An accessible guide to how semiconductor electronics work and how they are manufactured, for professionals and interested readers with no electronics engineering background
Semiconductor Basics is an accessible guide to how semiconductors work. It is written for readers without an electronic engineering background. Semiconductors are the basis for almost all modern electronic devices. The author—an expert on the topic—explores the fundamental concepts of what a semiconductor is, the different types in use, and how they are different from conductors and insulators. The book has a large number of helpful and illustrative drawings, photos, and figures.
The author uses only simple arithmetic to help understand the device operation and applications. The book reviews the key devices that can be constructed using semiconductor materials such as diodes and transistors and all the large electronic systems based on these two component such as computers, memories, LCDs and related technology like Lasers LEDs and infrared detectors. The text also explores integrated circuits and explains how they are fabricated. The author concludes with some projections about what can be expected in the future. This important book:
Offers an accessible guide to semiconductors using qualitative explanations and analogies, with minimal mathematics and equations
Presents the material in a well-structured and logical format
Explores topics from device physics fundamentals to transistor formation and fabrication and the operation of the circuits to build electronic devices and systems
Includes information on practical applications of p-n junctions, transistors, and integrated circuits to link theory and practice
Written for anyone interested in the technology, working in semiconductor labs or in the semiconductor industry, Semiconductor Basics offers clear explanations about how semiconductors work and its manufacturing process.
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Yes, you can access Semiconductor Basics by George Domingo in PDF and/or ePUB format, as well as other popular books in Technologie et ingénierie & Ingénierie de l'électricité et des télécommunications. We have over one million books available in our catalogue for you to explore.
To understand how semiconductors work and how they are used, we need to be familiar with the concept of allowed energy levels first proposed by Niels Bohr. How Bohr came up with the idea of a planetary model of the atom is very interesting. Science is a continuum: one observation leads to a hypothesis that leads to a theory that leads to more observations, and so on. Bohr did not come up with his model of the atom out of the blue – no apple fell on his head. A lot of observations and theories going back to the 1700s were proposed before he put them together in a now well‐known theory.
In this chapter, I discuss the experimental evidence and the scientific observations that led to Bohr's planetary model of the atom and the discrete energy levels it postulated. This brief journey will help us understand the significance of the Bohr atom that explains the strange behavior of light spectra.
1.1 Sinusoidal Waves
Before I start, I want to clarify the terms used to define a wave, which I use in the next few sections, and the relations between these terms (see Figure 1.1). There are four variables that we use to define any sinusoidal wave:
The amplitude, A: How high each peak of the wave is in relation to the middle, its zero value.
The frequency, f: The number of ups and downs in the wave in a given time. The units are Hertz or number of ups and downs per second: a number/s.
The wavelength, λ: The distance between two peaks, in meters (m), centimeters (cm), or micrometers (μm).
The wave number, ν (the Greek letter nu, not the letter v): The reciprocal of the wavelength. Some properties of waves are better expressed by the reciprocal of the wavelength. The units are therefore 1/m or m−1, or cm−1, or μm−1.
The last three variables are related by the velocity of the wave. Velocity is the distance that a moving object covers during a fixed amount of time, so the velocity v (this is now the letter v) has units of meters per second (m/s). The key relationships are
(1.1)
and the wave number – the reciprocal of the wavelength – is
(1.2)
For example, suppose that Figure 1.1 represents a sound wave. The velocity of sound in air is 343 m s−1. Take a look at Figure 1.1:
The figure shows 5 cycles in 0.001 seconds, which means the frequency is 5000 cycles per second or f = 5000 Hz, (where Hz, Hertz is the unit for frequency) which happens to be the middle of our hearing range.
The wavelength is the velocity divided by the frequency, or λ = 343 (m s−1)/5000 (1 s−1) = 0.069 m or 6.9 cm. Notice that the seconds cancel out, and therefore the units are in meters or centimeters.
The wave number is v = 1/0.069 m = 14.5 m−1.
As much as possible, I use the metric system of units (MKS, meter, kilogram, second). I have always found it very annoying when books keep changing the unit system. When necessary, I will give you the equivalents.
Figure 1.1 A sinusoidal wave is described in several ways: frequency, wavelength, and reciprocal of the wavelength plus its amplitude.
Now we are ready to dive into the pre‐history of the Bohr atom and understand how Dr. Bohr came up with his famous model.
1.2 The Case of the Missing Lines
To explain how semiconductors work, we start with the Bohr atom. Most readers are familiar with Bohr's planetary model of the atom. How Bohr came up with this model is a very interesting scientific historical path involving many famous scientists of the nineteenth and early twentieth centuries. Science goes one step at a time.
William Wollaston (1766–1826), shown on the left in Figure 1.2, was an English chemist who discovered a couple of atomic elements, including palladium and rhodium. Very early in the 1800s, he built the first spectrometer. Wollaston focused the light from the sun through a prism and, to his surprise, found black lines partitioning the spectra (Figure 1.3). What the heck was going on?
Figure 1.2 William Wollaston (left) looked at the sun's light through a prism and was the first to observe the missing lines.
Source:https://library.si.edu/image‐gallery/73731. Joseph von Fraunhofer (right) studied the missing lines with his spectrometer and named them A–K. where Hz, Hertz is the unit for frequency. https://www.kruess.com/en/campus/spectroscopy/history‐of‐spectroscopy/
Figure 1.3 The sun’s spectrum through a prism shows dark lines: wavelengths of light that seem to have disappeared.
