Computational Materials Science 50 (2010) 356–362 Contents lists available at ScienceDirect Computational Materials Science journal homepage: www.elsevier.com/locate/commatsci Surface stability of potassium nitrate (KNO3) from density functional theory O.M. Løvvik a,b,⇑, T.L. Jensen c,⇑⇑, J.F. Moxnes c, O. Swang a,d, E. Unneberg c a SINTEF Materials and Chemistry, PO Box 124, Blindern, NO-0314 Oslo, Norway Department of Physics, University of Oslo, PO Box 1048, Blindern, N-0316 Oslo, Norway c Norwegian Defence Research Establishment, PO Box 25, NO-2027 Kjeller, Norway d Department of Chemistry, University of Oslo, PO Box 1033, Blindern, N-0315 Oslo, Norway b a r t i c l e i n f o Article history: Received 7 April 2010 Received in revised form 25 August 2010 Accepted 26 August 2010 Keywords: Potassium nitrate Surface energy Density functional theory a b s t r a c t Potassium nitrate has been studied by accurate DFT calculations. The bulk crystal structure and electronic structure were calculated and compared to previous studies. In addition, the surface stability of various faces was quantified, confirming that the {0 0 1} face has the lowest surface energy of 0.19 Jm 2. Other surfaces terminated by nitrate ions exhibited reconstructions upon relaxation, rotating the ions into an orientation parallel to the surface plane. Ó 2010 Elsevier B.V. All rights reserved. 1. Introduction Potassium nitrate (KNO3) has many applications, e.g. as a fertilizer, as an oxidizing agent in pyrotechnics, and in food preservation. The metastable c phase has been extensively studied due to its ferroelectric properties [1–5]. It has, however, been difficult to take any practical advantage of this, due to the lack of stability [6–9]. KNO3 crystallizes at room temperature into the a phase (also called phase II). For a long time it was believed that this phase belonged to the space group Pmcn (orthorhombic, with Z = 4) [10–12]. However, a neutron diffraction study by Adiwidjaja and Pohl demonstrated that the crystal structure actually consists of a 2 2 1 supercell of the Pmcn unit cell, with Z = 16 and within the space group Cmc21 [13]. The crystal structure transforms into the b phase (I) at around 128 °C when heated, and passes through the ferroelectric c phase (III) between 124 and 110 °C upon cooling. A number of phases also exists at lower temperatures [14,15]. Transitions between these phases have been extensively studied by a variety of techniques [7,16–41]. The growth of KNO3 crystals has been examined by several authors [42–46], and it has been shown that the {0 0 1} face has the lowest surface energy [43]. Other crystal faces have also been observed, including the {0 1 0}, {1 0 0}, {1 1 0}, {0 1 1}, {0 2 1}, ⇑ Corresponding author at: SINTEF Materials and Chemistry, PO Box 124, Blindern, NO-0314 Oslo, Norway. ⇑⇑ Corresponding author. E-mail addresses: ole.martin.lovvik@sintef.no (O.M. Løvvik), tomas-lunde.jensen@ffi.no (T.L. Jensen). 0927-0256/$ - see front matter Ó 2010 Elsevier B.V. All rights reserved. doi:10.1016/j.commatsci.2010.08.027 {0 1 2}, and {1 1 1} faces. An overview of the possibilities of different kinds of growth is given by Rolfs et al. [43]. Previous theoretical studies on this system have focused on the ferroelectric properties of the c phase [5,47,48] and on phase transitions [30,49]. The Hartree–Fock study by Aydinol et al. also presented calculations of bonding characteristics and the structural stability of various phases of KNO3 [5]. The present contribution has a slightly different focus. We report a detailed computational study of the bulk electronic structure of the a phase of KNO3, followed by an investigation of the stability of various surfaces. All calculations are performed within the scope of density functional theory (DFT) using a plane wave description of the electron density and periodic boundary conditions. 2. Methodology Calculations were performed within density functional theory (DFT) as implemented in the Vienna ab initio simulation package (VASP) [50,51], using the PBE generalized gradient approximation (GGA) density functional [52]. The projector augmented wave (PAW) method [53] was used to represent the electron density. This is a generalization of the linearized augmented plane wave (LAPW) and the pseudopotential (PP) methods, with reliability comparable to that of LAPW and efficiency close to that of PP methods [53]. All calculations were spin unrestricted, allowing for spin polarization. Despite this, no net spin density was seen for any of the systems described herein. DFT calculations were also performed applying the ab initio simulation package Quantum Espresso (QE) v4.0.3 [67], using the BLYP 357 O.M. Løvvik et