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Ab initio investigations of magnetic properties of ultrathin transition ...

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16 2 The FLAPW method<br />

1<br />

0<br />

0 1<br />

Figure 2.1: The division <strong>of</strong> space in the APW method. The muffin-tin spheres (MT) are<br />

surrounded by the interstitial region (I).<br />

functions. The expansion coefficients cijk are determined from the secular equation, via<br />

the Rayleigh-Ritz principle [74]:<br />

�<br />

[Hjj ′(k) − ɛνkSjj ′(k)]cνjk =0, (2.2)<br />

j<br />

where<br />

�<br />

Hjj ′(k) = ϕjk(r)[<br />

Ω<br />

−∇2 ↑(↓)<br />

+ Veff 2 ]ϕj ′ k(r)d 3 r (2.3)<br />

are the elements <strong>of</strong> the Hamilton matrix and<br />

�<br />

Sjj ′(k) =<br />

ϕjk(r)ϕj<br />

Ω<br />

′ k(r)d 3 r (2.4)<br />

are the so-called overlap matrix elements. The integrals are evaluated over the volume <strong>of</strong><br />

the unit cell (Ω). The type <strong>of</strong> functions {ϕjk} chosen, may or may not be energy-dependent,<br />

determines the detailed solution <strong>of</strong> the secular equation. The eigenvalues always follow from<br />

the condition<br />

det |Hjj ′(k) − ɛνkSjj ′(k)| =0. (2.5)<br />

If plane waves are chosen as basis functions. They are orthogonal, diagonal in momentum<br />

and any power <strong>of</strong> momentum and the implementation <strong>of</strong> planewave based methods is<br />

rather straightforward because <strong>of</strong> their simplicity.<br />

The APW is powerful approach but requires a solution on non-linear equations due to<br />

the matching between augmented functions the plane waves. This problem is explained in<br />

the next section, and it will be shown how it is useful to linearize the equations around

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