Windowed Green Function MoM for Second-Kind Surface Integral Equation Formulations of Layered Media Electromagnetic Scattering Problems

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Windowed Green Function MoM for Second-Kind
Surface Integral Equation Formulations of Layered
Media Electromagnetic Scattering Problems
Rodrigo Arrieta1and Carlos Pérez-Arancibia2
1Department of Electrical Engineering, PUC Chile (riarrieta@uc.cl)
2Department of Applied Mathematics, University of Twente (c.a.perezarancibia@utwente.nl)
Abstract—This paper presents a second-kind surface integral
equation method for the numerical solution of frequency-domain
electromagnetic scattering problems by locally perturbed layered
media in three spatial dimensions. Unlike standard approaches,
the proposed methodology does not involve the use of layer Green
functions. It instead leverages an indirect Müller formulation in
terms of free-space Green functions that entails integration over
the entire unbounded penetrable boundary. The integral equation
domain is effectively reduced to a small-area surface by means
of the windowed Green function method, which exhibits high-
order convergence as the size of the truncated surface increases.
The resulting (second-kind) windowed integral equation is then
numerically solved by means of the standard Galerkin method of
moments (MoM) using RWG basis functions. The methodology
is validated by comparison with Mie-series and Sommerfeld-
integral exact solutions as well as against a layer Green function-
based MoM. Challenging examples including realistic structures
relevant to the design of plasmonic solar cells and all-dielectric
metasurfaces, demonstrate the applicability, efficiency, and accu-
racy of the proposed methodology.
Index Terms—layered media, layer Green function, Sommer-
feld integrals, method of moments, dielectric cavities, solar cells,
metasurfaces
I. INTRODUCTION
Problems of electromagnetic (EM) scattering and radiation
in the presence of planar layered media have played an
important role in the development of electromagnetics since
the beginning of the 20th century, when the seminal works
of Zenneck and Sommerfeld on the propagation of radio
waves over the surface of the earth appeared [1]. Their
relevance lies in that in many application areas it is crucial
to determine the scattering from localized perturbations (e.g.,
surface roughness, small-size inclusions, meta-atoms) and/or
the field produced by localized sources (e.g., antenna feeds)
embedded within physically large structures that, away from
a certain region of interest, can be effectively assumed as
planar and infinite (e.g., the surface of the earth, silicon
substrates). This is often the case in numerous problems
in radio communications [2], remote subsurface sensing [3],
microwave circuits [4], [5], nano-optical metamaterials [6],
photonics [7], and plasmonics [8].
Popular numerical approaches to layered media scattering
include differential equation-based methods, such as the finite
difference [9] and finite element methods [10], and surface in-
z
1, ǫ1, µ1
Γ
ˆ
n
Σ
2, ǫ2, µ2
y
x
(E1,H1)
(Esrc,Hsrc)
(Esrc,Hsrc)
Fig. 1: Illustration of the scattering of a plane electromag-
netic wave by a locally perturbed penetrable half-space. The
boundary Γand the planar surface Σcoincide for (x, y, 0) far
enough from the bounded local perturbation.
tegral equation (SIE) methods, such as the method of moments
(MoM) [11] (also known as the boundary element method)
and Nyström methods [12]. Unlike differential equation-based
methods, SIE methods do not suffer from dispersion errors,
and they can easily handle unbounded domains and radiation
conditions at infinity without recourse to perfectly matched
layers or approximate absorbing/transparent boundary condi-
tions for truncation of the computational domain. Additionally,
SIE methods rely on discretization of the relevant physical
boundaries, and they therefore give rise to linear systems
of reduced dimensionality which, although dense, can be
efficiently solved by means of iterative solvers in conjunction
with fast algorithms [13].
