# Electromagnetic scattering from a wire with perfectly matched layer condition

Copyright (C) 2022 Michele Castriotta, Igor Baratta, Jørgen S. Dokken

This demo is implemented in three files: one for the mesh generation with Gmsh, one for the calculation of analytical efficiencies, and one for the variational forms and the solver. It illustrates how to:

• Use complex quantities in FEniCSx

• Setup and solve Maxwell’s equations

• Implement (rectangular) perfectly matched layers

## Equations, problem definition and implementation

First, we import the required modules

import sys

try:
import gmsh
except ModuleNotFoundError:
print("This demo requires gmsh to be installed")
sys.exit(0)
import numpy as np

try:
import pyvista
have_pyvista = True
except ModuleNotFoundError:
print("pyvista and pyvistaqt are required to visualise the solution")
have_pyvista = False
from functools import partial
from typing import Tuple, Union

from efficiencies_pml_demo import calculate_analytical_efficiencies
from mesh_wire_pml import generate_mesh_wire

import ufl
from basix.ufl import element
from dolfinx import fem, mesh, plot
from dolfinx.io import VTXWriter, gmshio

from mpi4py import MPI
from petsc4py import PETSc


Since we want to solve time-harmonic Maxwell’s equation, we require that the demo is executed with DOLFINx (PETSc) complex mode.

if not np.issubdtype(PETSc.ScalarType, np.complexfloating):
print("Demo should only be executed with DOLFINx complex mode")
exit(0)


Now, let’s consider an infinite metallic wire immersed in a background medium (e.g. vacuum or water). Let’s now consider the plane cutting the wire perpendicularly to its axis at a generic point. Such plane $$\Omega=\Omega_{m} \cup\Omega_{b}$$ is formed by the cross-section of the wire $$\Omega_m$$ and the background medium $$\Omega_{b}$$ surrounding the wire. We limit the background medium with a squared perfectly matched layer (or shortly PML), which will act as an absorber for outgoing scattered waves.

The goal of this demo is to calculate the electric field $$\mathbf{E}_s$$ scattered by the wire when a background wave $$\mathbf{E}_b$$ impinges on it. We will consider a background plane wave at $$\lambda_0$$ wavelength, which can be written analytically as:

$\mathbf{E}_b = \exp(\mathbf{k}\cdot\mathbf{r})\hat{\mathbf{u}}_p$

with $$\mathbf{k} = \frac{2\pi}{\lambda_0}n_b\hat{\mathbf{u}}_k$$ being the wavevector of the plane wave, pointing along the propagation direction, with $$\hat{\mathbf{u}}_p$$ being the polarization direction, and with $$\mathbf{r}$$ being a point in $$\Omega$$. We will only consider $$\hat{\mathbf{u}}_k$$ and $$\hat{\mathbf{u}}_p$$ with components belonging to the $$\Omega$$ domain and perpendicular to each other, i.e. $$\hat{\mathbf{u}}_k \perp \hat{\mathbf{u}}_p$$ (transversality condition of plane waves). Using a Cartesian coordinate system for $$\Omega$$, and by defining $$k_x = n_bk_0\cos\theta$$ and $$k_y = n_bk_0\sin\theta$$, with $$\theta$$ being the angle defined by the propagation direction $$\hat{\mathbf{u}}_k$$ and the horizontal axis $$\hat{\mathbf{u}}_x$$, we have:

$\mathbf{E}_b = -\sin\theta e^{j (k_xx+k_yy)}\hat{\mathbf{u}}_x + \cos\theta e^{j (k_xx+k_yy)}\hat{\mathbf{u}}_y$

The function background_field below implements this analytical formula:

def background_field(theta: float, n_b: float, k0: complex,
x: np.typing.NDArray[np.float64]):

kx = n_b * k0 * np.cos(theta)
ky = n_b * k0 * np.sin(theta)
phi = kx * x + ky * x
return (-np.sin(theta) * np.exp(1j * phi), np.cos(theta) * np.exp(1j * phi))


For convenience, we define the $$\nabla\times$$ operator for a 2D vector

def curl_2d(a: fem.Function):
return ufl.as_vector((0, 0, a.dx(0) - a.dx(1)))


