A photon makes current only if it is absorbed in the active layer. Light absorbed in the transparent electrode, the transport layers or the metal contact is heat. A thin-film cell is therefore designed not for maximum absorption but for maximum absorption in one layer, and that needs the absorptance of every layer separately, which the transfer matrix provides from the fields it already computes. Pettersson, Roman and Inganäs (1999) wrote this out for organic cells, Peumans and Forrest and then Burkhard, Hoke and McGehee turned it into the standard optical model of thin-film photovoltaics, and the same calculation serves perovskite, CIGS and thin silicon cells alike.
The absorbed power density
In an absorbing layer of complex index the time-averaged power dissipated per unit volume is
proportional to the local intensity, with the absorption coefficient hidden in . The field in a layer is the sum of the forward and backward amplitudes the transfer matrix returns, , so contains the two decaying exponentials and their interference term, and integrated over the layer is a closed form in , and (Pettersson's equations), which is what PyStratify evaluates. The profile is the calculator's field panel; its integral layer by layer is the per-layer absorptance.
Absorptance from the Poynting flux
Equivalently, energy conservation in each layer says that what flows in and does not flow out is absorbed. With and the normal components of the time-averaged Poynting vector at the layer's two faces and the incident flux,
The two routes must agree, and the sum rule is the check: PyStratify computes for every layer, and the check under the example confirms that the layers' absorptances, and add to one to , Poynting's theorem applied to the whole stack. A layer with gets exactly whatever the field inside it, which a numerical integration of would not reproduce; the flux difference does.
- mean perovskite absorptance, 400–750 nm:
- mean ITO absorptance, 400–750 nm:
Code
import numpy as np
from pystratify import planar
from pystratify.docs import material # n + ik of a tabulated page (refractiveindex.info format)
n = lambda wl: [1.0, material('docs/data/tutorials/ITO_Konig.yml', wl), material('docs/data/tutorials/TiO2_Sarkar.yml', wl), material('docs/data/tutorials/MAPbI3_Phillips.yml', wl), 1.55, material('docs/data/tutorials/Au_Johnson.yml', wl), 1.0] # incident medium, layers, substrate
d = [np.inf, 0.1, 0.05, 0.3, 0.15, 0.1, np.inf] # thicknesses, µm
lam = (380 + 5 * np.arange(95)) * 1e-3 # wavelength, µm
th = np.radians(0)
R, T = {}, {}
for pol in ('s', 'p'):
rows = [planar.coh_tmm(pol, n(wl), d, th, wl) for wl in lam]
R[pol], T[pol] = np.array([r['R'] for r in rows]), np.array([r['T'] for r in rows])
R_avg, T_avg = (R['s'] + R['p']) / 2, (T['s'] + T['p']) / 2 # unpolarized
- agrees R + T + the absorptance of every layer = 1 (largest departure): 2.22×10⁻¹⁶ against 0 ± 10⁻⁹ (Poynting's theorem)
The standing wave, and thickness
In a stack this thin the field inside is a standing wave: the back contact reflects nearly everything, so the intensity has a node at the metal and antinodes a quarter wave (in the material) away from it. An absorber placed at an antinode absorbs strongly, at a node weakly, and since the node spacing is , a change of absorber thickness of 50–100 nm moves the active layer from one to the other for a given wavelength. This is why the absorption of a thin organic or perovskite cell oscillates with thickness and why its external quantum efficiency has interference fringes rather than the smooth Beer–Lambert rise of a thick absorber. Thickening the perovskite absorbs more of the red, up to the point where the light is gone before it reaches the back contact; beyond that the extra thickness only adds collection losses, and the optimum is found by the photocurrent, not by the absorptance at one wavelength.
The photocurrent
Weighting by the solar photon flux gives the current a perfect collector would deliver:
with the AM1.5 global photon flux (ASTM G173; about photons m⁻² s⁻¹ below 1100 nm, corresponding to 44 mA cm⁻² if every one were absorbed in silicon). This is the figure of merit the optical models of organic and perovskite cells optimise (Burkhard, Hoke and McGehee 2010), layer thickness by layer thickness, and the one the calculator's sweeps are for. A measured external quantum efficiency divided by the computed is the internal quantum efficiency, the electrical part of the problem separated from the optical one, which is the main practical use of the layer-resolved calculation: it tells whether a cell loses photons or carriers.
Parasitic absorption
Every other layer's is a loss, and the model tells which. Indium tin oxide absorbs in the blue (its band edge) and in the near infrared (its free electrons; the trade-off with sheet resistance of the low-emissivity section), typically 5–10 % of the current in a thin-film cell; a 20 nm PEDOT:PSS or a doped transport layer a few percent; the metal back contact a few percent of the long-wavelength light, more if the contact is rough or the stack is designed so that an antinode sits at the metal. Silver loses less than aluminium, and a thin dielectric spacer between the absorber and the metal (which pushes the antinode out of the metal) is the standard fix for both organic and silicon cells. The totals are what the layer absorptances add up to, and an optical loss budget of a cell is a bar chart of them.
Beyond a planar stack
A planar calculation assumes a single pass per reflection. Thick silicon cells trap light with textured surfaces, whose ceiling is Yablonovitch's , and thin cells with gratings and scattering back reflectors; the per-layer absorption of a textured cell comes from a ray-tracing or grating solver fed with the planar coefficients of each facet, which is how the calculator's textured surfaces compute it. The planar stack remains the reference case: it is exact, it is fast, and it is what the textured result must reduce to when the texture is removed.
References
- L. A. A. Pettersson, L. S. Roman and O. Inganäs, J. Appl. Phys. 86, 487 (1999), doi:10.1063/1.370757
- G. F. Burkhard, E. T. Hoke and M. D. McGehee, Adv. Mater. 22, 3293 (2010), doi:10.1002/adma.201000883
- P. Peumans, A. Yakimov and S. R. Forrest, J. Appl. Phys. 93, 3693 (2003), doi:10.1063/1.1534621
- ASTM G173-03, Standard Tables for Reference Solar Spectral Irradiances (AM1.5 global), https://www.nrel.gov/grid/solar-resource/spectra-am1.5.html
- S. J. Byrnes, Multilayer optical calculations, arXiv:1603.02720 (2016), https://arxiv.org/abs/1603.02720