qpms/Scattering and Shit.lyx

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\pdf_title "Sähköpajan päiväkirja"
\pdf_author "Marek Nečada"
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\begin_body

\begin_layout Standard
\begin_inset FormulaMacro
\newcommand{\vect}[1]{\mathbf{#1}}
\end_inset


\begin_inset FormulaMacro
\newcommand{\ud}{\mathrm{d}}
\end_inset


\end_layout

\begin_layout Title
Electromagnetic multiple scattering, spherical waves and ****
\end_layout

\begin_layout Author
Marek Nečada
\end_layout

\begin_layout Chapter
Zillion conventions for spherical vector waves
\end_layout

\begin_layout Section
Legendre polynomials and spherical harmonics: messy from the very beginning
\end_layout

\begin_layout Standard
\begin_inset Marginal
status open

\begin_layout Plain Layout
FIXME check the Condon-Shortley phases.
\end_layout

\end_inset


\end_layout

\begin_layout Standard
Associated Legendre polynomial of degree 
\begin_inset Formula $l\ge0$
\end_inset

 and order 
\begin_inset Formula $m,$
\end_inset

 
\begin_inset Formula $l\ge m\ge-l$
\end_inset

, is given by the recursive relation
\begin_inset Formula 
\[
P_{l}^{-m}=\underbrace{\left(-1\right)^{m}}_{\mbox{Condon-Shortley phase}}\frac{1}{2^{l}l!}\left(1-x^{2}\right)^{m/2}\frac{\ud^{l+m}}{\ud x^{l+m}}\left(x^{2}-1\right)^{l}.
\]

\end_inset

There is a relation between the positive and negative orders,
\end_layout

\begin_layout Standard
\begin_inset Formula 
\[
P_{l}^{-m}=\underbrace{\left(-1\right)^{m}}_{\mbox{C.-S. p.}}\frac{\left(l-m\right)!}{\left(l+m\right)!}P_{l}^{m}\left(\cos\theta\right),\quad m\ge0.
\]

\end_inset

The index 
\begin_inset Formula $l$
\end_inset

 (in certain notations, it is often 
\begin_inset Formula $n$
\end_inset

) is called 
\emph on
degree
\emph default
, index 
\begin_inset Formula $m$
\end_inset

 is the 
\emph on
order
\emph default
.
 These two terms are then transitively used for all the object which build
 on the associated Legendre polynomials, i.e.
 spherical harmonics, vector spherical harmonics, spherical waves etc.
\end_layout

\begin_layout Subsection
Kristensson 
\end_layout

\begin_layout Standard
Kristensson uses the Condon-Shortley phase, so (sect.
 [K]D.2)
\end_layout

\begin_layout Standard
\begin_inset Formula 
\[
Y_{lm}\left(\hat{\vect r}\right)=\left(-1\right)^{m}\sqrt{\frac{2l+1}{4\pi}\frac{\left(l-m\right)!}{\left(l+m\right)!}}P_{l}^{m}\left(\cos\theta\right)e^{im\phi}
\]

\end_inset


\begin_inset Formula 
\[
Y_{lm}^{\dagger}\left(\hat{\vect r}\right)=Y_{lm}^{*}\left(\hat{\vect r}\right)
\]

\end_inset


\begin_inset Formula 
\[
Y_{l,-m}\left(\hat{\vect r}\right)=\left(-1\right)^{m}Y_{lm}^{\dagger}\left(\hat{\vect r}\right)
\]

\end_inset


\end_layout

\begin_layout Standard
Orthonormality:
\begin_inset Formula 
\[
\int Y_{lm}\left(\hat{\vect r}\right)Y_{l'm'}^{\dagger}\left(\hat{\vect r}\right)\,\ud\Omega=\delta_{ll'}\delta_{mm'}
\]

\end_inset


\end_layout

\begin_layout Section
Pi and tau
\end_layout

\begin_layout Subsection
Taylor
\end_layout

\begin_layout Standard
\begin_inset Formula 
\begin{eqnarray*}
\tilde{\pi}_{mn}\left(\cos\theta\right) & = & \sqrt{\frac{2n+1}{4\pi}\frac{\left(n-m\right)!}{\left(n+m\right)!}}\frac{m}{\sin\theta}P_{n}^{m}\left(\cos\theta\right)\\
\tilde{\tau}_{mn}\left(\cos\theta\right) & = & \sqrt{\frac{2n+1}{4\pi}\frac{\left(n-m\right)!}{\left(n+m\right)!}}\frac{\ud}{\ud\theta}P_{n}^{m}\left(\cos\theta\right)
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Section
Vector spherical harmonics (?)
\end_layout