In classical layered media SIE formulations [14]–[19], how-
ever, all these attractive features come at the price of employ-
ing the dyadic Green function for layered media, also known
as the layer Green function (LGF), which naturally enforces
the exact transmission conditions at planar unbounded physical
boundaries. The use of the LGF poses difficulties in view of
the LGF evaluation cost (there is vast literature on this subject,
for which we refer the reader to the review articles [20]–[22]).
Moreover, problems involving localized perturbations (e.g.,
open cavities and bumps) give rise to additional challenges
to LGF-SIE formulations, as artificial/transparent interfaces
need to be introduced in order to properly represent the fields
surrounding the perturbations [23].
1
arXiv:2210.02565v1 [math.NA] 15 Aug 2022
This work presents a fully 3D EM layered-media windowed
Green function (WGF) method. The WGF method, which was
originally developed for scalar layered media problems [24]–
[26] and later extended to waveguides in the frequency and
time domains [27]–[30], completely bypasses the use of Som-
merfeld integrals or other problem-specific Green functions.
This is here achieved by first deriving an indirect Müller
SIE [31], [32] given in terms of free-space Green functions and
featuring only weakly-singular kernels, which is posed on the
entire unbounded penetrable interface (see Secs. III and IV).
The unbounded SIE domain is then effectively truncated to
a bounded surface containing the localized perturbations by
introducing (in the surface integrals) a smooth windowing
function that effectively acts like a reflectionless absorber
for the surface currents leaving the windowed region (see
Sec. V). As in the case of the Helmholtz SIEs [26], the
field errors introduced by the windowing approximation decay
faster than any negative power of the diameter of the truncated
region. A straightforward (Galerkin) MoM discretization using
Rao-Wilton-Glisson (RWG) functions is used to discretize
the resulting windowed SIE (see Sec. VI), although any
other Maxwell SIE method could be employed. A limitation
of the proposed approach is that transmission conditions at
unbounded penetrable interfaces need to be enforced via
second-kind SIEs such as Müller’s. First-kind SIEs, such as
the more popular Poggio–Miller–Chang–Harrington–Wu–Tsai
(PMCHWT) [33]–[35], could be considered provided they
are converted into equivalent second-kind SIEs by means of
Calderón preconditioners [36].
Compared to LGF-SIE formulations, the WGF formulation
involves additional unknown surface currents on planar por-
tions of the unbounded dielectric interfaces that eventually lead
to larger linear systems. In many cases this additional cost is
compensated by the fact that the associated matrix coefficients
involve evaluations of the inexpensive free-space Green func-
tions and that the resulting linear system can be efficiently
solved iteratively by means of GMRES (see Sec. VII-C).
For problems involving multiple dielectric layers and/or small
size PEC inclusions, however, LGF formulations that leverage
the discrete complex images method (DCIM) [37]–[39] for
the evaluation of the LGF, may well outperform the WGF
methodology.
The proposed approach amounts to a flexible and easy-
to-implement MoM for layered media EM problems, in the
sense that only minor modifications to existing electromag-
netic SIE solvers are needed to deliver the WGF capabilities.
The method is thoroughly validated (see Sec. VII) against
the exact Mie series scattering solution for a hemispherical
bump on a perfectly electrically conducting (PEC) half-space
(using a windowed MFIE formulation), and also against
the open-source LGF code [40]. A performance compari-
son against a LGF-MoM based on the state-of-the-art C++
library Strata [41] is presented in Sec. VII-C. Finally, the
proposed methodology is showcased by means of a variety of
challenging examples including EM scattering by a large open
cavity (Sec. VII-D), an all-dielectric metasurface (Sec. VII-E),
and a three-layer plasmonic solar cell (Sec. VII-F).
