As in the nonmagnetic BOPunscr, the unscreened bond integrals βτ have the GSP functional form described by eq. (3.2) [69], supplemented by the fifth-order polynomial as the cut-off function (see Section 3.1 for details). We use the same parameters as in Fe BOP developed by Mrovec et al. [35] with minor modification of the cut-off function to ensure that no unphysical bumps occur. This is achieved by increasing BI
cut
R from the original value of 3.7 Å used by Mrovec et al. to 4.0 Å with all the other parameters remaining the same. Table 5-1 summarizes the parameters used in the unscreened bond integrals, and Figure 5-1 shows the R-dependence of the bond integrals.
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Table 5-1. The parameters of unscreened bond integrals (eq. (3.2)) used in BOPunscr for
bcc Fe. The parameters are taken from [35], with only BI cut
R changed to a larger value in order to avoid any unphysical bumps in the tail function. The unit of βτ
( )
R0 is eV; R0,c
R , R1BI and RcutBI are in Å; na and nc are dimensionless.
( )
R0 τ β R0 Rc R1BI BI cut R na nc ddσ – 0.6450 2.4930 4.2336 3.0 4.0 3.5805 6.7179 ddπ 0.3380 2.4930 4.2336 3.0 4.0 5.0703 5.3437 ddδ – 0.0450 2.4930 4.2336 3.0 4.0 8.5802 0.027297
As in the nonmagnetic BOPs, screened bond integrals are analytically represented by the functional form ij
( )(
1 ij)
ij
R S
τ τ τ
β =β − (eq. (3.3)), where βτ
( )
Rij takes thesimplified GSP function eq. (3.4) and Sij
τ is defined in eq. (3.5). Again βτ
( )
Rij is cutoffby a fifth-order polynomial (see Section 3.1 for details). The parameters in βτ
( )
Rij andij
Sτ are used to fit the OTB-sd data obtained from the method of Urban et al. [32] for extracting bond integrals from DFT calculations using the projection formalism. The calculation of the OTB-sd bond integrals was done by our collaborator Dr. Mrovec. The parameters of screened bond integrals used in Fe BOPscr are summarized in Table 5-2.
The R-dependence of the OTB-sd bond integrals, deduced from DFT calculations, the screened bond integrals ij
τ
β and the simplified GSP function βτ
( )
Rij are shown in Figure5-2. The general features of the OTB-sd bond integrals are similar to those found in group 5 and 6 non-magnetic transition metals. In OTB-sd data, the discontinuity of bond integrals in the region between the first and second nearest neighbor of the bcc lattice is again apparent in ddπ and ddδ bond integrals and less pronounced in ddσ bond integral. This is well reproduced by the screened bond integrals represented by
ij
( )(
1 ij)
ij
R S
τ τ τ
β =β − . Although the reproduction of the discontinuity in ddδ bond
integrals is less satisfactory than for ddπ integrals, these bond integrals are approaching zero at the second nearest neighbors and, presumably, play only a minor role in the overall performance of the resulting BOPsrc.
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Table 5-2. Parameters entering equations (3.3), (3.4) and (3.5) for screened bond integrals used in BOPscr for bcc Fe. Units of βτ
( )
R0 and O Rτ( )
0 are eV; R0, Rc, R1BI and RcutBI inÅ.
( )
R0 τ β O Rτ( )
0 R0 Rc R1BI RcutBI sdσ 0.845 –0.045 2.4825 0.71 2.6 4.0 ddσ – 0.620 0.040 2.4825 0.71 2.6 4.0 ddπ 0.410 – 0.030 2.4825 0.47 2.6 4.0 ddδ – 0.062 0.020 2.4825 0.31 2.6 4.0Figure 5-2. Screened bond integrals used in BOPscr for bcc Fe. Dots: OTB-sd data. Solid
line: analytic screened bond integrals. Dashed line: simplified GSP function (eq. (3.4)). The red and blue color correspond to R from the regions of the first and second nearest neighbors, respectively.
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The repulsive part of the cohesive energy is again composed of two contributions, a pairwise interaction (Epair) and an environment dependent contribution (Eenv). The
functional forms of Epair and Eenv are the same as in the BOPs for non-magnetic metals
(see Chapter 3). The parameters in Epair and Eenv are adjusted so that the resulting BOPs
reproduce the fundamental physical properties of the equilibrium ferromagnetic bcc Fe, the cohesive energy, three elastic constants (C11, C12 and C44) and the equilibrium lattice
constant. The experimental values of these properties to which the BOPs are fitted are summarized in Table 5-3. Moreover, in order to assure the BOP behaves reasonably when atoms are significantly closer to each other than the first nearest neighbor spacing in the equilibrium bcc lattice, the parameter R0 in Epair is chosen to be slightly smaller than the first nearest neighbor spacing. The parameter B0 in Epair is then adjusted to
reproduce the energy dependence on the lattice parameter when the bcc lattice is hydrostatically compressed, calculated using a DFT method (VASP) with spin polarization included. Figure 5-3 shows the comparison for this energy dependence calculated using DFT and BOPs, respectively. The results obtained using BOPunscr and
BOPscr are both in a very good agreement with the DFT calculation. The parameters used
in Eenv and Epair for both BOP
unscr and BOPscr are summarized in Tables 5-4 and 5-5.
The R-dependence of the pair potential Φ in Epair is shown in Figure 5-4. As in the BOPs
for non-magnetic metals, a slight attractive part exists in the vicinity of the separation of the second nearest neighbors in both BOPunscr and BOPscr, which presumably arises from
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Table 5-3. Experimental values [81, 112] to which the BOPs for Fe are fitted. Cohesive energy (Ecoh) is in eV, elastic moduli in 1011 Pa, and lattice parameter (a) in Å.
Ecoh C
11 C12 C44 a
4.28 2.431 1.381 1.219 2.8665
Figure 5-3. Dependence of the energy difference between the hydrostatically compressed bcc lattice of Fe and its equilibrium bcc lattice, ∆E, on acom/a, where acom is the lattice
parameter of the compressed bcc lattice. Lines: BOPs. Dots: DFT.
Table 5-4. Parameters used in the environment dependent repulsion (Eenv), given by
equations (3.7), (3.8) and (3.9) in Chapter 3, for BOPunscr and BOPscr for bcc Fe. Rij is in
units of the lattice parameter a. Rs = 0.52 (in units of a). µ, g and ν are dimensionless.
Fe A [eV] µ g ν R1rep [Å] rep
cut
R [Å]
BOPunscr 5.498×101 7.0 20.0 6.0 3.0 4.0
101
Table 5-5. Parameters used in the pair potential Φ, given by eq. (3.10) in Chapter 3, for BOPunscr and BOPscr for bcc Fe. Rk is in Å and Bk in eV Å-3, when Rij is in Å. In all cases,
R0 is chosen to be 0.9 of the first nearest neighbor spacing of the equilibrium bcc lattice.
Fe BOPunscr BOPscr
k Rk Bk Rk Bk 0 2.23 35.0 2.23 30.0 1 2.75 − 0.486 028 26 2.75 − 0.972 681 58 2 2.90 2.428 666 99 2.90 2.516 912 64 3 3.50 1.198 115 96 3.50 0.693 543 45 4 3.70 − 0.780 182 45 3.80 − 0.412 698 08
Figure 5-4. The R-dependence of the pair potential Φ used in BOPunscr and BOPscr for Fe.
The first, second and third neighbor spacings in the equilibrium bcc lattice are marked as vertical lines denoted as 1st, 2nd and 3rd, respectively.
102