Summary

General Principles

The Wave Model

This model is based on the idea of a traveling wave, which is an organized disturbance traveling at a well-defined wave speed v.

  • In transverse waves the displacement is perpendicular to the direction in which the wave travels.

  • In longitudinal waves the particles of the medium are displaced parallel to the direction in which the wave travels.

A wave transfers energy, but no material or substance is transferred outward from the source.

The figure illustrates a transverse wave above a longitudinal wave one.

Two basic classes of waves:

  • Mechanical waves travel through a material medium such as water or air.

  • Electromagnetic waves require no material medium and can travel through a vacuum.

For mechanical waves, such as sound waves and waves on strings, the speed of the wave is a property of the medium. Speed does not depend on the size or shape of the wave.

Important Concepts

The displacement D of a wave is a function of both position (where) and time (when).

For a transverse wave on a string, the snapshot graph is a picture of the wave. The displacement of a longitudinal wave is parallel to the motion; thus the snapshot graph of a longitudinal sound wave is not a picture of the wave.

Sinusoidal waves are periodic in both time (period T) and space (wavelength λ):

D(x, t)=A sin[2π(x/λ−t/T)+ϕ0]=A sin(kx−ωt+ϕ0)

where A is the amplitude, k=2π/λ is the wave number, ω=2πf=2π/T is the angular frequency, and ϕ0 is the phase constant that describes initial conditions.

The fundamental relationship for any sinusoidal wave is v=λf.

Applications

The wave intensity is the power-to-area ratio: I=P/a

For a circular or spherical wave: I=Psource /4πr2

The sound intensity level is

β=(10 dB) log10 (I/1.0×10−12 W/m2)

The Doppler effect occurs when a wave source and detector are moving with respect to each other: the frequency detected differs from the frequency f0 emitted.

Approaching source Observer approaching a source
f+=f01−vs /v f+=(1+vo/v)f0
Receding source Observer receding from a source
f−=f01+vs/v f−=(1−vo/v)f0

The Doppler effect for light uses a result derived from the theory of relativity.

Terms and Notation