Atoms Entropy Quanta John D. Norton

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Atoms

Entropy

Quanta

John D. Norton

Department of History and Philosophy of Science

University of Pittsburgh

1

The Papers of

Einstein’s Year of

Miracles, 1905

2

The Papers of 1905

1

"Light quantum/photoelectric effect paper"

"On a heuristic viewpoint concerning the production and transformation of light."

Annalen der Physik , 17(1905), pp. 132-148.(17 March 1905)

2

Einstein's doctoral dissertation

"A New Determination of Molecular Dimensions"

Buchdruckerei K. J. Wyss, Bern, 1905. (30 April 1905)

Also: Annalen der Physik, 19(1906), pp. 289-305.

3

"Brownian motion paper."

"On the motion of small particles suspended in liquids at rest required by the molecular-kinetic theory of heat."

Annalen der Physik , 17(1905), pp. 549-560.(May 1905; received 11 May 1905)

4

Special relativity

“On the Electrodynamics of Moving Bodies,”

Annalen der Physik, 17 (1905), pp. 891-921. (June 1905; received 30 June, 1905)

5

E=mc 2

“Does the Inertia of a Body Depend upon its Energy

Content?”

Annalen der Physik, 18(1905), pp. 639-641. (September 1905; received 27

September, 1905)

Einstein inferred from the thermal properties of high frequency heat radiation that it behaves thermodynamically as if constituted of spatially localized, independent quanta of energy.

Einstein used known physical properties of sugar solution (viscosity, diffusion) to determine the size of sugar molecules.

Einstein predicted that the thermal energy of small particles would manifest as a jiggling motion, visible under the microscope.

Maintaining the principle of relativity in electrodynamics requires a new theory of space and time.

Changing the energy of a body changes its inertia in accord with E=mc 2 .

Einstein to Conrad Habicht

18th or 25th May 1905

“…and is very revolutionary”

Einstein’s assessment of his light quantum paper.

…So, what are you up to, you frozen whale, you smoked, dried, canned piece of sole…?

…Why have you still not sent me your dissertation? …Don't you know that I am one of the

1.5 fellows who would read it with interest and pleasure, you wretched man? I promise you four papers in return…

The [first] paper deals with radiation and the energy properties of light and is very revolutionary , as you will see if you send me your work first .

The second paper is a determination of the true sizes of atoms from the diffusion and the viscosity of dilute solutions of neutral substances.

The third proves that, on the assumption of the molecular kinetic theory of heat, bodies on the order of magnitude 1/1000 mm, suspended in liquids, must already perform an observable random motion that is produced by thermal motion;…

The fourth paper is only a rough draft at this point, and is an electrodynamics of moving bodies which employs a modification of the theory of space and time; the purely kinematical part of this paper will surely interest you.

Why is

only the light quantum

“very revolutionary”?

2

Einstein's doctoral dissertation

"A New Determination of Molecular Dimensions"

Buchdruckerei K. J. Wyss, Bern, 1905. (30 April 1905)

Also: Annalen der Physik, 19(1906), pp. 289-305.

3

"Brownian motion paper."

"On the motion of small particles suspended in liquids at rest required by the molecular-kinetic theory of heat."

Annalen der Physik , 17(1905), pp. 549-560.(May 1905; received 11 May 1905)

4

Special relativity

“On the Electrodynamics of Moving Bodies,”

Annalen der Physik, 17 (1905), pp. 891-921. (June 1905; received 30 June, 1905)

5

E=mc 2

“Does the Inertia of a Body Depend upon its Energy

Content?”

Annalen der Physik, 18(1905), pp. 639-641. (September 1905; received 27

September, 1905)

All

the rest develop or complete 19th century physics.

Advances the molecular kinetic program of Maxwell and

Boltzmann.

Establishes the real significance of the Lorentz covariance of

Maxwell’s electrodynamics.

Light energy has momentum; extend to all forms of energy.

6

Why is

only the light quantum

“very revolutionary”?

Well, not always.

"Monochromatic radiation of low density behaves--as long as Wien's radiation formula is valid [i.e. at high values of frequency/temperature]--in a thermodynamic sense, as if it consisted of mutually independent energy quanta of magnitude [h  ]."

All

the rest develop or complete 19th century physics.

