(Thin-layer approximation / Low-density approximation / Plane-wave
approximation)
Feynman derives a formula of Poynting’s vector that is based on thin-layer
approximation, low-density approximation, and plane-wave approximation.
1. Thin-layer approximation:
“All of our calculations have been made for a thin layer of material
whose index is not too far from 1, so that Ea
would always be much less than Es (just to make the calculations easier). In keeping with our
approximations, we should, therefore, leave out the term Ēa2, because it is much smaller than ĒsĒa (Feynman et al., 1963, p. 31–9).”
In this
section, Feynman only uses the term low-density
approximation to derive a formula of Poynting’s vector, ϵ0cE2. However, he mentions that all of his calculations are made for a thin
layer of material whose index is not too far from 1. We should recall that the angle between Es and Ea is almost a right angle and it can be related to the
approximation formula, e−iω(n−1)Δz/c ≈ 1−iω(n−1)Δz/c. To be precise, this method
of approximation is based on a “thin gas plate” in which Δz should be
relatively thin in the formula. Otherwise, the decrease in
E due to absorptions of light in a thicker plate would result in a significant
loss of light energy. In short, we may include the term “thin gas plate
approximation” or simply “thin-layer approximation.”
“For the first term we can
write αĒs2, where α is the as yet unknown constant
of proportionality which relates the average value of E2 to the energy being carried (Feynman
et al., 1963, p. 31–9).”
In section 31-2, Feynman states: “If the source S
(of Fig. 31–1) is far off to the left, then the field Es will have the same phase everywhere on the plate,
so we can write that in the neighborhood of the plate Es = E0eiω(t−z/c).” He did not
determine Ēs2 possibly because it involves calculations due to
the decrease in Es, that is, the absorption of light will end up as thermal energy in a material.
Perhaps it is good to emphasize that the
electric field Es is attenuated by a factor of e−kz in which k is the absorption index of the material. If the loss of energy is considered negligible, Feynman could have
determined Ēs2 instead of writing it as αĒs2. Note that in the next chapter, he changes the
notation Ēs2 to < Es2 >.
2. Low-density approximation:
“One way of checking that our calculations are consistent
is to see that we always keep terms which are proportional to NΔz, the area density of atoms in
the material, but we leave out terms which are proportional to (NΔz)2
or any higher power of NΔz. Ours is what should be called
a “low-density approximation” (Feynman
et al., 1963, p. 31–10).”
According to
Feynman, leaving out terms that are proportional to (NΔz)2 or any higher power of NΔz should be called a “low-density approximation.” However, it involves
a low-density approximation due to smaller N and thin layer approximation
due to shorter Δz. One may recall that η (= NΔz) is the number of charges per unit
area where N is the
number of atoms per unit volume of the thin plate.
In Volume II, Feynman mentions: “…we had to restrict ourselves to finding the
index only for materials of low density, like gases…. so we studied only the
rarefied gas, where such effects are not important (Feynman et al., 1964).” It
may be more accurate to state “rarefied gases approximation,”
but physicists have developed various models of refractive index based on different
atomic densities.
In section 32–3 Waves in a dielectric
of Volume II, Feynman adds: “… if N is
small enough so that n is close to one (as it is for a gas), then Eq. (32.27)
says that n2 is one plus a small number: n2 = 1 + ϵ. We can then
write n = √(1 + ϵ) ≈ 1 + ϵ/2, and the two
expressions are equivalent (Feynman et al., 1964).” It should be worth mentioning
that the refractive index of air is 1.0003. On the other hand, the term rarefied gas means
that the pressure of the gas is much less than
atmospheric pressure. Therefore, ϵ/2 is lesser than 0.0003, i.e., n is expected to be
very close to 1, but small N
may be known as a “rarefied gas approximation” or “low-pressure gas approximation.”
In Volume II,
Feynman elaborates that “S = ϵ0c2E×B, is called ‘Poynting’s
vector,’ after its discoverer. It tells us the rate at which the field energy
moves around in space. …… Believe it or not, we have already derived this
result in Section 31–5
of Vol. I, when we were studying light (Feynman
et al., 1964).” Perhaps Feynman could have said that he has derived Poynting’s
vector ϵ0cE2 using the definition of energy
density of electromagnetic wave and Poynting’s
theorem. (It is also known as Umov-Poynting vector because Nikolay Umov, a
Russian physicist, first proposed the concept of energy flux in a continuous
medium in 1874.) In a sense, it is paradoxical that the formula ϵ0cE2 can be exactly proved using Poynting’s
theorem, but Feynman’s proof is based on “low-density
approximation.”
3. Plane wave approximation:
“We now go back to Eq. (30.19), which
tells us that for large z Ea = NΔzqev(ret
by z/c)/2ϵ0c (31.26) (Feynman
et al., 1963, p. 31–10).”
Eq. (30.19), as
mentioned by Feynman, is based on the assumption of an infinite plane of constant density of oscillating charges.
More importantly, the phrase “for large z” means that a spherical wave may
appear like a plane wave because the curvature becomes negligible when it is significantly
farther away from the source. Some may prefer the term monochromatic plane
wave because this is a single-frequency spherical wave from a faraway source
that would look like a plane wave after traveling a very large distance. For
example, the wavefronts of light from stars are effectively parallel. It may be known as a plane wave approximation as the direction of electric
fields is perpendicular to the motion of the plane wave.
In section
31.2, Feynman explains that in the neighborhood of the plate Es = E0eiω(t−z/c) if the source
S (Fig. 31–1)
is far off to the left (Feynman et al., 1963, p. 31–4). That is, the source S is idealized to be infinitely far and thus the electric
fields of oscillating electrons are in the same direction and have the same
amplitude E0. Specifically, the field Es is weaker in the z-direction and it is
sometimes called an inhomogeneous plane wave
(Jackson, 1999). In short, the homogeneous plane wave becomes an inhomogeneous plane
wave when it enters a medium. Some may prefer to describe this method as “inhomogeneous
plane-wave approximation.”
Review Questions:
1. How would describe
Feynman’s method of calculations that is based on a thin layer
of material whose refractive index is close to 1?
2. Is the energy carried by an electric
wave calculated by only using low density approximation?
3. Would you describe
a wave of the electric field after traveling a large z as a “monochromatic
plane wave” (Griffiths, 2005) or “inhomogeneous plane wave” (Jackson, 1999)?
The moral of the
lesson: A simplified formula of Poynting’s vector ϵ0cE2 for a chromatic (or inhomogeneous) plane wave can be derived using thin-layer
approximation, low-density approximation, and plane-wave approximation.
References:
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.
2. Feynman, R. P., Leighton, R.
B., & Sands, M. (1964). The
Feynman Lectures on Physics,
Vol II: Mainly electromagnetism and matter. Reading, MA:
Addison-Wesley.
3. Griffiths, D. J. (2005). Introduction to Electrodynamics (3rd ed.). New Jersey: Pearson Education.
4. Jackson, J. D. (1999). Classical Electrodynamics (3rd ed.). New York: John Wiley & Sons.
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