al. / Computational Materials Science 50 (2010) 356–362 -117.8 -116.8 Fig. 1(b). The total energy convergence with respect to Ec is even worse for the norm-conserving potentials. We have plotted the behaviour for two different choices of the cut-off energy for charge Echarge; Echarge = 4 Ec (default) and Echarge = 2 Ec. Proper convergence has not been found in any of the cases, even when Ec is increased to more than 2000 eV (note the different scales on the axes of Fig. 1 (a) and (c)). This means that the convergence criterion we proposed (1 meV change of total energy/50 eV increase of Ec) may be too strict. After all, we are usually interested in relative energies, not the absolute total energy. To test another option, we plotted the calculated pressure of the experimental cell (which is non-zero because the applied density functional fails to predict the exact magnitude of the lattice parameters) as a function of Ec. The calculated pressure is an important quantity when performing automatic relaxation of the unit cell size (and shape), which can be used to search for unknown crystal structures [54]. For VASP, the pressure is apparently already converged (changes less than 1 kbar when Ec is increased by 50 eV) at 500 eV for the soft potentials (Fig. 1(b)). When using hard potentials, similar convergence is reached at a cut-off of 950 eV. In the case of QE using norm-conserving pseudopotentials, we see that a cut-off of 1360 eV is necessary to obtain proper convergence of the pressure (Fig. 1(d)). In this case we can clearly see that using Echarge = 2 Ec is necessary to obtain convergence; when the default value of Echarge = 4 Ec is used, the pressure seems to diverge when Ec is increased further. Another important set of parameters is the calculated forces, which are used when optimizing the ionic positions. We checked numeric convergence of the forces with respect to Ec in a similar vein as above. The convergence criterion was now that the force changes should be less than 0.05 eV/Å when Ec is increased with 50 eV. In the case of VASP we found converged of the forces for Ec = 450 and 600 eV for the soft and hard potentials, respectively. QE exhibited converged forces at Ec = 1224 eV when Echarge = 2 Ec; when Echarge = 4 Ec the forces were converged at 1496 eV. (b) Soft Hard -118 -117 -118.2 -117.2 400 900 Calculated pressure (kbar) (a) Total energy (eV) functional and norm-conserving pseudopotentials. The QE calculations allowed no spin polarization. The density of k points in the reciprocal space integration was always kept below 0.2 per Å 1. As an example, a gamma-centred 4 2 4 mesh was used for the Pmcn bulk unit cell. Convergence tests up to an 8 6 8 mesh confirmed that the uncertainty in total energy resulting from the chosen sampling was below 1 meV per unit cell. For slab calculations, only the gamma point was used in the vacuum direction. The tetrahedron method with Blöchl corrections was used to smear partial occupancies near the Fermi level. The criterion for self-consistence was a change in total electronic energy of less than 10 6 eV between consecutive electron density iterations. The QE calculations used the same density of k points. Computer codes for plane-wave calculations have often built in default values for energy cut-off. For KNO3, the default value would be 400 eV for the standard (soft) potentials in VASP. However, we expected an unusually strong perturbation of the N and/or O atoms upon formation of nitrate groups, and therefore conducted convergence tests of the total energy as a function of the kinetic energy cut-off Ec. Indeed, as seen in Fig. 1(a), the total energy changes dramatically with increasing Ec. The total energy is not properly converged (defined here as changing by less than 1 meV when increasing Ec by 50 eV) until Ec = 1250 eV. Even at this point the total energy continues to drop, and is 2.5 meV lower when Ec = 1500 eV. This indicates the existence of electron density changes uncommonly close to the atomic nuclei, and we found it necessary to repeat the test with harder potentials (smaller frozen core and higher plane wave cut-offs). These results are also shown in Fig. 1(a), and again we see that the default Ec (which is much higher (750 eV) for the hard potentials) is clearly insufficient to achieve convergence. This time, however, proper convergence is obtained at 950 eV, and the change in total energy is less than 0.1 meV when increasing Ec further to 1100 eV. We investigated the same convergence behaviour for QE, this is shown in 60 40 20 Hard 0 400 (d) -6420 4x -6422 2x -6424 -6426 400 900 1400 Energy cut-off (eV) 600 800 1000 Energy cut-off (eV) 1900 Calculated pressure (kbar) Total energy (eV) Energy cut-off (eV) (c) Soft 200 100 4x 2x 0 -100 -200 400 900 1400 Energy cut-off (eV) Fig. 1. Convergence of the calculated electronic total energy (a and c) and the calculated pressure (b and d) as a function of the energy cut-off of the kinetic energy plane wave expansion. The upper panels present VASP calculations with blue diamonds denoting standard (soft) potentials, and red squares denoting potentials with smaller frozen core and higher cut-offs (hard). The lower panels present data from QE calculations, with two different values of the charge density energy cut-off (augmentation cut-off); 4 and 2 times that of the kinetic energy cut-off, represented by blue diamonds and red squares, respectively. Lines are drawn as guides to the eye only. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) 358 O.M. Løvvik et al. / Computational Materials Science 50 (2010) 356–362 Table 1 Lattice constants, volume (V) and interatomic distances from experiment and DFT calculations using soft and hard PBE potentials with VASP as well as norm-conserving BLYPpotentials with QE The difference between the hard and soft potentials is the size of the core region, where the electron density is kept fixed. The energy cut-offs Ec are 400, 755.6, 950, and 1360 eV, respectively – the two former are default values for the respective potentials, while the latter are the converged values for the hard PBE and norm-conserving BLYP potentials. The number of formula units Z is 16 for the Cmc21 unit cell and 4 for the Pmcn unit cell. The minimum and maximum interatomic distances refer to the first coordination sphere – this includes three O atoms for N–O and nine O atoms for K–O. Ec (eV) Potential Z a (Å) b (Å) c (Å) V (Å3) N–O min. (Å) N–O max. (Å) K–O min. (Å) K–O max. (Å) Expt. (Ref. [13]) VASP PAW VASP PAW VASP PAW QE norm-cons 10.825 18.351 6.435 1278.3 1.23 1.26 2.81 2.95 400 PBE soft 16 10.58 17.87 6.00 1134 1.27 1.27 2.67 2.82 756 PBE hard 16 10.56 17.80 6.16 1159 1.26 1.26 2.70 2.83 950 PBE hard 16 10.97 18.57 6.56 1337 1.26 1.27 2.88 2.96 1360 BLYP 4 11.45 19.40 7.01 1558 1.28 1.29 3.03 3.13 It is necessary to use the hard version of the potentials for K, N, and O atoms in VASP to obtain a reliable calculated pressure. However, the largest effects are seen when going from the soft to hard version for oxygen; this suggests that oxygen has the largest electronic changes in the core region. Relaxations of bulk unit cells were performed by simultaneously optimizing atomic positions, unit cell size, and shape. A quasi–Newtonian formalism using the residual minimization scheme with direct inversion in the iterative subspace was used to minimize the forces. The convergence criterion for equilibrium was that all forces should be lower than 0.05 eV/Å. Most of the test calculations (finding convergence etc.) were performed using the Pmcn unit cell, rather than the four times larger Cmc21 structure. This saved much computational effort, but should pose no problems when it comes to reliability of the results, since the local bonding environment is very similar in the two structures. Also, the difference in calculated total energy per unit cell between the two models is within the error bar of the calculations (1 meV/unit cell), and the relaxed cell parameters were also very similar when using the different cells (differences were less than 0.3%). As an aside, we note that since our calculations are performed at 0 K, the crystal structure at room temperature will not necessarily coincide with the computed results, even assuming that the numerical model otherwise is perfect. An interesting future study would be to compare the energy of different KNO3 isomorphs as a function of temperature from phonon calculations. For the abovementioned reasons, it was decided to base all surface calculations on the Pmcn unit cell as well. Lattice constants were fixed at the bulk relaxed values, and positions were relaxed starting from the bulk relaxed positions. Surface energies were converged within 1 meV with a vacuum layer of 10 Å, which were used for initial calculations, screening surface energies for a number of different surfaces. In the calculations reported here, a vacuum layer of 16 Å was used to separate the slabs. Since the Cmc21 unit cell is a 2 2 1 supercell of the Pmcn unit cell, many of the surface indices are the same for the two models. Whenever there is room for doubt, it is specified for which crystal structure the index is valid. The number of atomic layers should be large enough to ensure bulk-like conditions in the middle of the slab without compromising numerical efficiency (one layer is here defined to consist of one formula unit). We found that six layers are sufficient to obtain converged atomic displacements after relaxation (less than 0.01 Å displacements in the mid layer). No atoms were kept fixed, as tests revealed that neither fixing a layer in the middle (to ensure bulk conditions) nor fixing a layer at one of the surfaces (to mimic bulk continuation) led to significant changes in energy or geometry compared to allowing all atoms to move freely. 