# 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 ```python import importlib.util if importlib.util.find_spec("petsc4py") is not None: import dolfinx if not dolfinx.has_petsc: print("This demo requires DOLFINx to be compiled with PETSc enabled.") exit(0) else: print("This demo requires petsc4py.") exit(0) import sys from functools import partial from typing import Union from mpi4py import MPI import numpy as np from scipy.special import h2vp, hankel2, jv, jvp import ufl from basix.ufl import element from dolfinx import default_real_type, default_scalar_type, fem, mesh, plot from dolfinx.fem.petsc import LinearProblem from dolfinx.io import gmshio try: from dolfinx.io import VTXWriter except ImportError: print("This demo requires DOLFINx to be configured with adios2.") exit(0) try: import gmsh except ModuleNotFoundError: print("This demo requires gmsh to be installed") exit(0) try: import pyvista have_pyvista = True except ModuleNotFoundError: print("pyvista and pyvistaqt are required to visualise the solution") have_pyvista = False 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(default_scalar_type, np.complexfloating): print("Demo should only be executed with DOLFINx complex mode") exit(0) # This file defines the `generate_mesh_wire` function, which is used to # generate the mesh used for the PML demo. The mesh is made up by a # central circle (the wire), and an external layer (the PML) divided in # 4 rectangles and 4 squares at the corners. The `generate_mesh_wire` # function takes as input: # - `radius_wire`: the radius of the wire # - `radius_scatt`: the radius of the circle where scattering efficiency # is calculated # - `l_dom`: length of real domain # - `l_pml`: length of PML layer # - `in_wire_size`: the mesh size at a distance `0.8 * radius_wire` from # the origin # - `on_wire_size`: the mesh size on the wire boundary # - `scatt_size`: the mesh size on the circle where scattering # efficiency is calculated # - `pml_size`: the mesh size on the outer boundary of the PML # - `au_tag`: the tag of the physical group representing the wire # - `bkg_tag`: the tag of the physical group representing the background # - `scatt_tag`: the tag of the physical group representing the boundary # where scattering efficiency is calculated # - `pml_tag`: the tag of the physical group representing the PML # (together with pml_tag+1 and pml_tag+2) # # from functools import reduce def generate_mesh_wire( radius_wire: float, radius_scatt: float, l_dom: float, l_pml: float, in_wire_size: float, on_wire_size: float, scatt_size: float, pml_size: float, au_tag: int, bkg_tag: int, scatt_tag: int, pml_tag: int, ): dim = 2 # A dummy circle for setting a finer mesh c1 = gmsh.model.occ.addCircle(0.0, 0.0, 0.0, radius_wire * 0.8, angle1=0.0, angle2=2 * np.pi) gmsh.model.occ.addCurveLoop([c1], tag=c1) gmsh.model.occ.addPlaneSurface([c1], tag=c1) c2 = gmsh.model.occ.addCircle(0.0, 0.0, 0.0, radius_wire, angle1=0, angle2=2 * np.pi) gmsh.model.occ.addCurveLoop([c2], tag=c2) gmsh.model.occ.addPlaneSurface([c2], tag=c2) wire, _ = gmsh.model.occ.fragment([(dim, c2)], [(dim, c1)]) # A dummy circle for the calculation of the scattering efficiency c3 = gmsh.model.occ.addCircle(0.0, 0.0, 0.0, radius_scatt, angle1=0, angle2=2 * np.pi) gmsh.model.occ.addCurveLoop([c3], tag=c3) gmsh.model.occ.addPlaneSurface([c3], tag=c3) r0 = gmsh.model.occ.addRectangle(-l_dom / 2, -l_dom / 2, 0, l_dom, l_dom) inclusive_rectangle, _ = gmsh.model.occ.fragment([(dim, r0)], [(dim, c3)]) delta_pml = (l_pml - l_dom) / 2 separate_rectangle, _ = gmsh.model.occ.cut(inclusive_rectangle, wire, removeTool=False) _, physical_domain = gmsh.model.occ.fragment(separate_rectangle, wire) bkg_tags = [tag[0] for tag in physical_domain[: len(separate_rectangle)]] wire_tags = [ tag[0] for tag in physical_domain[len(separate_rectangle) : len(inclusive_rectangle) + len(wire)] ] # Corner PMLS pml1 = gmsh.model.occ.addRectangle(-l_pml / 2, l_dom / 2, 0, delta_pml, delta_pml) pml2 = gmsh.model.occ.addRectangle(-l_pml / 2, -l_pml / 2, 0, delta_pml, delta_pml) pml3 = gmsh.model.occ.addRectangle(l_dom / 2, l_dom / 2, 0, delta_pml, delta_pml) pml4 = gmsh.model.occ.addRectangle(l_dom / 2, -l_pml / 2, 0, delta_pml, delta_pml) corner_pmls = [(dim, pml1), (dim, pml2), (dim, pml3), (dim, pml4)] # X pmls pml5 = gmsh.model.occ.addRectangle(-l_pml / 2, -l_dom / 2, 0, delta_pml, l_dom) pml6 = gmsh.model.occ.addRectangle(l_dom / 2, -l_dom / 2, 0, delta_pml, l_dom) x_pmls = [(dim, pml5), (dim, pml6)] # Y pmls pml7 = gmsh.model.occ.addRectangle(-l_dom / 2, l_dom / 2, 0, l_dom, delta_pml) pml8 = gmsh.model.occ.addRectangle(-l_dom / 2, -l_pml / 2, 0, l_dom, delta_pml) y_pmls = [(dim, pml7), (dim, pml8)] _, surface_map = gmsh.model.occ.fragment(bkg_tags + wire_tags, corner_pmls + x_pmls + y_pmls) gmsh.model.occ.synchronize() bkg_group = [tag[0][1] for tag in surface_map[: len(bkg_tags)]] gmsh.model.addPhysicalGroup(dim, bkg_group, tag=bkg_tag) wire_group = [tag[0][1] for tag in surface_map[len(bkg_tags) : len(bkg_tags + wire_tags)]] gmsh.model.addPhysicalGroup(dim, wire_group, tag=au_tag) corner_group = [ tag[0][1] for tag in surface_map[len(bkg_tags + wire_tags) : len(bkg_tags + wire_tags + corner_pmls)] ] gmsh.model.addPhysicalGroup(dim, corner_group, tag=pml_tag) x_group = [ tag[0][1] for tag in surface_map[ len(bkg_tags + wire_tags + corner_pmls) : len( bkg_tags + wire_tags + corner_pmls + x_pmls ) ] ] gmsh.model.addPhysicalGroup(dim, x_group, tag=pml_tag + 1) y_group = [ tag[0][1] for tag in surface_map[ len(bkg_tags + wire_tags + corner_pmls + x_pmls) : len( bkg_tags + wire_tags + corner_pmls + x_pmls + y_pmls ) ] ] gmsh.model.addPhysicalGroup(dim, y_group, tag=pml_tag + 2) # Marker interior surface in bkg group boundaries: list[np.typing.NDArray[np.int32]] = [] for tag in bkg_group: boundary_pairs = gmsh.model.get_boundary([(dim, tag)], oriented=False) boundaries.append(np.asarray([pair[1] for pair in boundary_pairs], dtype=np.int32)) interior_boundary = reduce(np.intersect1d, boundaries) gmsh.model.addPhysicalGroup(dim - 1, interior_boundary, tag=scatt_tag) gmsh.model.mesh.setSize([(0, 1)], size=in_wire_size) gmsh.model.mesh.setSize([(0, 2)], size=on_wire_size) gmsh.model.mesh.setSize([(0, 3)], size=scatt_size) gmsh.model.mesh.setSize([(0, x) for x in range(4, 40)], size=pml_size) gmsh.model.mesh.generate(2) return gmsh.model # This file contains a function for the calculation of the # absorption, scattering and extinction efficiencies of a wire # being hit normally by a TM-polarized electromagnetic wave. # # The formula are taken from: # Milton Kerker, "The Scattering of Light and Other Electromagnetic Radiation", # Chapter 6, Elsevier, 1969. # # ## Implementation # First of all, let's define the parameters of the problem: # # - $n = \sqrt{\varepsilon}$: refractive index of the wire, # - $n_b$: refractive index of the background medium, # - $m = n/n_b$: relative refractive index of the wire, # - $\lambda_0$: wavelength of the electromagnetic wave, # - $r_w$: radius of the cross-section of the wire, # - $\alpha = 2\pi r_w n_b/\lambda_0$. # # Now, let's define the $a_\nu$ coefficients as: # # $$ # \begin{equation} # a_\nu=\frac{J_\nu(\alpha) J_\nu^{\prime}(m \alpha)-m J_\nu(m \alpha) # J_\nu^{\prime}(\alpha)}{H_\nu^{(2)}(\alpha) J_\nu^{\prime}(m \alpha) # -m J_\nu(m \alpha) H_\nu^{(2){\prime}}(\alpha)} # \end{equation} # $$ # # where: # - $J_\nu(x)$: $\nu$-th order Bessel function of the first kind, # - $J_\nu^{\prime}(x)$: first derivative with respect to $x$ of # the $\nu$-th order Bessel function of the first kind, # - $H_\nu^{(2)}(x)$: $\nu$-th order Hankel function of the second kind, # - $H_\nu^{(2){\prime}}(x)$: first derivative with respect to $x$ of # the $\nu$-th order Hankel function of the second kind. # # We can now calculate the scattering, extinction and absorption # efficiencies as: # # $$ # & q_{\mathrm{sca}}=(2 / \alpha)\left[\left|a_0\right|^{2} ``` ```python :incorrectly_encoded_metadata: '{\nu=1}^{\infty}\left|a_\nu\right|^{2}\right] \\' :title: 2 \sum_ # & q_{\mathrm{ext}}=(2 / \alpha) \operatorname{Re}\left[ a_0 ``` ```python :incorrectly_encoded_metadata: '{\nu=1}^{\infty} a_\nu\right] \\' :title: 2 \sum_ # & q_{\mathrm{abs}} = q_{\mathrm{ext}} - q_{\mathrm{sca}} # $$ # The functions that we import from `scipy.special` correspond to: # # - `jv(nu, x)` ⟷ $J_\nu(x)$, # - `jvp(nu, x, 1)` ⟷ $J_\nu^{\prime}(x)$, # - `hankel2(nu, x)` ⟷ $H_\nu^{(2)}(x)$, # - `h2vp(nu, x, 1)` ⟷ $H_\nu^{(2){\prime}}(x)$. # # Next, we define a function for calculating the analytical efficiencies # in Python. The inputs of the function are: # # - `eps` ⟷ $\varepsilon$, # - `n_bkg` ⟷ $n_b$, # - `wl0` ⟷ $\lambda_0$, # - `radius_wire` ⟷ $r_w$. # # We also define a nested function for the calculation of $a_l$. For the # final calculation of the efficiencies, the summation over the different # orders of the Bessel functions is truncated at $\nu=50$. ``` ```python def compute_a(nu: int, m: complex, alpha: float) -> float: J_nu_alpha = jv(nu, alpha) J_nu_malpha = jv(nu, m * alpha) J_nu_alpha_p = jvp(nu, alpha, 1) J_nu_malpha_p = jvp(nu, m * alpha, 1) H_nu_alpha = hankel2(nu, alpha) H_nu_alpha_p = h2vp(nu, alpha, 1) a_nu_num = J_nu_alpha * J_nu_malpha_p - m * J_nu_malpha * J_nu_alpha_p a_nu_den = H_nu_alpha * J_nu_malpha_p - m * J_nu_malpha * H_nu_alpha_p return a_nu_num / a_nu_den def calculate_analytical_efficiencies( eps: complex, n_bkg: float, wl0: float, radius_wire: float, num_n: int = 50 ) -> tuple[float, float, float]: m = np.sqrt(np.conj(eps)) / n_bkg alpha = 2 * np.pi * radius_wire / wl0 * n_bkg c = 2 / alpha q_ext = c * np.real(compute_a(0, m, alpha)) q_sca = c * np.abs(compute_a(0, m, alpha)) ** 2 for nu in range(1, num_n + 1): q_ext += c * 2 * np.real(compute_a(nu, m, alpha)) q_sca += c * 2 * np.abs(compute_a(nu, m, alpha)) ** 2 return q_ext - q_sca, q_sca, q_ext # 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: # # $$ # \mathbf{E}_b = -\sin\theta e^{j (k_xx+k_yy)}\hat{\mathbf{u}}_x ``` ```python :incorrectly_encoded_metadata: '{j (k_xx+k_yy)}\hat{\mathbf{u}}_y' :title: \cos\theta e^ # $$ # # The function `background_field` below implements this analytical # formula: ``` ```python 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[0] + ky * x[1] 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 ```python def curl_2d(a: fem.Function): return ufl.as_vector((0, 0, a[1].dx(0) - a[0].