Custom Source


This tutorial demonstrates using a custom source to define a source with an arbitrary time profile.

Stochastic Dipole Emission in Light Emitting Diodes

In addition to the two source time profiles of a continuous wave (CW) and finite-bandwidth pulse, Meep supports a custom source for defining an arbitrary time profile. This feature can be used to model spatially incoherent random (i.e., white noise) dipole emission in a light-emitting diode (LED), spontaneously recombining excitonic emission in an organic light-emitting diode (OLED), as well as near-field heat transfer. Such incoherent emission processes are very different from coherent emission by a single collection of sources with a fixed phase relation, and more complicated modeling techniques are required.

This tutorial example involves computing the radiated flux from dipole emitters of a 2d LED-like periodic structure with a thin (1d) light-emitting layer. A schematic of the unit cell geometry and simulation layout is shown below. A silver (Ag) back reflector is used to direct nearly all the flux upwards into the direction. PML is used to terminate the air region at the top of the cell. (Note: PML is not necessary at the bottom of the cell due to the Ag layer which is effectively a lossless mirror with skin depth of a few nanometers at a wavelength of 1 μm.) The emitting layer is placed within a lossless dielectric substrate with wavelength-independent refractive index of 3.45.

One can take two different approaches to computing the radiated flux based on the type of emitter: (1) random or (2) deterministic. In Method 1 (brute-force Monte-Carlo), each emitter is a white-noise dipole: every timestep for every dipole is an independent random number. A single run involves all dipoles which are modeled using a CustomSource. The stochastic results for the radiated flux are averaged over multiple trials/iterations via Monte-Carlo sampling. Method 2 exploits the property of linear time-invariance of the materials/geometry and involves a sequence of separate runs each with a single deterministic dipole (i.e., pulse time profile, GaussianSource) at different positions in the emitting layer. Because dipoles at different positions are uncorrelated, the radiated flux from the ensemble is simply the average of all the individual iterations. The two approaches converge towards identical results, but Method 1 is more computationally expensive than Method 2 due to the much larger number of trials/iterations () required to attain low noise variance. (Even more sophisticated deterministic methods exist to reduce the number of separate simulations, especially at high resolutions; for example, replacing the point-dipole sources with a rapidly converging set of smooth basis functions, or fancier methods that exploit trace-estimation methods and/or transform volumetric sources to surface sources.)

Note regarding normalization: To directly compare the results for the radiated flux from the two methods, one might scale the spectrum from Method 2 in post processing to correct for the difference in spectrum between a Gaussian pulse and white noise. However, it is usually more convenient to nondimensionalize the results (for both methods) by dividing the flux spectrum for the textured surface with a reference spectrum computed by the same method, for example emission from a flat surface or in a homogeneous medium. This way, the details of the source spectra cancel automatically, and the nondimensionalized results can be compared as-is without any tricky scaling calculations. This kind of nondimensionalized comparison is useful to determine the emission enhancement (or suppression) of one structure relative to another as well as the light-extraction efficiency (the ratio of the radiated flux to the total flux emitted by the dipoles). In order to compute the absolute (not relative) light emission by a particular structure, using either Method 1 or Method 2, one would need to rescale the output (thanks to linearity) to convert the input spectrum (from white noise or Gaussian) to the actual emission spectrum (e.g. determined from the gain spectrum of a light-emitting diode).

The simulation script is in examples/stochastic_emitter.py. The notebook is examples/stochastic_emitter.ipynb.

import meep as mp
from meep.materials import Ag
import numpy as np

import argparse
parser = argparse.ArgumentParser()
parser.add_argument('-res', type=int, default=50, help='resolution (pixels/um)')
parser.add_argument('-nr', type=int, default=20, help='number of random trials (method 1)')
parser.add_argument('-nd', type=int, default=10, help='number of dipoles')
parser.add_argument('-nf', type=int, default=500, help='number of frequencies')
parser.add_argument('-textured', action='store_true', default=False, help='flat (default) or textured surface')
parser.add_argument('-method', type=int, choices=[1,2], default=1, help='type of method: (1) random dipoles with nr trials or (2) single dipole with 1 run per dipole')
args = parser.parse_args()

resolution = args.res

dpml = 1.0
dair = 1.0
hrod = 0.7
wrod = 0.5
dsub = 5.0
dAg = 0.5

sx = 1.1
sy = dpml+dair+hrod+dsub+dAg

cell_size = mp.Vector3(sx,sy)

pml_layers = [mp.PML(direction=mp.Y,
                     thickness=dpml,
                     side=mp.High)]

fcen = 1.0
df = 0.2
nfreq = args.nf
ndipole = args.nd
ntrial = args.nr
run_time = 2*nfreq/df

