This page should give you a brief introduction to the theoretical
This page should give you a brief introduction to the theoretical background of the KKRsusc program. To find more details on the theory and a detailed description on the method follow these links:
background of the KKRsusc program. To find more details on the theory
and a detailed description on the method follow these links:
*[S. Lounis et al., Phys. Rev. Lett. 105, 187205 (2010)](http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.105.187205)
\*[S. Lounis et al., Phys. Rev. Lett. 105, 187205 (2010)](http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.105.187205)\*[S. Lounis et al., Phys. Rev. B 83, 035109 (2011)](http://journals.aps.org/prb/abstract/10.1103/PhysRevB.83.035109)\*[B. Schweflinghaus et al., Phys. Rev. B 89, 235439 (2014)](http://journals.aps.org/prb/abstract/10.1103/PhysRevB.89.235439)
*[S. Lounis et al., Phys. Rev. B 83, 035109 (2011)](http://journals.aps.org/prb/abstract/10.1103/PhysRevB.83.035109)
*[B. Schweflinghaus et al., Phys. Rev. B 89, 235439 (2014)](http://journals.aps.org/prb/abstract/10.1103/PhysRevB.89.235439)
## Projected Green function
## Projected Green function
The Kohn-Sham (KS) Green function (GF) is the resolvent of the
The Kohn-Sham (KS) Green function (GF) is the resolvent of the corresponding Hamiltonian, <spandir="">G\_{\\text{KS}}(E) = (E - \\mathcal{H}\_{\\text{KS}})^{-1}</span>. In the Korringa-Kohn-Rostoker Green function (KKR-GF) method, space is partitioned into nonoverlapping regions surrounding the atoms, labeled <spandir="">i</span>. These regions are taken as spherical in the atomic sphere approximation (ASA), and the KS potential is also assumed to be spherical around each atom, <spandir="">V\\^{\\text{KS}}\_i(r)</span>, with <spandir="">r = |\\vec{r}\\,|</span> and <spandir="">\\hat{r} = \\vec{r}/r</span>. Then the KS GF is expressed in terms of energy-dependent scattering solutions for each atomic potential, <spandir="">R\_{i\\ell}\\^\\sigma(r;E)\\,Y\_{L}(\\hat{r})</span> and <spandir="">H\_{i\\ell}\\^\\sigma(r;E)\\,Y\_{L}(\\hat{r})</span>, which are products of radial functions and (real) spherical harmonics, for each spin <spandir="">\\sigma = \\;\\uparrow,\\,\\downarrow</span> and angular momentum <spandir="">L = (\\ell,m)</span>. <spandir="">R\_{i\\ell}\\^\\sigma(r;E)</span> is regular at the center of the ASA sphere, and <spandir="">H\_{i\\ell}\\^\\sigma(r;E)</span> diverges there.
corresponding Hamiltonian, $G_{\text{KS}}(E) = (E -
\mathcal{H}_{\text{KS}})^{-1}$. In the Korringa-Kohn-Rostoker Green
function (KKR-GF) method, space is partitioned into nonoverlapping
regions surrounding the atoms, labeled $i$. These regions are taken as
spherical in the atomic sphere approximation (ASA), and the KS potential
is also assumed to be spherical around each atom,
$V\^{\text{KS}}_i(r)$, with $r = |\vec{r}\,|$ and $\hat{r} =
\vec{r}/r$. Then the KS GF is expressed in terms of energy-dependent
scattering solutions for each atomic potential,
$R_{i\ell}\^\sigma(r;E)\,Y_{L}(\hat{r})$ and
$H_{i\ell}\^\sigma(r;E)\,Y_{L}(\hat{r})$, which are products of
radial functions and (real) spherical harmonics, for each spin $\sigma
= \;\uparrow,\,\downarrow$ and angular momentum $L = (\ell,m)$.
$R_{i\ell}\^\sigma(r;E)$ is regular at the center of the ASA
sphere, and $H_{i\ell}\^\sigma(r;E)$ diverges there.
The Korringa-Kohn-Rostoker Green function is given by
The Korringa-Kohn-Rostoker Green function is given by
where $r_{\text{min}} = \min(r,r')$ and $r_{\text{max}} = \max(r,r')$, and $G^{\sigma,\text{str}}_{iL,jL'}(E)$ is the structural GF, describing backscattering effects.
where <spandir="">r\_{\\text{min}} = \\min(r,r')</span> and <spandir="">r\_{\\text{max}} = \\max(r,r')</span>, and <spandir="">G^{\\sigma,\\text{str}}\_{iL,jL'}(E)</span> is the structural GF, describing backscattering effects.
Near the Fermi energy (<spandir="">E\_\\text{F}</span>) one may approximate <spandir="">R\_{i\\ell}\\^\\sigma(r;E) \\approx R\_{i\\ell}\\^\\sigma(r;E\_\\text{F})</span>.
We now notice that the quantities present in the Green's function (The regular <spandir="">R(\\mathbf{r};E)</span>, and irregular <spandir="">H(\\mathbf{r};E)</span> component of the radial wave function) depend on both the energy and the position. This would make many calculations unfeasable, thus a separation of the energetic and spatial components is used.
Near the Fermi energy ($E_\text{F}$) one may approximate
Using a new basis set <spandir="">\\ket{\\phi\_{ilb}}</span>, where <spandir="">i</span> accounts for the lattice site, <spandir="">l</span> for the orbital, and <spandir="">b</span> for the energy. One can disentangle the spatial dependence using
@@ -61,10 +53,7 @@ The transverse magnetic Kohn-Sham susceptibility is given by
...
@@ -61,10 +53,7 @@ The transverse magnetic Kohn-Sham susceptibility is given by
\end{aligned}
\end{aligned}
```
```
Here, <spandir="">\\chi\_{\\uparrow\\downarrow}</span> and <spandir="">\\chi\_{\\downarrow\\uparrow}</span> correspond to <spandir="">\\chi\_{+-}</span> and <spandir="">\\chi\_{-+}</span>, respectively.
Here, $\chi_{\uparrow\downarrow}$ and
$\chi_{\downarrow\uparrow}$ correspond to $\chi_{+-}$ and
$\chi_{-+}$, respectively.
### Dyson-like equation
### Dyson-like equation
...
@@ -72,8 +61,7 @@ $\chi_{-+}$, respectively.
...
@@ -72,8 +61,7 @@ $\chi_{-+}$, respectively.
#### Dyson equation
#### Dyson equation
Let us turn our attention to the Dyson equation for the GF, including
Let us turn our attention to the Dyson equation for the GF, including the self-energy describing the coupling to the magnetic excitations:
the self-energy describing the coupling to the magnetic excitations: