A brief History of Brownian Motion
- Jan Ingenhousz 1785 (1st to record
an observation?).
- Robert Brown 1828 (1st to study
systematically and publish).
- Various explanations and
experiments:
- Regnault 1858 (irregular heating
by light?).
- Weiner 1863 (not temperature
differences or evaporation).
- Cantoni and Oehl 1865
(persistence for over a year).
- S. Exner 1867 (more rapid with
smaller particles).
- Jevons 1870 (electrical forces?).
- Dancer 1870 (not electrical
forces).
- Delsaux 1877 (1st to say motion
is from molecular bombardment).
- Gouy 1888 (motion is more lively
in less viscous liquid, illumination nor e.m. field has an effect,
first experimental work).
- Ramsay 1892 (not electrical,
pressure differences?).
- Maede Bache 1894 (confirmation of
Gouy).
- Quincke 1898 (temperature
fluctuations?).
- F. M. Exner 1900 (not temperature
fluctuations, particle size and temperature dependence).
- Louis Bachelier 1900 (correct
mathematical theory in doctoral dissertation 'Theory of Speculation').
- A. Einstein 1905.
- Various explanations and
experiments:
- Smoluchowski 1905 (similar
results as Einstein using different methods).
- de Broglie et. al. 1908 (makes a
movie from still photos at 1/20 sec. intervals).
- J. Perrin 1921 (Les Atoms) Nobel
prize in 1926:
- Starts with the law of definite proportions and collects all
known arguments in favor of the existence of atoms. A real tour de force.
Perrin's experiments
- Observations under a microscope, both horizontal and vertical orientations.
- Preparation of gamboge grains of various sizes.
- Measurement of grain size and mass by three techniques (direct camera measurments, weight, Stokes' law).
In the following:
- NA is Avogadro's number.
- g is the acceleration of gravity.
- R is the ideal gas constant.
- T is the absolute temperature.
- a is the radius of the particles.
is
the viscosity of the liquid.
1. Vertical distribution in emulsions (balance between Brownian
motion and gravity)
Here
n is the concentration of particles, no is the
concentration at hight h, m the mass of the particles, d the density
of the liquid, D the density of the material of the particles.
Experimental value of Avogadro's number is determined to be 68.2 x 1022.
2.
Direct random walk displacement measurements (Einstein)
Here
x is the the projection of the horizontal displacement along an
arbitrary axis in time t.
Experimental value of Avogadro's number is determined to be 64 x 1022.
3. Brownian rotation (Einstein)
Here
A is the change in the angle of rotation in time t.
Experimental value of Avogadro's number is determined to be 65 x 1022.
4. Diffusion
(Einstein)
Here
D is the diffusion coefficient.
Experimental value of Avogadro's number is determined to be 69 x 1022.
Perrin's summary in 1923:
- Brownian motion has now been
investigated by Perrin or others under various conditions:
- Temperature variations.
- Light intensity variations.
- Light color variations.
- Disturbances due to local mechanical vibrations.
- In other fluids (acids, bases,
salts).
- In fluids with other viscosities (glycerin,
gases).
- Water droplets on soap films.
- Over periods of days, weeks years
and in quartz inclusions (i.e. 1000's of years).
- With various size particles (0.2
microns up to 5.5 microns) of various materials (pollen, mastic,
gamboge).
- Brownian motion is truly random, eternal,
spontaneous; an essential property of fluids in equilibrium.
- Brownian motion breaks the 2nd law of
thermodynamics ('Carnot's Principle') on a microscopic scale (Perrin
anticipates Feynman's thermal ratchet problem).
- Agreement of various methods of calculating Avogadro's
number, NA is proof of the atomic theory.
|
Experiment
|
NA/1022
|
|
Viscosity of gases (kinetic theory)
|
62
|
|
Vertical distribution in dilute emulsions
|
68
|
|
Vertical distribution in concentrated emulsions
|
60
|
|
Brownian motion, Displacements
|
64
|
|
Brownian motion, Rotations
|
65
|
|
Brownian motion, Diffusion
|
69
|
|
Density fluctuations in concentrated emulsions
|
60
|
|
Critical opalescence
|
75
|
|
Blueness of the sky
|
65
|
|
Diffusion of light in argon
|
69
|
|
Blackbody spectrum
|
61
|
|
Charge in microscopic particles [Millikan like experiments]
|
61
|
|
Radioactivity, Projected charges
|
62
|
|
Radioactivity, Helium produced
|
66
|
|
Radioactivity, Radium lost
|
64
|
|
Radioactivity, Energy radiated
|
60
|
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