Brownian molecular motion / Mirror wobbling / Johnson noise
In this section,
Feynman discusses three related phenomena: the random motion of a suspended
particle (classical Brownian motion), the wobbling of a mirror due to
radiation pressure (rotational Brownian motion), and the Johnson noise of an
electrical resistor (Brownian motion of electrons). They can be understood as
three manifestations of thermal fluctuation—governed by the Equipartition Theorem
and Fluctuation-Dissipation Theorem. Thus, a fitting title for the section
might be “Three Types of Brownian Motion,” instead of simply “Equipartition of energy.” It is worth
mentioning that the explanation of classical Brownian motion was first
established by Einstein in his 1905 “Miracle Year” paper, On the
Movement of Small Particles Suspended in a Stationary Liquid, Required by the
Molecular-Kinetic Theory of Heat.
1. Brownian molecular motion
“This was later proved to
be one of the effects of molecular motion, and we can
understand it qualitatively by thinking of a great push ball on a playing
field, seen from a great distance, with a lot of people underneath, all pushing
the ball in various directions. We cannot see the people because we imagine
that we are too far away, but we can see the ball, and we notice that it moves
around rather irregularly. We also know, from the theorems that we have
discussed in previous chapters, that the mean kinetic energy of a small
particle suspended in a liquid or a gas will be 3/2kT even
though it is very heavy compared with a molecule (Feynman et al., 1963, p. 41-1).”
Brownian motion is
the continuous, rapid, and irregular zigzag movement of particles (such as
pollen grains) suspended in a fluid (liquid or gas). This phenomenon serves as direct
evidence for the molecular-kinetic theory of heat, confirming that fluids are
composed of perpetually moving molecules.
We can define Brownian
motion by three interconnected features:
(1) Random motion: The
suspended particles undergo continuous, chaotic, and non-directional
translational and rotational movements. Its path is described as a random walk
because the direction of motion is unpredictable.
(2) Thermal
fluctuations: The motion or collisions arise from thermal fluctuations instead
of simply absolute temperature. The temperature sets the strength of those
fluctuations, so higher temperature means more vigorous Brownian motion.
(3) Diffusion: The
particle’s motion is quantitatively related to diffusion. The mean square distance
of the particle is directly proportional to the observation time and it is
related to the diffusion coefficient (Einstein, 1905).
In short, Einstein’s
theory allows for the calculation of fundamental constants, such as Avogadro’s
number and the size of molecules, by measuring the observable particle
movements.
“The Brownian movement
was discovered in 1827 by Robert Brown, a botanist. While he was studying
microscopic life, he noticed little particles of plant pollens jiggling around
in the liquid he was looking at in the microscope, and he was wise enough to
realize that these were not living, but were just little pieces of dirt moving
around in the water. In fact he helped to demonstrate that this had nothing to
do with life by getting from the ground an old piece of quartz in which there
was some water trapped. It must have been trapped for millions and millions of
years, but inside he could see the same motion. What one sees is that very tiny
particles are jiggling all the time (Feynman et al., 1963, p. 41-1).”
In De Rerum Natura (about 60 BCE), Lucretius
described the motion of dust particles in the sunlight as evidence of atomic
collisions (Powles, 1978). Although
this is not exactly the Brownian motion in the modern sense, it is an
early recognition that “random walk” can be explained by the presence of
invisible microscopic particles. In 1827, Robert Brown established the
phenomenon through meticulous microscopic observations of pollen grains
suspended in water and explained that the motion was not biological but
physical in origin. Almost 80 years later, Einstein (1905) and
Smoluchowski (1906) provided the theoretical foundation of Brownian
motion quantitatively in terms of molecular collisions, thereby offering
decisive evidence for the atomic nature of matter. However, Jean
Baptiste Perrin was awarded the Nobel Prize for Physics in 1926 for his
experimental work on Brownian motion.
2. Mirror wobbling
“What
is the mean-square angle over which the mirror will wobble? Suppose we find the
natural vibration period of the mirror by tapping on one side and seeing how
long it takes to oscillate back and forth, and we also know the moment of inertia, I
(Feynman et al., 1963, p. 41-2).”
When a mirror is suspended freely—typically by a thin fiber or wire—it
exhibits an irregular, continuous wobbling motion even in the absence of
external, visible disturbances. This mirror wobbling is the rotational
equivalent of classical translational Brownian motion and serves as a direct,
macroscopic demonstration of thermal energy fluctuations. The phenomenon is
characterized by:
(1) Random Angular
displacement: The mirror undergoes small, continuous, and unpredictable angular
displacements. This erratic oscillation is readily observed as a “random
walk" in the reflected light beam.
(2) Thermal origin:
The random motion originates from the fluctuating net torque applied to the
mirror. This torque is caused by incessant, unequal bombardment from the
surrounding air molecules, whose energy is determined by the absolute
temperature.
(3) Fluctuation-Dissipation:
The amplitude and frequency of the wobble are determined by the balance between
the fluctuating thermal torque (fluctuation) and the mechanical forces
opposing it (dissipation). This involves the mirror’s moment of inertia,
the stiffness of the fiber (restoring force), and the damping from the
surrounding air.
In essence, mirror
wobbling is the random, thermally driven angular motion of a suspended mirror,
observable as the jitter of its reflected beam—a macroscopic manifestation of
microscopic molecular agitation.
It should be worth mentioning that the mirrors in the
interferometers have the function to split the incoming laser beam into two
perpendicular beams. The mirrors are made of fused silica (very pure glass) and
suspended by glass fibers, but they still have thermal noise from (translational
and rotational) Brownian motion. Today’s mirror stabilization control injects
harmful noise, constituting a major obstacle to sensitivity improvements, e.g.,
in the Laser Interferometer Gravitational-Wave Observatory (LIGO). This would affect
accuracy in the detection of black holes, where gravitational waves emerge from
events like black hole mergers produce minuscule changes in the length of an
interferometer's arms, often smaller than a proton's diameter. If the random,
thermal vibrations of the mirrors are larger than the gravitational wave
signal, they will obscure it, rendering the event undetectable.
“We
know the formula for the kinetic energy of rotation—it is given by Eq. (19.8): T=½Iω2.
That is the kinetic energy, and the potential energy that goes with it will be
proportional to the square of the angle—it is V=½αθ2.
But, if we know the period t0 and calculate from
that the natural frequency ω0=2π/t0,
then the potential energy is V=½Iω02θ2
(Feynman et al., 1963, p. 41-2).”
Feynman’s brief
explanations of a rotational harmonic oscillator could be unpacked as follows:
1. Rotational Kinetic Energy
The kinetic energy T for
rotational motion is given by T=½Iω2, where I is the moment of
inertia and ω is the
angular velocity.
2. Restoring torque
In a torsional system, the restoring torque t is proportional to
the angular displacement q. This means: t = -kq where k is the
torsional constant (a measure of the stiffness of the system).
3. Potential Energy of a Torsional Oscillator
The potential energy V stored in this twist is analogous to
that of a spring and is given by: V=½kθ2. (In Feynman’s text, this is written as V=½αθ2, where α is equivalent to k.
4. Natural angular frequency
The system undergoes simple harmonic motion with a period t0.
The natural angular frequency ω0 (in radians per second) is
related to the period by: ω0 = 2π/t0.
5. Equation of motion of a torsional oscillator
For a torsional oscillator, the equation of motion is: Id2q/dt2 = -kq.
This simplifies to: d2q/dt2 = -(k/I)q which is the
standard form for simple harmonic motion with angular frequency ω0 = Ö(k/I). Solving
for k: k = Iω02
6. Substituting Torsional constant into Potential Energy
Substituting this into the potential energy formula: V = ½kθ2 = ½Iω02θ2
The constant α in the initial potential energy
expression is commonly known as the torsional constant k.
3. Johnson noise
“So now we can design
circuits and tell when we are going to get what is called Johnson noise,
the noise associated with thermal fluctuations! Where do the fluctuations come
from this time? They come again from the resistor—they come from
the fact that the electrons in the resistor are jiggling around because they
are in thermal equilibrium with the matter in the resistor, and they make
fluctuations in the density of electrons (Feynman et al., 1963, p. 41-2).”
Johnson noise (or thermal noise)
is the random, electrically measurable voltage (or current) fluctuation
produced by a resistor at thermodynamic equilibrium. It arises from the
universal requirement of thermal equilibrium: any system that absorbs energy
must also emit it to maintain a constant temperature.
Three Perspectives
on the Phenomenon
Dynamical
Perspective (Brownian Motion of Electrons): The noise manifests as the Brownian
motion of electrons (charge carriers) within the resistor. The electrons are
constantly being scattered by thermal vibrations of the lattice atoms, causing
their velocity to fluctuate randomly. This random motion of charge creates the
tiny, ever-changing voltage fluctuations across the resistor's terminals.
Thermodynamic
Perspective (Black-Body Analogy): The resistor behaves like a
one-dimensional black-body radiator, emitting and absorbing thermal radiation
in the form of fluctuating electromagnetic fields. At thermal equilibrium, the
strength of these fluctuations is precisely balanced, which ensures zero net
energy flow.
Electrodynamical Perspective
(Nyquist's Theorem): The noise is governed by Nyquist's (1928) theorem, an example of the
Fluctuation-Dissipation Theorem, states that the mean-square noise voltage is
directly proportional to the absolute temperature and the dissipation
(resistance) of the system: <V²> = 4kTRΔf. In this equation, k
is the Boltzmann constant, T is the absolute temperature, R is
the resistance, and Δf is the bandwidth over which the noise is measured.
In short, we can unify the concepts of Brownian motion and Johnson noise under the
Fluctuation-Dissipation Theorem. However, Johnson noise is not just a technical
limitation in sensitive electrical circuits, it is fundamentally a
manifestation of the intrinsic thermal fluctuations present in any resistive
material.