3. Results and discussion As mentioned in the methodology section, it was important to use significantly increased cut-off energies to achieve reliable calculated pressures. It is interesting to see how this influences the predicted bulk crystal structure when using the experimental structure as input. Lattice constants of the relaxed crystal structure of KNO3 are given in Table 1 for different choices of potentials and Fig. 2. The PBE relaxed crystal structure of KNO3 in the Cmc21 crystal structure using a ball- and stick model seen along the c axis (a) and along the a axis (b). K, N, and O atoms are drawn as grey, blue, and red balls. In (c), the coordination of K by nine oxygen atoms is outlined with a polyhedron. The oxygen atoms are then drawn small when belonging to the first coordination sphere of the K atom, and large otherwise. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) 359 O.M. Løvvik et al. / Computational Materials Science 50 (2010) 356–362 (a) (b) O 0 O O N N O O 7.4 0 O 1 Fig. 3. Contour plot of the valence electron density (a) and the electron localization function (b) in a plane intersecting an NO3 unit. The electron density is plotted in units of e/Å3, and the scales are logarithmic. energy cut-offs, compared to the experimental structure reported by Adiwidjaja and Pohl [13]. The relaxed crystal structure using the hard potential in VASP with the highest cut-off is shown in Fig. 2. These results illustrate quite clearly the importance of using a high enough cut-off for the relaxation: while the default (non-converged) cut-off of the hard potentials (755.6 eV) leads to predicted lattice constants between 2.4% and 4.2% lower than experiment, the converged cut-off (950 eV) implies lattice constants between 1.2 and 1.9% higher than experiment. The numerical error resulting from using the default cut-off is thus up to 6% for the lattice constants, and more than 13% for the predicted volume. The case is even worse when using the soft potentials; the predicted lattice constants are then off by up to 8.5% and the volume by more than 15% from the converged values. This clearly demonstrates the necessity to use increased cut-off energies when performing automatic relaxation; an increase of approximately 30% is sufficient to approach reliable forces (see Fig. 1(b)), which is in accordance with general recommendations in the VASP guide. When the norm-conserving BLYP potentials are used in the relaxation, the lattice parameters are up to 9% higher than experiment, and the volume is 22% higher than experiment. This deviation is much larger than normally seen in band-structure calculations. To ensure that the automatic relaxation was not to blame, we performed a manual optimization of the cell volume keeping the relative lattice constants fixed. This gave an optimized cell volume within 0.1% of that obtained by the automatic relaxation, so we believe that the results presented in Table 1 are representative for the BLYP potential. The BLYP potentials are fitted to a set of atomic and molecular test systems, and this could be the explanation for being less suited to extended systems. Also, a recent test of various DFT potentials concluded that the largest deviation of the enthalpy of formation from the experimental one was found for NO2 in the case of BLYP [55]. The predicted enthalpy of formation was significantly lower than the experimental one, indicating that BLYP is underbinding the N–O system. This is consistent with the significant over-estimation of the unit cell volume found in the present study. It is important to note that the converged values of the PBE predicted lattice constants are larger than the experimental ones, even if the temperature was higher in the experiments (room temperature) than in our calculations (in principle 0 K). If temperature effects were taken into account, the predicted lattice constants would most probably be even larger, particularly since it is known that the aragonite structure can exhibit large anisotropy of the thermal expansion [30]. The difference between predicted and measured lattice constants would thus be more than 2%. We believe that except for the temperature, the PBE functional is the only significant remaining source of errors in the VASP calculations. Therefore, the DFT prediction of lattice constants is not so good for