size and oxygen coordination number of the rare earths, placement of a rare earth dopant in the B complexes can almost immediately be excluded. A rare earth substitution for the B atom sites would result in a very large distortion of the lithium tetraborate lattice that does not fit with our experimental EXAFS data. Table 1 supports our position as to why a rare earth in a B substitution site can be neglected. To have a rare earth substitute for B in either the BO3 or BO4 clusters would result in coordination numbers of 3 and 4, less than the observed 7–10 oxygen coordination obtained from the EXAFS data. The RE-O bond length is reduced if placed in a boron site, even in the best fit to the EXAFS data. In the case for Nd, the Nd-O bond length is 1.92 Å for a boron site, still significantly less than the 2.7 Å observed, but this fit (Table 1) to the EXAFS data requires an unphysical shift in the adsorption edge, as discussed below in the context of our near edge X-ray absorption experimental data. It is noteworthy that for Nd substituting for boron in the BO3 structure, the fit to the EXAFS data would still require a expansion of the bonding distance from the B-O approximately 1.3–1.9 Å, which would greatly distort the interlocking BO3-BO4 portions of the unit cell. In general, substituting a rare earth element such as Nd with a radius of roughly 1.123 Å with a coordination number of 6 into a site where the B3+ radius is, on average, 0.15–0.25 Å for oxygen coordination numbers of 3 and 4 respectively, is unphysical. Substituting a rare earth element, such as Nd, in a manner that would in a way that would result in a bond length of 1.273 to 1.373 Å, so as to achieve less distortion of the interlocking BO3-BO4 portions of the unit cell, is possible only if we ignore the obvious problem of coordination number mismatch and the very large resulting charge distributions, as partly elaborated by theory below.
X-ray absorption near edge structure
In Figure 8, the experimental X-ray absorption near edge structure (XANES) region for Li2B4O7:Nd has been plotted in more detail than in Figure 4. The solid black line is the experimental data and the dotted red line is the theoretical calculation using FEFF 9.05 and full metal scattering with a cluster size of 5.1 Å and a small convergence factor of 0.05. The Hedin-Lundqvist to ground state exchange correlation was used.
Figure 8

Plotted is the experimental data (solid black line) for Li2B4O7:Nd in the nominal X-ray absorption near edge structure region. FEFF 9.05 has been used to calculate a theoretical X-ray absorption near edge structure spectrum (red dotted line) using full multiple scattering. The theory has been shifted to higher binding energy by 2.8 eV (reflective of the +3 charge of the Nd dopant).
Peak fitting to the XANES data was accomplished by using an arctangent function to represent the bare atom absorption background and two Voigt functions to fit the peaks. The results are listed in Table 2. Two broad peaks are identified in the XANES spectra; one at approximately 4.00 eV beyond the experimentally determined core binding energy (6212 eV) and the other at approximately 37.57 eV above the core L3 edge. A similar peak structure is observed in a rare earth oxygen environment in Joseph et al. [
Table 2
| Dopant | Peak 1–Eo (eV) | Peak 2–Eo (eV) | Peak 1/Nd yield ratio | Peak 2/Nd yield ratio | Reduced chi2 |
|---|---|---|---|---|---|
| Nd | 2.22 (6.71) | 35.93 (15.24) | 1.00 | 1.00 | 1.64 |
| Gd | 1.76 (6.65) | 37.46 (16.54) | 1.08 | 1.07 | 2.13 |
| Dy | 1.86 (6.97) | 36.75 (14.95) | 0.98 | 0.98 | 1.91 |
| Er | 2.19 (7.16) | 39.00 (14.87) | 1.07 | 0.93 | 1.42 |
| Average | 2.00 | 37.57 | 1.04 | 0.99 |
Tabulated are the results for fitting the XANES region of the doped samples with an arctangent function and two Voigt functions.
The “error” given in parenthesis in the Peak 1 and Peak 2 shifts from the inflection point (Eo), are the full width half maximums FWHM.
For rare earth materials where the rare earth atom is in the +3 valence state, the XANES spectra have a single peak white line, whereas for RE elements that adopt the +4 valence state (e.g., Ce and Pr), the XANES spectra typically have a double peaked white line which occurs due to additional interactions with the ligand environment [
Density functional theory studies of RE doped lithium tetraborate
To better ascertain the role the host matrix does play in the f to f transitions of the +3 rare earth ions in doped lithium tetraborate, we modeled the electron structure of Li2B4O7 doped with Nd, Gd, Dy, Er and Yb. Our calculations are carried out within density function theory (DFT) as implemented in the CASTEP software [
We built a cubic cell of Li16B32O56, as shown in Figure 9. Based on our EXAFS results that place the RE dopant in a Li+ site, one Li+ atom is then substituted by a Nd, Gd, Dy, Er, or Yb atom, representing 6.25% atomic doping which is much higher than the experimental level, but computationally tractable. Monkhorst-Pack [
Figure 9

The schematic of the structural geometry for Li15B32O56RE (RE = Nd, Gd, Dy, Er, or Yb). Oxygen (red), boron (gray), lithium (blue), and rare earth (green) are indicated.
Figure 10

