chapter 9 introduction to quantum mechanics (may. 20, 2005)

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Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

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Page 1: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Chapter 9

Introduction to Quantum Mechanics

(May. 20, 2005)

Page 2: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Conduction ( 传导 ), convection ( 对流 ), radiation ( 辐射 )

Hypothesis ( 假设 ), postulate (假定,基本原理) ,

Blackbody radiation , Photoelectric effect ( 光电效应 )

Thermotics ( 热学 ) , thermodynamics ( 热力学 )

ultraviolet Catastrophe (disaster) ( 紫外灾难 )

Reinforce ( 加强 ) irradiate , shine

Page 3: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.1 Blackbody radiation and Planck hypothesis

• Two patches of clouds in physics sky at the beginning of 20th century.

• The speed of light Relativity

• The blackbody radiation foundation of Quantum theory

Page 4: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.1.1 Blackbody radiation and Planck’s hypothesis ( 假设 ).

• Types of heat energy transmission are conduction, convection and radiation.

• Conduction is transfer of heat energy by molecular vibrations not by actual motion of material. For example, if you hold one end of an iron rod ( 铁杆 ) and the other end of the rod is put on a flame, you will feel hot some time later. You can say that the heat energy reaches your hand by heat conduction.

Page 5: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Convection is transfer of heat by actual motion of. The hot-air furnace, the hot-water heating system, and the flow of blood in the body are examples.

• Radiation The heat reaching the earth from the sun cannot be transferred either by conduction or convection since the space between the earth and the sun has no material medium. The energy is carried by electromagnetic waves that do not require a material medium for propagation. The kind of heat transfer is called thermal radiation.

Page 6: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Blackbody is defined as the body which can absorb all energies that fall on it. It is something like a black hole. No lights or material can get away from it as long as it is trapped. A large cavity with a small hole on its wall can be taken as a blackbody.

Page 7: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

•Blackbody radiation: Any radiation that enters the hole is absorbed in the interior of the cavity, and the radiation emitted from the hole is called blackbody radiation.

Fig. 9.1 Blackbody concave.

Page 8: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Fig. 9.2 the blackbody radiation of spectra for four different temperatures.

1. Stefan and Boltzmann’s law: it is found that the radiation energy is proportional to the fourth power of the associated temperature.

4)( TTM M(T) is actually the area under each curve, σ is called Stefan’s constant and T is absolute temperature.

Page 9: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

2. Wien’s displacement law: the peak of the curve shifts towards longer wavelength as the temperature falls and it satisfies

bTpeak

This law is quite useful for measuring the temperature of a blackbody with a very high temperature. You can see the example for how to measure the temperature on the surface of the sun.

where b is called the Wein’s constant.

Page 10: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• The above laws describes the blackbody radiation very well.

• The problem exists in the relation between the radiation power Mλ(T) and the wavelength λ.

• Blackbody radiation has nothing to do with both the material used in the blackbody concave wall and the shape of the concave wall.

• Two typical theoretical formulas for blackbody radiation : One is given by Rayleigh and Jeans and the other by Wein.

Page 11: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Rayleigh and Jeans

In 1890, Rayleigh and Jeans obtained a formula using the classical electromagnetic (Maxwell) theory and the classical equipartition theorem of energy ( 能均分定理 ) in thermotics (热学 ). The formula is given by

TCTM 41)(

Page 12: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Rayleigh-Jeans formula was correct for very long wavelength in the far infrared but hopelessly wrong in the visible light and ultraviolet region. Maxwell’s electromagnetic theory and thermodynamics are known ascorrect theory. The failure in explaining blackbody radiation puzzled physicists! It was regarded as ultraviolet Catastrophe (disaster).

Fig. 9.3 Blackbody radiation

Rayleigh-Jeans’ line

Wein’s line

Page 13: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Wein’s formula:

Later on in 1896, Wein derived another important formula using thermodynamics.

TC

eCTM

352)(

Unfortunately, this formula is only valid in the region of short wavelengths.

Page 14: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Rayleigh-Jeans’ line

Wein’s line

( m) T=1500K

1 2 3

M(T)

Page 15: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Planck’s Magic formula

In 1900, after studying the above two formulas carefully, Planck proposed ( 提出 ) an empirical formula.