this compound, for any of the methods studied. The PBE potential is otherwise known to perform very well when it comes to prediction of lattice constants, but the present results suggest that at least in some cases this could be due to cancellation of errors. We have performed additional tests with VASP to see if this large discrepancy is due to the PBE potential, details are not presented here. Changing to the PW91 potential did not make a significant contribution to the overall picture; this also exhibited painstakingly slow convergence and clear over-estimation of the lattice constants. We will discuss possible reasons for the difficulties of predicting lattice constants in this system in the following. It is interesting to see how the choice of potential and cut-off influences the interatomic distances. We can see from Table 1 that the N–O distances are relatively unaffected by this choice, with all the potentials predicting slightly too high values. The largest difference is seen in the K–O distances, which can serve to explain the spread in predicted lattice constants. The potentials with default cut-off predict significantly diminished K–O distances compared to the experimental ones, while the hard potential with converged cut-off predict a K–O distance 2.3% larger than the experimental value. The latter difference is exactly the same as for the N–O distance when using the hard potential with converged cut-off. Since there is no direct bond between K and N, the K–N distances reflect the sum of the K–O and O–N distances. Thus, the poor performance of the soft potentials mainly influences the K–O bond lengths, predicting a too close contact. Some insight into why the soft potentials are insufficient for the system under study can be achieved by considering the electronic density in the plane defined by a nitrate ion. Fig. 3 shows how the absence of atomic symmetry stretches far into the core region of both nitrogen and oxygen atoms. This indicates a significant overlap of the N valence charge with the O core charge (and vice versa), increasing the importance of the core region for the bonding behaviour. The electron localization function (ELF) is also shown in Fig. 3. The ELF is related to the kinetic energy of the electrons, and can thus give a graphic picture of the chemical bonds [56]. The ELF confirms that significant parts of the N–O bond are located in the middle between the atoms, indicating a mainly covalent bond. There are no such bonds between K and O, reflecting the strong ionic character of the interaction between K+ and NO3 . There are suggestions of directional bonds towards K around the O atoms, but clearly centred at the O sites (they are seen as the strong red areas in two directions, perpendicular to the N–O bond, from the O atoms in Fig. 3 (b)). This can be seen more clearly in Fig. 4, where the valence charge density is plotted as lines between nearest O.M. Løvvik et al. / Computational Materials Science 50 (2010) 356–362 Valence charge density (e/Å3) 360 7 6 K-O 5 N-O 4 3 2 1 0 0.0 0.2 0.4 0.6 0.8 1.0 Normalized interatomic distance Fig. 4. The valence charge density in e/Å3 between N and O (red solid curve) and between K and O (blue dashed curve) as a function of the interatomic distance. The distance has been normalized for ease of comparison. Oxygen is placed at relative distance 1 in both cases. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) neighbour N–O and K–O pairs. It can be clearly seen how there remains a significant valence charge between N and O, while it vanishes in the middle between K and O. It is also notable how far into the core of the oxygen atom the bond is reaching in the case of K– O; this is probably why a small core region and high energy plane waves are needed to describe this bond properly. We may regard the potassium atom as a spherical, rather hard cation polarizing the nitrate anion. The calculated density of states (DOS) of bulk KNO3 with the PBE functional is shown in Fig. 5. The PBE–GGA calculated band gap is 3.0 eV. Since GGA tends to significantly underestimate the band gap, we expect that the real band gap is somewhat higher; strongly suggesting that KNO3 is an insulator. Indeed, an experimental band gap of 6–7 eV has been reported [57]. Three distinct regions are clearly visible in the valence region. Between approximately 8 and 7 eV a relatively narrow section is seen with very similar shape for all the three elements; the N states are of purely p character, the O states are both s and p, while the K states exhibit both s, p, and d character. These features thus suggest both N–O and K–O interactions. The next filled region is between 2.5 and 1.5 eV, and is dominated by pure O-p states, as