(Angular frequency w / Wave number k / w-k relationship)
The three
interesting points discussed in this section are angular frequency (angular temporal
frequency), wave number (angular spatial frequency), and the relationship
between angular frequency and wave number.
1. Angular
frequency:
“The angular
frequency ω can be defined as the rate of change of phase with time (radians
per second). (Feynman et al., 1963, section 29–3 Sinusoidal waves).”
Feynman defines angular frequency (ω) as the rate
of change of phase with time (radians per second). For a sinusoidal wave,
angular frequency can be simply described as the ratio of an angular
displacement to the time taken (e.g., ω = 2p/T in which T is the period of oscillation). Alternatively, we may use the term angular temporal frequency because ω is
related to time and it helps to distinguish the concept of wave number that is
the rate of change of phase with distance. Similarly, the term acceleration could be defined
either as the rate of change of velocity “with time” or “with distance.” To be
more specific, we can define angular temporal frequency as the rate of change
of an oscillator’s phase (or angular displacement) with respect to time that is
applicable to a sinusoidal wave.
To recall the concept of phase, we can refer to Chapter
21 in which Feynman suggests: “The constant Δ is sometimes called the phase of the oscillation, but that is a confusion, because other people
call ω0t+Δ the phase, and say the phase changes with time. We might say that Δ
is a phase shift from some defined zero. Let us
put it differently. Different Δ’s correspond to motions in
different phases. That is true, but whether we want to call Δ the
phase, or not, is another question...” In short, a phase is a state of an oscillator pertaining to
its position and direction of motion. The term phase has been used
traditionally to describe the successive stages of various cycles, such as the periodical
appearance of the Moon as it orbits the Earth.
2. Wave number:
“… we
can define a quantity called the wave number, symbolized as k.
This is defined as the rate of change of phase with distance (radians
per meter). (Feynman et al., 1963, section 29–3 Sinusoidal waves).”
Feynman defines wave
number (k) as the rate of change of
phase with distance (radians per meter). However, this term is a misnomer because
it is not strictly a number and k is sometimes used as a
complex function. In dispersive media (e.g.,
water), k is a complex function of frequency that has both real and
imaginary parts. Thus, a better term could be angular spatial frequency instead
of angular wavenumber or wave number. Specifically, we can define angular
spatial frequency as the rate of change of an oscillator’s phase with respect
to distance that is applicable to a sinusoidal wave (instead of a wave packet).
From an operational perspective, k can be measured as the number of the
oscillator’s cycles per unit distance (e.g., k = 2p/l).
According to Feynman, the formula for a cosine wave
moving in a direction x with a wave number k and an angular
frequency ω will be written in general as cos (ωt−kx). Perhaps he
could have elaborated that it can be written as a sine function or cosine
function, and it can be written as either cos (ωt−kx) or cos (kx−ωt)
because cos q =
cos (−q). In general, cos (kx−ωt) may refer to a wave
moving to the right, whereas cos (kx+ωt) may refer to another
wave moving to the left. If we fix t as a specific instant in time
(e.g., t = 0), we can have a snapshot graph that shows how a
wave’s vertical displacement changes as a function of x. If we fix x
as a specific point in space (e.g., x = 0), we can have a history
graph that shows how a wave’s vertical displacement changes with time.
3. w-k relationship:
“Now in
our particular wave there is a definite relationship between the
frequency and the wavelength, but the above definitions of k and ω
are actually quite general (Feynman et
al., 1963, section 29–3
Sinusoidal waves).”
Feynman clarifies that there is a definite
relationship between the frequency and the wavelength in our particular wave,
but the definitions of ω and k provided in this section are quite
general. That is, ω and k are not related in the same way in
other physical circumstances. Perhaps Feynman could simply explain that the
definite relationship shown is applicable only to sinusoidal waves that have
only one frequency and one wavelength. In other words, ω and k are
related in a complicated manner for a wave packet. This leads to the concept of
group velocity and phase velocity that will be covered in chapter 48 when
Feynman emphasizes that “[t]he group velocity is the
derivative of ω with respect to k, and the phase velocity is ω/k.”
In the end of the section, Feynman mentions that
equation (29.1) is a legitimate formula because it is applicable
to the “wave zone” (the region that is beyond a few wavelengths). However, the
term “wave zone” is not commonly used in this context. More interestingly, in
section 34-7 The ω, k four-vector, Feynman says, “if ω is
thought of as being like t, and k is thought of as being like x
divided by c2, then the new ω′ will be like t′, and
the new k′ will be like x′/c2.” That is, the angular frequency ω of a sinusoidal wave and its wave
number k transform in the same way as space and time under the Lorentz
transformation. Thus, it is worthwhile mentioning that the wave number k
and the angular frequency ω are interrelated to the extent they are analogous
to the space and time in special relativity.
Review Questions:
1. Would you use the term angular frequency and define it as the rate of change of phase with time?
2.
Would you use the term wave number and define it as the rate of change of phase with distance?
3. How would you describe the relationship between
the angular frequency and wave number of an oscillator?
The moral of the lesson: the angular frequency (ω) is the rate of change
of phase with time, whereas the wave number (k) is the
rate of change of phase with distance; ω = 2p/T = 2pf and k
= 2p/l implies ω/k = fl = c (for
a sinusoidal wave).
Reference:
1. Feynman, R. P., Leighton, R. B., & Sands, M. (1963). The Feynman Lectures on Physics, Vol I: Mainly mechanics, radiation, and heat. Reading, MA: Addison-Wesley.
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