The great achievements of 19th century physics:

•The wave theory of light; Newton’s corpuscular theory fails.

•Maxwell’s electrodynamic and its development and perfection by

Hertz, Lorentz…

•The synthesis: light waves just are electromagnetic waves.

Einstein’s light quantum paper initiated a reappraisal of the physical constitution of light that is not resolved over 100 years later.

7

How did Einstein find the quantum?

The content of Einstein’s discovery was quite unanticipated:

High frequency light energy exists in

• spatially independent,

• spatially localized points.

The method of Einstein’s discovery was familiar and secure.

Einstein’s research program in statistical physics from first publication of 1901:

How can we infer the microscopic properties of matter from its macroscopic properties?

The statistical papers of 1905: the analysis of thermal systems consisting of

• spatially independent

• spatially localized, points.

(Dilute sugar solutions,

Small particles in suspension)

8

If….

If

we locate

Einstein’s light quantum paper against the background of electrodynamic theory, its claims are so far beyond bold as to be foolhardy.

If

we locate

Einstein’s light quantum paper against the background of his work in statistical physics, its methods are an inspired variation of ones repeated used and proven effective in other contexts on very similar problems.

9

Einstein’s Early Program in Statistical Physics

10

Einstein’s first two “worthless” papers

Einstein to Stark, 7 Dec 1907, “…I am sending you all my publications excepting my two worthless beginner’s works…”

“Conclusions drawn from the phenomenon of

Capillarity,”

Annalen der Physik ,

4(1901), pp. 513-

523.

“On the thermodynamic theory of the difference in potentials between metals and fully dissociated solutions of their salts and on an electrical method for investigating molecular forces,” Annalen der

Physik , 8(1902), pp.

798-814.

11

Einstein’s first two “worthless” papers

Einstein’s hypothesis:

Forces between molecules at distance r apart are governed by a potential P satisfying

P = P

- c

 c



 (r) for constants c

 and c

 characteristic of the two molecules and universal function  (r).

From macroscopic properties of capillarity and electrochemical potentials infer coefficients in the microscopic force law.

12

Independent Discovery of the Gibbs Framework

Einstein, Albert.

'Kinetische Theorie des

Waermegleichgewichtes und des zweiten Hauptsatzes der

Thermodynamik'. Annalen der Physik, 9 (1902)

3 papers 1902-

1904

13

Independent Discovery of the Gibbs Framework

Einstein, Albert. 'Eine

Theorie der Grundlagen der Thermodynamik'.

Annalen der Physik, 9

(1903)

3 papers 1902-

1904

14

Independent Discovery of the Gibbs Framework

Einstein, Albert. 'Zur allgemeinen molekularen

Theorie der Waerme'.

Annalen der Physik, 14

(1904)

3 papers 1902-

1904

15

The Hidden Gem

16



Einstein’s Fluctuation Formula

Any canonically distributed system p ( E )

 exp





E kT



Variance of energy from mean

2 

( E

E )

2  kT

2 d E

 kT

2

C dT

Heat capacity is macroscopically measureable.



(1904)

17





Applied to an Ideal Gas

Ideal monatomic gas, n molecules

E

3 nkT

2

C

3 nk

2

2 

( E

E )

2  kT

2 d E dT

 kT

2

C

E

 

3 n / 2 kT

(3 n / 2) kT

1

3 n / 2 n=10 24 …. negligible n=1

1

3/ 2

0.816



18







Applied to heat radiation

Volume V of heat radiation (Stefan-Boltzmann law)

E

 

VT

4

C

4

VT

3

In 1904, no one had any solid idea of the constitution of heat radiation!

2 

( E

E ) 2  kT 2 d E dT

 kT 2 C



E

2

 kVT

5/2

VT

4

2 k

V

1

T

3/2

Hence estimate volume V in which fluctuations are of the size of the mean energy.

2 

E

2

(1904)

19

Einstein’s Doctoral

Dissertation

"A New Determination of

Molecular Dimensions”

20

21

How big are molecules?

= How many fit into a gram mole? = Loschmidt’s number N

Find out by determining how the presence of sugar molecules in dilute solutions increases the viscosity of water. The sugar obstructs the flow and makes the water seem thicker.