1

12)( 52

Tkhc

ehcTM

Where c is the speed of light, k is Boltzmann’s constant, h is Planck’s constant and e is the base of natural logarithm.

It is surprising that the experience formula can describe the curve of blackbody radiation exactly for all wavelengths.

Page 16: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Other unbelievable deductions:

(1) For very large wavelength, the Rayleigh-Jeans formula can be obtained from Planck’s formula;

1Tk

hc

1Tk

hc

2

2

11

Tk

hc

Tk

hce Tk

hc

Drop the second order and higher order terms, and RJ formula could be obtained.

Page 17: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(2) For smaller wavelength of blackbody radiation, the Wein’s formula can be achieved also from Planck’s experience formula;

Tk

hc

Tk

hc e

e

1

1

Then Wein’s formula could be obtained.

Page 18: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(3) Integrating Planck’s formula with respect to wavelength, the Stefan and Boltzmann’s law can be obtained as well.

4

0

)()( TdTMTM

Is called Stefen constant.

Page 19: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(4) Finally, according to the basic mathematical theory and differentiating the Planck’s formula with respect to wavelength, Wien’s displacement law can also be derived!

0)(

d

TdM

bT max

Page 20: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Planck’s empirical formula matched all the different classical physics results obtained by the Maxwell electromagnetic theory, thermodynamics and statistics! However, no one knew why at that time. This phenomenon seemed unbelievable, incredible and even impossible, but is true!

In order to derive this formula theoretically, Planck proposed a brave hypothesis which is also incredible.

Page 21: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Planck’s Hypotheses:

• The molecules and atoms composing the blackbody concave can be regarded as the linear harmonic oscillator with electrical charge;

• The oscillators can only be in a special energy state. All these energies must be the integer multiples of a smallest energy (ε0 = hν). Therefore the energies of the oscillators are E = n hν with n = 1, 2, 3, …

Page 22: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Using the hypothesis and classical physics, Planck arrived at his experience formula in two months later. The correct result shows that Planck’s hypothesis is correct!

Quantum theory and modern physics was founded by these hypotheses!

Page 23: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

• Planck-Einstein Energy Quantization Law:

hc

hE

Quantum energy

Planck constant

Frequency

seV

sJh

15

34

10136.4

10626.6

eVJ

JeV18

19

10242.61

10602.11

Page 24: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

It is pity that Planck himself did not believe his such a wonderful hypothesis and he spent about ten years to solve the same problem using classical physics, but obviously in vain ( 徒劳的 ). Planck’s case is similar to Newton’s experience as he spent the rest of his life to show the existence of God.

Page 25: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Example: Calculate the photon energies for the following types of electromagnetic radiation: (a) a 600kHz radio wave; (b) the 500nm (wavelength of) green light; (c) a 0.1 nm (wavelength of) X-rays.

Solution: (a) for the radio wave, we can use the Planck-Einstein law directly

eV

HzseVhE9

315

1048.2

1060010136.4

Page 26: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(b) The light wave is specified by wavelength, we can use the law explained in wavelength:

eVm

meVhcE 26.2

10550

10241.19

6

(c). For X-rays, we have

keVeVm

meVhcE 4.121024.1

101.0

10241.1 49

6

Page 27: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Therefore you can see that the higher frequency corresponds to the higher energy. The X-rays have quite high energy, so they have high power of penetration.

Here we emphasize that the particle properties of light and the photon will be defined. As we know the light is electromagnetic waves and it has the properties of waves.

Planck associated the energy quanta only with the light emission in the cavity walls and Einstein extended them to the absorption of radiation in his explanation of the photoelectric effect.

Page 28: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.2 Photoelectric Effect

The quantum nature of light had its origin in the theory of thermal radiation and was strongly reinforced by the discovery of the photoelectric effect.

Page 29: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.2.1 Photoelectric Effect

Fig. 9.4 Apparatus to investigate the photoelectric effect that was first found in 1887 by Hertz.

