Non-collinear magnetism in WIEN2k
Non-collinear magnetism in WIEN2k
Non-collinear magnetism in WIEN2k
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Augmentation (...)ϕ AP W⃗Gσ(⃗k)ϕ LO⃗Gσ α == ∑ σ α ∑(LA ⃗ Gσ αL(A ⃗ Gσσ αu σαlLu σαl+ B ⃗ Gσσ αL+ B ⃗ Gσσ αL˙u σαl+ C ⃗ Gσ αL)˙u σαl Y L χ σ α,)u σα2,l Y L χ σ αA L , B L , C L are calculated from sphere boundary conditions.for APW/LAPW match<strong>in</strong>g is done to ↑ and ↓ plane waves <strong>in</strong> aglobal sp<strong>in</strong> coord<strong>in</strong>ate frame. Thus A L , B L depend on global σand local σ α sp<strong>in</strong> <strong>in</strong>dexes, and on k-po<strong>in</strong>t.LO has to vanish at a sphere boundary. It is a pure sp<strong>in</strong>or <strong>in</strong> alocal coord<strong>in</strong>ate frame (A L , B L , C L depend only on σ α ).for APW type of basis B = 0 <strong>in</strong> PW and LO, and additional localorbital “lo” is <strong>in</strong>troduced with C = 0, and B ≠ 0.wien workshop 2003 – p.19/40