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Callister - An introduction - 8th edition

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858 • Chapter 21 / Optical Properties<br />

photoconductivity<br />

21.12 PHOTOCONDUCTIVITY<br />

The conductivity of semiconducting materials depends on the number of free electrons<br />

in the conduction band and also the number of holes in the valence band, according<br />

to Equation 18.13. Thermal energy associated with lattice vibrations can<br />

promote electron excitations in which free electrons and/or holes are created, as<br />

described in Section 18.6. Additional charge carriers may be generated as a consequence<br />

of photon-induced electron transitions in which light is absorbed; the attendant<br />

increase in conductivity is called photoconductivity. Thus, when a specimen<br />

of a photoconductive material is illuminated, the conductivity increases.<br />

This phenomenon is used in photographic light meters. A photoinduced current<br />

is measured, and its magnitude is a direct function of the intensity of the incident<br />

light radiation, or the rate at which the photons of light strike the photoconductive<br />

material. Of course, visible light radiation must induce electronic transitions in the<br />

photoconductive material; cadmium sulfide is commonly used in light meters.<br />

Sunlight may be directly converted into electrical energy in solar cells, which<br />

also employ semiconductors. The operation of these devices is, in a sense, the reverse<br />

of that for the light-emitting diode. A p–n junction is used in which photoexcited<br />

electrons and holes are drawn away from the junction, in opposite directions,<br />

and become part of an external current, as illustrated in the (a) chapter-opening<br />

diagram for this chapter.<br />

Concept Check 21.7<br />

Is the semiconductor zinc selenide (ZnSe), which has a band gap of 2.58 eV, photoconductive<br />

when exposed to visible light radiation? Why or why not?<br />

[The answer may be found at www.wiley.com/college/callister (Student Companion Site).]<br />

21.13 LASERS<br />

laser<br />

All the radiative electron transitions heretofore discussed are spontaneous; that is,<br />

an electron falls from a high energy state to a lower one without any external provocation.<br />

These transition events occur independently of one another and at random<br />

times, producing radiation that is incoherent; that is, the light waves are out of phase<br />

with one another. With lasers, however, coherent light is generated by electron transitions<br />

initiated by an external stimulus; in fact, laser is just the acronym for light<br />

amplification by stimulated emission of radiation.<br />

Although there are several different varieties of laser, the principles of operation<br />

are explained using the solid-state ruby laser. Ruby is simply a single crystal<br />

of Al 2 O 3 (sapphire) to which has been added on the order of 0.05% Cr 3 ions. As<br />

previously explained (Section 21.9), these ions impart to ruby its characteristic red<br />

color; more important, they provide electron states that are essential for the laser<br />

to function. The ruby laser is in the form of a rod, the ends of which are flat, parallel,<br />

and highly polished. Both ends are silvered such that one is totally reflecting<br />

and the other partially transmitting.<br />

The ruby is illuminated with light from a xenon flash lamp (Figure 21.13).<br />

Before this exposure, virtually all the Cr 3 ions are in their ground states; that is,<br />

electrons fill the lowest energy levels, as represented schematically in Figure 21.14.<br />

However, photons of wavelength 0.56 m from the xenon lamp excite electrons<br />

from the Cr 3 ions into higher energy states. These electrons can decay back into

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