\begin_layout Subsection
Kristensson
\end_layout

\begin_layout Standard
Original formulation, sect.
 [K]D.3.3
\end_layout

\begin_layout Standard
\begin_inset Formula 
\begin{eqnarray*}
\vect A_{1lm}\left(\hat{\vect r}\right) & = & \frac{1}{\sqrt{l\left(l+1\right)}}\left(\hat{\vect{\theta}}\frac{1}{\sin\theta}\frac{\partial}{\partial\phi}Y_{lm}\left(\hat{\vect r}\right)-\hat{\vect{\phi}}\frac{\partial}{\partial\theta}Y_{lm}\left(\hat{\vect r}\right)\right)\\
\vect A_{2lm}\left(\hat{\vect r}\right) & = & \frac{1}{\sqrt{l\left(l+1\right)}}\left(\hat{\vect{\theta}}\frac{\partial}{\partial\phi}Y_{lm}\left(\hat{\vect r}\right)-\hat{\vect{\phi}}\frac{1}{\sin\theta}\frac{\partial}{\partial\theta}Y_{lm}\left(\hat{\vect r}\right)\right)\\
\vect A_{3lm}\left(\hat{\vect r}\right) & = & \hat{\vect r}Y_{lm}\left(\hat{\vect r}\right)
\end{eqnarray*}

\end_inset

Normalisation:
\begin_inset Formula 
\[
\int\vect A_{n}\left(\hat{\vect r}\right)\cdot\vect A_{n'}^{\dagger}\left(\hat{\vect r}\right)\,\ud\Omega=\delta_{nn'}
\]

\end_inset

Here 
\begin_inset Formula $\mbox{ }^{\dagger}$
\end_inset

 means just complex conjugate, apparently (see footnote on p.
 89).
\end_layout

\begin_layout Section
Spherical Bessel functions
\begin_inset CommandInset label
LatexCommand label
name "sec:Spherical-Bessel-functions"

\end_inset


\end_layout

\begin_layout Standard
The radial dependence of spherical vector waves is given by the spherical
 Bessel functions and their first derivatives.
 Commonly, the following notation is adopted
\begin_inset Formula 
\begin{eqnarray*}
z_{n}^{(1)}(x) & = & j_{n}(x),\\
z_{n}^{(2)}(x) & = & y_{n}(x),\\
z_{n}^{(3)}(x) & = & h_{n}^{(1)}(x)=j_{n}(x)+iy_{n}(x),\\
z_{n}^{(4)}(x) & = & h_{n}^{(2)}(x)=j_{n}(x)-iy_{n}(x).
\end{eqnarray*}

\end_inset

Here, 
\begin_inset Formula $j_{n}$
\end_inset

 is the spherical Bessel function of first kind (regular), 
\begin_inset Formula $y_{j}$
\end_inset

 is the spherical Bessel function of second kind (singular), and 
\begin_inset Formula $h_{n}^{(1)},h_{n}^{(2)}$
\end_inset

 are the Hankel functions a.k.a.
 spherical Bessel functions of third kind.
 In spherical vector waves, 
\begin_inset Formula $j_{n}$
\end_inset

 corresponds to regular waves, 
\begin_inset Formula $h^{(1)}$
\end_inset

 corresponds (by the usual convention) to outgoing waves, and 
\begin_inset Formula $h^{(2)}$
\end_inset

 corresponds to incoming waves.
 To describe scattering, we need two sets of waves with two different types
 of spherical Bessel functions 
\begin_inset Formula $z_{n}^{(J)}$
\end_inset

.
 Most common choice is 
\begin_inset Formula $J=1,3$
\end_inset

, because if we decompose the field into spherical waves centered at 
\begin_inset Formula $\vect r_{0}$
\end_inset

, the field produced by other sources (e.g.
 spherical waves from other scatterers or a plane wave) is always regular
 at 
\begin_inset Formula $\vect r_{0}$
\end_inset

.
 Second choice which makes a bit of sense is 
\begin_inset Formula $J=3,4$
\end_inset

 as it leads to a nice expression for the energy transport.
\end_layout

\begin_layout Section
Spherical vector waves
\end_layout

\begin_layout Standard
TODO 
\begin_inset Formula $M,N,\psi,\chi,\widetilde{M},\widetilde{N},u,v,w,\dots$
\end_inset

