Photoluminescence Spectroscopy for Understanding Light Management in Solar Cells
Abstract
The purpose of applying a light management structure in a solar
cell is to absorb the largest possible amount of incident
radiation in the active layer. Independent of the material,
thickness and structure of the solar cell, the fundamental
approaches for light management are: A) reducing the proportion
of the light being reflected out at the front surface and B)
increasing the path length of the light within the absorbing
substrate. Therefore, characterizing and optimizing the light
management technique is essential for further improving solar
cell efficiency.
In this thesis, a method based on the generalized
Planck’s law of radiation is developed to extract the
band-to-band absorptance from the photoluminescence spectra of
semiconductor materials. Unlike the traditional way of obtaining
absorptance from the reflection and transmission measurement,
this method is only sensitive to absorbed photons that can
generate electron-hole pairs. Therefore, the parasitic losses
such as free carrier absorption and the absorption in non-active
layers can be automatically eliminated. With the extracted
band-to-band absorptance, the implied photo-current of the sample
is accurately estimated without the need of forming a p-n
junction. By comparing the band-to-band absorptance of silicon
wafers with and without light trapping structure, the optical
enhancement is rapidly accessed. Using this method, a wide range
of light trapping structures are studied on crystalline silicon
wafers to improve the photo-current generation.
Self-assembled plasmonic Ag particles (AgNP) together
with a dielectric based diffuse reflector (DR) are applied on the
rear side of silicon wafers to provide excellent optical
enhancement without sacrificing the electrical performance of the
device. AgNP have proven to scatter the light at wide angles, so
that total internal reflection occurs and the light can be
trapped in the solar cell. Dielectric based diffuse reflectors
have the advantage of high reflectivity and low absorption loss
compared to metal reflectors. The combination of DR and AgNP
provides light trapping performance (62% of Lambertian
enhancement) which is comparable with inverted pyramids (67% of
Lambertian enhancement) on a 200 mm thick silicon wafer. By
applying AgNP in the back of a silicon wafer with an
interdigitated back contact (IBC) structure, a maximum of 53% of
fraction of the Lambertian enhancement is achieved with an
optimized capping layer. For a standard IBC cell with AgNP
embedded in the rear side, the short circuit current density is
estimated to enhance by 18% in the spectral range from 1000 nm to
1200 nm.
Texturing is still the most widely applied light
management technique in the c-Si solar cell industry. The
textured surface produces broad-band anti-reflection properties
as well as effective light trapping to the solar cell. We extend
the application of the PL technique to evaluate the optical
performance of textured samples. Several structures including
reactive ion etched textures (RIE), metal-assisted textures (MET)
and random pyramid textures (RAN) are experimentally evaluated
with the photoluminescence technique. By fabricating a silicon
wafer with RIE and RAN textures on the front and rear side
respectively, we demonstrate a structure with near ideal
absorption in the ultraviolet and visible spectrum and a light
trapping efficiency of 55% in the near infrared region of the
solar spectrum. Using an analytical model with independent
angular distribution parameters on both surfaces, we carry out a
quantitative analysis on the impact of front reflection, rear
absorption and the angular distribution on the implied current
generation of these silicon samples. With the origins of the
optical loss of these light management structures revealed, the
effective approach for reaching maximum photo-current for high
efficiency silicon solar cells is discussed. We conclude that the
non-perfect angular distribution is the main limitation for
approaching Lambertian light trapping in high efficiency silicon
solar cells.
Dielectric based diffuse reflectors have excellent optical
properties and can be applied on a wide range of solar cells. A
diffuse reflector prepared by Snow Globe coating is applied on
a-Si:H/mc-Si:H tandem solar cell. The reflector has close to 100%
reflectance over a spectral range of 500-1300 nm which indicates
much lower parasitic optical losses compared to the standard
textured ZnO:Al/Ag reflector. The application of DR avoids the
localized surface plasmon and propagating surface plasmon
resonances existing on randomly textured ZnO:Al/Ag back contacts.
Both of the resonances can couple with the incident light and
introduce significant amount of parasitic absorption and thereby
reducing the overall cell performance. By replacing ZnO:Al/Ag
with SGC reflector on tandem thin film silicon solar cells as a
rear reflector, the short circuit current of the bottom solar
cell is enhanced and the overall cell efficiency is improved from
10.2% to 10.4%.
Organic/inorganic hybrid perovskite material has the
potential for being a lowcost and high efficiency photovoltaic
technology. The knowledge of absorption coefficient of such novel
absorber materials is essential in understanding the extent to
which perovskite solar cells may suffer from parasitic
absorption. The fundamental relationship between band-to-band
absorptance and photoluminescence is used to measure the
absorption coefficient absorption coefficient of
organic-inorganic hybrid perovskite methylammonium lead iodide
(CH3NH3PbI3) films from 675 nm to 1400 nm. Unlike other methods
used to extract the absorption coefficient, photoluminescence is
only affected by band-to-band absorption and is capable of
detecting absorption events at very low energy levels. Absorption
coefficients as low as 10e-14 cm-1 are detected at room
temperature for long wavelengths, which is 14 orders of magnitude
lower than reported values at shorter wavelengths. The
temperature dependence of absorption coefficient is calculated
from the photoluminescence spectra of CH3NH3PbI3 in the
temperature range 80-360K with 10K intervals. Based on the
temperature dependent absorption coefficient, a polynomial
parameterization describing the product of the radiative
recombination coefficient and square of the intrinsic carrier
density is also presented.
This thesis focuses on understanding and improving the light
management of solar cells. The method of extracting band-to-band
absorptance from photoluminescence spectra is used to compare a
wide range of light trapping structures on silicon wafers and to
extract the absorption coefficient of perovskite film at very low
energy levels.
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