Let’s now see how we can implement PMLs for our problem. PMLs are artificial layers surrounding the real domain that gradually absorb waves impinging them. Mathematically, we can use a complex coordinate transformation of this kind to obtain this absorption:

\begin{align} & x^\prime= x\left{1+j\frac{\alpha}{k_0}\left[\frac{|x|-l_{dom}/2} {(l_{pml}/2 - l_{dom}/2)^2}\right] \right}\ \end{align}

with $$l_{dom}$$ and $$l_{pml}$$ being the lengths of the domain without and with PML, respectively, and with $$\alpha$$ being a parameter that tunes the absorption within the PML (the bigger the $$\alpha$$, the faster the absorption). In DOLFINx, we can define this coordinate transformation in the following way:

def pml_coordinates(x: ufl.indexed.Indexed, alpha: float, k0: complex, l_dom: float, l_pml: float):
return (x + 1j * alpha / k0 * x * (ufl.algebra.Abs(x) - l_dom / 2) / (l_pml / 2 - l_dom / 2)**2)


We use the following domain specific parameters.

# Constants
epsilon_0 = 8.8541878128 * 10**-12
mu_0 = 4 * np.pi * 10**-7

# Radius of the wire and of the boundary of the domain
l_dom = 0.8
radius_scatt = 0.8 * l_dom / 2
l_pml = 1

# The smaller the mesh_factor, the finer is the mesh
mesh_factor = 1

# Mesh size inside the wire
in_wire_size = mesh_factor * 6e-3

# Mesh size at the boundary of the wire
on_wire_size = mesh_factor * 3.0e-3

# Mesh size in the background
scatt_size = mesh_factor * 15.0e-3

# Mesh size at the boundary
pml_size = mesh_factor * 15.0e-3

# Tags for the subdomains
au_tag = 1
bkg_tag = 2
scatt_tag = 3
pml_tag = 4


We generate the mesh using GMSH and convert it to a dolfinx.mesh.Mesh.

model = None
gmsh.initialize(sys.argv)
if MPI.COMM_WORLD.rank == 0:
in_wire_size, on_wire_size, scatt_size, pml_size,
au_tag, bkg_tag, scatt_tag, pml_tag)
model = MPI.COMM_WORLD.bcast(model, root=0)
msh, cell_tags, facet_tags = gmshio.model_to_mesh(model, MPI.COMM_WORLD, 0, gdim=2)

gmsh.finalize()
MPI.COMM_WORLD.barrier()


We visualize the mesh and subdomains with PyVista

if have_pyvista:
topology, cell_types, geometry = plot.create_vtk_mesh(msh, 2)
grid = pyvista.UnstructuredGrid(topology, cell_types, geometry)
plotter = pyvista.Plotter()
num_local_cells = msh.topology.index_map(msh.topology.dim).size_local
grid.cell_data["Marker"] = cell_tags.values[cell_tags.indices < num_local_cells]
grid.set_active_scalars("Marker")
plotter.view_xy()
if not pyvista.OFF_SCREEN:
plotter.show(interactive=True)
else:
pyvista.start_xvfb()
figure = plotter.screenshot("wire_mesh_pml.png", window_size=[800, 800])


We observe five different subdomains: one for the gold wire (au_tag), one for the background medium (bkg_tag), one for the PML corners (pml_tag), one for the PML rectangles along $$x$$ (pml_tag + 1), and one for the PML rectangles along $$y$$ (pml_tag + 2). These different PML regions have different coordinate transformation, as specified here below:

\begin{align} \text{PML}\text{corners} \rightarrow \mathbf{r}^\prime & = (x^\prime, y^\prime) \ \text{PML}\text{rectangles along x} \rightarrow \mathbf{r}^\prime & = (x^\prime, y) \ \text{PML}_\text{rectangles along y} \rightarrow \mathbf{r}^\prime & = (x, y^\prime). \end{align}

Now we define some other problem specific parameters:

wl0 = 0.4  # Wavelength of the background field
n_bkg = 1  # Background refractive index
eps_bkg = n_bkg**2  # Background relative permittivity
k0 = 2 * np.pi / wl0  # Wavevector of the background field
theta = 0  # Angle of incidence of the background field


We use a degree 3 Nedelec (first kind) element to represent the electric field:

degree = 3
curl_el = element("N1curl", msh.basix_cell(), degree)
V = fem.FunctionSpace(msh, curl_el)


Next, we interpolate $$\mathbf{E}_b$$ into the function space $$V$$, define our trial and test function, and the integration domains:

Eb = fem.Function(V)
f = partial(background_field, theta, n_bkg, k0)
Eb.interpolate(f)