, sine/cosine convention (B&H), ...
\end_layout

\begin_layout Standard
There are two mutually orthogonal types of divergence-free (everywhere except
 in the origin for singular waves) spherical vector waves, which I call
 electric and magnetic, given by the type of multipole source to which they
 correspond.
 This is another distinction than the regular/singular/ingoing/outgoing
 waves given by the type of the radial dependence (cf.
 section 
\begin_inset CommandInset ref
LatexCommand ref
reference "sec:Spherical-Bessel-functions"

\end_inset

).
 Oscillating electric current in a tiny rod parallel to its axis will generate
 electric dipole waves (net dipole moment of magnetic current is zero) moment
 , whereas oscillating electric current in a tiny circular loop will generate
 magnetic dipole waves (net dipole moment of electric current is zero).
\end_layout

\begin_layout Standard
In the usual cases we encounter, the part described by the magnetic waves
 is pretty small.
\end_layout

\begin_layout Subsection
Taylor
\end_layout

\begin_layout Standard
Definition [T](2.40); 
\begin_inset Formula $\widetilde{\vect N}_{mn}^{(j)},\widetilde{\vect M}_{mn}^{(j)}$
\end_inset

 are the electric and magnetic waves, respectively:
\end_layout

\begin_layout Standard
\begin_inset Formula 
\begin{eqnarray*}
\widetilde{\vect N}_{mn}^{(j)} & = & \frac{n(n+1)}{kr}\sqrt{\frac{2n+1}{4\pi}\frac{\left(n-m\right)!}{\left(n+m\right)!}}P_{n}^{m}\left(\cos\theta\right)e^{im\phi}z_{n}^{j}\left(kr\right)\hat{\vect r}\\
 &  & +\left[\tilde{\tau}_{mn}\left(\cos\theta\right)\hat{\vect{\theta}}+i\tilde{\pi}_{mn}\left(\cos\theta\right)\hat{\vect{\phi}}\right]e^{im\phi}z_{n}^{j}\left(kr\right)\\
\widetilde{\vect M}_{mn}^{(j)} & = & \left[i\tilde{\pi}_{mn}\left(\cos\theta\right)\hat{\vect{\theta}}-\tilde{\tau}_{mn}\left(\cos\theta\right)\hat{\vect{\phi}}\right]e^{im\phi}z_{n}^{j}\left(kr\right)
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Subsection
Kristensson
\end_layout

\begin_layout Standard
Definition [K](2.4.6); 
\begin_inset Formula $\vect u_{\tau lm},\vect v_{\tau lm},\vect w_{\tau lm}$
\end_inset

 are the waves with 
\begin_inset Formula $j=3,1,4$
\end_inset

 respectively, i.e.
 outgoing, regular and incoming waves.
 The first index distinguishes between the electric (
\begin_inset Formula $\tau=2$
\end_inset

) and magnetic (
\begin_inset Formula $\tau=1$
\end_inset

).
 Kristensson uses a multiindex 
\begin_inset Formula $n\equiv(\tau,l,m)$
\end_inset

 to simlify the notation.
\begin_inset Formula 
\begin{eqnarray*}
\left(\vect{u/v/w}\right)_{2lm} & = & \frac{1}{kr}\frac{\ud\left(kr\, z_{l}^{(j)}\left(kr\right)\right)}{\ud\, kr}\vect A_{2lm}\left(\hat{\vect r}\right)+\sqrt{l\left(l+1\right)}\frac{z_{l}^{(j)}(kr)}{kr}\vect A_{3lm}\left(\hat{\vect r}\right)\\
\left(\vect{u/v/w}\right)_{1lm} & = & z_{l}^{(j)}\left(kr\right)\vect A_{1lm}\left(\hat{\vect r}\right)
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Subsection
Relation between Kristensson and Taylor
\begin_inset CommandInset label
LatexCommand label
name "sub:Kristensson-v-Taylor"

\end_inset


\end_layout

\begin_layout Standard
Kristensson's and Taylor's VSWFs seem to differ only by an 
\begin_inset Formula $l$
\end_inset

-dependent normalization factor, and notation of course (n.b.
 the inverse index order)
\begin_inset Formula 
\begin{eqnarray*}
\left(\vect{u/v/w}\right)_{2lm} & = & \frac{\widetilde{\vect N}_{ml}^{(3/1/4)}}{\sqrt{l\left(l+1\right)}}\\
\left(\vect{u/v/w}\right)_{1lm} & = & \frac{\widetilde{\vect M}_{ml}^{(3/1/4)}}{\sqrt{l\left(l+1\right)}}
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Section
Plane wave expansion
\end_layout

\begin_layout Subsection
Taylor
\end_layout

\begin_layout Standard
\begin_inset Formula $x$
\end_inset

-polarised, 
\begin_inset Formula $z$
\end_inset

-propagating plane wave, 
\begin_inset Formula $\vect E=E_{0}\hat{\vect x}e^{i\vect k\cdot\hat{\vect z}}$
\end_inset

 (CHECK):
\begin_inset Formula 
\begin{eqnarray*}
\vect E & = & -i\left(p_{mn}\widetilde{\vect N}_{mn}^{(1)}+q_{mn}\widetilde{\vect M}_{mn}^{(1)}\right)\\
p_{mn} & = & E_{0}\frac{4\pi i^{n}}{n(n+1)}\tilde{\tau}_{mn}(1)\\
q_{mn} & = & E_{0}\frac{4\pi i^{n}}{n(n+1)}\tilde{\pi}_{mn}(1)
\end{eqnarray*}

\end_inset

while it can be shown that
\begin_inset Formula 
\begin{eqnarray*}
\tilde{\pi}_{mn}(1) & = & -\frac{1}{2}\sqrt{\frac{\left(2n+1\right)\left(n\left(n+1\right)\right)}{4\pi}}\left(\delta_{m,1}+\delta_{m,-1}\right)\\
\tilde{\tau}_{mn}(1) & = & -\frac{1}{2}\sqrt{\frac{\left(2n+1\right)\left(n\left(n+1\right)\right)}{4\pi}}\left(\delta_{m,1}-\delta_{m,-1}\right)
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Subsection
Kristensson
\end_layout

\begin_layout Standard
\begin_inset Formula $x$
\end_inset

-polarised, 
\begin_inset Formula $z$
\end_inset

-propagating plane wave, 
\begin_inset Formula $\vect E=E_{0}\hat{\vect x}e^{i\vect k\cdot\hat{\vect z}}$
\end_inset

 (CHECK, ):
\begin_inset Formula 
\[
\vect E=\sum_{n}a_{n}\vect v_{n}
\]

\end_inset


\begin_inset Formula 
\begin{eqnarray*}
a_{1lm} & = & E_{0}i^{l+1}\sqrt{\left(2l+1\right)\pi}\left(\delta_{m,1}+\delta_{m,-1}\right)\\
a_{2lm} & = & E_{0}i^{l+1}\sqrt{\left(2l+1\right)\pi}\left(\delta_{m,1}+\delta_{m,-1}\right)
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Section
Radiated energy
\end_layout

\begin_layout Standard
In this section I summarize the formulae for power 
\begin_inset Formula $P$
\end_inset

 radiated from the system.
 For an absorbing scatterer, this should be negative (n.b.
 sign conventions can be sometimes confusing).
 If the system is excited by a plane wave with intensity 
\begin_inset Formula $E_{0}$
\end_inset

, this can be used to calculate the absorption cross section (TODO check
 if it should be multiplied by the 2),
\begin_inset Formula 
\[
\sigma_{\mathrm{abs}}=-\frac{2P}{\varepsilon\varepsilon_{0}\left|E_{0}\right|^{2}}.
\]

\end_inset


\end_layout

\begin_layout Subsection
Kristensson
\begin_inset CommandInset label
LatexCommand label
name "sub:Radiated enenergy-Kristensson"

\end_inset


\end_layout

\begin_layout Standard
Sect.
 [K]2.6.2; here this form of expansion is assumed:
\begin_inset Formula 
\begin{equation}
\vect E\left(\vect r,\omega\right)=k\sqrt{\eta_{0}\eta}\sum_{n}\left(a_{n}\vect v_{n}\left(k\vect r\right)+f_{n}\vect u_{n}\left(k\vect r\right)\right).\label{eq:power-Kristensson-E}
\end{equation}

\end_inset

Here 
\begin_inset Formula $\eta_{0}=\sqrt{\mu_{0}/\varepsilon_{0}}$
\end_inset

 is the wave impedance of free space and 
\begin_inset Formula $\eta=\sqrt{\mu/\varepsilon}$
\end_inset

 is the relative wave impedance of the medium.
 