The band structure and density of states of Li15B32O56Nd (A), Li15B32O56Dy (B), Li15B32O56Er (C), Li15B32O56Yb (D). In band structure plots vs. wave vector, spin up is black and spin down is red, while in the density of states plots the rare earth d state densities are blue, f state densities are red and boron p state density is green while the total density of states envelope is black. The density of states are plotted spin resolved.
In Li2B4O7:Nd (Figure 10A) and Li2B4O7:Dy (Figure 10B), we observe that nearly all the unoccupied 4f levels hybridize with the lithium tetraborate conduction bands. This could explain the similarity of the edge shift uncovered by the Latin hyper cube sampling (LHS) analysis summarized in Table 1 between Nd and Dy doped samples. We find that in Er the 4f levels, particularly the spin down component situated at EF do not mix with the host lithium tetraborate, whereas at 2–4 eV above EF, the f state population is very low (Figure 10C). For Li2B4O7:Yb (Figure 10D), there are few unoccupied 4f states, which leads to little depletion of the Yb 4f14 occupancy, unlike GaN:Yb [
The correlation U has been applied, as noted, to the rare earth 4f orbitals only, the remaining various orbital subset of orbitals may in some cases have applicable correlation energies as well. There is no a priori exclusion of multiple correlation energies, nor of wave vector dependence of the various possible correlation energies and such complications might well exist. This could lead to an incomplete (or insufficient) description of orbital hybridization effects including the luminescent and optical properties. In general, the increased hybridization will decrease excited state lifetimes and increase luminescent spectral feature widths, including the f to f transition spectral features. The contributions to f to f transition spectral broadening, nonetheless, arising from the strong rare earth hybridization with the lithium tetraborate lattice, are significant even without considering the variations in oxygen coordination, although Li2B4O7:Yb (Figure 10D) may be the exception. The variations in oxygen coordination evident from the EXAFS, and expected for a glassy lithium tetraborate, will be even more significant because of the strong rare earth hybridization with the lithium tetraborate lattice, affecting the f to f transition spectral broadening to a great degree.
Conclusion
Previous studies of rare earth doped lithium tetraborate glasses revealed asymmetry in the RE 4f spectral emission lines. In order to determine the source of the spectral line distortion, X-ray absorption fine structure studies were conducted in order to extract the local environment surrounding the rare earth dopants. The near edge absorption spectra data analysis indicates that for all of the rare earth doped samples studied (Li2B4O7:Nd, Li2B4O7:Gd, Li2B4O7:Dy, and Li2B4O7:Er), the dopant substitutes into the Li+ ion sites as RE3+. The empirically determined site was then used to perform a density functional theory calculation and determine the electronic source of the asymmetry in the spectral emission lines.
As a result of the doping, there is a slight expansion of the coordination shells (O and B atoms) that surrounded the original Li+ atom from approximately 2.0 Å to approximately 2.5 Å, the exact value depending upon the size of the rare earth. The results for rare earth doped borates compare well with expected bonding distances when compared with rare earth coordination number and atomic radii from Shannon [93], the radial distributions functions obtained from X-ray diffraction [
A qualitative XANES analysis confirms a +3 valence state and is consistent with our theoretical expectations. The resulting density functional theory calculations indicate there is strong hybridization with the unoccupied 4f orbitals with the host lithium tetraborate matrix. This hybridization is a likely the source of the spectral emission line distortion observed when the glass oxygen positional disorder is also taken into account.
Conflict of interest statement
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Statements
Acknowledgments
This work was supported by the Nebraska Public Power District through the Nebraska Center for Energy Sciences Research competitive grant program, the Defense Threat Reduction Agency (Grant No. HDTRA1-07-1-0008, HDTRA1-09-1-0060, and BRBAA08-I-2-0128), the NSF through the “QSPINS” MRSEC (DMR-0820521) at UNL. The views expressed in this article are those of the authors and do not reflect the official policy or position of the Air Force, Department of Defense or the U.S. Government.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
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Summary
Keywords
rare earth luminescence, lithium tetraborate, hyrbridization, x-ray absorption, local structure
Citation
Kelly TD, Petrosky JC, McClory JW, Adamiv VT, Burak YV, Padlyak BV, Teslyuk IM, Lu N, Wang L, Mei W-N and Dowben PA (2014) Rare earth dopant (Nd, Gd, Dy, and Er) hybridization in lithium tetraborate. Front. Physics 2:31. doi: 10.3389/fphy.2014.00031
Received
21 March 2014
Accepted
07 May 2014
Published
27 May 2014
Volume
2 - 2014
Edited by
Peter Fischer, Lawrence Berkeley National Laboratory, USA
Reviewed by
Fengqi Song, Nanjing University, China; Cesare Franchini, University of Vienna, Austria; Khim Karki, Brookhaven National Laboratory, USA
Copyright
© 2014 Kelly, Petrosky, McClory, Adamiv, Burak, Padlyak, Teslyuk, Lu, Wang, Mei and Dowben.
This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Peter A. Dowben, Department of Physics and Astronomy, University of Nebraska-Lincoln, Theodore Jorgensen Hall, 855 N 16th Street, Lincoln, NE, 68588-0299, USA e-mail: pdowben1@unl.edu
This article was submitted to Condensed Matter Physics, a section of the journal Frontiers in Physics.
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