Generalized Bloch condition
Spin spirals may be conveniently modeled using a generalization of the Bloch condition (set LNONCOLLINEAR=.TRUE. and LSPIRAL=.TRUE.):
i.e., from one unit cell to the next the up- and down-spinors pick up an additional phase factor of and , respectively,
where R is a lattice vector of the crystalline lattice, and q is the so-called spin-spiral propagation vector.
The spin-spiral propagation vector is commonly chosen to lie within the first Brillouin zone of the reciprocal space lattice, and has to be specified by means of the QSPIRAL-tag.
The generalized Bloch condition above gives rise to the following behavior of the magnetization density:
This is schematically depicted in the figure at the top of this page:
the components of the magnization in the xy-plane rotate about the spin-spiral propagation vector q.
Basis set considerations
The generalized Bloch condition redefines the Bloch functions as follows:
This changes the Hamiltonian only minimally:
where in and the kinetic energy of a plane wave component changes to:
In the case of spin-spiral calculations the cutoff energy of the basis set of the individual spinor components is specified by means of the ENINI-tag.
Additionally one needs to set ENMAX appropriately:
ENMAX needs to be chosen larger than ENINI, and large enough so that the plane wave components of both the up-spinors as well as the components of the down-spinor all have a kinetic energy smaller than ENMAX.
This is the case when:
where
In most cases it is more than sufficient to set ENMAX=ENINI+100.
To judge whether ENMAX is chosen large enough one will always get a warning at runtime, e.g.
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| |
| W W AA RRRRR N N II N N GGGG !!! |
| W W A A R R NN N II NN N G G !!! |
| W W A A R R N N N II N N N G !!! |
| W WW W AAAAAA RRRRR N N N II N N N G GGG ! |
| WW WW A A R R N NN II N NN G G |
| W W A A R R N N II N N GGGG !!! |
| |
| To represent the spin spiral you requested, with a kinetic |
| energy cutoff of ENINI= 300.00 eV, choose ENMAX > 331.21 eV |
| Currently ENMAX= 400.00 eV |
| |
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