In figure 9.4, a glass tube contains two electrodes ( 电极 ) of the same material, one of which is irradiated ( 被照射 ) by light. The electrodes are connected to a battery and a sensitive current detector measures the current flow between them.

The current flow is a direct measure of the rate of emission of electrons from the irradiated electrode.

Page 30: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

The electrons in the electrodes can be ejected by light and have a certain amount of kinetic energy.Now we change:

(1) the frequency and intensity of light,

(2) the electromotive force (e.m.f. 电动势 or voltage),

(3) the nature of electrode surface.

It is found that:

Page 31: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(1). For a given electrode material, no photoemission exists at all below a certain frequency of the incident light. When the frequency increases, the emission begins at a certain frequency. The frequency is called threshold frequency of the material. The threshold frequency has to be measured in the existence of e.m.f. (electromotive force) as at such a case the photoelectrons have no kinetic energy to move from the cathode ( 阴极 ) to anode ( 阳极 ). Different electrode material has different threshold frequency.

Page 32: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(2). The rate of electron emission is directly proportional to the intensity of the incident light.

Photoelectric current The intensity of light∝

(3). Increasing the intensity of the incident light does not increase the kinetic energy of the photoelectrons.

Intensity of light kinetic energy of ∝photoelectron

However increasing the frequency of light does increase the kinetic energy of photoelectrons even for very low intensity levels.

Frequency of light kinetic energy of ∝photoelectron

Page 33: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(4). There is no measurable time delay between irradiating the electrode and the emission of photoelectrons, even when the light is of very low intensity. As soon as the electrode is irradiated, photoelectrons are ejected.

(5) The photoelectric current is deeply affected by the nature of the electrodes and chemical contamination of their surface.

Page 34: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

It is found that the second and the fifth conclusions can be explained easily by explained easily by classical theory of physics — classical theory of physics — Maxwell’s electromagnetic theory of Maxwell’s electromagnetic theory of light, but the other three cases conflict light, but the other three cases conflict with any reasonable interpretation of with any reasonable interpretation of the classical theory of physics.the classical theory of physics.

Page 35: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Let’s have a look at the three trouble cases:

(a) The existence of a threshold frequency: Classical theory cannot explain the phenomenon as the light energy does not depend on the frequency of light. Light energies should depend on its intensity and the irradiating time.

(b) In third case, it is unbelievable that the kinetic energies of photoelectrons do not depend on the intensity of incident light as the intensity indicates the light energy!

Page 36: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(c). No time delay in the photoelectric effect

Since the rate of energy supply to the electrode surface is proportional to the intensity of the light, we would expect to find a time delay in photoelectron emission for a very low intensity light beam. The delay would allow the light to deliver adequate energy to the electrode surface to cause the emission. Therefore “the no time delay phenomenon” puzzled us.

Page 37: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

In 1905, Einstein solved the photoelectric effect problem by applying the Planck’s hypothesis. He pointed out that Planck’s quantization hypothesis applied not only to the emission of radiation by a material object but also to its transmission and its absorption by another material object. The light is not only electromagnetic waves but also a quantum. All the effects of photoelectric emission can be readily explained from the following assumptions:

Page 38: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

(1) The photoemission of an electron from a cathode occurs when an electron absorbs a photon of the incident light;

(2) The photon energy is calculated by the Planck’s quantum relationship: E = hν.

(3) The minimum energy is required to release an electron from the surface of the cathode. The minimum energy is the characteristic of the cathode material and the nature of its surface. It is called work function.

Page 39: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

The equation for the photoelectric emission can be written out by supposing the photon energy is completely absorbed by the electron. After this absorption, the kinetic energy of the electron should have the energy of the photon. If this energy is greater than the work function of the material, the electron should become a photoelectron and jumps out of the material and probably have some kinetic energy.

Page 40: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Therefore we have the equation of photoelectric effect:

2

2

1mvAh

Photon energy

Work function

Photoelectron kinetic energy

Using this equation and Einstein’s assumption, you could readily explain all the results in the photoelectric effect: why does threshold frequency exist (problem)? why is the number of photoelectrons proportional to the light intensity? why does high intensity not mean high photoelectron energy (problem)? why is there no time delay (problem)?