# Definition of Trial and Test functions
Es = ufl.TrialFunction(V)
v = ufl.TestFunction(V)

# Definition of 3d fields
Es_3d = ufl.as_vector((Es, Es, 0))
v_3d = ufl.as_vector((v, v, 0))

# Measures for subdomains
dx = ufl.Measure("dx", msh, subdomain_data=cell_tags)
dDom = dx((au_tag, bkg_tag))
dPml_xy = dx(pml_tag)
dPml_x = dx(pml_tag + 1)
dPml_y = dx(pml_tag + 2)


Let’s now define the relative permittivity $$\varepsilon_m$$ of the gold wire at $$400nm$$ (data taken from Olmon et al. 2012 , and for a quick reference have a look at refractiveindex.info):

# Definition of relative permittivity for Au @400nm
eps_au = -1.0782 + 1j * 5.8089


We can now define a space function for the permittivity $$\varepsilon$$ that takes the value $$\varepsilon_m$$ for cells inside the wire, while it takes the value of the background permittivity $$\varepsilon_b$$ in the background region:

D = fem.FunctionSpace(msh, ("DG", 0))
eps = fem.Function(D)
au_cells = cell_tags.find(au_tag)
bkg_cells = cell_tags.find(bkg_tag)
eps.x.array[au_cells] = np.full_like(au_cells, eps_au, dtype=np.complex128)
eps.x.array[bkg_cells] = np.full_like(bkg_cells, eps_bkg, dtype=np.complex128)
eps.x.scatter_forward()


Now we need to define our weak form in DOLFINx. Let’s write the PML weak form first. As a first step, we can define our new complex coordinates as:

x = ufl.SpatialCoordinate(msh)
alpha = 1

# PML corners
xy_pml = ufl.as_vector((pml_coordinates(x, alpha, k0, l_dom, l_pml),
pml_coordinates(x, alpha, k0, l_dom, l_pml)))

# PML rectangles along x
x_pml = ufl.as_vector((pml_coordinates(x, alpha, k0, l_dom, l_pml), x))

# PML rectangles along y
y_pml = ufl.as_vector((x, pml_coordinates(x, alpha, k0, l_dom, l_pml)))


We can then express this coordinate systems as a material transformation within the PML region. In other words, the PML region can be interpreted as a material having, in general, anisotropic, inhomogeneous and complex permittivity $$\boldsymbol{\varepsilon}_{pml}$$ and permeability $$\boldsymbol{\mu}_{pml}$$. To do this, we need to calculate the Jacobian of the coordinate transformation:

$\begin{split} \mathbf{J}=\mathbf{A}^{-1}= \nabla\boldsymbol{x}^ \prime(\boldsymbol{x}) = \left[\begin{array}{ccc} \frac{\partial x^{\prime}}{\partial x} & \frac{\partial y^{\prime}}{\partial x} & \frac{\partial z^{\prime}}{\partial x} \\ \frac{\partial x^{\prime}}{\partial y} & \frac{\partial y^{\prime}}{\partial y} & \frac{\partial z^{\prime}}{\partial y} \\ \frac{\partial x^{\prime}}{\partial z} & \frac{\partial y^{\prime}}{\partial z} & \frac{\partial z^{\prime}}{\partial z} \end{array}\right]=\left[\begin{array}{ccc} \frac{\partial x^{\prime}}{\partial x} & 0 & 0 \\ 0 & \frac{\partial y^{\prime}}{\partial y} & 0 \\ 0 & 0 & \frac{\partial z^{\prime}}{\partial z} \end{array}\right]=\left[\begin{array}{ccc} J_{11} & 0 & 0 \\ 0 & J_{22} & 0 \\ 0 & 0 & 1 \end{array}\right] \end{split}$

Then, our $$\boldsymbol{\varepsilon}_{pml}$$ and $$\boldsymbol{\mu}_{pml}$$ can be calculated with the following formula, from Ward & Pendry, 1996:

$\begin{split} {\boldsymbol{\varepsilon}_{pml}} &= A^{-1} \mathbf{A} {\boldsymbol{\varepsilon}_b}\mathbf{A}^{T},\\ {\boldsymbol{\mu}_{pml}} &= A^{-1} \mathbf{A} {\boldsymbol{\mu}_b}\mathbf{A}^{T}, \end{split}$

with $$A^{-1}=\operatorname{det}(\mathbf{J})$$.