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: $$ x^\prime= x\left\{1+j\frac{\alpha}{k_0}\left[\frac{|x|-l_{dom}/2} {(l_{pml}/2 - l_{dom}/2)^2}\right] \right\} $$ 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: ```python 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. ```python # 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 radius_wire = 0.05 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`. ```python model = None gmsh.initialize(sys.argv) if MPI.COMM_WORLD.rank == 0: model = generate_mesh_wire( radius_wire, radius_scatt, l_dom, l_pml, 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) partitioner = dolfinx.cpp.mesh.create_cell_partitioner(dolfinx.mesh.GhostMode.shared_facet) mesh_data = gmshio.model_to_mesh(model, MPI.COMM_WORLD, 0, gdim=2, partitioner=partitioner) assert mesh_data.cell_tags is not None, "Cell tags are missing" assert mesh_data.facet_tags is not None, "Facet tags are missing" gmsh.finalize() MPI.COMM_WORLD.barrier() ``` We visualize the mesh and subdomains with [PyVista](https://docs.pyvista.org/) ```python tdim = mesh_data.mesh.topology.dim if have_pyvista: topology, cell_types, geometry = plot.vtk_mesh(mesh_data.mesh, 2) grid = pyvista.UnstructuredGrid(topology, cell_types, geometry) plotter = pyvista.Plotter() num_local_cells = mesh_data.mesh.topology.index_map(tdim).size_local grid.cell_data["Marker"] = mesh_data.cell_tags.values[ mesh_data.cell_tags.indices < num_local_cells ] grid.set_active_scalars("Marker") plotter.add_mesh(grid, show_edges=True) 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: ```python 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)](https://defelement.com/elements/nedelec1.html) element to represent the electric field: ```python degree = 3 curl_el = element("N1curl", mesh_data.mesh.basix_cell(), degree, dtype=default_real_type) V = fem.functionspace(mesh_data.mesh, curl_el) ``` Next, we interpolate $\mathbf{E}_b$ into the function space $V$, define our trial and test function, and the integration domains: ```python 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[0], Es[1], 0)) v_3d = ufl.as_vector((v[0], v[1], 0)) # Measures for subdomains dx = ufl.Measure("dx", mesh_data.mesh, subdomain_data=mesh_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*](https://doi.org/10.1103/PhysRevB.86.235147) , and for a quick reference have a look at [refractiveindex.info]( https://refractiveindex.info/?shelf=main&book=Au&page=Olmon-sc)): ```python # 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: ```python D = fem.functionspace(mesh_data.mesh, ("DG", 0)) eps = fem.Function(D) au_cells = mesh_data.cell_tags.find(au_tag) bkg_cells = mesh_data.cell_tags.find(bkg_tag) eps.x.array[au_cells] = np.full_like(au_cells, eps_au, dtype=eps.x.array.dtype) eps.x.array[bkg_cells] = np.full_like(bkg_cells, eps_bkg, dtype=eps.x.array.dtype) 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: ```python x = ufl.SpatialCoordinate(mesh_data.mesh) alpha = 1 # PML corners xy_pml = ufl.as_vector( (pml_coordinates(x[0], alpha, k0, l_dom, l_pml), pml_coordinates(x[1], alpha, k0, l_dom, l_pml)) ) # PML rectangles along x x_pml = ufl.as_vector((pml_coordinates(x[0], alpha, k0, l_dom, l_pml), x[1])) # PML rectangles along y y_pml = ufl.as_vector((x[0], pml_coordinates(x[1], 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: $$ \mathbf{J}=\mathbf{A}^{-1}= \nabla\boldsymbol{x}^ \prime(\boldsymbol{x}) = \left[\begin{array}{ccc} \frac{\partial x^{\prime}}{\partial x} & \frac{\partial y^{\prime}}{\partial x} & \frac{\partial z^{\prime}}{\partial x} \\ \frac{\partial x^{\prime}}{\partial y} & \frac{\partial y^{\prime}}{\partial y} & \frac{\partial z^{\prime}}{\partial y} \\ \frac{\partial x^{\prime}}{\partial z} & \frac{\partial y^{\prime}}{\partial z} & \frac{\partial z^{\prime}}{\partial z} \end{array}\right]=\left[\begin{array}{ccc} \frac{\partial x^{\prime}}{\partial x} & 0 & 0 \\ 0 & \frac{\partial y^{\prime}}{\partial y} & 0 \\ 0 & 0 & \frac{\partial z^{\prime}}{\partial z} \end{array}\right]=\left[\begin{array}{ccc} J_{11} & 0 & 0 \\ 0 & J_{22} & 0 \\ 0 & 0 & 1 \end{array}\right] $$ Then, our $\boldsymbol{\varepsilon}_{pml}$ and $\boldsymbol{\mu}_{pml}$ can be calculated with the following formula, from [Ward & Pendry, 1996]( https://www.tandfonline.com/doi/abs/10.1080/09500349608232782): $$ \begin{align} {\boldsymbol{\varepsilon}_{pml}} &= A^{-1} \mathbf{A} {\boldsymbol{\varepsilon}_b}\mathbf{A}^{T},\\ {\boldsymbol{\mu}_{pml}} &= A^{-1} \mathbf{A} {\boldsymbol{\mu}_b}\mathbf{A}^{T}, \end{align} $$ 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: ```python 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]: J = ufl.grad(pml) # 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: ```python # 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) # For factorisation prefer MUMPS, then superlu_dist, then default sys = PETSc.Sys() # type: ignore use_superlu = PETSc.IntType == np.int64 if sys.hasExternalPackage("mumps") and not use_superlu: # type: ignore mat_factor_backend = "mumps" elif sys.hasExternalPackage("superlu_dist"): # type: ignore mat_factor_backend = "superlu_dist" else: if mesh_data.mesh.comm > 1: raise RuntimeError("This demo requires a parallel LU solver.") else: mat_factor_backend = "petsc" problem = LinearProblem( a, L, bcs=[], petsc_options={ "ksp_type": "preonly", "pc_type": "lu", "pc_factor_mat_solver_type": mat_factor_backend, }, ) Esh = problem.solve() assert problem.solver.getConvergedReason() > 0, "Solver did not converge!" ``` 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. ```python gdim = mesh_data.mesh.geometry.dim V_dg = fem.functionspace(mesh_data.mesh, ("DG", degree, (gdim,))) Esh_dg = fem.Function(V_dg) Esh_dg.interpolate(Esh) with VTXWriter(mesh_data.mesh.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]( https://docs.fenicsproject.org/dolfinx/main/python/demos/demo_interpolation-io.html) DOLFINx demo. ```python if have_pyvista: V_cells, V_types, V_x = plot.vtk_mesh(V_dg) V_grid = pyvista.UnstructuredGrid(V_cells, V_types, V_x) Esh_values = np.zeros((V_x.shape[0], 3), dtype=np.float64) Esh_values[:, :tdim] = Esh_dg.x.array.reshape(V_x.shape[0], tdim).real V_grid.point_data["u"] = Esh_values plotter = pyvista.Plotter() plotter.add_text("magnitude", font_size=12, color="black") plotter.add_mesh(V_grid.copy(), show_edges=True) plotter.view_xy() plotter.link_views() 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: ```python 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(mesh_data.mesh.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: ```python 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: ```python # 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[0], Esh[1], 0)) E_3d = ufl.as_vector((E[0], E[1], 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 gcs = 2 * radius_wire n = ufl.FacetNormal(mesh_data.mesh) n_3d = ufl.as_vector((n[0], n[1], 0)) # Create a marker for the integration boundary for the scattering # efficiency marker = fem.Function(D) scatt_facets = mesh_data.facet_tags.find(scatt_tag) incident_cells = mesh.compute_incident_entities( mesh_data.mesh.topology, scatt_facets, tdim - 1, tdim ) mesh_data.mesh.topology.create_connectivity(tdim, tdim) midpoints = mesh.compute_midpoints(mesh_data.mesh, tdim, 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", mesh_data.mesh, subdomain_data=mesh_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 = mesh_data.mesh.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 = mesh_data.mesh.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 mesh_data.mesh.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}%") ``` ```python # Check if errors are smaller than 1% assert err_abs < 0.01 # assert err_sca < 0.01 assert err_ext < 0.01 ```