well as more K states with s, p, and d character. This indicates an interaction between K and O. The last valence region lies between 0.5 and 0 eV, and contains O-p states as well as K-p and d states. The narrow and non-connected shape of the DOS confirms the picture of an ionic solid with strong N–O and K–O interactions at low energies. We now turn to the calculations of surface energies. The surface energy of a particular face can be calculated by inserting a vacuum layer between two opposite faces; the difference in total energy between the resulting slab and the bulk is then equal to twice the surface energy. The surface energy is converged already when the size of the vacuum layer is 10 Å, but we have nevertheless used vacuum layers of 16 Å between the slabs in order to manipulate surfaces in a later study without the risk of interaction between images. In calculations of surface energies of metals, it is important to use an alternative way of defining the bulk reference energy to avoid linear divergence of the surface energy as the number of layers is increased [58]. One typical way to obtain this is to calculate the total energy of a series of slabs with increasing number of layers, and use the (interpolated) difference in energy between such slabs as the bulk reference energy [58]. It has later been shown that this is not so important for insulators, for which only a few layers usually are sufficient to obtain convergent surface energies, and the Fig. 5. The calculated local and total density of states (DOS) calculated by VASP. The s-projected (filled blue), p-projected (solid black) and d-projected (dotted red) DOS are shown for K, N, and O, as well as the total DOS for KNO3 (filled green). The energy is measured in eV relative to the Fermi level, and the DOS units are states/ (atomunit cell volume) for the local DOS and states/unit cell volume for the total DOS. (For color interpretation given in this figure legend the reader is referred to see the web version of this article.) true bulk energy can be used as the bulk reference energy [59]. We have found this to be the case for KNO3, and in the data in Table 2 show that the three methods give surface energies differing by only a few percent. All other surface energies are thus calculated using the true bulk energy as the reference energy. Whether to relax the fractional coordinates for the whole slab or only parts of it, is also a matter of choice. It is sometimes chosen to keep one or more layers at one side of the slab frozen; this side then represents a continuation into the bulk geometry [60]. This approach makes it possible to induce an unphysical polarization, and is often avoided for dielectric materials. Another option is to keep one or more layers frozen in the middle of the slab to ensure bulk geometry. We have compared these options with calculations allowing all atoms to relax. No significant differences were found, except for movements of the atoms that were kept fixed. Even the neighbour atoms of the fixed ones changed very similarly in all the three cases. We have therefore chosen to relax all atoms in the Table 2 Surface energies (in J/m2) for different faces of KNO3. Relaxed and unrelaxed slabs are compared in some cases. For the {0 0 1} face, two different bulk reference energies were tested: The true bulk energy (‘‘Bulk”) and an interpolated energy representing the middle layer of the slab for an increasing number of slab layers (‘‘Slab series”; see text and Ref. [58] for details). Some of the faces can be chosen to be terminated by either NO3 (‘‘NO3 top”) or K (‘‘K top”). The {1 1 2} face of the Cmc21 unit cell corresponds to the {1 1 1} face of the smaller Pmcn unit cell. Similarly, the {1 1 4} face corresponds to the {1 1 2} face. The results marked with an asterisk are calculated by QE, other results are by VASP. Face {0 0 1} {0 0 1} {0 1 0} {0 1 0} {1 0 0} {1 1 0} {1 1 0} {1 1 2} {1 1 4} {0 0 1} Bulk NO3 top K top NO3 top K top NO3 top K top NO3 top* Slab series Unrelaxed Relaxed Unrelaxed Relaxed 0.235 0.671 0.894 0.410 0.593 0.862 0.410 1.020 0.658 0.148 0.199 0.544 0.666 0.344 0.250 0.297 0.337 0.219 0.662 0.193 O.M. Løvvik et al. / Computational Materials Science 50 (2010) 356–362 remaining calculations. The change in surface energy when going from the unrelaxed to the relaxed slab varies from around 10% to 65%, see Table 2. This reflects the very different degree of surface reconstruction for the different surfaces, as illustrated in Fig. 6, where side-views of some of the surfaces of this study are shown. It is clear from Fig. 6 that the reconstruction of the NO3 terminated {1 1 0} surface involves rotating the NO3 units into the surface plane. Thus, the O