# Absorbed Power Density Map of a Lossy Cylinder¶

The dft_flux routines (add_flux) described in the previous examples compute the total power in a given region (FluxRegion). It is also possible to compute the local (i.e., position-dependent) absorbed power density in a dispersive (lossy) material. This quantity is useful for obtaining a spatial map of the photon absorption. The absorbed power density is defined as $$\mathrm{Re}\, \left[ {\mathbf{E}^* \cdot \frac{d\mathbf{P}}{dt}} \right]$$ where $\mathbf{P}$ is the total polarization field. In the Fourier (frequency) domain with time-harmonic fields, this expression is $$\mathrm{Re}\, \left[ {\mathbf{E}^* \cdot (-i \omega \mathbf{P})} \right] = \omega\, \mathrm{Im}\, \left[ {\mathbf{E}^* \cdot \mathbf{P}} \right]$$ where $\mathbf{E}^* \cdot \mathbf{P}$ denotes the dot product of the complex conjugate of $\mathbf{E}$ with $\mathbf{P}$. However, since $\mathbf{D}=\mathbf{E}+\mathbf{P}$, this is equivalent to $$\omega\, \mathrm{Im}\, \left[ {\mathbf{E}^* \cdot (\mathbf{D}-\mathbf{E})} \right] = \omega\, \mathrm{Im}\, \left[ {\mathbf{E}^* \cdot \mathbf{D}} \right]$$ since $\mathbf{E}^* \cdot \mathbf{E} = |\mathbf{E}|^2$ is purely real. Calculating this quantity involves two steps: (1) compute the Fourier-transformed $\mathbf{E}$ and $\mathbf{D}$ fields in a region via the dft_fields feature and (2) in post processing, compute $\omega\, \mathrm{Im}\, \left[ {\mathbf{E}^* \cdot \mathbf{D}} \right]$.

This tutorial example involves computing the absorbed power density for a two-dimensional cylinder (radius: 1 μm) of silicon dioxide (SiO2, from the materials library) at a wavelength of 1 μm given an incident $E_z$-polarized planewave. (The attenuation length of SiO2 at this wavelength is $\lambda/\mathrm{Im}\, \sqrt{\varepsilon}$ = ~3000 μm.) We will also verify that the total power absorbed by the cylinder obtained by integrating the absorbed power density over the entire cylinder is equivalent to the same quantity computed using the alternative method involving a closed, four-sided dft_flux box (Poynting's theorem).

In [1]:
import numpy as np
import matplotlib.pyplot as plt

import meep as mp
from meep.materials import SiO2

resolution = 100  # pixels/um

dpml = 1.0
pml_layers = [mp.PML(thickness=dpml)]

r = 1.0     # radius of cylinder
dair = 2.0  # air padding thickness

s = 2*(dpml+dair+r)
cell_size = mp.Vector3(s,s)

wvl = 1.0
fcen = 1/wvl

# is_integrated=True necessary for any planewave source extending into PML
sources = [mp.Source(mp.GaussianSource(fcen,fwidth=0.1*fcen,is_integrated=True),
center=mp.Vector3(-0.5*s+dpml),
size=mp.Vector3(0,s),
component=mp.Ez)]

symmetries = [mp.Mirror(mp.Y)]

geometry = [mp.Cylinder(material=SiO2,
center=mp.Vector3(),
height=mp.inf)]

sim = mp.Simulation(resolution=resolution,
cell_size=cell_size,
boundary_layers=pml_layers,
sources=sources,
k_point=mp.Vector3(),
symmetries=symmetries,
geometry=geometry)

fcen,0,1,
center=mp.Vector3(),
size=mp.Vector3(2*r,2*r),
yee_grid=True)

# closed box surrounding cylinder for computing total incoming flux
mp.FluxRegion(center=mp.Vector3(x=-r),size=mp.Vector3(0,2*r),weight=+1),
mp.FluxRegion(center=mp.Vector3(x=+r),size=mp.Vector3(0,2*r),weight=-1),
mp.FluxRegion(center=mp.Vector3(y=+r),size=mp.Vector3(2*r,0),weight=-1),
mp.FluxRegion(center=mp.Vector3(y=-r),size=mp.Vector3(2*r,0),weight=+1))

sim.run(until_after_sources=100)

Dz = sim.get_dft_array(dft_fields,mp.Dz,0)
Ez = sim.get_dft_array(dft_fields,mp.Ez,0)
absorbed_power_density = 2*np.pi*fcen * np.imag(np.conj(Ez)*Dz)

dxy = 1/resolution**2
absorbed_power = np.sum(absorbed_power_density)*dxy
absorbed_flux = mp.get_fluxes(flux_box)[0]
err = abs(absorbed_power-absorbed_flux)/absorbed_flux
print("flux:, {} (dft_fields), {} (dft_flux), {} (error)".format(absorbed_power,absorbed_flux,err))

-----------
Initializing structure...
Halving computational cell along direction y
time for choose_chunkdivision = 0.00278592 s
Working in 2D dimensions.
Computational cell is 8 x 8 x 0 with resolution 100
cylinder, center = (0,0,0)
radius 1, height 1e+20, axis (0, 0, 1)
dielectric constant epsilon diagonal = (1,1,1)
time for set_epsilon = 0.94641 s
lorentzian susceptibility: frequency=9.67865, gamma=0.0806554
-----------

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run 0 finished at t = 200.0 (40000 timesteps)
flux:, 0.13120421825956843 (dft_fields), 0.13249534167200247 (dft_flux), 0.0097446702362583 (error)


There is one important item to note: in order to eliminate discretization artifacts when computing the $\mathbf{E}^* \cdot \mathbf{D}$ dot-product, the add_dft_fields definition includes yee_grid=True which ensures that the $E_z$ and $D_z$ fields are computed on the Yee grid rather than interpolated to the centered grid. As a corollary, we cannot use get_array_metadata to obtain the coordinates of the dft_fields region or its interpolation weights because this involves the centered grid.

The two values for the total absorbed power which are displayed at the end of the run are nearly equivalent. The relative error between the two methods is ~1.0%.

A schematic of the simulation layout generated using plot2D shows the line source (red), PMLs (green hatch region), dft_flux box (solid blue contour line), and dft_fields surface (blue hatch region).

In [2]:
plt.figure()
sim.plot2D()

Out[2]:
<matplotlib.axes._subplots.AxesSubplot at 0x7f450c399110>

The spatial map of the absorbed power density shows that most of the absorption occurs in a small region near the back surface of the cylinder (i.e., on the opposite side of the incident planewave).

In [3]:
plt.figure()
x = np.linspace(-r,r,Dz.shape[0])
y = np.linspace(-r,r,Dz.shape[1])
plt.pcolormesh(x,
y,
np.transpose(absorbed_power_density),
cmap='inferno_r',

<matplotlib.colorbar.Colorbar at 0x7f44ecab7f90>