Created
March 27, 2023 00:23
-
-
Save oskooi/b95220b00e63ddc42f97532ae3a7710c to your computer and use it in GitHub Desktop.
radiated flux of a point dipole in 3d Cartesian coordinates
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
import argparse | |
import meep as mp | |
import numpy as np | |
parser = argparse.ArgumentParser() | |
parser.add_argument( | |
'-res', | |
type=float, | |
help='resolution (pixels/μm)', | |
default=100.0, | |
) | |
args = parser.parse_args() | |
resolution = args.res # pixels/um | |
s = 5.0 | |
dpml = 1.0 | |
cell_size = mp.Vector3(s+2*dpml,s+2*dpml,s+2*dpml) | |
pml_layers = [mp.PML(dpml)] | |
n = 1.0 # refractive index of surrounding medium | |
wvl = 1.0 # source wavelength | |
fcen = 1/wvl | |
src_cmpt = mp.Ex | |
sources = [mp.Source(src=mp.GaussianSource(fcen,fwidth=0.1*fcen), | |
center=mp.Vector3(), | |
component=src_cmpt)] | |
if src_cmpt == mp.Ex: | |
symmetries = [mp.Mirror(mp.X,phase=-1), | |
mp.Mirror(mp.Y), | |
mp.Mirror(mp.Z)] | |
elif src_cmpt == mp.Ez: | |
symmetries = [mp.Mirror(mp.X), | |
mp.Mirror(mp.Y), | |
mp.Mirror(mp.Z,phase=-1)] | |
else: | |
symmetries = [] | |
sim = mp.Simulation(cell_size=cell_size, | |
resolution=resolution, | |
sources=sources, | |
symmetries=symmetries, | |
boundary_layers=pml_layers, | |
default_material=mp.Medium(index=n)) | |
flux_box = sim.add_flux(fcen, | |
0, | |
1, | |
mp.FluxRegion(center=mp.Vector3(0.5*s,0,0), | |
size=mp.Vector3(0,s,s)), | |
mp.FluxRegion(center=mp.Vector3(-0.5*s,0,0), | |
size=mp.Vector3(0,s,s), | |
weight=-1.0), | |
mp.FluxRegion(center=mp.Vector3(0,0.5*s,0), | |
size=mp.Vector3(s,0,s)), | |
mp.FluxRegion(center=mp.Vector3(0,-0.5*s,0), | |
size=mp.Vector3(s,0,s), | |
weight=-1.0), | |
mp.FluxRegion(center=mp.Vector3(0,0,0.5*s), | |
size=mp.Vector3(s,s,0)), | |
mp.FluxRegion(center=mp.Vector3(0,0,-0.5*s), | |
size=mp.Vector3(s,s,0), | |
weight=-1.0)) | |
sim.run( | |
mp.dft_ldos(fcen,0,1), | |
until_after_sources=mp.stop_when_fields_decayed( | |
50, | |
src_cmpt, | |
mp.Vector3(), | |
1e-8, | |
), | |
) | |
flux = mp.get_fluxes(flux_box)[0] | |
dV = 1/(resolution**3) | |
ldos = -np.real(sim.ldos_Fdata[0]*np.conj(sim.ldos_Jdata[0]))*dV | |
ratio = flux/ldos | |
print(f"flux:, {int(resolution):d}, {ldos:.6f}, {flux:.6f}, {ratio:.6f}") |
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment