2015-11-11 13:02:08 +02:00
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\end_header
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\begin_body
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\begin_layout Standard
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2015-11-23 21:04:18 +02:00
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\begin_inset FormulaMacro
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{\boldsymbol{\hat{\mathbf{#1}}}}
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\begin_inset FormulaMacro
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\newcommand{\ud}{\mathrm{d}}
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\end_layout
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\begin_layout Title
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Technical notes on quantum electromagnetic multiple scattering
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\end_layout
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\begin_layout Author
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2015-11-09 19:01:25 +02:00
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Marek Nečada
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2015-11-09 10:57:22 +02:00
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\end_layout
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\begin_layout Affiliation
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COMP Centre of Excellence, Department of Applied Physics, Aalto University,
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P.O.
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Box 15100, Fi-00076 Aalto, Finland
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\end_layout
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\begin_layout Date
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\begin_inset ERT
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status open
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\begin_layout Plain Layout
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\backslash
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today
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\end_layout
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\end_inset
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\end_layout
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\begin_layout Abstract
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...
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\end_layout
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\begin_layout Section
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Theory of quantum electromagnetic multiple scattering
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\end_layout
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\begin_layout Subsection
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Incoherent pumping
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\end_layout
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\begin_layout Standard
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Cf.
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Wubs
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\begin_inset CommandInset citation
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LatexCommand cite
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key "wubs_multiple-scattering_2004"
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\end_inset
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, Delga
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\begin_inset CommandInset citation
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LatexCommand cite
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key "delga_quantum_2014,delga_theory_2014"
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\end_inset
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.
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\end_layout
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\begin_layout Subsection
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General initial states
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\end_layout
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\begin_layout Standard
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Look at
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\begin_inset CommandInset citation
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LatexCommand cite
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key "landau_computational_2015"
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\end_inset
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for an inspiration for solving the LS equation with an arbitrary initial
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state.
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\end_layout
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\begin_layout Section
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Computing classical Green's functions
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\end_layout
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2015-12-28 16:32:18 +02:00
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\begin_layout Standard
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The formulae below might differ depending on the conventions used by various
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authors.
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For instance, Taylor
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\begin_inset CommandInset citation
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LatexCommand cite
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key "taylor_optical_2011"
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\end_inset
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uses normalized spherical wavefunctions
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\begin_inset Formula $\widetilde{\vect M}_{mn}^{(j)},\widetilde{\vect N}_{mn}^{(j)}$
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\end_inset
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which are designed in a way that avoids float number overflow of some of
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the variables during the numerical calculation.
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\end_layout
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\begin_layout Standard
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Beware of various conventions in definitions of Legendre functions etc.
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(the implementation in py-gmm differs, for example, by a factor of
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\begin_inset Formula $(-1)^{m}$
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\end_inset
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from scipy.special.lpmn.
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\end_layout
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2015-11-09 10:57:22 +02:00
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\begin_layout Subsection
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2015-11-23 21:04:18 +02:00
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T-Matrix method
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2015-11-09 10:57:22 +02:00
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\end_layout
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2015-11-23 21:04:18 +02:00
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\begin_layout Subsubsection
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VSWF decomposition
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\end_layout
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\begin_layout Standard
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Expressions for VSWF in Xu
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(2)"
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2015-12-03 03:49:29 +02:00
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key "xu_electromagnetic_1995"
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\end_inset
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:
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\end_layout
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\begin_layout Standard
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\begin_inset Formula
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\begin{eqnarray}
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\vect M_{mn}^{(J)} & = & \left(i\uvec{\theta}\pi_{mn}(\cos\theta)-\uvec{\phi}\tau_{mn}(\cos\theta)\right)z_{n}^{(J)}(kr)e^{im\phi},\nonumber \\
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\vect N_{mn}^{(J)} & = & \uvec rn(n+1)P_{n}^{m}(\cos\theta)\frac{z_{n}^{(J)}(kr)}{kr}e^{im\phi}\label{eq:vswf}\\
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& & +\left(\uvec{\theta}\tau_{mn}(\cos\theta)+i\uvec{\phi}\pi_{mn}(\cos\theta)\right)\nonumber \\
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& & \phantom{+}\times\frac{1}{kr}\frac{\ud\left(rz_{n}^{(J)}(kr)\right)}{\ud r}e^{im\phi},\nonumber \\
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& = & ...\nonumber
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\end{eqnarray}
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2015-11-23 21:04:18 +02:00
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\end_inset
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where
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\begin_inset Formula $z_{n}^{(J)}$
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\end_inset
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denotes
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\begin_inset Formula $j_{n},y_{n},h_{n}^{+},h_{n}^{-}$
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\end_inset
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for
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\begin_inset Formula $J=1,2,3,4$
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\end_inset
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, respectively, and
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\begin_inset Formula
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\begin{eqnarray*}
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\pi_{mn}(\cos\theta) & = & \frac{m}{\sin\theta}P_{n}^{m}(\cos\theta),\\
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\tau_{mn}(\cos\theta) & = & \frac{\ud P_{n}^{m}(\cos\theta)}{\ud\theta}=-\sin\theta\frac{\ud P_{n}^{m}(\cos\theta)}{\ud\cos\theta}.
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\end{eqnarray*}
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\end_inset
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The expressions for
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\begin_inset Formula $\vect M_{mn}^{(J)},\vect N_{mn}^{(J)}$
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\end_inset
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are dimensionless.
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\end_layout
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\begin_layout Standard
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Expansions for the scattered fields are
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(4)"
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2015-12-03 03:49:29 +02:00
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key "xu_electromagnetic_1995"
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2015-11-23 21:04:18 +02:00
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\end_inset
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:
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\begin_inset Formula
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\begin{eqnarray*}
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\vect E_{s}(j) & = & \sum_{n=1}^{\infty}\sum_{m=-n}^{n}iE_{mn}\left[a_{mn}^{j}\vect N_{mn}^{(3)}+b_{mn}^{j}\vect M_{mn}^{(3)}\right],\\
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\vect H_{s}(j) & = & \frac{k}{\omega\mu}\sum_{n=1}^{\infty}\sum_{m=-n}^{n}E_{mn}\left[b_{mn}^{j}\vect N_{mn}^{(3)}+a_{mn}^{j}\vect M_{mn}^{(3)}\right].
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\end{eqnarray*}
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\end_inset
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These expansions should be OK in SI units (take the Fourier transform of
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\begin_inset Formula $\nabla\times\vect E=-\partial\vect B/\partial t$
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\end_inset
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and
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\begin_inset Formula $\vect B=\mu\vect H$
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\end_inset
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).
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For internal field of a sphere, the (regular-wave) expansion reads
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\begin_inset Formula
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\begin{eqnarray*}
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\vect E_{I}(j) & = & -\sum_{n=1}^{\infty}\sum_{m=-n}^{n}iE_{mn}\left[d_{mn}^{j}\vect N_{mn}^{(1)}+c_{mn}^{j}\vect M_{mn}^{(1)}\right],\\
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\vect H_{I}(j) & = & -\frac{k}{\omega\mu}\sum_{n=1}^{\infty}\sum_{m=-n}^{n}E_{mn}\left[c_{mn}^{j}\vect N_{mn}^{(1)}+d_{mn}^{j}\vect M_{mn}^{(1)}\right]
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\end{eqnarray*}
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\end_inset
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(note the minus sign; I am not sure about its role) and the incident field
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(incl.
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field from the other scatterers) is assumed to have the same regular-wave
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form
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\begin_inset Formula
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\begin{eqnarray*}
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\vect E_{i}(j) & = & -\sum_{n=1}^{\infty}\sum_{m=-n}^{n}iE_{mn}\left[p_{mn}^{j}\vect N_{mn}^{(1)}+q_{mn}^{j}\vect M_{mn}^{(1)}\right],\\
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\vect H_{i}(j) & = & -\frac{k}{\omega\mu}\sum_{n=1}^{\infty}\sum_{m=-n}^{n}E_{mn}\left[q_{mn}^{j}\vect N_{mn}^{(1)}+p_{mn}^{j}\vect M_{mn}^{(1)}\right].
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\end{eqnarray*}
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\end_inset
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The common multipole-dependent factor is given by
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\begin_inset Formula
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\[
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E_{mn}=\left|E_{0}\right|i^{n}(2n+1)\frac{\left(n-m\right)!}{\left(n+m\right)!}
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\]
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\end_inset
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which
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\begin_inset Quotes eld
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\end_inset
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is desired for keeping the formulation of the multisphere scattering theory
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consistent with that of the Mie theory.
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It ensures that all the expressions in the multisphere theory turn out
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to be identical to those in the Mie theory when one is dealing with a cluster
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containing only one sphere and illuminated by a single plane wave
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\begin_inset Quotes erd
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\end_inset
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.
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(According to Bohren&Huffman
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(4.37)"
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key "bohren_absorption_1983"
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\end_inset
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, the decomposition of a plane wave reads
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\begin_inset Formula
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\[
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\vect E=E_{0}\sum_{n=1}^{\infty}i^{n}\frac{2n+1}{n(n+1)}\left(\vect M_{o1n}^{(1)}-i\vect N_{e1n}^{(1)}\right),
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\]
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\end_inset
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where the even/odd VSWF and
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\begin_inset Formula $m\ge0$
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\end_inset
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convention is used.)
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\end_layout
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\begin_layout Standard
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\emph on
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It should be possible to just take it away and the abovementioned expansions
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are still consistent, are they not?
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\end_layout
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2015-12-03 03:49:29 +02:00
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\begin_layout Standard
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In
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\begin_inset CommandInset citation
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LatexCommand cite
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after "sec. 4A"
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key "xu_electromagnetic_1995"
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\end_inset
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, there are formulae for translation of the plane wave between VSWF with
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different origins.
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\end_layout
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\begin_layout Standard
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o
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\end_layout
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2015-11-23 21:04:18 +02:00
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\begin_layout Subsubsection
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Mie scattering
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\end_layout
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\begin_layout Standard
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For the exact form of the coefficients following from the boundary conditions
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on the spherical surface, cf.
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(12–13)"
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2015-12-03 03:49:29 +02:00
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key "xu_electromagnetic_1995"
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2015-11-23 21:04:18 +02:00
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\end_inset
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.
