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Lecture 1 Discretization of energies (c) So Hirata, Department of Chemistry, University of Illinois at Urbana- Champaign. This material has been developed and made available online by work supported jointly by University of Illinois, the National Science Foundation under Grant CHE-1118616 (CAREER), and the Camille & Henry Dreyfus Foundation, Inc. through the Camille Dreyfus Teacher-Scholar program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the sponsoring agencies.

Lecture 1 Discretization of energies

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Page 1: Lecture 1 Discretization of energies

Lecture 1Discretization of energies

(c) So Hirata, Department of Chemistry, University of Illinois at Urbana-Champaign. This material has been developed and made available online by work supported jointly by University of Illinois, the

National Science Foundation under Grant CHE-1118616 (CAREER), and the Camille & Henry Dreyfus Foundation, Inc. through the Camille Dreyfus Teacher-Scholar program. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not

necessarily reflect the views of the sponsoring agencies.

Page 2: Lecture 1 Discretization of energies

Discretization of Energies

Energies are discrete (quantized) and not continuous.

This quantization principle cannot be derived – rather it should be accepted as physical reality.

We will survey historical developments in physics that led to the important discovery that energies are quantized. The details of each of the experiments or theories are not so important – the conclusion is important.

Page 3: Lecture 1 Discretization of energies

Quantization of Energy

Classical mechanics: Any value of energy is allowed. Energy is continuous.

Quantum mechanics: Not all values of energy are allowed. Energy is discrete (quantized).

Page 4: Lecture 1 Discretization of energies

Black-body radiation

A heated metal emits light.

As the temperature becomes higher, the color of the emitted light shifts from red to white to blue.

How can physics explain this effect?

Page 5: Lecture 1 Discretization of energies

Light

Wavelength (λ) and frequency (ν) of light are inversely proportional: c = νλ (c is the speed of light).

Page 6: Lecture 1 Discretization of energies

What is “temperature”? – translation, rotation, vibrations, etc. of atoms in molecules and solids.

Light of frequency v can also be viewed as an oscillator having temperature.

Equipartition principle: Heat flows from high to low temperature area; each oscillator has the same thermal energy kT at equilibrium.

Black-body radiation

Page 7: Lecture 1 Discretization of energies

Black-body radiation

Experimentally, increasing the temperature increases the intensity and decreases the maximum of wavelengths of light.

Page 8: Lecture 1 Discretization of energies

Black-body radiation

short wavelengthlarge frequency v

Rayleigh-Jeans ~ kTv2

Experimental

c = vλ

Classical explanation – Rayleigh-Jeans law – has the limitation.

energy distribution~ kT / λ4 ~ kTv2

Ultraviolet catastrophe.

Page 9: Lecture 1 Discretization of energies

Black-body radiation

Planck could explain the experimental energy density by postulating that the energy of each electromagnetic oscillator is limited to discrete values (quantized).

E = nhν (n = 0,1,2,…). h is Planck’s constant.

Page 10: Lecture 1 Discretization of energies

Black-body radiation

0 ν ∞

kT

vDe

nsi

ty o

f lig

hts

with

freq

uen

cy v

Each electromagnetic

oscillator of a frequency v is given an equal share of energy

kT

v2

Page 11: Lecture 1 Discretization of energies

Black-body radiation

hνhνhν

0 ν ∞

kT hν hν hν hν hν hν hν hν hνhν

vDe

nsi

ty o

f lig

hts

with

freq

uen

cy v

Electromagnetic oscillators with

smaller frequencies are

unaffected, leading to

Rayleigh-Jeans results

v2

v2 × hv/(ehv/kT−1)

hv/(ehv/kT−1) Bose-Einstein statistics

Page 12: Lecture 1 Discretization of energies

Continuous vs. quantized

Higher frequencies

Each oscillator has a price tag of hv and kT may not be enough to buy one hv if v is high

kT kT kT kT

Page 13: Lecture 1 Discretization of energies

Planck’s constant h

E = nhν (n = 0,1,2,…) h = 6.63 x 10–34 J s. (Joule is the units of

energy and is equal to Nm or Newton x meter). The frequency has the units s–1.

Because h is small, classical limit works well in so many cases.

In the limit h → 0, E becomes continuous and any arbitrary value of E is allowed. This is the classical limit.

Page 14: Lecture 1 Discretization of energies

Heat capacities

Heat capacity is the amount of energy one needs to heat up a substance by 1 K. The greater the heat capacity, the more thermally responsive the substance is.

“Heat” is a macroscopic concept of a flow of energies of a collection of oscillators.

Dulong-Petit’s law of heat capacity: molar heat capacity of monatomic solids is the same.

Page 15: Lecture 1 Discretization of energies

Heat capacities

There are NA (Avogadro’s) number of atoms in a mole of a monatomic solid. Each can act as a three-way oscillator (that oscillates in x, y, and z directions independently).

According to the equipartition principle, each of the three degrees of freedom of an oscillator is entitled to kT energy.

E = 3NAkT → C = dE/dT = 3NAk = 3RR is the gas constant.

Page 16: Lecture 1 Discretization of energies

Heat capacities

Dulong-Petit’s law holds for large T.

For small T, it does not.

The deviation at low T has been explained by Einstein

Page 17: Lecture 1 Discretization of energies

Heat capacities

For smaller T, the thermal energy kT ceases to be able to afford the smallest allowed quantum hν (ν is the frequency of oscillation).

hv…hv

hv hv

hvhv

hv

hvhv

hv

hv

hv

Small T Large T

kTkT

kT

Page 18: Lecture 1 Discretization of energies

Heat capacities

Einstein assumed that there was only one available frequency of oscillation v.

When Debye used a more realistic distribution of frequencies, he obtained a better agreement between theory and experiment.

Page 19: Lecture 1 Discretization of energies

Atomic & molecular spectra

Colors of matter originate from the light emitted or absorbed by constituent atoms and molecules.

The frequencies of light emitted or absorbed are discrete.

Page 20: Lecture 1 Discretization of energies

Atomic & molecular spectra

This has been explained by atoms and molecules having discrete energies (E1, E2, …).

When light is emitted or absorbed, an atom or molecule shifts in energy, so hv = En – Em.

Page 21: Lecture 1 Discretization of energies

Summary

Energies of stable atoms, molecules, electromagnetic radiation, and vibrations of atoms, etc. are discrete (quantized). They are not continuous.

Macroscopically observed phenomena, such as red color of hot metals, heat capacity of solids at a low temperature, and colors of matter are all due to quantum effects.

Quantized nature of energy cannot be derived. We should simply accept this.