Dear Wien2k users, Is there any detailed introduction of the spin-orbit coupling calculation?
I have a couple of questions, for example: 1.What’s the context of this case.normso, is it the density in the spherical sphere? 2.How does the density of full BZ calculated from B type symmetry operations on irre k points in lapw2 procedure since B type invert the spin dn to spin up? It seems the input files of “lapw2 -up -so” only use the up information, without dn information. 3.If one use the scaler relativistic in the sphere and non-relativistic in interstitial, will the radius function at the transition radius Rc be discontinuous? Looking forward to your reply. Best wishes, Rossie.
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