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
70%
Electrons and holes will recombine by emitting photons.
This is unavoidable and will lead to a reduction in the current.
This our third fundamental loss and is called emission loss.
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