We use ufl.grad to calculate the Jacobian of our coordinate transformation for the different PML regions, and then we can implement this Jacobian for calculating $$\boldsymbol{\varepsilon}_{pml}$$ and $$\boldsymbol{\mu}_{pml}$$. The here below function named create_eps_mu() serves this purpose:



def create_eps_mu(pml: ufl.tensors.ListTensor,
eps_bkg: Union[float, ufl.tensors.ListTensor],
mu_bkg: Union[float, ufl.tensors.ListTensor]) -> Tuple[ufl.tensors.ComponentTensor,
ufl.tensors.ComponentTensor]:

# Transform the 2x2 Jacobian into a 3x3 matrix.
J = ufl.as_matrix(((J[0, 0], 0, 0),
(0, J[1, 1], 0),
(0, 0, 1)))

A = ufl.inv(J)
eps_pml = ufl.det(J) * A * eps_bkg * ufl.transpose(A)
mu_pml = ufl.det(J) * A * mu_bkg * ufl.transpose(A)
return eps_pml, mu_pml

eps_x, mu_x = create_eps_mu(x_pml, eps_bkg, 1)
eps_y, mu_y = create_eps_mu(y_pml, eps_bkg, 1)
eps_xy, mu_xy = create_eps_mu(xy_pml, eps_bkg, 1)


The final weak form in the PML region is:

$\int_{\Omega_{pml}}\left[\boldsymbol{\mu}^{-1}_{pml} \nabla \times \mathbf{E} \right]\cdot \nabla \times \bar{\mathbf{v}}-k_{0}^{2} \left[\boldsymbol{\varepsilon}_{pml} \mathbf{E} \right]\cdot \bar{\mathbf{v}}~ d x=0,$

while in the rest of the domain is:

$& \int_{\Omega_m\cup\Omega_b}-(\nabla \times \mathbf{E}_s) \cdot (\nabla \times \bar{\mathbf{v}})+\varepsilon_{r} k_{0}^{2} \mathbf{E}_s \cdot \bar{\mathbf{v}}+k_{0}^{2}\left(\varepsilon_{r} -\varepsilon_b\right)\mathbf{E}_b \cdot \bar{\mathbf{v}}~\mathrm{d}x. = 0.$

Let’s solve this equation in DOLFINx:

# Definition of the weak form
F = - ufl.inner(curl_2d(Es), curl_2d(v)) * dDom \
+ eps * (k0**2) * ufl.inner(Es, v) * dDom \
+ (k0**2) * (eps - eps_bkg) * ufl.inner(Eb, v) * dDom \
- ufl.inner(ufl.inv(mu_x) * curl_2d(Es), curl_2d(v)) * dPml_x \
- ufl.inner(ufl.inv(mu_y) * curl_2d(Es), curl_2d(v)) * dPml_y \
- ufl.inner(ufl.inv(mu_xy) * curl_2d(Es), curl_2d(v)) * dPml_xy \
+ (k0**2) * ufl.inner(eps_x * Es_3d, v_3d) * dPml_x \
+ (k0**2) * ufl.inner(eps_y * Es_3d, v_3d) * dPml_y \
+ (k0**2) * ufl.inner(eps_xy * Es_3d, v_3d) * dPml_xy

a, L = ufl.lhs(F), ufl.rhs(F)

problem = fem.petsc.LinearProblem(a, L, bcs=[], petsc_options={"ksp_type": "preonly", "pc_type": "lu"})
Esh = problem.solve()


Let’s now save the solution in a bp-file. In order to do so, we need to interpolate our solution discretized with Nedelec elements into a compatible discontinuous Lagrange space.

V_dg = fem.VectorFunctionSpace(msh, ("DG", degree))
Esh_dg = fem.Function(V_dg)
Esh_dg.interpolate(Esh)

with VTXWriter(msh.comm, "Esh.bp", Esh_dg) as vtx:
vtx.write(0.0)


For more information about saving and visualizing vector fields discretized with Nedelec elements, check this DOLFINx demo.

if have_pyvista:
V_cells, V_types, V_x = plot.create_vtk_mesh(V_dg)
V_grid = pyvista.UnstructuredGrid(V_cells, V_types, V_x)
Esh_values = np.zeros((V_x.shape, 3), dtype=np.float64)
Esh_values[:, :msh.topology.dim] = Esh_dg.x.array.reshape(V_x.shape, msh.topology.dim).real
V_grid.point_data["u"] = Esh_values

plotter = pyvista.Plotter()
plotter.view_xy()

if not pyvista.OFF_SCREEN:
plotter.show()
else:
pyvista.start_xvfb()
plotter.screenshot("Esh.png", window_size=[800, 800])