\end_layout

\begin_layout Standard
The radiated power is then (2.28): 
\begin_inset Formula 
\[
P=\frac{1}{2}\sum_{n}\left(\left|f_{n}\right|^{2}+\Re\left(f_{n}a_{n}^{*}\right)\right).
\]

\end_inset

The first term is obviously the power radiated away by the outgoing waves.
 The second term must then be minus the power sucked by the scatterer from
 the exciting wave.
 If the exciting wave is plane, it gives us the extinction cross section
\begin_inset Formula 
\[
\sigma_{\mathrm{tot}}=-\frac{\sum_{n}\Re\left(f_{n}a_{n}^{*}\right)}{\varepsilon\varepsilon_{0}\left|E_{0}\right|^{2}}
\]

\end_inset


\end_layout

\begin_layout Subsection
Taylor
\end_layout

\begin_layout Standard
Here I derive the radiated power in Taylor's convention by applying the
 relations from subsection 
\begin_inset CommandInset ref
LatexCommand ref
reference "sub:Kristensson-v-Taylor"

\end_inset

 to the Kristensson's formulae (sect.
 
\begin_inset CommandInset ref
LatexCommand ref
reference "sub:Radiated enenergy-Kristensson"

\end_inset

).
\end_layout

\begin_layout Standard
Assume the external field decomposed as (here I use tildes even for the
 expansion coefficients in order to avoid confusion with the 
\begin_inset Formula $a_{n}$
\end_inset

 in 
\begin_inset CommandInset ref
LatexCommand eqref
reference "eq:power-Kristensson-E"

\end_inset

) 
\begin_inset Formula 
\[
\vect E\left(\vect r,\omega\right)=\sum_{mn}\left[-i\left(\tilde{p}_{mn}\vect{\widetilde{N}}_{mn}^{(1)}+\tilde{q}_{mn}\widetilde{\vect M}_{mn}^{(1)}\right)+i\left(\tilde{a}_{mn}\widetilde{\vect N}_{mn}^{(3)}+\tilde{b}_{mn}\widetilde{\vect M}_{mn}^{(3)}\right)\right]
\]

\end_inset

(there is minus between the regular and outgoing part!).
 The coefficients are related to those from 
\begin_inset CommandInset ref
LatexCommand eqref
reference "eq:power-Kristensson-E"

\end_inset

 as 
\begin_inset Formula 
\[
\tilde{p}_{mn}=\frac{k\sqrt{\eta_{0}\eta}}{-i\sqrt{n(n+1)}}a_{2nm},\quad\tilde{q}_{mn}=\frac{k\sqrt{\eta_{0}\eta}}{-i\sqrt{n(n+1)}}a_{1nm},
\]

\end_inset


\begin_inset Formula 
\[
\tilde{a}_{mn}=\frac{k\sqrt{\eta_{0}\eta}}{i\sqrt{n(n+1)}}f_{2nm},\quad\tilde{b}_{mn}=\frac{k\sqrt{\eta_{0}\eta}}{i\sqrt{n(n+1)}}f_{1nm}.
\]

\end_inset

The radiated power is then
\begin_inset Formula 
\[
P=\frac{1}{2}\sum_{m,n}\frac{n\left(n+1\right)}{k^{2}\eta_{0}\eta}\left(\left|a_{mn}\right|^{2}+\left|b_{mn}\right|^{2}-\Re\left(a_{mn}p_{mn}^{*}\right)-\Re\left(b_{mn}q_{mn}^{*}\right)\right).
\]

\end_inset

If the exciting wave is a plane wave, the extinction cross section is
\begin_inset Formula 
\[
\sigma_{\mathrm{tot}}=\frac{\Re\left(a_{mn}p_{mn}^{*}\right)+\Re\left(b_{mn}q_{mn}^{*}\right)}{\varepsilon\varepsilon_{0}\left|E_{0}\right|^{2}}
\]

\end_inset


\end_layout

\begin_layout Section
Limit solutions
\end_layout

\begin_layout Subsection
Far-field asymptotic solution
\end_layout

\begin_layout Standard
TODO start from 
\begin_inset CommandInset citation
LatexCommand cite
after "(A7)"
key "pustovit_plasmon-mediated_2010"

\end_inset


\end_layout

\begin_layout Subsection
Near field limit
\end_layout

\begin_layout Chapter
Single particle scattering and Mie theory
\end_layout

\begin_layout Standard
The basic idea is simple.
 For an exciting spherical wave (usually the regular wave in whatever convention
) of a given frequency 
\begin_inset Formula $\omega$
\end_inset