atoms initially pointing out of the surface move closer to neighbouring K+ ions, which leads to electrostatic stabilization. This does not happen in the {010} face covered by K+ ions, as the surface is covered by spherically symmetric ions. We note that the most stable face – {0 0 1} – is the only face with the NO3 units already oriented parallel to the surface. This compares favourably with experiments, which have shown that the {0 0 1} face is indeed the most stable one. The calculated surface energy of 0.19 Jm 2 is very similar to that of other ionic crystals, e.g. 0.16 Jm 2 for NaCl [61,62] and 0.17 Jm 2 for Li2CO3 [63]. It is in many cases possible to create different surface terminations for a specific face. As an example, the {1 1 0} face can have at least three different terminations, even when enforcing stoichiometry. The structure shown in Fig. 6 is terminated by NO3 on both sides of the slab – this is called ‘‘NO3 top” in Table 2 Alternatively, the lower two NO3 units may be moved to the top of the slab, yielding a slab with two different terminations – NO3 on one side and K+ on the other. (This would create an unphysical dipole moment, and has not been studied here.) If the lower pair of K+ ions (one is hidden behind the other) is also moved from bottom to top, the slab is terminated by K+ ions on both sides. This is called ‘‘K top” in Table 2. Reconstructions play different roles for different surface terminations. This can be illustrated by the three various situations in Fig. 6. In the case of the {0 0 1} face, there is little energy to be gained by reconstruction, since the NO3 ions are already parallel to the surface. Neither does reconstruction take place for the K terminated {0 1 0} face; in this case electrostatic interaction energy can only be slightly increased by reconstruction. This changes, however, when moving to the NO3 covered {1 1 0} face. The bulk cut structure exhibits oxygen ions pointing directly out of the surface plane, which obviously is an expensive construction as the surface energy is relatively high for this surface before relaxation. 361 After relaxation, however, the surface energy is 65% lower, due to the reconstruction of NO3 ions. This brings the NO3-covered {1 1 0} face lower in energy than the K-covered analogue. The opposite was the case before relaxation, emphasizing the importance of the reconstruction. 4. Conclusions Density functional calculations of KNO3 have been performed within the generalized gradient (PBE) approximation using hard PAW potentials and norm-conserving potential. Thorough investigations of convergence demonstrated that very high cut-off energies were required to obtain reliable energies, forces, and pressure. This tendency proved particularly strong for the default (‘‘soft”) potentials, and harder versions were required for proper convergence. We attribute this to the unusual bonding within the nitrate group, with electronic changes taking place far into the core region of the oxygen atoms. Analysis of the electron density and electron localization functions gives a picture of strongly ionic interactions between K+ and NO3 , and strongly covalent bonds between N and O. Standard potentials predict lattice constants up to 8.5% higher for the VASP calculations and 9% for the QE calculations, compared to the results found using the proper choice of parameters. The converged calculations predict slightly elongated lattice constants (up to 2%) compared to experimental values. Various crystal faces were constructed using a slab structure with vacuum between the slabs. Relaxation of the slabs demonstrated that NO3 units with oxygen pointing out of the surface plane reconstructed upon relaxation, bringing oxygen into the surface plane. The surface with the lowest surface energy was the {0 0 1} face, in which the NO3 ions are parallel to the surface already in the bulk cut structure. The surface energy was found to be 0.19 Jm 2. Acknowledgements A generous grant of computer time from the Norwegian Metacenter for Computing Science (NOTUR) and Norwegian Defence Research Establishment are gratefully acknowledged. References Bulk cut 001 010 110 Relaxed Fig. 6. Some of the faces of this study, seen from the side. The slabs are bulk cut (not relaxed, upper row) and relaxed (lower row). The {0 0 1} (NO3 top), {0 1 0} (K top), and {1 1 0} (NO3 top) faces are shown from left to right. Note the orientation of the NO3 ions (blue and red balls), which in the case of the {1 1 0} face is rotated parallel to the surface plane upon relaxation. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) [1] A. Chen, F. Chernow, Physical Review 154 (2) (1967) 493. 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