Yet another form of motion is called harmonic or periodic motion
An object moves over the same path repeatedly. Examples of harmonic motion include:
Consider a mass attached to a compressed spring.
The maximum distance from the equilibrium position, here it is A, is called the amplitude.
In SHM the displacement, the velocity, and the acceleration all follow sine curves.
Small oscillations of a pendulum are another case of SHM.
The longer the pendulum the longer the period.
A pendulum has period T on Earth. If the same pendulum were moved to the Moon, how does the new period compare to the old period?
Two pendula have the same length, but different masses attached to the string. How do their periods compare?
Waves can be divided into two types called transverse and longitudinal.
For transverse waves, the disturbance is perpendicular – transverse – to the wave motion.
For longitudinal waves the disturbance is in the same direction as the wave motion.
Some media can support both types of wave.
Waves are also divided into wave pulses (or pulse waves) which are disturbances localized in space, and periodic waves (harmonic waves) where the disturbance is spread out in space.
A harmonic wave is one that repeats in space and time.
At a fixed point in space, the disturbance in the medium will also oscillate with the same period as the wave passes by. A
t a fixed time, the disturbance will be periodic in space.
At a fixed time, the disturbance as a function of distance from the source, will look something like
The amplitude A is the 'height' of the wave – the maximum deviation from the equilibrium.
The distance between successive identical points on the wave – e.g. between adjacent crests – is called the wavelength λ.
At a fixed point in space, the disturbance as a function of time will also look something like:
The period T is the amount of time it takes to cycle through one oscillation.
The frequency f is the number of oscillation cycles per unit time which pass by a fixed point
The wave velocity is the ratio of the distance traveled by a feature on the wave, e.g. a crest, and the time elapsed.
It takes one period T for the wave to move one wavelength λ.
The wave velocity (phase velocity) is v=λ/T=λ f
In some cases the wave speed does depend upon the frequency. This effect is called dispersion. This effect is used by a prism to 'split' white light: the speed of light in the glass is different for each color.
In the ocean, long wavelengths travel faster than short wavelengths.
The velocity of the wave is different from the velocity of the medium.
Does a longitudinal wave, such as a sound wave, have an amplitude?
Consider a wave on a string moving to the right. What is the motion of point A?
Consider point B on the string What is the velocity of point B? B
In 2D and 3D we can have more kinds of waves.
Wavefront – lines in 2D or 3D which connect the same feature on the wave e.g. a crest.
Ray – a line in the direction of wave motion and perpendicular to the wavefronts.
The amplitude of circular and spherical waves decreases with distance from the source.
The reason a wave in 2D and 3D attenuates is because of conservation of energy.
All waves transport energy at a rate which varies as the square of the amplitude.
The energy passing through a circle (2D) or sphere (3D) surrounding the source must be constant.
In 2D the amplitude must vary as A ∝1/√r.
In 3D the amplitude must vary as A ∝1/r.
A1 r1=A2 r2
When a wave reaches a boundary with a medium that has a different wave speed, some of the wave is reflected and some is transmitted.
For a wave in 1D the reflected wave simply propagates in the reverse direction.
In 2D and 3D the direction the reflected wave propagates depends upon the angle at which it hit the boundary.
At every point upon a boundary we can draw a line perpendicular to the surface called the normal.
The angle between the incoming ray and the normal – called the angle of incidence – is equal to the angle between the reflected ray and the normal – the angle of reflection.
This relationship is called the Law of Reflection.
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That part of the wave which is not reflected is transmitted.
In 1D the transmitted wave continues in the same direction as the incident wave.
In 2D and 3D the direction the transmitted wave propagates depends upon the angle at which is strikes the surface.
This effect is called refraction.
A wave travels faster in a thin rope than in a thick rope (if the tension is the same in both). A wave traveling along a thin rope meets and enters a thick section of rope. Which property of the wave in the thick rope is the same as in the thin rope?
Unlike objects, two or more waves can exist at the same point in space at the same time. The net disturbance at a given point in space is the sum of the disturbances of the individual waves.
When two waves pass through each other, the net disturbance at some point in space follows the principle of superposition.
The two waves are said to interfere.
If the net disturbance is greater than the disturbance of either wave separately the interference is constructive.
If the net disturbance is less than the maximum disturbance of the two waves, the interference is destructive.
More generally, for waves in 1D we have three situations:
Synonymously we use in phase to mean constructive interference and out of phase to mean destructive
In 2D and 3D the interference between two circular/spherical waves depends upon the distance from the sources.
Consider two coherent sources of sound waves with the same frequency. The net sound wave at a given location depends upon the distance from that point to the sources.
If the difference in distance to the sources is an integer number of wavelengths then the waves constructively interfere.
If the difference in distance to the sources is half-integral then the two waves destructively interfere.
It is possible to set up a vibrating medium where the wave appears to be standing still.
The system can be decomposed into two waves traveling in opposite directions which interfere
At some places the two waves constructively interfere, at other they destructively interfere.
At special frequencies of the two waves the locations of destructive and constructive interference are fixed.
These locations are called nodes and antinodes respectively.
The most common example of this phenomenon is a taut string.
For a string of fixed length, only certain wavelengths can produce standing waves.
Knowing the wave velocity, the frequencies can be found
The lowest frequency, f1, is called the fundamental.
The higher allowed frequencies are called overtones.
When the overtones are multiples of the fundamental, the overtones are also called harmonics.
Now let's consider a taut string of length L which is fixed only at one end while the other end at is able to move. The fixed end point corresponds to the location of a node: the free end is an antinode. Again, only certain wavelengths of the standing wave can fulfill this condition.
If a source is moving with respect to an observer, the frequency is perceived to be different than when there is no relative motion.
If the source is moving towards an observer the frequency appears to be higher than when the source and observer are at rest.
If the source is moving away from an observer the frequency of the sound wave appears to be lower.
This change in perceived frequency is called the Doppler Effect.
The change in frequency depends upon whether the source or receiver is stationary with respect to the medium.
Consider a source located one wavelength from a receiver.
When the source moves toward the receiver the wavelength of the wave in that direction shrinks.
The Doppler effect also occurs when the source is stationary and the detector moves.
If the detector moves towards the source the receiver perceives a shorter time period T' for the wave.
Consider the case where a stationary source emits a wave towards an object moving toward the source.
The object perceives the wave to have a higher frequency because it is moving towards the source.
The object reflects a wave (i.e. it becomes a source) with the same (higher) perceived frequency.
The original source perceives the reflected wave to have an even higher frequency because the object is moving toward it.
The Doppler Effect also occurs for light. Astronomers use the Doppler Effect to measure the speed of an object towards or away from Earth.