II. LAYERED MEDIA SCATTERING
We consider here the problem of time-harmonic electro-
magnetic scattering of an incident field (Einc,Hinc)by a
penetrable locally perturbed half-space 2, with boundary
Γ = 2, as depicted in Fig. 1. Letting 1=R3\2, we
express the total electromagnetic field as
(Etot,Htot)=(Esrc,Hsrc)+(Ej,Hj)in j(1)
for j= 1,2.The known auxiliary source field (Esrc,Hsrc)
which is given in terms of the incident field (Einc,Hinc)under
consideration, is constructed so that the fields (Ej,Hj),j=
1,2,satisfy the homogeneous Maxwell equations
×EjµjHj=0and ×Hj+iωjEj=0in j(2)
for j= 1,2, where ω > 0is the angular frequency, and j
and µjare respectively the permittivity and the permeability
within the subdomain j. (We have assumed here that the
time dependence of the EM fields is given by et.) For
planewave incidences, for instance, (Esrc,Hsrc)is taken as
the exact total field solution of the problem of scattering of the
planewave by the flat lower half-space with planar boundary
Σ = {(x, y, 0) R3}and constants 2and µ2(see Fig. 1).
The rationale for introducing (Esrc,Hsrc)lies in ensuring that
(Ej,Hj),j= 1,2,are outgoing wavefields propagating away
from the localized perturbations or, more precisely, that they
satisfy the Silver-Müller radiation condition:
lim
|r|→∞ µjHj×r− |r|jEj=0in j, j = 1,2,(3)
uniformly in all directions r/|r|. The explicit expressions of
the source fields utilized throughout the paper are provided in
Sec. III below.
The transmission conditions at the material interfaces,
meaning that the tangential components of (Etot,Htot)are
continuous across Γ, lead to the jump conditions
ˆ
n× {E2|E1|+}=Msrc (4a)
ˆ
n× {H2|H1|+}=Jsrc (4b)
on Γ, with
Msrc := ˆ
n× {Esrc|+Esrc|}(5a)
Jsrc := ˆ
n× {Hsrc|+Hsrc|}(5b)
where we have adopted the notation F(r)|±= limδ0+ F(r±
δˆ
n(r)) for rΓ. As usual, the unit normal vector at rΓis
denoted as ˆ
n(r)and is assumed directed from 2to 1(see
Fig.1). Existence and uniqueness of solutions of the resulting
EM transmission problem are established in [42].
III. INCIDENT AND SOURCE FIELDS
Two types of incident fields (Einc,Hinc)and corresponding
auxiliary source fields (Esrc,Hsrc)are considered in this
paper, namely planewaves and electric dipoles.
Upon impinging on the planar surface Σat the interface
between the half spaces D1={z > 0}and D2={z < 0}
2
with wavenumbers k1and k2(kj=ωµjj, for j= 1,2),
respectively, the incident planewave
Einc(r)=(p×k)eik·rand Hinc(r) = 1
ωµ1
k×Einc(r)(6)
with p= (px, py, pz)and k= (0, k1y,k1z)where k1z0
and |k|=qk2
1y+k2
1z=k1, gives rise to a reflected
field (Eref ,Href )in D1and a transmitted field (Etrs,Htrs)
in D2. The resulting x-independent total field, given by
(Einc +Eref ,Hinc +Href )in D1and (Etrs,Htrs)in D2,
is completely determined by the transverse component of the
fields [43]:
Einc
x(r)
Hinc
x(r)=E0
H0exp(ik1yyik1zz)
Eref
x(r)
Href
x(r)=E0RTE
H0RTMexp(ik1yy+ik1zz)
Etrs
x(r)
Htrs
x(r)=E0TTE
H0TTMexp(ik2yyik2zz)
depending on the reflection coefficients:
RTE =µ2k1zµ1k2z
µ2k1z+µ1k2z
, RTM =2k1z1k2z
2k1z+1k2z
the transmission coefficients:
TTE =2µ2k1z
µ2k1z+µ1k2z
, T TM =22k1z
2k1z+1k2z
the amplitudes:
E0=pzk1ypyk1z, H0=k2
1
ωµ1
px
and the propagation constants k2y=k1yand k2z=
qk2
2k2
2ywith the complex square root defined so that
Im k2z0. The EM field can be retrieved from the transverse
components via
E=Exˆ
x1
Hx
z ˆ
y+1
Hx
y ˆ
z
H=Hxˆ
x+1
µ
Ex
z ˆ
y1
µ
Ex
y ˆ
z.