Next we can calculate the total electric field $$\mathbf{E}=\mathbf{E}_s+\mathbf{E}_b$$ and save it:

E = fem.Function(V)
E.x.array[:] = Eb.x.array[:] + Esh.x.array[:]

E_dg = fem.Function(V_dg)
E_dg.interpolate(E)

with VTXWriter(msh.comm, "E.bp", E_dg) as vtx:
vtx.write(0.0)


## Post-processing

To validate the formulation we calculate the absorption, scattering and extinction efficiencies, which are quantities that define how much light is absorbed and scattered by the wire. First of all, we calculate the analytical efficiencies with the calculate_analytical_efficiencies function defined in a separate file:

q_abs_analyt, q_sca_analyt, q_ext_analyt = calculate_analytical_efficiencies(eps_au, n_bkg, wl0, radius_wire)


We calculate the numerical efficiencies in the same way as done in demo_scattering_boundary_conditions.py, with the only difference that now the scattering efficiency needs to be calculated over an inner facet, and therefore it requires a slightly different approach:

# Vacuum impedance
Z0 = np.sqrt(mu_0 / epsilon_0)

# Magnetic field H
Hsh_3d = -1j * curl_2d(Esh) / (Z0 * k0 * n_bkg)

Esh_3d = ufl.as_vector((Esh, Esh, 0))
E_3d = ufl.as_vector((E, E, 0))

# Intensity of the electromagnetic fields I0 = 0.5*E0**2/Z0
# E0 = np.sqrt(ax**2 + ay**2) = 1, see background_electric_field
I0 = 0.5 / Z0

# Geometrical cross section of the wire

n = ufl.FacetNormal(msh)
n_3d = ufl.as_vector((n, n, 0))

# Create a marker for the integration boundary for the scattering
# efficiency
marker = fem.Function(D)
scatt_facets = facet_tags.find(scatt_tag)
incident_cells = mesh.compute_incident_entities(msh.topology, scatt_facets, msh.topology.dim - 1,
msh.topology.dim)

midpoints = mesh.compute_midpoints(msh, msh.topology.dim, incident_cells)
inner_cells = incident_cells[(midpoints[:, 0]**2 + midpoints[:, 1]**2) < (radius_scatt)**2]

marker.x.array[inner_cells] = 1

# Quantities for the calculation of efficiencies
P = 0.5 * ufl.inner(ufl.cross(Esh_3d, ufl.conj(Hsh_3d)), n_3d) * marker
Q = 0.5 * eps_au.imag * k0 * (ufl.inner(E_3d, E_3d)) / (Z0 * n_bkg)

# Define integration domain for the wire
dAu = dx(au_tag)

# Define integration facet for the scattering efficiency
dS = ufl.Measure("dS", msh, subdomain_data=facet_tags)

# Normalized absorption efficiency
q_abs_fenics_proc = (fem.assemble_scalar(fem.form(Q * dAu)) / (gcs * I0)).real
# Sum results from all MPI processes
q_abs_fenics = msh.comm.allreduce(q_abs_fenics_proc, op=MPI.SUM)

# Normalized scattering efficiency
q_sca_fenics_proc = (fem.assemble_scalar(fem.form((P('+') + P('-')) * dS(scatt_tag))) / (gcs * I0)).real

# Sum results from all MPI processes
q_sca_fenics = msh.comm.allreduce(q_sca_fenics_proc, op=MPI.SUM)

# Extinction efficiency
q_ext_fenics = q_abs_fenics + q_sca_fenics

# Error calculation
err_abs = np.abs(q_abs_analyt - q_abs_fenics) / q_abs_analyt
err_sca = np.abs(q_sca_analyt - q_sca_fenics) / q_sca_analyt
err_ext = np.abs(q_ext_analyt - q_ext_fenics) / q_ext_analyt

if msh.comm.rank == 0:
print()
print(f"The analytical absorption efficiency is {q_abs_analyt}")
print(f"The numerical absorption efficiency is {q_abs_fenics}")
print(f"The error is {err_abs*100}%")
print()
print(f"The analytical scattering efficiency is {q_sca_analyt}")
print(f"The numerical scattering efficiency is {q_sca_fenics}")
print(f"The error is {err_sca*100}%")
print()
print(f"The analytical extinction efficiency is {q_ext_analyt}")
print(f"The numerical extinction efficiency is {q_ext_fenics}")
print(f"The error is {err_ext*100}%")

# Check if errors are smaller than 1%
assert err_abs < 0.01
# assert err_sca < 0.01
assert err_ext < 0.01