, type 
\begin_inset Formula $\zeta$
\end_inset

 (electric or magnetic), degree 
\begin_inset Formula $l$
\end_inset

 and order 
\begin_inset Formula $m$
\end_inset

, the particle responds with waves from the complementary set (e.g.
 outgoing waves), with the same frequency 
\begin_inset Formula $\omega$
\end_inset

, but any type 
\begin_inset Formula $\zeta'$
\end_inset

, degree 
\begin_inset Formula $l'$
\end_inset

 and order 
\begin_inset Formula $m'$
\end_inset

, in a way that the Maxwell's equations are satisfied, with the coefficients
 
\begin_inset Formula $T_{l',m';l,m}^{\zeta',\zeta}(\omega)$
\end_inset

.
 This yields one row in the scattering matrix (often called the 
\begin_inset Formula $T$
\end_inset

-matrix) 
\begin_inset Formula $T(\omega)$
\end_inset

, which fully characterizes the scattering properties of the particle (in
 the linear regime, of course).
 Analytical expression for the matrix is known for spherical scatterer,
 otherwise it is computed numerically (using DDA, BEM or whatever).
 So if we have the two sets of spherical wave functions 
\begin_inset Formula $\vect f_{lm}^{J_{1},\zeta}$
\end_inset

, 
\begin_inset Formula $\vect f_{lm}^{J_{2},\zeta}$
\end_inset

 and the full 
\begin_inset Quotes sld
\end_inset

exciting
\begin_inset Quotes srd
\end_inset

 wave has electric field given as
\begin_inset Formula 
\[
\vect E_{\mathrm{ext}}=\sum_{\zeta=\mathrm{E,M}}\sum_{l,m}c_{lm}^{\zeta}\vect f_{lm}^{\zeta},
\]

\end_inset

the 
\begin_inset Quotes sld
\end_inset

scattered
\begin_inset Quotes srd
\end_inset

 field will be
\begin_inset Formula 
\[
\vect E_{\mathrm{scat}}=\sum_{\zeta',l',m'}\sum_{\zeta,l,m}T_{l',m';l,m}^{\zeta',\zeta}c_{lm}^{\zeta}\vect f_{l'm'}^{\zeta'},
\]

\end_inset

and the total field around the scaterer is 
\begin_inset Formula $\vect E=\vect E_{\mathrm{ext}}+\vect E_{\mathrm{scat}}$
\end_inset

.
\end_layout

\begin_layout Section
Mie theory – full version
\end_layout

\begin_layout Standard
\begin_inset Formula $T$
\end_inset

-matrix for a spherical particle is type-, degree- and order- diagonal,
 that is, 
\begin_inset Formula $T_{l',m';l,m}^{\zeta',\zeta}(\omega)=0$
\end_inset

 if 
\begin_inset Formula $l\ne l'$
\end_inset

, 
\begin_inset Formula $m\ne m'$
\end_inset

 or 
\begin_inset Formula $\zeta\ne\zeta'$
\end_inset

.
 Moreover, it does not depend on 
\begin_inset Formula $m$
\end_inset

, so
\begin_inset Formula 
\[
T_{l',m';l,m}^{\zeta',\zeta}(\omega)=T_{l}^{\zeta}\left(\omega\right)\delta_{\zeta'\zeta}\delta_{l'l}\delta_{m'm}
\]

\end_inset

where for the usual choice 
\begin_inset Formula $J_{1}=1,J_{2}=3$
\end_inset


\begin_inset Formula 
\begin{eqnarray*}
T_{l}^{E}\left(\omega\right) & = & TODO,\\
T_{l}^{M}(\omega) & = & TODO.
\end{eqnarray*}

\end_inset


\end_layout

\begin_layout Section
Long wave approximation for spherical nanoparticle
\end_layout

\begin_layout Standard
TODO start from 
\begin_inset CommandInset citation
LatexCommand cite
after "(A11)"
key "pustovit_plasmon-mediated_2010"

\end_inset

 and around.
\end_layout

\begin_layout Chapter
Green's functions
\end_layout

\begin_layout Section
xyz pure free-space dipole waves in terms of SVWF
\end_layout

\begin_layout Section
Mie decomposition of Green's function for single nanoparticle
\end_layout

\begin_layout Chapter
Translation of spherical waves: getting insane
\end_layout

\begin_layout Chapter
Multiple scattering: nice linear algebra born from all the mess
\end_layout

\begin_layout Standard
\begin_inset CommandInset bibtex
LatexCommand bibtex
bibfiles "dipdip"
options "plain"

\end_inset


\end_layout

\end_body
\end_document