GTBL042-19 GTBL042-Callister-v2 September 17, 2007 17:39
Revised Pages
Learning Objectives
After careful study of this chapter you should be able to do the following:
1.Compute the energy of a photon given its
frequency and the value of Planck’s constant.
2.Briefly describe electronic polarization that
results from electromagnetic radiation-atomic
interactions. Cite two consequences of electronic
polarization.
3.Briefly explain why metallic materials are opaque
to visible light.
4.Defineindex of refraction.
5.Describe the mechanism of photon absorption for
(a) high-purity insulators and semiconductors,
and (b) insulators and semiconductors that
contain electrically active defects.
6.For inherently transparent dielectric materials,
note three sources of internal scattering that can
lead to translucency and opacity.
7.Briefly describe the construction and operation
of ruby and semiconductor lasers.
19.1 INTRODUCTION
By “optical property” is meant a material’s response to exposure to electromagnetic
radiation and, in particular, to visible light. This chapter first discusses some of the ba-
sic principles and concepts relating to the nature of electromagnetic radiation and its
possible interactions with solid materials. Next to be explored are the optical behav-
iors of metallic and nonmetallic materials in terms of their absorption, reflection, and
transmission characteristics. The final sections outline luminescence, photoconduc-
tivity, and light amplification by stimulated emission of radiation (laser), the practical
utilization of these phenomena, and optical fibers in communications.
Basic Concepts
19.2 ELECTROMAGNETIC RADIATION
In the classical sense, electromagnetic radiation is considered to be wave-like, consist-
ing of electric and magnetic field components that are perpendicular to each other
and also to the direction of propagation (Figure 19.1). Light, heat (or radiant en-
ergy), radar, radio waves, and x-rays are all forms of electromagnetic radiation. Each
is characterized primarily by a specific range of wavelengths, and also according to the
technique by which it is generated. Theelectromagnetic spectrumof radiation spans
the wide range fromγ-rays (emitted by radioactive materials) having wavelengths
on the order of 10−^12 m (10−^3 nm), through x-rays, ultraviolet, visible, infrared, and
finally radio waves with wavelengths as long as 10^5 m. This spectrum, on a logarithmic
scale, is shown in Figure 19.2.
H
Position
Figure 19.1 An
electromagnetic
wave showing
electric fieldeand
magnetic fieldH
components, and the
wavelengthλ.