P = radius of sugar molecule, idealized as a sphere

After a long and very hard calculation…

And after very many special assumptions…

Apparent viscosity m *

=viscosity m of pure water x (1 + fraction of volume taken by sugar  )

 = ( r /m) N (4 p /3) P

3 r = sugar density in the solution m = molecular weight of sugar

Well, not quite. Einstein made a mistake in the calculation. The correct result is m * = m (1 + 5/2  )

The examiners did not notice.

PhD. He later corrected the mistake.

22

Recovering N

Turning the expression for apparent viscosity inside out:

N =

(3m/ 4 pr ) x ( m * / m - 1) x

1/P 3

All measurable quantities

P = radius of molecule.

Unknown!

ONE equation in TWO unknowns.

Einstein needs another equation.

The rate of diffusion of sugar in water is fixed by the measurable diffusion coefficient D.

Einstein shows:

N =

(RT/6 pm D) x

1/P

All measurable quantities

TWO equations in TWO unknowns.

Einstein determined

N = 2.1 x 10 23

After later correction for his calculation error

N = 6.6 x 10

23

23

The statistical physics of dilute sugar solutions

Dilute sugar solution in a gravitational field.

Sugar in dilute solution consists of a fixed, large number of component molecules that do not interact with each other.

Hence they can be treated by exactly the same analysis as an ideal gas!

Sugar in dilute solution exerts an osmotic pressure P that obeys the ideal gas law

PV = nkT

24

Recovering the equation for diffusion

The equilibrium sugar concentration gradient arises from a balance of:

Sugar molecules falling under the effect of gravity.

Stokes’ law F = 6 pm Pv, F = gravitational force

And

Sugar molecules diffusing upwards because of the concentration gradient.

density gradient pressure gradient

(ideal gas law) upward force

The condition for perfect balance is

N

= (RT/6 pm D) x

1/P

25

Equilibration of pressure by a field instead of a semi-permeable membrane…

… was a device Einstein used repeatedly but casually in 1905, but had been introduced with great caution and ceremony in his 1902 “Potentials” paper.

26

“Brownian motion paper.”

“On the motion of small particles suspended in liquids at rest required by the molecularkinetic theory of heat.”

27

28

An easier way to estimate N?

Doctoral dissertation: Einstein determined N from TWO equations in TWO unknowns N, P.

N = (3m/ 4 pr ) x ( m * / m - 1) x

1/P 3

N = (RT/6 pm D) x

1/P

What if sugar molecules were so big that we could measure their diameter P under the microscope?

Why not just do the same analysis with microscopically visible particles?! Then P is observable.

Only ONE equation is needed.

Particles in suspension in a gravitational field

Particles in suspension = a fixed, large number of component that do not interact with each other.

Hence they can be treated by exactly the same analysis as an ideal gas and dilute sugar solution!

The particles exert a pressure due to their thermal motions.

PV=nkT

…and this leads to their diffusion according to the same relation N = (RT/6 pm D ) x 1/P .

Measure D and we can find N.

29

Brownian motion

Einstein predicted thermal motions of tiny particles visible under the microscope and suspected that this explained Brown’s observations of the motion of pollen grains.

For particles of size 0.001mm, Einstein predicted a displacement of approximately

6 microns in one minute.

“If it is really possible to observe the motion discussed here … then classical thermodynamics can no longer be viewed as strictly valid even for microscopically distinguishable spaces, and an exact determination of the real size of atoms becomes possible.”

30

Estimating the coefficient of diffusion for suspended particles

…and hence determine N.

To describe the thermal motions of small particles, Einstein laid the foundations of the modern theory of stochastic processes and solved the “random walk problem.”

Particles spread over time t, distributed on a bell curve.

Their mean square displacement is 2Dt.

Hence we can read D from the observed displacement of particles over time.

Then find N using N

= (RT/6 pm D) x

1/P

31

Unexpected properties of the motion

Displacement is proportional to square root of time. So an average velocity cannot be usefully defined.

displacement time

 0 as time gets large.

The “jiggles” are not the visible result of single collisions with water molecules, but each jiggle is the accumulated effect of many collision.

32

Thermodynamics of

Systems of Independent

Components

(ideal gas law)

33

The simplest case: an ideal gas

(e.g. most ordinary gases at ordinary temperatures and low pressures)

Pressure P x volume V = number of molecules n x Boltzmann’s constant k x temperature T

PV = nkT

What we shall see:

The law depends only the gases having a very few simple properties: they consist of very many spatially localized, independent components, fixed in number.

The remarkable fact: Very few micro-properties of the gas enter into the law. Only n and k.

Boltzmann’s constant k

= ideal gas constant R

/Loschmidt’s number N k = R/N

34

From micro to macro…

An ideal gas in a gravitational field.

h

Micro-structure

A dilute gas is a fixed, large number of component molecules that do not interact with each other.

Because of their thermal energy at temperature

T, the molecules spread to fill the volume

V

, exerting a pressure

P on the vessel walls.

We can infer the ideal gas law from the micro-structure.

Observed property

Ideal gas law

PV = nkT

35

…and back

An ideal gas in a gravitational field.

Micro-structure

A dilute gas is a fixed, large number of component molecules that do not interact with each other.

h

The ideal gas law is the macroscopic signature of…

…And we can invert the inference.

Observed property

Ideal gas law

PV = nkT

36

A much simpler derivation

Very many, independent, small particles at equilibrium in a gravitational field.

Independence expressed: energy E(h) of each particle is a function of height h only.

Pull of gravity equilibrated by pressure P.

37

A much simpler derivation

Boltzmann distribution of energies

P robability of one molecule at height h

P(h) = const. exp(-E(h)/kT)

D ensity of gas at height h

r = r

0 exp(-E(h)/kT)

D ensity gradient due to gravitational field d r /dh = -1/kT (dE/dh) r = 1/kT f = 1/kT dP/dh where f = - (dE/dh) r is the gravitational force density, which is balanced by a pressure gradient P for which f = dP/dh.

Ideal gas law

R earrange d/dh(P r kT) = 0

S o that P = r kT PV = nkT since r = n/V

Reverse inference possible, but messy. Easier with

Einstein’s 1905 derivation.

38

“Light quantum/photoelectric effect paper”

"On a heuristic viewpoint concerning the production and transformation of light."

39

Einstein’s astonishing idea

The light quantum hypothesis

“Monochromatic radiation of low density (within the range of validity of Wien’s radiation formula) behaves thermodynamically as if it consisted of mutually independent energy quanta of magnitude

[h  ].” i.e. Electromagnetic radiation does not always behave like waves, contrary to the most successful science of the nineteenth century.

Sometimes it behaves like little lumps of energy of size h .

Einstein’s reasons:

Certain experimental effects are only plausibly explained by light consisting of quanta: especially the photoelectric effect.

There is an atomistic signature in the thermodynamics of high frequency radiation.

40

Why the atomistic signature of radiation is hard to see

Atomistic signature of systems with

• fixed, large number

• spatially localized

• independent components is the ideal gas law.

High frequency radiation is a system with

• variable , large number

• spatially localized

• independent components, so the ideal gas law is hard to see .

Constant temperature expansion of an ideal gas. The number of molecules is constant and the pressure drops, as the ideal gas law demands.

Constant temperature expansion of high frequency radiation. The number of quanta increases and the pressure stays constant.

41

Einstein noticed a new signature of independent atoms…

An ideal gas can spontaneously compress to half its volume (with very small probability) .

Probability one molecule is on the left is (1/2).

Probability all n molecules are on the left is (1/2) n

.

Entropy S =

- k log (probability)

Entropy difference

D S = - kn log 2

The signature of independent atoms: entropy depends on the logarithm of volume ratios.

42

…which he found in high frequency radiation

Spontaneous volume fluctuations in high frequency radiation are also possible.

Radiation of energy E may spontaneously halve in volume with very small probability.

Probability of spontaneous compression is (1/2)

E/h 

Just as is the radiation consisted of n = E/h  spatially localized, independent quanta of energy.

log (probability)

= - Entropy s/k

Entropy difference

D S = - k (E/h  ) log 2

Determined from measured properties of radiation.

43

Conclusion

44

Unity in

Einstein’s statistical physics of

1905

Einstein investigated many different thermal systems in 1905.

What made these investigations tractable was a common feature:

Each consisted of a large number of spatially localized component that do not interact with each other. And so:

Ideal gas is just like

Dilute sugar solution is just like

Particles in suspension is just like

High frequency radiation

45

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