TEST 3 Flashcards
What is a wave?
A wave is an oscillation or periodic movement that can transport energy from one point in space to another. (kinetic energy is transferred through matter (the rope, water, or air) while the matter remains essentially in place.)
electromagnetic waves consist of
an electric field oscillating in step with a perpendicular magnetic field, both of which are perpendicular to the direction of travel. These waves can travel through a vacuum at a constant speed of 2.998 × 10^8 m/s, the speed of light (denoted by c)
waves are characterized by
a wavelength, a frequency and an amplitude
wavelength
lamda; the distance between two consecutive peaks or troughs in a wave measured in meters
frequency
Hz, v or nu; the number of wave cycles that pass a specified point in space in a specified amount of time (seconds.) A cycle corresponds to one complete wavelength.
amplitude
corresponds to the magnitude of the wave’s displacement. The amplitude is related to the intensity of the wave, which for light is the brightness, and for sound is the loudness.
speed of a wave
The product of a wave’s wavelength (λ) and its frequency (ν
for electromagnetic radiation in a vacuum, speed is equal to
the fundamental constant, c
what is the relationship between wavelength and frequency
inversely proportional. As the wavelength increases, the frequency decreases.
what happens when two or more waves come into contact?
they interfere with one another
standing waves
remain constrained within some region of space. A system with fixed end points such as this restricts the number and type of the possible waveforms. This is an example of quantization, in which only discrete values from a more general set of continuous values of some property are observed.
nodes
waves displaying more than one-half wavelength) all have one or more points between the two end points that are not in motion called nodes. number of nodes= n-1
what is a blackbody?
A blackbody is a convenient, ideal emitter that approximates the behavior of many materials when heated. It is “ideal” in the same sense that an ideal gas is a convenient, simple representation of real gases that works well, provided that the pressure is not too high nor the temperature too low. BUT the theoretical curves did not show a peak, and absurdly showed the intensity becoming infinitely large as the wavelength became smaller, which would imply that everyday objects at room temperature should be emitting large amounts of UV light. This became known as the “ultraviolet catastrophe” Planck resolved this by restricting the vibrational energies to discrete values for each frequency, he could derive an expression for blackbody radiation that correctly had the intensity dropping rapidly for the short wavelengths in the UV region.
E=
hc/lamda
Planck’s constant (a.k.a. h)
h= 6.626 ×× 10−34 joule seconds (J s)