geometry = [mp.Block(material=mp.Medium(index=3.45),
                     center=mp.Vector3(0,0.5*sy-dpml-dair-hrod-0.5*dsub),
                     size=mp.Vector3(mp.inf,dsub,mp.inf)),
            mp.Block(material=Ag,
                     center=mp.Vector3(0,-0.5*sy+0.5*dAg),
                     size=mp.Vector3(mp.inf,dAg,mp.inf))]

if args.textured:
    geometry.append(mp.Block(material=mp.Medium(index=3.45),
                             center=mp.Vector3(0,0.5*sy-dpml-dair-0.5*hrod),
                             size=mp.Vector3(wrod,hrod,mp.inf)))

def compute_flux(m=1,n=0):
    if m == 1:
        sources = []
        for n in range(ndipole):
            sources.append(mp.Source(mp.CustomSource(src_func=lambda t: np.random.randn()),
                                     component=mp.Ez,
                                     center=mp.Vector3(sx*(-0.5+n/ndipole),-0.5*sy+dAg+0.5*dsub)))
    else:
        sources = [mp.Source(mp.GaussianSource(fcen,fwidth=df),
                             component=mp.Ez,
                             center=mp.Vector3(sx*(-0.5+n/ndipole),-0.5*sy+dAg+0.5*dsub))]

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

    flux_mon = sim.add_flux(fcen,
                            df,
                            nfreq,
                            mp.FluxRegion(center=mp.Vector3(0,0.5*sy-dpml),size=mp.Vector3(sx)))

    sim.run(until=run_time)

    flux = mp.get_fluxes(flux_mon)
    freqs = mp.get_flux_freqs(flux_mon)

    return freqs, flux


if args.method == 1:
    fluxes = np.zeros((nfreq,ntrial))
    for t in range(ntrial):
        freqs, fluxes[:,t] = compute_flux(m=1)
else:
    fluxes = np.zeros((nfreq,ndipole))
    for d in range(ndipole):
        freqs, fluxes[:,d] = compute_flux(m=2,n=d)


if mp.am_master():
    with open('method{}_{}_res{}_nfreq{}_ndipole{}.npz'.format(args.method,"textured" if args.textured else "flat",resolution,nfreq,ndipole),'wb') as f:
        np.savez(f,freqs=freqs,fluxes=fluxes)

There are five items to note in this script. (1) The frequency discretization of the flux spectrum must be sufficiently fine to resolve noisy features. In this example, the frequency range is 0.9 to 1.1 with spacing of 0.0004. (2) The runtime must be long enough for the DFT spectrum to resolve these oscillations. Due to the Fourier Uncertainty Principle, the runtime should be at least ~1/frequency resolution. Here, we found that a larger runtime of 2/frequency resolution was sufficient to converge to the desired accuracy. Technically, what we are doing is spectral density estimation of the periodogram by an ensemble average with a rectangular window, but many variations on this general idea exist. (3) The material properties for Ag are imported from the materials library. (4) At the end of the run, the flux spectra from all iterations are saved to a file using NumPy's uncompressed .npz format. This data is used to plot the results in post processing. (5) For Method 1, independent random numbers can be used for the white-noise dipole emitters in the trial runs for the two cases of a flat and textured surface, since all that matters is that they average to the same power spectrum.

Results for Methods 1 and 2 for the two cases of a flat and textured surface are generated using the following shell script:

#!/bin/bash

# Method 1: flat surface
python stochastic_emitter.py -method 1 -res 50 -nf 500 -nd 10 -nr 500

# Method 1: textured surface
python stochastic_emitter.py -method 1 -res 50 -nf 500 -nd 10 -nr 500 -textured

# Method 2: flat surface
python stochastic_emitter.py -method 2 -res 50 -nf 500 -nd 10

# Method 2: textured surface
python stochastic_emitter.py -method 2 -res 50 -nf 500 -nd 10 -textured

Afterwards, the four NumPy files produced by each run are used to plot the normalized flux for each method.

import numpy as np
import matplotlib.pyplot as plt

method1_f0 = np.load('method1_flat_res50_nfreq500_ndipole10.npz')
method1_f1 = np.load('method1_textured_res50_nfreq500_ndipole10.npz')

method1_freqs = method1_f0['freqs']
method1_f0_mean = np.mean(method1_f0['fluxes'],axis=1)
method1_f1_mean = np.mean(method1_f1['fluxes'],axis=1)

method2_f0 = np.load('method2_flat_res50_nfreq500_ndipole10.npz')
method2_f1 = np.load('method2_textured_res50_nfreq500_ndipole10.npz')

method2_freqs = method2_f0['freqs']
method2_f0_mean = np.mean(method2_f0['fluxes'],axis=1)
method2_f1_mean = np.mean(method2_f1['fluxes'],axis=1)

plt.semilogy(method1_freqs,method1_f1_mean/method1_f0_mean,'b-',label='Method 1')
plt.semilogy(method2_freqs,method2_f1_mean/method2_f0_mean,'r-',label='Method 2')
plt.xlabel('frequency')
plt.ylabel('normalized flux')
plt.legend()
plt.show()

