The effect of perovskite
material properties on the power conversion
to electricity and, especially, to heat and the operation temperature
of perovskite solar cells (PSCs) was simulated. The operation temperature
is topical because the technology is progressing toward commercialization:
first, because cells are subject to varying outdoor conditions, and
second, because commercial use benefits from accurate power production
prediction, in which the cell temperature is an influential factor.
This article products insights into how perovskite absorber properties,
including the band gap (E
g), diffusion
length, and layer thickness, affect the heat production and temperature
coefficient of planar PSCs based on optoelectronic simulations. The
change in heat production with an increasing band gap was observed
to be quasi-linear: self-heating decreased by approximately −0.38
W/(m2 meV) until E
g = 1.7 eV,
after which the slope slightly relaxed. Over the studied band gap
range of 1.2–2.2 eV, the change in heat production as a function
of the band gap resulted in the self-heating of a small band gap (E
g = 1.2 eV) device, 575 W/m2, to
be more than twice that of a large band gap (E
g = 2.2 eV) device, 253 W/m2. Further, the steady-state
operating temperature at the maximum power point was modeled and shown
to significantly vary between 30 °C for a large (2.2 eV) band
gap device and 44 °C for a small (1.2 eV) band gap device in
the example outdoor conditions of 1000 W/m2 irradiance,
20 °C ambient temperature, and ca. 1 m/s wind speed. The self-heating-induced
temperature increment subsequently affected the power production predictions
of different band gap devices, from −6 to −1%. The results
presented here can improve the operation temperature and power production
predictions of PSCs with alternative perovskite absorbers.