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For the particular case of spherical nanoparticle, it is important that
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they can be written as
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(14–15)"
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2015-12-03 03:49:29 +02:00
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key "xu_electromagnetic_1995"
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2015-11-23 21:04:18 +02:00
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\end_inset
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\begin_inset Formula
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\begin{alignat*}{1}
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a_{mn}^{j} & =a_{n}^{j}p_{mn}^{j},\quad b_{mn}^{j}=b_{n}^{j}q_{mn}^{j},\\
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c_{mn}^{j} & =c_{n}^{j}q_{mn}^{j},\quad d_{mn}^{j}=d_{n}^{j}p_{mn}^{j},
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\end{alignat*}
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\end_inset
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in other words, the Mie coefficients do not depend on
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\begin_inset Formula $m$
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\end_inset
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but solely on
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\begin_inset Formula $n$
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\end_inset
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(which is not surprising and probably follows from the Wigner-Eckart theorem).
|
2015-11-09 10:57:22 +02:00
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\end_layout
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2015-12-03 03:49:29 +02:00
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\begin_layout Subsubsection
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Translation coefficients
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\end_layout
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\begin_layout Standard
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A quite detailed study can be found in
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\begin_inset CommandInset citation
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LatexCommand cite
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key "xu_calculation_1996"
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\end_inset
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, I have not read the recenter one
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\begin_inset CommandInset citation
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LatexCommand cite
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key "xu_efficient_1998"
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\end_inset
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which deals with efficient evaluation of Wigner 3jm symbols and Gaunt coefficie
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nts.
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\end_layout
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\begin_layout Standard
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With the VSWF as in
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\begin_inset CommandInset ref
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LatexCommand eqref
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reference "eq:vswf"
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\end_inset
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and translation relations in the form
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(38,39)"
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key "xu_calculation_1996"
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\end_inset
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\begin_inset Formula
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\begin{eqnarray*}
|
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|
|
\vect M_{\mu\nu}^{(J)l} & = & \sum_{n=1}^{\infty}\sum_{m=-n}^{n}\left[A_{mn}^{\mu\nu}\vect M_{mn}^{(1)j}+B_{mn}^{\mu\nu}\vect N_{mn}^{(1)j}\right],\quad r\le d_{lj},\\
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|
|
\vect N_{\mu\nu}^{(J)l} & = & \sum_{n=1}^{\infty}\sum_{m=-n}^{n}\left[B_{mn}^{\mu\nu}\vect M_{mn}^{(1)j}+A_{mn}^{\mu\nu}\vect N_{mn}^{(1)j}\right],\quad r\le d_{lj},\\
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|
|
\vect M_{\mu\nu}^{(J)l} & = & \sum_{n=1}^{\infty}\sum_{m=-n}^{n}\left[A_{mn}^{\mu\nu}\vect M_{mn}^{(J)j}+B_{mn}^{\mu\nu}\vect N_{mn}^{(J)j}\right],\quad r\ge d_{lj},\\
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|
|
\vect N_{\mu\nu}^{(J)l} & = & \sum_{n=1}^{\infty}\sum_{m=-n}^{n}\left[B_{mn}^{\mu\nu}\vect M_{mn}^{(J)j}+A_{mn}^{\mu\nu}\vect N_{mn}^{(J)j}\right],\quad r\ge d_{lj},
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|
|
\end{eqnarray*}
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\end_inset
|
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|
the translation coefficients (which should in fact be also labeled with
|
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|
|
their origin indices
|
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|
\begin_inset Formula $l,j$
|
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|
\end_inset
|
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) are
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\begin_inset CommandInset citation
|
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|
LatexCommand cite
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|
after "(82,83)"
|
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|
key "xu_calculation_1996"
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\end_inset
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\end_layout
|
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\begin_layout Standard
|
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|
\begin_inset Formula
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|
\begin{multline*}
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|
|
A_{mn}^{\mu\nu}=\\
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|
|
\frac{(-1)^{m}i^{\nu+n}(n+2)_{n-1}\left(\nu+2\right)_{\nu+1}(n+\nu+m-\mu)!}{4n(n+\nu+1)_{n+\nu}(n-m)!(\nu+m)!}\\
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|
\times e^{i(\mu-m)\phi_{lj}}\sum_{q=0}^{q_{\mathrm{max}}}(-1)^{q}\left[n(n+1)+\nu(\nu+1)-p(p+1)\right]\\
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|
|
\times\tilde{a}_{1q}\begin{pmatrix}z_{p}^{(J)}(kd_{lj})\\
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|
|
j_{p}(kd_{lj})
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|
|
\end{pmatrix}P_{p}^{\mu-m}(\cos\theta_{lj}),\qquad\begin{pmatrix}r\le d_{lj}\\
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|
|
r\ge d_{lj}
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|
\end{pmatrix};
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|
\end{multline*}
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\end_inset
|
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\begin_inset Formula
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|
\begin{multline*}
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|
B_{mn}^{\mu\nu}=\\
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|
|
\frac{(-1)^{m}i^{\nu+n+1}(n+2)_{n+1}\left(\nu+2\right)_{\nu+1}(n+\nu+m-\mu+1)!}{4n(n+1)(n+m+1)(n+\nu+2)_{n+\nu+1}(n-m)!(\nu+m)!}\\
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|
\times e^{i(\mu-m)\phi_{lj}}\sum_{q=0}^{Q_{\mathrm{max}}}(-1)^{q}\Big\{2(n+1)(\nu-\mu)\tilde{a}_{2q}-\\
|
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|
|
-\left[p(p+3)-\nu(\nu+1)-n(n+3)-2\mu(n+1)\right]\tilde{a}_{3q}\Big\}\\
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|
\times\begin{pmatrix}z_{p+1}^{(J)}(kd_{lj})\\
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|
j_{p+1}(kd_{lj})
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|
\end{pmatrix}P_{p+1}^{\mu-m}(\cos\theta_{lj}),\qquad\begin{pmatrix}r\le d_{lj}\\
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|
r\ge d_{lj}
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|
\end{pmatrix};
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|
\end{multline*}
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\end_inset
|
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where
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|
\begin_inset CommandInset citation
|
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|
|
|
LatexCommand cite
|
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|
|
after "(79,80)"
|
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|
key "xu_calculation_1996"
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\end_inset
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|
\begin_inset Formula
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|
\begin{eqnarray*}
|
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|
|
|
\tilde{a}_{1q} & = & a(-m,n,\mu,\nu,n+\nu-2q)/a(-m,n,\mu,\nu,n+\nu),\\
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|
|
\tilde{a}_{2q} & = & a(-m-1,n+1,\mu+1,\nu,n+\nu+1-2q)/\\
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|
|
& & /a(-m-1,n+1,\mu+1,\nu,n+\nu+1),\\
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|
\tilde{a}_{3q} & = & a(-m,n+1,\mu,\nu,n+\nu+1-2q)/\\
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|
|
& & /a(-m,n+1,\mu,\nu,\mu+\nu+1),
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|
\end{eqnarray*}
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\end_inset
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\begin_inset Formula
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|
\begin{eqnarray*}
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|
|
p & = & n+\nu-2q\\
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|
|
q_{\max} & = & \min\left(n,\nu,\frac{n+\nu-\left|m-\mu\right|}{2}\right),\\
|
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|
Q_{\max} & = & \min\left(n+1,\nu,\frac{n+\nu+1-\left|m-\mu\right|}{2}\right),
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|
\end{eqnarray*}
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\end_inset
|
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|
2015-12-28 16:32:18 +02:00
|
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|
|
where the parentheses with lower index mean most likely the Pochhammer symbol
|
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/
|
2015-12-03 03:49:29 +02:00
|
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|
|
\emph on
|
2015-12-28 16:32:18 +02:00
|
|
|
|
rising
|
2015-12-03 03:49:29 +02:00
|
|
|
|
\emph default
|
2015-12-28 16:32:18 +02:00
|
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|
|
factorial
|
2015-12-03 03:49:29 +02:00
|
|
|
|
\begin_inset Formula
|
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|
|
|
\[
|
2015-12-28 16:32:18 +02:00
|
|
|
|
\left(x\right)_{n}=x(x+1)(x+2)\dots(x+n-1)=\frac{(x+n-1)!}{(x-1)!}=\frac{\Gamma(x+n)}{\Gamma(x)},
|
2015-12-03 03:49:29 +02:00
|
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|
|
\]
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|
\end_inset
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|
2015-12-28 16:32:18 +02:00
|
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|
|
which is damn confusing (because this can also mean the falling factorial,
|
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|
|
cf.
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|
|
Wikipedia); and Xu does not bother explaining the notation
|
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|
\emph on
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|
|
anywhere
|
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|
\emph default
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.
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|
|
The fact that it is the rising factorial has been checked by comparing
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|
\begin_inset Formula $a_{0}$
|
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|
|
\end_inset
|
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|
\begin_inset CommandInset citation
|
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|
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|
LatexCommand cite
|
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|
|
|
after "(78)"
|
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|
|
|
key "xu_calculation_1996"
|
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|
\end_inset
|
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|
to some implementation from the internets
|
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|
\begin_inset Foot
|
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|
status open
|
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|
\begin_layout Plain Layout
|
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|
\family typewriter
|
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|
|
|
\begin_inset CommandInset href
|
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|
|
LatexCommand href
|
|
|
|
|
name "https://raw.githubusercontent.com/michael-hartmann/gaunt/master/gaunt.py"
|
|
|
|
|
target "https://raw.githubusercontent.com/michael-hartmann/gaunt/master/gaunt.py"
|
2015-12-03 03:49:29 +02:00
|
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|
\end_inset
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|
2015-12-28 16:32:18 +02:00
|
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\end_layout
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|
2015-12-03 03:49:29 +02:00
|
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|
\end_inset
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|
2015-12-28 16:32:18 +02:00
|
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|
.
|
2015-12-03 03:49:29 +02:00
|
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|
\end_layout
|
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|
\begin_layout Standard
|
|
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|
|
The implementation should be checked with
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
after "Table II"
|
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|
|
key "xu_calculation_1996"
|
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\end_inset
|
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\end_layout
|
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|
\begin_layout Subsubsection
|
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|
|
Equations for the scattering problem
|
|
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|
|
\end_layout
|
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|
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|
\begin_layout Standard
|
|
|
|
|
The linear system for the scattering problem reads
|
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|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
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|
|
|
after "(30)"
|
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|
|
key "xu_electromagnetic_1995"
|
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\end_inset
|
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|
\begin_inset Formula
|
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|
\begin{eqnarray*}
|
|
|
|
|
a_{mn}^{j} & = & a_{n}^{j}\left\{ p_{mn}^{j,j}-\sum_{l\neq j}^{(1,L)}\sum_{\nu=1}^{\infty}\sum_{\mu=-\nu}^{\nu}\left[a_{\mu\nu}^{l}A_{mn}^{\mu\nu;lj}+b_{\mu\nu}^{l}B_{mn}^{\mu\nu;lj}\right]\right\} \\
|
|
|
|
|
b_{mn}^{j} & = & b_{n}^{j}\left\{ q_{mn}^{j,j}-\sum_{l\neq j}^{(1,L)}\sum_{\nu=1}^{\infty}\sum_{\mu=-\nu}^{\nu}\left[a_{\mu\nu}^{l}B_{mn}^{\mu\nu;lj}+b_{\mu\nu}^{l}A_{mn}^{\mu\nu;lj}\right]\right\}
|
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|
\end{eqnarray*}
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|
\end_inset
|
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where
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\begin_inset Formula $p_{mn}^{j,j},q_{mn}^{j,j}$
|
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\end_inset
|
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are the expansion coefficients of the initial incident waves in the
|
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\begin_inset Formula $j$
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\end_inset
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-th particle's coordinate system
|
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\begin_inset CommandInset citation
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LatexCommand cite
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after "sec. 4A"
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key "xu_electromagnetic_1995"
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\end_inset
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.
