courses:ast201:8
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courses:ast201:8 [2023/12/09 02:00] – asad | courses:ast201:8 [2023/12/09 22:39] (current) – [4.2 Photoabsorbers or photoconductors] asad | ||
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- | ==== - Intrinsic photoabsorbers | + | ==== - Photoabsorbers |
So far we have talked about the emancipation of electrons via lattice vibration and collision, but an a photon with a wavelength larger than the **curoff wavelength** can also emancipate an electron. The cutoff wavelength | So far we have talked about the emancipation of electrons via lattice vibration and collision, but an a photon with a wavelength larger than the **curoff wavelength** can also emancipate an electron. The cutoff wavelength | ||
$$ \lambda_c = \frac{hc}{E_G} = \frac{1.24 \ \mu\text{m}}{E_G \text{ eV}}. $$ | $$ \lambda_c = \frac{hc}{E_G} = \frac{1.24 \ \mu\text{m}}{E_G \text{ eV}}. $$ | ||
- | For Si, the value of 1.1 $\mu$m. | + | For Si, the value of 1.1 $\mu$m. In astronomy we use semiconductors as photoabsorbers. A simple example is shown below. |
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+ | The photon stream promotes electrons to the conduction band leaving behind an equal number of holes in the valence band. This is a basic **detector** or **sensor** or **receiver** that converts energy into matter, photons into electrons. The greater the stream the higher the conductivity of the detector. If the voltage across the semiconductor is constant, the electrical current $i$ through the resistor $R_L$ would depend on the number of photons absorbed per second. | ||
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+ | So the voltage measured at $V_o$ will be directly related to the **intensity** of light. | ||
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==== - Extrinsic semiconductors ==== | ==== - Extrinsic semiconductors ==== |
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