With these expressions at hand we define the auxiliary
planewave source field as
(Esrc,Hsrc) = ((Einc,Hinc)+(Eref ,Href )in 1
(Etrs,Htrs)in 2.(7)
Since by construction the source field (7) satisfies the exact
transmission conditions at Σ, it holds that the current sources
Msrc and Jsrc defined in (5) are supported on the (bounded)
local perturbation Γ\Σ.
In the special case when 2is occupied by a PEC, in
which the boundary condition ˆ
n×Etot =0holds on the
interface Γ, we have that (Esrc,Hsrc)takes the form (7) with
(Etrs,Htrs)=(0,0)and (Eref ,Href )given in terms of the
reflection coefficients RTE =RTM =1.
Finally, we take
Hinc =1
µj∇×{Gj(·,r0)p},Einc =1
j×Hinc (8)
with
Gj(r,r0) := eikj|rr0|
4π|rr0|(9)
being the (Helmholtz) free-space Green function, as the in-
cident field produced by an electric dipole at r0j. The
corresponding source field is thus selected as
(Esrc,Hsrc) = ((Einc,Hinc)in j
(0,0)otherwise (10)
for j= 1,2.
IV. SECOND-KIND INTEGRAL EQUATION FORMULATION
In order to approximate the unknown EM fields (Ej,Hj),
j= 1,2, we resort to a second-kind indirect Müller formula-
tion. We start by introducing the off-surface integral operators
(Sjϕ)(r) := ZΓ
Gj(r,r0)ϕ(r0) ds0+
1
k2
jZΓ
Gj(r,r0)0
s·ϕ(r0) ds0
(11)
(Djϕ)(r) := ∇ × ZΓ
Gj(r,r0)ϕ(r0) ds0(12)
for rR3\Γ, with ϕbeing a vector field tangential to Γ. (In
what follows the surface integrals over Γmust be interpreted as
conditionally convergent.) The unknown EM fields (Ej,Hj)
are thus sought as
Ej(r) := k2
j(Sjv)(r) + µj(Dju)(r)(13a)
Hj(r) := k2
j(Sju)(r)j(Djv)(r)(13b)
for rj,j= 1,2, in terms of unknown surface currents u
and vthat are to be determined by means of a SIE posed on Γ.
Clearly, the field defined in (13) satisfy Maxwell equations (2),
in view of the fact that ∇×Sj=Djand ∇×Dj=k2
jSj.
In order to derive a SIE for the currents we make use of
the well-known jump relations:
ˆ
n×(Sjϕ)|±=Tjϕand ˆ
n×(Djϕ)|±=Kjϕ±ϕ
2(14)
on rΓ, where
(Tjϕ)(r) := ˆ
n(r)×ZΓ
Gj(r,r0)ϕ(r0) ds0+
1
k2
j
ˆ
n(r)× ∇ZΓ
Gj(r,r0)0
s·ϕ(r0) ds0(15)
and
(Kjϕ)(r) := ˆ
n(r)×∇×ZΓ
Gj(r,r0)ϕ(r0) ds0.(16)
Evaluating the integral representation formulae (13) on Γ
and using (14) we obtain
ˆ
n×Ej|±=k2
jTjv+µjn±u
2+Kjuo(17a)
3
摘要:

WindowedGreenFunctionMoMforSecond-KindSurfaceIntegralEquationFormulationsofLayeredMediaElectromagneticScatteringProblemsRodrigoArrieta1andCarlosPérez-Arancibia21DepartmentofElectricalEngineering,PUCChile(riarrieta@uc.cl)2DepartmentofAppliedMathematics,UniversityofTwente(c.a.perezarancibia@utwente.nl...

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