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\emph on
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TODO expressions for
|
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\begin_inset Formula $p_{mn}^{j,j},q_{mn}^{j,j}$
|
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\end_inset
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in the case of dipole initial wave.
|
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\end_layout
|
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\begin_layout Subsubsection
|
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Solving the linear system
|
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\end_layout
|
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\begin_layout Standard
|
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\begin_inset CommandInset citation
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LatexCommand cite
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after "sec. 5"
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key "xu_electromagnetic_1995"
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\end_inset
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\end_layout
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|
2015-11-09 10:57:22 +02:00
|
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\begin_layout Subsection
|
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|
T-Matrix resummation (multiple scatterers)
|
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\end_layout
|
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|
2015-11-23 21:04:18 +02:00
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\begin_layout Subsection
|
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Boundary element method
|
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\end_layout
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|
2015-11-09 10:57:22 +02:00
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\begin_layout Subsection
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BEM→TM
|
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\end_layout
|
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\begin_layout Standard
|
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Cf.
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|
SCUFF-TMATRIX (
|
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|
\begin_inset CommandInset ref
|
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LatexCommand ref
|
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reference "sub:SCUFF-TMATRIX"
|
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\end_inset
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)
|
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\end_layout
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\begin_layout Section
|
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|
Available software
|
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\end_layout
|
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|
2015-11-18 19:52:48 +02:00
|
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|
\begin_layout Itemize
|
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|
|
TODO which of them can calculate the VSWF translation coefficients?
|
|
|
|
|
\end_layout
|
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|
2015-11-09 10:57:22 +02:00
|
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\begin_layout Subsection
|
2015-11-09 19:01:25 +02:00
|
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|
SCUFF-EM
|
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|
\begin_inset CommandInset citation
|
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LatexCommand cite
|
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|
key "reid_scuff-em_2015"
|
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\end_inset
|
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2015-11-09 10:57:22 +02:00
|
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|
\end_layout
|
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\begin_layout Subsubsection
|
2015-11-09 19:01:25 +02:00
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\family typewriter
|
2015-11-09 10:57:22 +02:00
|
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SCUFF-TMATRIX
|
2015-11-09 19:01:25 +02:00
|
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|
\family default
|
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|
2015-11-09 10:57:22 +02:00
|
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|
\begin_inset CommandInset label
|
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LatexCommand label
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name "sub:SCUFF-TMATRIX"
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\end_inset
|
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\end_layout
|
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|
2015-11-09 19:01:25 +02:00
|
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|
\begin_layout Subsubsection
|
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|
\family typewriter
|
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|
SCUFF-SCATTER
|
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|
\family default
|
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\begin_inset CommandInset label
|
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|
LatexCommand label
|
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|
name "sub:SCUFF-SCATTER"
|
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\end_inset
|
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|
\end_layout
|
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\begin_layout Subsubsection
|
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|
|
Caveats
|
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|
|
\end_layout
|
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|
\begin_layout Description
|
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|
Units.
|
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|
\family typewriter
|
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|
SCUFF-SCATTER
|
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|
\family default
|
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|
|
's Angular frequencies specified using the
|
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|
|
\family typewriter
|
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|
|
--Omega
|
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|
\family default
|
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|
or
|
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|
|
\family typewriter
|
|
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|
|
--OmegaFile
|
|
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|
|
\family default
|
|
|
|
|
arguments are interpreted in units of
|
|
|
|
|
\begin_inset Formula $c/1\,\mathrm{μm}=3\cdot10^{14}\,\mathrm{rad/s}$
|
|
|
|
|
\end_inset
|
|
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|
|
\begin_inset Foot
|
|
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|
|
status open
|
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|
|
\begin_layout Plain Layout
|
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|
|
\family typewriter
|
|
|
|
|
\begin_inset CommandInset href
|
|
|
|
|
LatexCommand href
|
|
|
|
|
name "http://homerreid.dyndns.org/scuff-EM/scuff-scatter/scuffScatterExamples.shtml"
|
|
|
|
|
target "http://homerreid.dyndns.org/scuff-EM/scuff-scatter/scuffScatterExamples.shtml"
|
|
|
|
|
|
|
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|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
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|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
.
|
|
|
|
|
|
|
|
|
|
\emph on
|
|
|
|
|
TODO what are the output units?
|
|
|
|
|
\end_layout
|
|
|
|
|
|
2015-11-09 10:57:22 +02:00
|
|
|
|
\begin_layout Subsection
|
2015-11-09 19:01:25 +02:00
|
|
|
|
MSTM
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
key "mackowski_mstm_2013"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
The incident field is a gaussian beam or a plane wave in the vanilla code
|
|
|
|
|
(no multipole radiation as input!).
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
The bulk of the useful code is in the
|
|
|
|
|
\family typewriter
|
|
|
|
|
mstm-modules-v3.0.f90
|
|
|
|
|
\family default
|
|
|
|
|
file.
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
For solving the interaction equations
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
after "(14)"
|
|
|
|
|
key "mackowski_mstm_2013"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
, the BCGM (biconjugate gradient method) is used.
|
2015-11-11 13:02:08 +02:00
|
|
|
|
(According to Wikipedia, this method is numerically unstable but has a
|
|
|
|
|
stabilized version (stabilized BCGM).)
|
2015-11-09 19:01:25 +02:00
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
According to the manual
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
after "2.3"
|
|
|
|
|
key "mackowski_mstm_2013"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
, they use some method (rotational-axial translation decomposition of the
|
|
|
|
|
translation operation), which
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
reduces the operation from an
|
|
|
|
|
\begin_inset Formula $L_{S}^{4}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
process to
|
|
|
|
|
\begin_inset Formula $L_{S}^{3}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
process where
|
|
|
|
|
\begin_inset Formula $L_{S}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
is the truncation order of the expansion
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
(more details can probably be found at
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
after "around (68)"
|
|
|
|
|
key "mackowski_calculation_1996"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
.
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
|
|
|
|
|
\emph on
|
|
|
|
|
Not sure if this holds also for nonspherical particles, I should either
|
|
|
|
|
read carefully
|
|
|
|
|
\emph default
|
|
|
|
|
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
key "mackowski_calculation_1996"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
\emph on
|
|
|
|
|
or look into
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
key "mishchenko_electromagnetic_2003"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
which is also cited in the manual.
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\end_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
By default spheres, it is possible to add own T-Matrix coefficients instead.
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
|
|
|
|
|
\emph on
|
|
|
|
|
Is it then possible to insert a T-Matrix of an arbitrary shape, or is it
|
|
|
|
|
somehow limited to
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
spherical-like
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
particles?
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\end_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Why the heck are the T-matrix options listed in the
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
Options for random orientation calculations
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
2015-11-18 19:52:48 +02:00
|
|
|
|
? Well, it seems that for fixed orientation, it is not possible to specify
|
|
|
|
|
the T-matrix, cf.
|
|
|
|
|
the description of
|
|
|
|
|
\family typewriter
|
|
|
|
|
fixed_or_random_orientation
|
|
|
|
|
\family default
|
|
|
|
|
option in
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
after "3.2.3"
|
|
|
|
|
key "mackowski_mstm_2013"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
.
|
2015-11-09 19:01:25 +02:00
|
|
|
|
\end_layout
|
|
|
|
|
|
2015-11-12 16:06:31 +02:00
|
|
|
|
\begin_layout Subsubsection
|
|
|
|
|
Interesting subroutines
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
2015-11-18 19:52:48 +02:00
|
|
|
|
|
|
|
|
|
\family typewriter
|
|
|
|
|
rottranfarfield
|
|
|
|
|
\family default
|
|
|
|
|
: it states
|
2015-11-12 16:06:31 +02:00
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
far field formula for outgoing vswf translation
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
.
|
|
|
|
|
What is that and how does it differ from whatever else (near field?) formula?
|
|
|
|
|
\end_layout
|
|
|
|
|
|
2015-11-18 19:52:48 +02:00
|
|
|
|
\begin_layout Subsection
|
|
|
|
|
py_gmm
|
|
|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
key "pellegrini_py_gmm_2015"
|
|
|
|
|
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Fortran code, already (partially) pythonized using
|
|
|
|
|
\family typewriter
|
|
|
|
|
f2py
|
|
|
|
|
\family default
|
|
|
|
|
by the authors(?); under GNU GPLv3.
|
|
|
|
|
This could save my day.
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Lots of unnecessary code duplication (see e.g.
|
|
|
|
|
|
|
|
|
|
\family typewriter
|
|
|
|
|
coeff_sp2
|
|
|
|
|
\family default
|
|
|
|
|
and
|
|
|
|
|
\family typewriter
|
|
|
|
|
coeff_sp2_dip
|
|
|
|
|
\family default
|
|
|
|
|
subroutines).
|
|
|
|
|
\end_layout
|
|
|
|
|
|
2015-11-12 16:06:31 +02:00
|
|
|
|
\begin_layout Itemize
|
2015-11-18 19:52:48 +02:00
|
|
|
|
Has comments!!! (Sometimes they are slightly inaccurate due to the copy-pasting,
|
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but it is still one of the most readable FORTRAN codes I have seen.)
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\end_layout
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\begin_layout Itemize
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The subroutines seem not to be bloated with dependencies on static/global
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variables, so they should be quite easily reusable.
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\end_layout
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\begin_layout Itemize
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The FORTRAN code was apparently used in
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\begin_inset CommandInset citation
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LatexCommand cite
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key "pellegrini_interacting_2007"
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\end_inset
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.
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Uses the multiple-scattering formalism described in
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\begin_inset CommandInset citation
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LatexCommand cite
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key "xu_efficient_1998"
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\end_inset
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.
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\end_layout
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\begin_layout Subsubsection
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Interesting subroutines
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\end_layout
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\begin_layout Standard
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Mie scattering:
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\end_layout
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\begin_layout Itemize
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\family typewriter
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coeff_sp2
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\family default
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: calculation of the Mie scattering coefficients (
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\begin_inset Formula $\overline{a}_{n}^{l},\overline{b}_{n}^{l}$
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\end_inset
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as in
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\begin_inset CommandInset citation
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LatexCommand cite
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after "(1), (2), \\ldots"
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key "pellegrini_py_gmm_2015"
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\end_inset
|
2015-11-12 16:06:31 +02:00
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2015-11-18 19:52:48 +02:00
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), for a set of spheres (therefore all the parameters have +1 dimension).