“Let P(ω)dω be
the power that the generator would deliver in the frequency range dω into
the very same resistor. Then we can prove (we shall prove it for another case,
but the mathematics is exactly the same) that the power comes out P(ω)dω
= (2/π)kTdω, and is independent of the resistance when
put this way (Feynman et al., 1963, p. 41-3).”
Feynman’s equation P(ω)dω
= (2/π)kTdω is
potentially confusing. Below is a brief note on the conversions (with units)
step-by-step, so that the relations between voltage spectral density, power
spectral density, and units/conventions are clearer.
1) Voltage Spectral
Density (Source Noise)
Based on the
Johnson–Nyquist noise formula, a resistor R at temperature T exhibits
an open‑circuit mean‑square voltage (voltage noise) of
<V2(f)> = 4 kT
R (Units: V2/Hz)
(Unit check: kT
has units J = V·A·s = V²·s / Ω, so kT R→ V²·s. Dividing by s (1/Hz) yields
V²/Hz.)
2) Power delivered
to a matched load (per Hz)
When the source and
load resistances are equal (impedance‑matched), the available thermal‑noise
power is maximized. By voltage division, half the open‑circuit voltage appears
across the load, so the mean‑square voltage across the load is <VL2>rms
= <V2(f)>/4.
Power spectral
density delivered to the load (W/Hz): P(f) = <V2(f)>/4R = 4 kT R/4R
= kT
Thus, the
available noise power per unit bandwidth is independent of R and
equal to kT (the “Johnson noise power formula”).
3. Power Density
per Angular Frequency (ω)
Power spectral
densities expressed per hertz (
Hence, P(ω) = P(f)(df/dω)
= kT/2π
Conclusion
The correct power
delivered by the resistor into a matched load in the angular frequency range ω
is: P(ω) dω = (kT/2π) dω
Feynman's
expression P(ω) dω
= (2/π)kT dω is larger by a factor of 4. The discrepancy could arise from a different
convention for defining P(ω) or from omitting the factor 1/4 that
comes from the matched‑load voltage division. Importantly, the power
delivered to a matched load is a universal quantity defined solely by
temperature and the Boltzmann constant, independent of the resistor's specific
value R.
Key Takeaways: Three Types of Thermal Fluctuation
These
three distinct phenomena—translational, rotational, and electrical
fluctuations—are unified by the Equipartition Theorem, demonstrating how
thermal energy, kT, dictates the average energy stored in every degree
of freedom, regardless of the system's nature (mechanical or electrical).
Fluctuation–Dissipation
Theorem (FDT): All three examples serve as evidence for the FDT, which states
that the magnitude of thermal fluctuations (the jiggling, wobbling, or noise)
is directly proportional to the system's ability to dissipate energy (viscosity
or resistance) and the absolute temperature.
Macroscopic Proof
of Atomism: Collectively, these "three types of Brownian motion"
provide compelling, measurable proof that matter and energy are composed of
discrete, constantly moving microscopic entities, turning atomic theory from a
hypothesis into an established, quantitative physical fact.
The Moral of the
Lesson:
The random motion
of smoke particles—readily visible in a sunlit beam of air—is another classic
example of Brownian motion. While there is no historical account of
Einstein having a flash of insight about Brownian motion while watching his
pipe smoke, it would not be surprising if he reflected on such everyday
phenomena. Einstein was known to be a dedicated pipe smoker throughout
his life and was famously quoted as asserting:
“I believe that
pipe smoking contributes to a somewhat calm and objective judgment in all human
affairs (Oeijord, 2011).”
He died in 1955 at
age 76 from a ruptured abdominal aortic aneurysm (Tesler, 2020), a condition
for which smoking is now a well-established risk factor (Aune et al., 2018). In
the end, Einstein’s relationship with smoking stands as a humbling reminder
that even the most extraordinary physicist remains subject to the ordinary
physical consequences of human habit.
Review Questions:
1. How would you define Brownian motion?
2. How would you explain the wobbling of a freely
suspended mirror?
3. How would you explain Johnson noise?
References:
Aune, D.,
Schlesinger, S., Norat, T., & Riboli, E. (2018). Tobacco smoking and the
risk of abdominal aortic aneurysm: a systematic review and meta-analysis of
prospective studies. Scientific reports, 8(1), 14786.
Einstein, A.
(1905). On the movement of small particles suspended in a stationary liquid
demanded by the molecular-kinetic theory of heat (English translation, 1956). Investigations
on the Theory of the Brownian Movement.
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.
Nyquist, H. (1928).
Certain topics in telegraph transmission theory. Transactions of the
American Institute of Electrical Engineers, 47(2), 617-644.
Oeijord, N. K.
(2011). The General Genetic Catastrophe: On the Discovery and the Discoverer.
iUniverse.
Powles, J. G.
(1978). Brownian motion-June 1827 (for teachers). Physics Education, 13(5),
310.
Smoluchowski, M.
(1906), Zur kinetischen Theorie der Brownschen Molekularbewegung
und der Suspensionen. Annalen der Physik, 21(14), 756–780.
Tesler, U. F.
(2020). A history of cardiac surgery: an adventurous voyage from antiquity
to the artificial heart. Cambridge Scholars Publishing.
