Mind the gap between theory and experiment Andrei Kiselev Jeonghyeon Kim and Olivier J. F. Martin Abstract After briefly introducing the surface integral equation method for the nu-

2025-05-02 0 0 1.12MB 18 页 10玖币
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Mind the gap between theory and experiment
Andrei Kiselev, Jeonghyeon Kim, and Olivier J. F. Martin
Abstract After briefly introducing the surface integral equation method for the nu-
merical solution of Maxwell’s equations, we discuss some examples where numerical
simulations based on effectively fabricated nanostructures can provide additional in-
sights into an experiment. Focusing on plasmonics, we study Fano resonant systems
for optical trapping, realistic dipole antennas for near-field enhancement, and hy-
brid nanostructures that combine plasmonic metals with dielectrics refractive index
sensing. For those systems, the same experimental detail can play a very different
role, depending on the type of physical observable. For example, roughness can
significantly influence the near-field, but be totally unnoticed in the far-field. It can
affect molecules adsorbed on the surface, while refractive index sensing can be fully
immune to such roughness. Approaching the experimental situation as closely as
possible is certainly a challenging task and we demonstrate a simple approach based
on SEM images for that. Altogether, bridging the gap between theory and experiment
is not such a trivial task. However, some of the simple steps illustrated in this chapter
can help build numerical models that match the experiment better.
1
Introduction
We did not have the pleasure to meet Werner S. Weiglhofer and only know of him
through his scientific publications. In spite of his too short career, they are extremely
numerous, diverse and impactful. Following the Web of Science categories, one
notices that these contributions do not only cover optics and electromagnetics, but
also reach out to applied physics, materials sciences andof coursemathematics.
They are very well cited; his works on demystified negative index of refraction [1],
and that on light-propagation in helicoidal bianisotropic media [2], at the top of
his list of citations. Working at the Department of Mathematics of the University
Nanophotonics and Metrology Laboratory, Swiss Federal Institute of Technology Lausanne (EPFL),
EPFL-STI-NAM, Station 11, CH-1015 Lausanne, e-mail: olivier.martin@epfl.ch
1
2 Andrei Kiselev, Jeonghyeon Kim, and Olivier J. F. Martin
of Glasgow, it is not surprising that Werner’s publications have a strong theoretical
flavour and have inspired many theoretical works. Yet, analysing their citations
further indicates that these theoretical developments inspired numerous experimental
projects. As an example, among the citations of his work on light-propagation in
helicoidal bianisotropic media [2], a third of the citing articles report experiments.
This illustrates how well Werner succeeded in bridging the gap between theory and
experiments! Obviously, theory is very important and progress within the realm of
theoretical physics is often fascinating in itself. Evidently, new theories are often the
driver behind new experimental work. This chapter, however, focuses on the inverse
process, where experimental work requires numerical support as close as possible to
the experimental situation. After briefly presenting the numerical technique we have
developed for over a decade to solve Maxwell’s equations, we discuss three different
experimental situations where we attempted to model the real experiment as closely
as possible.
2
Computational electromagnetics
At the onset of studying a given experimental situation lies the fundamental question
of the choice of the most appropriate numerical method. It is fair to say that there is
not one single numerical technique that is fit for all situations and even for the narrow
field of plasmonics, which is the focus of our work, numerous approaches exist as
illustrated in a recent review article [3]. Furthermore, each numerical method can
be put to good use as long as it is utilized wisely and carefully. Especially, sufficient
efforts must be undertaken to characterize the algorithm beforehand, to make sure
that it will converge well for the problem at hand and is free from spurious behaviours.
This task is especially thankless, but of paramount importance if the numerical results
are to be trusted. Note that it does not only apply to home-developed numerical codes,
but should be equally undertaken with commercial packages that should never be
trusted blindly, even if they produce beautiful and colourful images!
To assess the accuracy of a numerical technique and obtain a metric to quantify it,
one usually resorts to canonical problems. Unfortunately, there are essentially only
two such problems for which a reference solution exists (the quasi analytical Mie
solution): the scattering by a sphere for three-dimensional (3D) problems or by a
cylinder for two-dimensional (2D) geometries [5]. Figure 1 illustrates this approach
for a 2D solution obtained with a volumetric Green’s tensor approach [4]. In this
case, two different incident polarizations must be considered, with the electric field
either perpendicular to the cylinder axis (transverse electric or TE field) or parallel
to the cylinder axis (transverse magnetic or TM field). The differential cross section
can be computed as a function of the scattering angle and compared with the quasi
analytical Mie solution, Fig. 1(a). This panel indicates that many features exist in
that response, which need to be reproduced accurately with the numerical method. A
more quantitative metric is obtained by integrating the difference between this cross
section and the Mie solution over all scattering angles and repeating the calculations
Mind the gap between theory and experiment 3
Mie (TM)
Numerical result (TM)
Mie (TE)
Numerical result (TE)
Error
/
with an increasing number of discretized elements, Fig. 1(b). In principle, the error
should decrease as the number of elements increases. However, this behaviour is
far from monotonous since it includes different facets of the numerical problem:
on the one side, a finer mesh approximates the scatterer better and should provide
a more accurate solution; on the other hand, it requires a larger numerical matrix
to be solved, which is more difficult, especially when the matrix condition number
increases, as is the case here [6,7]. Consequently, plateaus appear in the convergence
curve, Fig. 1(b). We also notice that the polarization influences the solution accuracy,
reminiscent that in electromagnetics all field components do not behave in the same
way: some are continuous across materials’ boundaries, others are not [8].
Experimental situations are usually much more complicated than a sphere or a
cylinder and we will show in Sec. 3.2 that it is possible to use reciprocity to assess
the accuracy of numerical results produced for complex geometries.
In this chapter, we focus on the surface integral equation (SIE) method for the
numerical solution of Maxwell’s equations. An interesting feature of such a formu-
lation is that the boundary conditions at the edge of the computation window are
included in the equations and need not be taken care of by using ad hoc prescriptions,
such as absorbing boundary conditions or perfectly matched layers [9]. Indeed, these
boundary conditions are already included in the kernel of the integral equation, and
can take different forms, like infinite homogeneous space [10], surfaces or stratified
media [11, 12], or waveguide cavities [13]. There is of course a price to pay for this:
except for infinite homogeneous space where the kernel is known analytically [10],
(a) (b)
2.4
10
2.2
2.0
10
1.8
1.6
10
1.4
1.2
1.0
10
0.8
−6
0.6
0.4
0.2
0.0
0
60
120
180
Scattering angle [degree]
10
10
100
1000
Number of elements
Fig. 1 Measuring the numerical solution accuracy for light scattering by an infinite cylinder in
vacuum illuminated by a plane wave normal to the cylinder. Two polarizations are considered:
transverse electric (TE) with the electric field normal to the cylinder axis and transverse magnetic
(TM) with the electric field along the cylinder axis. (a) Comparison between the numerical solution
and the reference Mie solution for a dielectric cylinder with relative permittivity = 4 and a size
parameter = = 10.43, where is the cylinder diameter, its relative permittivity and
the wavelength in vacuum. (b) Relative error between the Mie and numerical solutions (defined
as the square of the difference between the numerical and Mie far-field amplitudes, normalized to
the square of the analytical amplitude) as a function of the number of discretized elements for two
different materials , for TE (solid lines) and TM (dashed lines) polarizations. Adapted from Ref.
4 with permission, copyright IEEE 2000.
=λ6 64+0 23
i
=4 0
Differential scattering cross section
4 Andrei Kiselev, Jeonghyeon Kim, and Olivier J. F. Martin
it must be evaluated numerically, usually by resorting to plane waves or eigenmodes
expansions [11, 14].
The SIE is constructed from the combination of an equation for the electric
field and one for the magnetic field; different weighted combinations can be used
here [15]. The volume integral form of Maxwell’s equations is transformed into a
surface equation using Gauss’ theorem and the solution is computed from unknown
electric and magnetic currents defined only on the surface of the scatterer [16]. This
is very advantageous since only that surface needs to be discretized; on the other
hand, a limitation of this approach is that the resulting matrix is dense since each
mesh is connected to all the other meshes in the system, different, e.g., from the finite
difference time domain method, where only nearest neighbours are connected [17].
The resulting system of linear equations is constructed through a Galerkin procedure,
where Rao-Wilton-Glisson functions are used both as basis and test functions [18].
The accuracy of the method strongly depends on the order used for the quadrature in
the Galerkin scheme [19]. Once the surface currents are known, different observables
can be computed, from the near-field to the different cross-sections [20], or even the
force and torque produced by the incident light on the nanostructure [21, 22].
3
Approaching experimental situations
Having settled for the numerical technique, we wish to address the question of
modelling the geometry of a real experiment as accurately as possible and will
do that in the context of three different plasmonic systems. This field of research
studies the interaction of light with coinage metals, like gold, silver, aluminium or
heavily doped semiconductors [23]. When light impinges on a nanostructure made
from such a metal, it resonantly excites the free electrons in the metal, producing
a very strong near-field at the vicinity of the nanostructure [24, 25]. It is quite
remarkable that nanostructures much smaller than the wavelength can exhibit such
strong resonances; the reason being the localisation of the free charges in a specific
pattern associated with each optical resonance [26, 27].
3.1
Fano-resonant systems
In principle, any resonant system has an optical response with a Lorentzian shape [5].
This is also true for a plasmonic nanostructure, as long as only one single resonance
is excited like in a small particle or a dipole antenna [28]. On the other hand, as soon
as more than one resonances are present, the lineshape can become very complicated
with several different peaks. A prominent family of such irregular responses is the so-
called Fano lineshape, following the name of Ugo Fano who discovered them while
interpreting atomic spectroscopy experiments [29]. In the context of plasmonics,
Fano resonances occur when two modes are present in the system, often a bright
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MindthegapbetweentheoryandexperimentAndreiKiselev,JeonghyeonKim,andOlivierJ.F.MartinAbstractAfterbrieflyintroducingthesurfaceintegralequationmethodforthenu-mericalsolutionofMaxwell’sequations,wediscusssomeexampleswherenumericalsimulationsbasedoneffectivelyfabricatednanostructurescanprovideadditional...

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