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2015-11-12 16:06:31 +02:00
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\end_layout
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2015-11-18 19:52:48 +02:00
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\begin_deeper
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\begin_layout Itemize
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What does the input parameter
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\family typewriter
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v_req
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\family default
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(
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\emph on
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vettore raggi equivalenti
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\emph default
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) mean?
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\end_layout
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\begin_layout Itemize
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How do I put in the environment permittivity?
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\end_layout
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\begin_layout Itemize
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\family typewriter
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m_epseq
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\family default
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are real and imaginary parts of the permittivity (which are then transformed
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into complex
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\family typewriter
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v_epsc
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\family default
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)
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\end_layout
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\begin_layout Itemize
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\family typewriter
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ref_index
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\family default
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is the environment refractive index (called
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\family typewriter
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n_matrix
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\family default
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in the example ipython notebook)
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\end_layout
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\begin_layout Itemize
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\family typewriter
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v_req
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\family default
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are the sphere radii?
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\end_layout
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\begin_layout Itemize
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\family typewriter
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nstop
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\family default
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is the maximum order of the
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\begin_inset Formula $n$
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\end_inset
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-expansion
|
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\end_layout
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\begin_layout Itemize
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\family typewriter
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neq
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\family default
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is ns, number of spheres for which the calculation is performed apparently,
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it is connected to some
|
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\begin_inset Quotes eld
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\end_inset
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dirty hack to interface fortran and python properly
|
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\begin_inset Quotes erd
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\end_inset
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(cf.
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\family typewriter
|
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|
gmm_f2py_module.f90
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\family default
|
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)
|
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\end_layout
|
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\end_deeper
|
2015-11-09 19:01:25 +02:00
|
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|
\begin_layout Section
|
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|
Code integration
|
2015-11-09 10:57:22 +02:00
|
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|
\end_layout
|
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|
2015-11-11 13:02:08 +02:00
|
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|
\begin_layout Section
|
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|
Testing and reproduction of foreign results
|
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|
\end_layout
|
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|
\begin_layout Subsection
|
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|
|
|
Delga PRL
|
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|
|
|
\begin_inset CommandInset citation
|
|
|
|
|
LatexCommand cite
|
|
|
|
|
key "delga_quantum_2014"
|
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|
\end_inset
|
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|
\end_layout
|
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|
\begin_layout Subsubsection
|
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|
|
Parameters
|
|
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|
|
\end_layout
|
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|
\begin_layout Itemize
|
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|
|
Surrounding lossless dielectric
|
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|
|
\series bold
|
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|
medium
|
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|
\series default
|
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|
with permittivity
|
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|
|
\begin_inset Formula $\epsilon_{d}=2.13$
|
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|
\end_inset
|
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|
.
|
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|
\end_layout
|
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|
\begin_layout Itemize
|
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|
\series bold
|
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|
QEs:
|
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|
\series default
|
|
|
|
|
dipole moment
|
|
|
|
|
\begin_inset Formula $\mu=0.19\, e\cdot\mathrm{nm}=9.12\,\mathrm{D}$
|
|
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|
|
\end_inset
|
|
|
|
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|
|
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|
|
, count
|
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|
\begin_inset Formula $N\in\left\{ 1,50,100,200\right\} $
|
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|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
, radial orientation,
|
|
|
|
|
\begin_inset Formula $h=1\,\mathrm{nm}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
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|
|
|
above the sphere (except for Fig.
|
|
|
|
|
5 where variable), natural frequency
|
|
|
|
|
\begin_inset Formula $\Omega_{n}=\omega_{0}-i\gamma_{\mathrm{QE}}/2,$
|
|
|
|
|
\end_inset
|
|
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|
|
\begin_inset Formula $\omega_{0}=$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
varies,
|
|
|
|
|
\begin_inset Formula $\gamma_{\mathrm{QE}}=15\,\mathrm{meV}$
|
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|
|
|
\end_inset
|
|
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|
.
|
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|
\end_layout
|
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|
\begin_layout Itemize
|
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|
|
|
|
|
|
|
|
\series bold
|
|
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|
|
Sphere:
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
radius
|
|
|
|
|
\begin_inset Formula $a=7\,\mathrm{nm}$
|
|
|
|
|
\end_inset
|
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|
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|
,
|
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|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Drude model
|
|
|
|
|
\begin_inset Formula $\epsilon_{m}(\omega)=\epsilon_{\infty}-\frac{\omega_{p}^{2}}{\omega\left(\omega+i\gamma_{p}\right)}$
|
|
|
|
|
\end_inset
|
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|
\end_layout
|
|
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|
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|
|
|
|
|
\begin_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Drude parameters
|
|
|
|
|
\begin_inset Formula $\omega_{p}=9\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
|
|
|
|
\begin_inset Formula $\epsilon_{\infty}=4.6$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
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|
|
\begin_inset Formula $\gamma_{p}=0.1\,\mathrm{eV}$
|
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|
|
|
\end_inset
|
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|
\end_layout
|
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|
|
|
\end_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
background permittivity
|
|
|
|
|
\begin_inset Formula $\epsilon_{d}(\omega)=2.13$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
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|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
(approximate?; not really a parameter) LSP resonances
|
|
|
|
|
\begin_inset Formula $\omega_{l}=\omega_{p}/\sqrt{\epsilon_{\infty}+\left(1+1/l\right)\epsilon_{d}}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
; particularly,
|
|
|
|
|
\begin_inset Formula $\omega_{1}\approx3.0236\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
|
|
|
|
\begin_inset Formula $\omega_{2}\approx3.2236\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
2015-11-11 17:00:58 +02:00
|
|
|
|
\begin_inset Formula $\omega_{3}\approx3.30\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
|
|
|
|
\begin_inset Formula $\omega_{4}\approx3.34\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
,
|
|
|
|
|
\begin_inset Formula $\omega_{5}\approx3.364\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
|
2015-11-11 13:02:08 +02:00
|
|
|
|
\begin_inset Formula $\omega_{\infty}\approx3.4692\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
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|
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|
\end_layout
|
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|
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|
\end_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
|
|
|
|
|
\series bold
|
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|
Detector:
|
|
|
|
|
\series default
|
|
|
|
|
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_deeper
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Far field:
|
|
|
|
|
\begin_inset Formula $1\,\mathrm{\mu m}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
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|
|
away from the center of the nanoparticle along the
|
|
|
|
|
\begin_inset Formula $y$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
axis (Fig.
