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.
