Where n ( E ) is the spatial density of conduction band electrons that would be present in thermal equilibrium if the Fermi level were at E, and p ( E ) is the spatial density of holes that would be present in thermal equilibrium if the Fermi level were at E.
12.
Where n ( E ) is the spatial density of conduction band electrons that would be present in thermal equilibrium if the Fermi level were at E, and p ( E ) is the spatial density of holes that would be present in thermal equilibrium if the Fermi level were at E.
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