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
86%
Similarly we separate holes with a hole membrane:
a layer that is highly conductive for holes but not for electrons.
This is often refered to as Back Surface Field (or BSF) in a conventional solar cell.
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