|
|
|
|
|
3).
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Itemize
|
|
|
|
|
Near field: position not specified in the paper; but in Fig.
|
|
|
|
|
4(b) there are
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
polarization spectra
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
instead of
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
light spectra
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
(eq.
|
|
|
|
|
4) in Fig.
|
|
|
|
|
4(a).
|
|
|
|
|
Does this mean that they are evaluated somewhere in/on the sphere? Or in
|
|
|
|
|
the particle? The latter is likely, as it is given by
|
|
|
|
|
\begin_inset Formula $P_{n}\left(\omega\right)=\left\langle \sigma_{n}^{+}\left(-\omega\right)\sigma_{n}^{-}(\omega)\right\rangle $
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
(cf.
|
|
|
|
|
the column below Fig.
|
|
|
|
|
3).
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\end_deeper
|
|
|
|
|
\begin_layout Subsubsection
|
|
|
|
|
Testing
|
|
|
|
|
\end_layout
|
|
|
|
|
|
|
|
|
|
\begin_layout Standard
|
|
|
|
|
In my
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
old
|
|
|
|
|
\begin_inset Quotes erd
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
code, there no splitting observable around
|
|
|
|
|
\begin_inset Formula $\omega\approx\omega_{0}\approx\omega_{\infty}\approx3.46\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
.
|
|
|
|
|
This is perhaps because the couplings to the higher multipoles is miscalculated
|
|
|
|
|
(too small).
|
|
|
|
|
No splitting around the NP dipole (
|
|
|
|
|
\begin_inset Formula $\approx3,02\,\mathrm{eV}$
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
) should be OK for single QE in far field (cf.
|
|
|
|
|
Fig.
|
|
|
|
|
3).
|
|
|
|
|
And there are yet the
|
|
|
|
|
\begin_inset Quotes eld
|
|
|
|
|
\end_inset
|
|
|
|
|
|
|
|
|
|
switched axes
|
|
|
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\begin_inset Quotes erd
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\end_inset
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...
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\end_layout
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2015-11-18 19:52:48 +02:00
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\begin_layout Standard
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If I set the dipole reflection coefficients RH[1], RV[1] to zero, and multiply
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the the quadrupole reflection coefficients RH[2], RV[2] by
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\begin_inset Formula $10^{6}$
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\end_inset
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, the peak at
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\begin_inset Formula $3.0\,\mathrm{eV}$
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\end_inset
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dissapears and a tiny(!) peak appears around the (expected) position of
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\begin_inset Formula $3.0\,\mathrm{eV}$
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\end_inset
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.
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Have I fucked up the Mie reflection coefficients? Sounds like if I forgot
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a factor of
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\begin_inset Formula $c$
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\end_inset
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somewhere.
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\end_layout
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2015-11-11 13:02:08 +02:00
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\begin_layout Subsection
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Delga JoO
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\begin_inset CommandInset citation
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LatexCommand cite
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key "delga_theory_2014"
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\end_inset
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\end_layout
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\begin_layout Subsubsection
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Parameters
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\end_layout
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\begin_layout Itemize
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\series bold
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QEs:
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\series default
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dipole moment
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\begin_inset Formula $\mu=0.38\, e\cdot\mathrm{nm}=18.24\,\mathrm{D}$
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\end_inset
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(double), otherwise the same parameters as in
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\begin_inset CommandInset citation
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LatexCommand cite
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key "delga_quantum_2014"
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\end_inset
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.
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\end_layout
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\begin_layout Itemize
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\series bold
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Sphere:
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\series default
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as in
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\begin_inset CommandInset citation
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LatexCommand cite
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key "delga_quantum_2014"
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\end_inset
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\end_layout
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\begin_layout Itemize
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\series bold
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Detector:
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\series default
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not stated in the paper
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\end_layout
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2015-11-11 17:00:58 +02:00
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\begin_layout Itemize
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\series bold
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Numerics:
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\series default
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looking at the leftmost ball in Fig.
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3, it seems that their SVW cutoff is around 12.
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\end_layout
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2015-11-12 16:06:31 +02:00
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\begin_layout Section
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TODO
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\end_layout
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\begin_layout Itemize
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Päivi's suggestion: suppress the dipole and let it interact only with the
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higher multipoles.
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\end_layout
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2015-11-09 10:57:22 +02:00
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\begin_layout Standard
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\begin_inset CommandInset bibtex
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LatexCommand bibtex
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bibfiles "dipdip"
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options "apsrev"
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\end_inset
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\end_layout
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\end_body
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\end_document
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