Book cover for Physics

Physics

John D. Cutnell, Kenneth W. Johnson, David Young, Shane Stadler

ISBN #9781118486894

10th Edition

2,562 Questions

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Summary

Learning Objectives

Key Concepts

Example Problems

Explanations

Common Mistakes

Summary

This module covers the dual nature of light and matter, illustrating how particles such as electrons can exhibit wave behavior and how waves such as light can exhibit particle-like characteristics. Key experiments such as the double-slit experiment, photoelectric effect, and Compton scattering demonstrate that classical ideas must be extended to include quantum concepts like quantization of energy, de Broglie wavelengths, and the uncertainty principle. These quantum phenomena are fundamental to modern technologies ranging from digital imaging to X-ray spectroscopy.

Learning Objectives

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Key Concepts

CONCEPT

DEFINITION

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Example Problems

Example 1

The dissociation energy of a molecule is the energy required to break the molecule apart into its separate atoms. The dissociation energy for the cyanogen molecule is $1.22 \times 10^{-18} \mathrm{J} .$ Suppose that this energy is provided by a single photon. Determine the (a) wavelength and (b) frequency of the photon. (c) In what region of the electromagnetic spectrum (see Figure 24.9) does this photon lie?

Example 2

An AM radio station broadcasts an electromagnetic wave with a frequency of $665 \mathrm{kHz}$, whereas an $\mathrm{FM}$ station broadcasts an electromagnetic wave with a frequency of 91.9 MHz. How many AM photons are needed to have a total energy equal to that of one FM photon?

Example 3

ssm Ultraviolet light with a frequency of $3.00 \times 10^{15} \mathrm{Hz}$ strikes a metal surface and ejects electrons that have a maximum kinetic energy of $6.1 \mathrm{eV} .$ What is the work function (in eV) of the metal?

Example 4

Light is shining perpendicularly on the surface of the earth with an intensity of $680 \mathrm{W} / \mathrm{m}^{2}$. Assuming that all the photons in the light have the same wavelength (in vacuum) of $730 \mathrm{nm},$ determine the number of photons per second per square meter that reach the earth.

Example 5

ssm Ultraviolet light is responsible for sun tanning. Find the wavelength (in nm) of an ultraviolet photon whose energy is $6.4 \times 10^{-19} \mathrm{J}$.

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Step-by-Step Explanations

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Common Mistakes

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