Introduction
Basics
Fundamental Losses
Below Bandgap Losses
Thermalisation Losses
Emission Losses
Boltzmann Losses
Carnot Losses
Practical Losses
Recombination Losses
Resistive Losses
Optical Losses
Ressources
About
20%
Some have high energies (like ultra-violet, violet, blue and other visible photons).
These are always absorbed by the absorber.
This is because they have enough energy to create an electron-hole pair.
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