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Surface and bulk passivation of multicrystalline silicon solar cells by ...

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6<br />

bond is called a hole. It too can be easily removed from the vicinity <strong>of</strong> the B atom <strong>and</strong><br />

move freely in the semiconductor material. A semiconductor doped with acceptors is<br />

known as p-type material. As the two types <strong>of</strong> semiconductors are brought together, a<br />

p-n junction is formed <strong>and</strong> the concentration gradient <strong>of</strong> carriers near the metallurgical<br />

junction leads to a carrier flow. As the junction region gets "depleted" <strong>of</strong> carriers, the<br />

ionized dopant cores left behind build up an electric field across the junction, which<br />

introduces drift current that is opposite to the diffusion current. An equilibrium<br />

situation will be arrived at as the two currents match. In the dark, the equilibrated p-n<br />

junction should have a spatially uniform Fermi level <strong>and</strong> no net macroscopic current<br />

flow is observed.<br />

When a p-n junction is illuminated, excess electron-hole pairs are generated <strong>by</strong><br />

light throughout the cell. This disturbs the equilibrium state <strong>of</strong> carriers everywhere.<br />

The excess electrons (holes) in n-type (p-type) region diffuse towards the junction <strong>and</strong><br />

are quickly pulled across the depletion region <strong>by</strong> the electric field. This is the<br />

photovoltaic effect.<br />

A simplified <strong>solar</strong> cell model is usually illustrated as a current source in<br />

parallel with a diode <strong>and</strong>, a shunt resistance <strong>and</strong> a series resistance component as well<br />

are added. The resulting equivalent circuit <strong>of</strong> a <strong>solar</strong> cell is shown in Figure 1.3.<br />

Notice that the current generated <strong>by</strong> the photons is represented <strong>by</strong> an independent<br />

source. The two resistors shown in Figure 1.3 represent two <strong>of</strong> the losses in a <strong>solar</strong><br />

cell. Rs is a series resistance loss due, primarily, to the ohmic loss in the surface <strong>of</strong><br />

the <strong>solar</strong> cell. The shunt resistance, Rsh, is used to model leakage currents. A shunt<br />

resistance <strong>of</strong> a few hundred ohms does not reduce the output power <strong>of</strong> the <strong>solar</strong> cell<br />

appreciably. In reality, Rsh is much larger than a few hundred ohms <strong>and</strong> can in most

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