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###### Perform Impurity calculations using kkrflex {#perform_impurity_calculations_using_kkrflex}
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##### Theory
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#### Motivation
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STS (Scanning tunnelling spectroscopy) is an experimental technique
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which provides information about the electrons charge density resolved
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on energy and position. This allows to extract a compound surface
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properties such its surface states and densities. One main features STS
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allows to access are the standing waves patterns which correspond to
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charge oscillations generated by an impurity and which decays with a
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power law from it. Due to the presence of many impurities at different
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positions and the superposition of different standing waves the
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topographic data is very difficult to interpret. For this reason a
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Fourier transform (FT) is performed in order to access main scattering
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processes.
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#### Stationary phase approximation (SPA) {#stationary_phase_approximation_spa}
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The spin, energy and position resolved density in presence of an
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impurity is: \\\\ \$\\Delta n (\\vec{r}
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\\sigma;E)=-\\frac{1}{\\pi}\\mathrm{Im} \\left\\langle \\vec{r}\\sigma
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\\left\| G\_{imp}(E)-G\_{host}(E) \\right\| \\vec{r} \\sigma
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\\right\\rangle\$. \\\\ In a non-degenerate case this Green\'s function
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difference can be written under the form: \\\\ \$\\Delta G(\\vec{r} +
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\\vec{R}\_n,\\vec{r} + \\vec{R}\_n;E) = - \\frac{1}{\\Omega\_{rec}\^2}
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\\int\\limits\_{0}\^{+\\infty} dt \\ dt\' \\int d\^2\\vec{k} \\
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d\^2\\vec{k}\' \\Psi\_{\\vec{k}}(\\vec{r})
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\\mathcal{T}\_{\\vec{k}\\vec{k}\'} \\Psi\^{\*}\_{\\vec{k}\'}(\\vec{r})
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e\^{i\\Phi}\$ \\\\ where \$\\Phi=(E-\\epsilon\_{\\vec{k}}+\\eta)t +
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(E-\\epsilon\_{\\vec{k}\'}+\\eta\')t\' +
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(\\vec{k}-\\vec{k}\')\\cdot\\vec{R}\_n\$.
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The main idea behind the SPA is to suppress the quick \$\\vec{k}\$ and
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\$t\$ oscillations in the above integral. The waves having the same
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phase will sum constructively while the ones with different phases will
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sum incoherently cancelling their contribution.This can be done looking
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for points \$\\{ \\vec{k}\_0,\\vec{k}\_0\',t\_0,t\_0\' \\}\$ which makes
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the phase \$\\Phi\$ stationary. This gives the following set of
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equations: \\\\ \$\\left\\{\\begin{array}{ll}\\vec{R}\_n &= -
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v\_{\\vec{k}\_0\'}t\_0\'\\\\\\vec{R}\_n &= v\_{\\vec{k}\_0}t\_0 \\\\E &=
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\\epsilon\_{\\vec{k}\_0} \\\\E &=
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\\epsilon\_{\\vec{k}\_0\'}\\end{array}\\right.\$ \\\\
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This means that the velocities at \$\\vec{k}\_0\$ and \$\\vec{k}\_0\'\$
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must be parallel but with an opposite direction. Furthermore the states
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defined by the previous wave vectors must lie in the same energy shell.
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Within these conditions one can obtain the difference in the density
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performing the integrals and trace calculation on spins, which results
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in : \\\\
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\$\\Delta n
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(\\vec{R}\_n+\\vec{r};E)=\|A\_{\\vec{k}\_0,\\vec{k}\_0\'}(\\vec{r})\|
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\\frac{\\sin((\\vec{k}\_0-\\vec{k}\_0\')\\cdot
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\\vec{R}\_n+\\phi\_{\\vec{k}\_0,\\vec{k}\_0\'})}{\|\\vec{R}\_n\|}\$
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where \$\|A\_{\\vec{k}\_0,\\vec{k}\_0\'}(\\vec{r})\| \\propto
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\|\\mathcal{T}\_{\\vec{k}\_0,\\vec{k}\_0\'}\|\$. The above relation
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shows that the density oscillates with respect to the position of the
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site n. It is also observed that this oscillation on the density has an
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\$1/\|\\vec{R}\_n\|\$ envelope. More generally the envelope has a power
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law shape which depends on the type of impurity (point defect, edge
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defect, magnetic defect \... ) and of the dimensionality of the crystal:
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\$\\frac{1}{R}\$ for a surface and \$\\frac{1}{R\^2}\$ for the bulk.
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This envelope also rely on the symmetries connecting the scattered
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states, in particular TRS. On Q. Liu et al.((Liu et al. Phys. Rev. B 85
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2012)) established a chart depicting the shape of the envelop with
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respect to these last considerations.
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#### Accessing scattering processes beyond JDOS : the extended joint density of states (exJDOS) {#accessing_scattering_processes_beyond_jdos_the_extended_joint_density_of_states_exjdos}
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STS experiments allow to observe standing waves in the density however
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mainly because of the presence of multiple impurities and because of the
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superposition of distinctive standing waves with different scattering
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vectors it\'s difficult to extract information from the raw density map.
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For this reason a FT is performed on the density map highlighting the
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main scattering processes. \\\\
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There is a general method exhibiting directly the FT depicted above and
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is commonly named joint density of states (JDOS). The formula describing
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this method gives the contribution of all scattering processes, having a
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scattering vector \$\\vec{q}=\\vec{k}\_f-\\vec{k}\_i\$, lying in the
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same energy shell : \\begin{equation}\\label{eq:JDOS formula}
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\\mbox{JDOS}(\\vec{q})=\\int d\^2 \\vec{k} \\ A\_{\\vec{k}}(E)
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A\_{\\vec{k}+\\vec{q}}(E) % \\quad \\mbox{with} \\quad %
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A\_{\\vec{k}}(E)=\\int\\limits\_{surface} d\^2 \\vec{r} \\
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\|\\Psi\_{\\vec{k}}(\\vec{r})\|\^2 \\delta(E-\\epsilon\_{\\vec{k}})
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\\end{equation} However according to this formula all scattering
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processes have the same weight which is in general not the case.
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Furthermore this formula leads to homogeneous quasiparticle
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interferences which is erroneous. In order to highlight the real
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scattered processes the extended joint density of states (exJDOS) method
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is used. Within this method the scattering processes are weighted as
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following:
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` * by the transition rate between states thanks to "Fermi's golden rule" and the $\mathcal{T}_{\vec{k},\vec{k}'}$ components: $\mbox{P}_{\vec{k},\vec{k}'}=2\pi |\mathcal{T}_{\vec{k},\vec{k}'}|^2\delta(\epsilon_{\vec{k}}-\epsilon_{\vec{k}'})$`\
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` * by the velocity-dependent scattering probability.States having velocities with opposite directions are most likely to scatter: $1-\cos(\vec{v}_{\vec{k}},\vec{v}_{\vec{k}'})$`
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The first point gives the probability of transition from one state to
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another in presence of a perturbation (here an impurity in the host
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system). The second point stems directly from the SPA. With the above
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considerations the convenient quantity exhibiting the FT of the
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quasiparticle interference map is : \\begin{multline}\\label{eq:exJDOS
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formula} \\mbox{exJDOS}(\\vec{q})=\\int d\^2 \\vec{k} \\
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A\_{\\vec{k}}(E) M\_{\\vec{k},\\vec{k}+\\vec{q}}
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A\_{\\vec{k}+\\vec{q}}(E) \\\\ \\quad \\mbox{with} \\quad %
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M\_{\\vec{k},\\vec{k}+\\vec{q}}=\\mbox{P}\_{\\vec{k},\\vec{k}+\\vec{q}}
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% \\left( 1-\\cos(\\vec{v}\_{\\vec{k}},\\vec{v}\_{+\\vec{q}}) \\right)
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\\end{multline}
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The method called JDOS-\$\\gamma\$STM only takes into account the group
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velocity contribution of exJDOS. In the case where the transition rate
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is not known there exists a phenomenological result, obtained by Rushan,
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and valid in topological insulators surfaces which asserts that states
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having spins with same directions are most likely to scatter :
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\$\\mathrm{P}\_{\\vec{k},\\vec{k}\'} \\approx \\left(
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1-\\cos(\\vec{s}\_{\\vec{k}},\\vec{s}\_{\\vec{k}+\\vec{q}}) \\right)\$.
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This approach is called spin-dependent scattering probability (SSP).
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##### A key object : the \$\\mathcal{T}\$-matrix {#a_key_object_the_mathcalt_matrix}
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In the calculation of electron scattering properties induced by defects
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within the KKR method, the transition matrix \$T\_{kk\'}\$ (where
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\$k=(\\mathbf{k},\\nu)\$ comprises the crystal momentum \$\\mathbf{k}\$
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and another index \$\\nu\$ for additional degeneracies) takes the
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central role. It is defined as \\begin{equation}
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` T_{k'k} =\int{ \mathrm{d} \mathbf{x} \, \mathrm{d} \mathbf{x}\,' ~ \boldsymbol{\psi}^{\dagger}_{k'}(\mathbf{x}) \, \Delta \mathbf{V}(\mathbf{x},\mathbf{x}\,') \, \boldsymbol{\psi}^{\mathrm{imp}}_{k}(\mathbf{x}\,') }~,`
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\\end{equation} and, using the expansions that are made in the KKR
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formalism, takes the form \\begin{equation}
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` T_{k'k} = \sum_{i,i'} \sum_{\Lambda,\Lambda'} {c^i}^*_{k',\Lambda} T^{ii'}_{\Lambda \Lambda'} ~ c^{i'}_{k,\Lambda'}~.`
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\\end{equation} with \\begin{equation}
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` T^{ii'}_{\Lambda \Lambda'} = \sum_{\Lambda`*`}`` ``\Delta^{i}_{\Lambda`` ``\Lambda`*`} \, \left( \delta_{ii'} \, \delta_{\Lambda'' \Lambda'} + \sum_{\Lambda`**`}`` ``G^{\mathrm{imp},ii'}_{\Lambda''`` ``\Lambda`**`} ~ \Delta t^{\mathrm{imp},i'}_{\Lambda''' \Lambda'} \right)~.`
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\\end{equation} The matrix \$T\^{ii\'}\_{\\Lambda \\Lambda\'}\$ is
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independent on the state vector \$k\$, but it depends only on the energy
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(often equal to the Fermi energy). All \$k\$-dependencies enter via the
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.
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In order to calculate scattering properties off defects, several steps
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have to be performed.
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` - converge a potential of an ideal host system with the Jülich-München code`\
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` - calculate the Fermi surface and wave-functions on the Fermi surface `\
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` - converge a potential of the defect (=impurity cluster) with the KKRimp code` |