Implement some Päivi's comments.
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@ -597,11 +597,11 @@ Category: Methods and Algorithms for Scientific Computing?
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\end_layout
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\begin_layout Abstract
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The (somewhat underrated) T-matrix multiple scattering method (TMMSM) can
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be used to solve the electromagnetic response of systems consisting of
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many compact scatterers, retaining a good level of accuracy while using
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relatively few of degrees of freedom, largely surpassing other methods
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in the number of scatterers it can deal with.
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The T-matrix multiple scattering method (TMMSM) can be used to solve the
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electromagnetic response of systems consisting of many compact scatterers,
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retaining a good level of accuracy while using relatively few degrees of
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freedom, largely surpassing other methods in the number of scatterers it
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can deal with.
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\end_layout
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\begin_layout Abstract
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@ -488,7 +488,7 @@ noprefix "false"
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around the origin (typically due to presence of a scatterer), one has to
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add the outgoing VSWFs
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\begin_inset Formula $\vswfrtlm{\tau}lm\left(\kappa\vect r\right)$
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\begin_inset Formula $\vswfouttlm{\tau}lm\left(\kappa\vect r\right)$
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\end_inset
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to have a complete basis of the solutions in the volume
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@ -608,7 +608,7 @@ transition matrix,
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\begin_inset Formula $T$
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\end_inset
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-matrix we can solve the single-patricle scatering prroblem simply by substituti
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-matrix we can solve the single-particle scattering problem simply by substituti
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ng appropriate expansion coefficients
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\begin_inset Formula $\rcoefftlm{\tau'}{l'}{m'}$
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\end_inset
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@ -680,12 +680,12 @@ literal "false"
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, but in general one can find them numerically by simulating scattering
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of a regular spherical wave
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\begin_inset Formula $\vswfouttlm{\tau}lm$
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\begin_inset Formula $\vswfrtlm{\tau}lm$
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\end_inset
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and projecting the scattered fields (or induced currents, depending on
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the method) onto the outgoing VSWFs
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\begin_inset Formula $\vswfrtlm{\tau}{'l'}{m'}$
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\begin_inset Formula $\vswfouttlm{\tau'}{l'}{m'}$
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\end_inset
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.
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@ -974,15 +974,67 @@ noprefix "false"
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\begin_inset Formula $\mezikuli{R^{<}}{R^{>}}{\vect 0}$
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\end_inset
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via by electromagnetic radiation is
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by electromagnetic radiation is
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\begin_inset Formula
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\begin{equation}
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P=\frac{1}{2\kappa^{2}\eta_{0}\eta}\left(\Re\left(\rcoeffp{}^{\dagger}\outcoeffp{}\right)+\left\Vert \outcoeffp{}\right\Vert ^{2}\right)=\frac{1}{2\kappa^{2}\eta_{0}\eta}\rcoeffp{}^{\dagger}\left(\Tp{}^{\dagger}\Tp{}+\frac{\Tp{}^{\dagger}+\Tp{}}{2}\right)\rcoeffp{}.\label{eq:Power transport}
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P=\frac{1}{2\kappa^{2}\eta_{0}\eta}\left(\Re\left(\rcoeffp{}^{\dagger}\outcoeffp{}\right)+\left\Vert \outcoeffp{}\right\Vert ^{2}\right)=\frac{1}{2\kappa^{2}\eta_{0}\eta}\rcoeffp{}^{\dagger}\left(\Tp{}^{\dagger}\Tp{}+\frac{\Tp{}^{\dagger}+\Tp{}}{2}\right)\rcoeffp{},\label{eq:Power transport}
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\end{equation}
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\end_inset
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where
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\begin_inset Formula $\eta_{0}=\sqrt{\mu_{0}/\varepsilon_{0}}$
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\end_inset
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and
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\begin_inset Formula $\eta=\sqrt{\mu/\varepsilon}$
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\end_inset
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are wave impedance of vacuum and relative wave impedance of the medium
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in
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\begin_inset Formula $\mezikuli{R^{<}}{R^{>}}{\vect 0}$
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\end_inset
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, respectively.
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\family roman
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\series medium
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\shape up
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\size normal
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\emph off
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\nospellcheck off
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\bar no
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\strikeout off
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\xout off
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\uuline off
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\uwave off
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\noun off
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\color none
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\begin_inset Formula $P$
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\end_inset
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is well-defined only when
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\begin_inset Formula $\eta$
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\end_inset
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is real.
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\family default
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\series default
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\shape default
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\size default
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\emph default
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\nospellcheck default
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\bar default
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\strikeout default
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\xout default
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\uuline default
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\uwave default
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\noun default
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\color inherit
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In realistic scattering setups, power is transferred by radiation into
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\begin_inset Formula $\openball{R^{<}}{\vect 0}$
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\end_inset
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@ -1357,8 +1409,11 @@ In practice, the multiple-scattering problem is solved in its truncated
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\begin_inset Formula $\tau lm$
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\end_inset
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-multiindices left.
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-multi-indices left.
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The truncation degree can vary for different scatterers (e.g.
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\begin_inset space \space{}
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\end_inset
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due to different physical sizes), so the truncated block
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\begin_inset Formula $\left[\tropsp pq\right]_{l_{q}\le L_{q};l_{p}\le L_{q}}$
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\end_inset
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@ -1394,7 +1449,7 @@ If no other type of truncation is done, there remain
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\begin_inset Formula $\tau lm$
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\end_inset
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-multiindices for
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-multi-indices for the
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\begin_inset Formula $p$
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\end_inset
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@ -117,7 +117,7 @@ Some refs here?
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\end_inset
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The most commonly used general approaches used in computational electrodynamics
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The most common general approaches used in computational electrodynamics
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are often unsuitable for simulating systems with larger number of scatterers
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due to their computational complexity: differential methods such as the
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finite difference time domain (FDTD) method or the finite element method
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@ -159,8 +159,8 @@ literal "false"
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\begin_layout Standard
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The natural way to overcome both limitations of CDA mentioned above is to
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include higher multipoles into account.
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Instead of polarisability tensor, the scattering properties of an individual
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take higher multipoles into account.
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Instead of a polarisability tensor, the scattering properties of an individual
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particle are then described with more general
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\begin_inset Formula $T$
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\end_inset
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@ -280,20 +280,10 @@ TODO refs to the code repositories once it is published.
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The features include computations of electromagnetic response to external
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driving, the related cross sections, and finding resonances of finite structure
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s.
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Moreover, it includes the improvements covered in this paper, enabling
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Moreover, it includes the improvements covered in this article, enabling
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to simulate even larger systems and also infinite structures with periodicity
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in one, two or three dimensions, which can be used e.g.
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for quickly evaluating dispersions of such structures
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\begin_inset Marginal
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status open
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\begin_layout Plain Layout
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And also their topological invariants (TODO)?
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\end_layout
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\end_inset
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.
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in one or two or three dimensions, which can be used e.g.
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for quickly evaluating dispersions of such structures.
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The QPMS suite contains a core C library, Python bindings and several utilities
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for routine computations.
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\begin_inset Marginal
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