Results for Method 1 for three different numbers of trials/iterations (10, 50, and 500) are shown in the following three figures. Each trial/iteration involves two runs: one each for the flat and textured surface. As the number of trials/iterations is increased, the "noisiness" in the plot is gradually reduced. However, the total runtime increases significantly.

The next figure shows a comparison of the normalized radiated flux for Method 1 (500 trials) and 2 (20 runs; 10 runs each for the flat and textured surface). The results show good agreement over the entire bandwidth spectrum. The Method 1 results required almost four days of compute time using an Intel Xeon processor with two single-threaded cores at 3.8 GHz whereas the Method 2 results were obtained in 24 minutes. In general, deterministic approaches tend to be more efficient than brute-force Monte-Carlo.

One situation in which you may need to perform brute-force Monte-Carlo simulations is that of nonlinear or time-varying media, because the equivalence between random and deterministic simulations above relied on linearity and time-invariance. However, in such media one also cannot directly employ white-noise sources, but you must instead input the noise with the correct spectrum for your desired emission process. For example, to model thermal emission in a nonlinear medium one must have a noise spectrum consistent with the fluctuation-dissipation theorem, which can be achieved using the NoisyLorentzianSusceptibility feature in Meep.

For cases involving a large number of spatially incoherent dipole emitters, a more computationally efficient approach than single-dipole simulations (Method 2) is separate simulations involving a line source with a different set of basis functions (Method 3). is typically independent of the resolution and . (For Method 2, the number of point dipoles comprising the same line source increases with resolution.) The mathematical details of Method 3 are described in Physical Review A, vol. 80, 012119, (2010). The source amplitude function of the th run in the ensemble is defined by a cosine Fourier series:

where if and otherwise, is the length of the line source.

As a demonstration of Method 3 and to compare with Method 2, a similar 2d LED-like periodic structure with a 1d light-emitting layer is used (the geometric parameters are slightly different). As before, results for the radiated flux of the textured surface are normalized using the flat surface so that the two methods can be directly compared without any additional post processing.

The simulation script is in examples/stochastic_emitter_line.py.

import meep as mp
from meep.materials import Ag
import numpy as np

import argparse
parser = argparse.ArgumentParser()
parser.add_argument('-res', type=int, default=50, help='resolution (pixels/um)')
parser.add_argument('-nf', type=int, default=500, help='number of frequencies')
parser.add_argument('-nsrc', type=int, default=15, help='number of line sources with cosine Fourier series amplitude function (method 3)')
parser.add_argument('-textured', action='store_true', default=False, help='flat (default) or textured surface')
parser.add_argument('-method', type=int, choices=[2,3], default=2,
                    help='type of method: (2) single dipole with 1 run per dipole or (3) line source with cosine Fourier series amplitude function')
args = parser.parse_args()

resolution = args.res

dpml = 1.0
dair = 0.9
hrod = 0.6
wrod = 0.8
dsub = 5.4
dAg = 0.4

sx = 1.5
sy = dpml+dair+hrod+dsub+dAg

cell_size = mp.Vector3(sx,sy)

pml_layers = [mp.PML(direction=mp.Y,
                     thickness=dpml,
                     side=mp.High)]

fcen = 1.0
df = 0.2
nfreq = args.nf
nsrc = args.nsrc
ndipole = int(sx*resolution)
run_time = 2*nfreq/df

geometry = [mp.Block(material=mp.Medium(index=3.45),
                     center=mp.Vector3(0,0.5*sy-dpml-dair-hrod-0.5*dsub),
                     size=mp.Vector3(mp.inf,dsub,mp.inf)),
            mp.Block(material=Ag,
                     center=mp.Vector3(0,-0.5*sy+0.5*dAg),
                     size=mp.Vector3(mp.inf,dAg,mp.inf))]

if args.textured:
    geometry.append(mp.Block(material=mp.Medium(index=3.45),
                             center=mp.Vector3(0,0.5*sy-dpml-dair-0.5*hrod),
                             size=mp.Vector3(wrod,hrod,mp.inf)))

def src_amp_func(n):
    def _src_amp_func(p):
        if n == 0:
            return 1/np.sqrt(sx)
        else:
            return np.sqrt(2/sx) * np.cos(n*np.pi*(p.x+0.5*sx)/sx)
    return _src_amp_func

def compute_flux(m,n):
    if m == 2:
        sources = [mp.Source(mp.GaussianSource(fcen,fwidth=df),
                             component=mp.Ez,
                             center=mp.Vector3(sx*(-0.5+n/ndipole),-0.5*sy+dAg+0.5*dsub))]
    else:
        sources = [mp.Source(mp.GaussianSource(fcen,fwidth=df),
                             component=mp.Ez,
                             center=mp.Vector3(0,-0.5*sy+dAg+0.5*dsub),
                             size=mp.Vector3(sx,0),
                             amp_func=src_amp_func(n))]

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

    flux_mon = sim.add_flux(fcen, df, nfreq,
                            mp.FluxRegion(center=mp.Vector3(0,0.5*sy-dpml),size=mp.Vector3(sx)))

    sim.run(until=run_time)

    flux = mp.get_fluxes(flux_mon)
    freqs = mp.get_flux_freqs(flux_mon)

    return freqs, flux


if args.method == 2:
    fluxes = np.zeros((nfreq,ndipole))
    for d in range(ndipole):
        freqs, fluxes[:,d] = compute_flux(2,d)
else:
    fluxes = np.zeros((nfreq,nsrc))
    for d in range(nsrc):
        freqs, fluxes[:,d] = compute_flux(3,d)


if mp.am_master():
    with open('method{}_{}_res{}_nfreq{}_{}{}.npz'.format(args.method,
                                                          "textured" if args.textured else "flat",
                                                          resolution,
                                                          nfreq,
                                                          "ndipole" if args.method == 2 else "nsrc",
                                                          ndipole if args.method == 2 else nsrc),'wb') as f:
        np.savez(f,freqs=freqs,fluxes=fluxes)

There are three items to note in this script. (1) The line source spans the entire length of the cell in the x direction (i.e., is sx). (2) The number of point dipoles in Method 2 is sx*resolution, one per pixel. (3) The source amplitude function in Method 3 is specified by the amp_func property of the Source object. In the case of a Fourier cosine series as conventionally written, is defined over the interval such that corresponds to the edge of the source, not the center. Since the source region in this example is defined in , the amplitude function must shift its coordinate argument by or 0.5*sx.

Method 3 requires a convergence check in which (nsrc) is repeatedly doubled until the change in the results are within a desired tolerance of e.g., < 1%. For this example, was found to be sufficient.

Results for Methods 2 and 3 for the two cases of a flat and textured surface are generated using the following shell script:

#!/bin/bash

# Method 2: flat surface
python stochastic_emitter_line.py -method 2 -res 50 -nf 500

# Method 2: textured surface
python stochastic_emitter_line.py -method 2 -res 50 -nf 500 -textured

# Method 3: flat surface
python stochastic_emitter_line.py -method 3 -res 50 -nf 500 -nsrc 15

# Method 3: textured surface
python stochastic_emitter_line.py -method 3 -res 50 -nf 500 -nsrc 15 -textured

Afterwards, the four NumPy files produced by each run are used to plot the normalized flux for each method.

import numpy as np
import matplotlib.pyplot as plt

method2_f0 = np.load('method2_flat_res50_nfreq500_ndipole75.npz')
method2_f1 = np.load('method2_textured_res50_nfreq500_ndipole75.npz')

method2_freqs = method2_f0['freqs']
method2_f0_mean = np.mean(method2_f0['fluxes'],axis=1)
method2_f1_mean = np.mean(method2_f1['fluxes'],axis=1)

method3_f0 = np.load('method3_flat_res50_nfreq500_nsrc15.npz')
method3_f1 = np.load('method3_textured_res50_nfreq500_nsrc15.npz')

method3_freqs = method3_f0['freqs']
method3_f0_mean = np.mean(method3_f0['fluxes'],axis=1)
method3_f1_mean = np.mean(method3_f1['fluxes'],axis=1)

plt.semilogy(method2_freqs,method2_f1_mean/method2_f0_mean,'b-',label='Method 2')
plt.semilogy(method3_freqs,method3_f1_mean/method3_f0_mean,'r-',label='Method 3')
plt.xlabel('frequency')
plt.ylabel('normalized flux')
plt.legend()
plt.show()

Results for Method 2 and 3 are shown in the following figure. The agreement is good but there is a significant difference in the runtime. Method 2 involves simulations each for the flat and textured surface for a total of 150 runs which required 10.6 hours. Method 3 involves simulations for the flat/textured surface for a total of 30 runs which required just 2.0 hours.