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Q.What is the function of a solar cell ? Briefly explain its working and draw its I-V characteristic curve.

CBSECBSE Class XII Board 2020Subjective· 3mImportance★★★★★est
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A solar cell converts light energy directly into electrical energy through the photovoltaic effect. When photons strike a p-n junction, they generate electron-hole pairs that are separated by the built-in electric field, producing a voltage and current. The I-V curve shows that current decreases from IscI_{sc} to zero as voltage increases from zero to VocV_{oc}.

I-V characteristic of a solar cell: current stays nearly constant at the short-circuit value I_sc as voltage increases from zero, then bends at the maximum power point (V_m, I_m) and falls steeply to the open-circuit voltage V_oc where current is zero.
I-V characteristic of a solar cell: current stays nearly constant at the short-circuit value I_sc as voltage increases from zero, then bends at the maximum power point (V_m, I_m) and falls steeply to the open-circuit voltage V_oc where current is zero.

Function of a Solar Cell

A solar cell is a semiconductor device that converts light energy (photons) directly into electrical energy through the photovoltaic effect. It acts as an energy transducer, transforming electromagnetic radiation into usable electric power without any moving parts or chemical reactions.

The fundamental principle relies on the behavior of a p-n junction when exposed to light. Unlike a regular diode that operates in darkness, a solar cell is designed to absorb photons and use their energy to create charge carriers that can drive an external current.

Working Principle

The operation hinges on three key processes:

1. Photon Absorption and Carrier Generation

When light strikes the solar cell, photons with energy E=hνE = h\nu greater than the band gap EgE_g of the semiconductor are absorbed. Each absorbed photon excites an electron from the valence band to the conduction band, creating an electron-hole pair. Silicon solar cells typically use Eg≈1.1 eVE_g \approx 1.1 \text{ eV}, which matches well with the solar spectrum.

2. Charge Separation by the Built-in Field

The p-n junction creates a depletion region with a built-in electric field pointing from the n-side to the p-side. This field is crucial: when electron-hole pairs are generated in or near the depletion region, the field sweeps electrons toward the n-side and holes toward the p-side before they can recombine. This spatial separation of charges creates a potential difference across the junction.

3. Current Collection

The separated charges accumulate on opposite sides of the junction, with the n-side becoming negative and the p-side positive. When an external circuit is connected, electrons flow from the n-side through the load to the p-side, delivering electrical power. The illuminated junction thus acts as a current source, with the light-generated current ILI_L flowing opposite to the normal diode current.

Note

The solar cell is essentially a diode that operates in the fourth quadrant of the I-V plane (negative current, positive voltage), delivering power rather than consuming it.

Current-Voltage Characteristic

The I-V relationship of an illuminated solar cell is given by:

I=IL−I0(eqVkT−1)I = I_L - I_0 \left( e^{\frac{qV}{kT}} - 1 \right)

where ILI_L is the light-generated current, I0I_0 is the reverse saturation current, qq is electron charge, kk is Boltzmann's constant, and TT is temperature.

Key points on the characteristic:

  • Short-circuit current (IscI_{sc}): When V=0V = 0 (terminals shorted), I=Isc≈ILI = I_{sc} \approx I_L. This is the maximum current the cell can deliver.

  • Open-circuit voltage (VocV_{oc}): When I=0I = 0 (open terminals), solving gives Voc=kTqln⁡(ILI0+1)V_{oc} = \frac{kT}{q} \ln\left(\frac{I_L}{I_0} + 1\right). This is the maximum voltage across the cell. …

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