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Chapter V July 15, 2015 Junctions of Photovoltaics
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Electron Affinity and Vacuum Level
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Quasi Thermal Equilibrium under applied electric bias or exposure of light Quasi Fermi level distribution
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Quasi Thermal Equilibrium under applied electric bias or exposure of light Quasi Fermi level In general, T n =T B =T
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Quasi Thermal Equilibrium under applied electric bias or exposure of light
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Current Density under Bias – Boltzmann Transport Equation and the Relaxation Time Approximation J(r) = J n (r) + J p (r)
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Transport Equation in Crystal
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Charge Separation of a Photovoltaic Device
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Origin of Photovoltaic Action
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Difference in work function Difference in electron affinity due to compositional gradient creating an effective field A gradient in the effective conduction band density of states
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Contact of n-type semiconductor and metal with Φ m >Φ n Electron flow Hole flow
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Electron flow Hole flow
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Reverse biasForward bias
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Contact of p-type semiconductor and metal with Φ m <Φ p
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Ohmic Contacts: a low resistance contact for the majority carriers Φ m >Φ p Φ m <Φ n Upon illumination, no photovoltage across the junction can be established.
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Limitations of the Schottky Barrier Junction
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The junction region is depleted of both electrons and holes and always presents a barrier to majority carriers, and a low resistance path to minority carriers. It drives the collection of minority carriers which are photogenerated throughout the p and n layers, and reach the junction by diffusion.
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Can lead to enhanced recombination in the junction region
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Surface and Interface States
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V bi
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Effect of Interface States on a p-n Junction More of the potential difference is dropped on the n side, large amount of mobile holes will accumulate beside the interface
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Interface States at a metal- semiconductor junction This is small for n-type- metal contact, but is large for p-type-metal contact.
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