Page 41: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Example: Ultraviolet light of wavelength 150nm falls on a chromium electrode. Calculate the maximum kinetic energy and the corresponding velocity of the photoelectrons (the work function of chromium is 4.37eV).

Solution: using the equation of the photoelectric effect, it is convenient to express the energy in electron volts. The photon energy is

eVm

meVhchE 27.8

10150

10241.19

6

and

eVeVmv

mvAh

90.3)37.427.8(2

12

1

2

2

Page 42: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

22191919 10602.110602.110602.11 smkgmNJeV

∴ 22192 10602.190.390.32

1 smkgeVmv

∴ smm

eVv /1017.1

1011.9

10496.1290.32 631

19

Page 43: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.2.2 The mass and momentum of photon

According to relativity, the particles with zero static mass are possibly existent. From the relativistic equation of energy-momentum,

420

222 cmcpE

when m0 = 0, E = pc = mc2 = hν

Page 44: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

∴ the mass of photon is

22 c

h

c

Emp

and the momentum of photon should be

h

c

h

c

Ep

Page 45: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.3 Compton effectA phenomenon called Compton scattering, first observed in 1924 by Compton, provides additional direct confirmation of the quantum nature of electromagnetic radiation. When X-rays impinges ( 冲击 , 撞击 ) on matter, some of the radiation is scattered ( 散射 ), just as the visible light falling on a rough surface undergoes diffuse reflection ( 漫射 ). Observation shows that some of the scattered radiation has smaller frequency and longer wavelength than the incident radiation, and that the change in wavelength depends on the angle through which the radiation is scattered. Specifically, if the scattered radiation emerges at an angle φ with the respect to the incident direction, and if and are the wavelength of the incident and scattered radiation, respectively, it is found that

Page 46: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

··P

, p

, p

2sin2cos1 2

mc

h

mc

h

where m is the electron mass.

Fig. 8.4 Schematic diagram of Compton

scattering.

In figure 8.4, the electron is initially at rest with incident photon of wavelength and momentum p; scattered photon with longer wavelength and momentum p and recoiling (反冲 , 后退 ) electron withmomentum P. The direction of the scattered photon makes an angle φ with that of the incident photon, and the angle between p and p is also φ.

φ

nmmc

hc 00243.0 called Compton

wavelength.

Page 47: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Compton scattering cannot be understood on the basis classical electromagnetic theory. On the basis of classical principles, the scattering mechanism is induced by motion of electrons in the material, caused by the incident radiation. This motion must have the same frequency as that of incident wave because of forced vibration, and so the scattered wave radiated by the oscillating charges should have the same frequency. There is no way the frequency can shifted by this mechanism.

The quantum theory, by contrast, provides a beautifully simple explanation. We imagine the scattering process as a collision of two particles, the incident photon and an electron at rest as shown in Fig. 8.4. The photon gives up some of its energy and momentum to the electron, which recoils as a result of this impact; and the final photon has less energy, smaller frequency and longer wavelength than the initial one. The equation can be derived as in our Chinese text book.

Page 48: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.4 The wave-particle duality of light

The concept that waves carrying energy may have a corpuscular (particle) aspect and that particles may have a wave aspect; which of the two models is the more appropriate will depend

Page 49: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

on the properties the model is seeking to explain. For example, waves of electromagnetic radiation need to be visualized as particles, called photons to explain the photoelectric effect. Now you may confuse the two properties of light and ask what the light actually is?

The fact is that the light shows the property of waves in its interference and diffraction and performances the particle

P

OS0

=d sin = x/L

d

property in blackbody radiation and photoelectric effect. Till now we can only say that the light has duality property.

We can say that light is wave when it is involved in its propagation only like interference and diffraction. This means that light interacts with itself. The light shows photon property when it interact with other materials. Let’s see another example of photon.

Page 50: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.5 Line spectra and Energy quantization in atoms

The quantum hypothesis, used in the preceding section for the analysis of the photoelectric effect, also plays an important role in the understanding of atomic spectra.

9.4.1 Line spectra of Hydrogen atoms

It is found that hydrogen always gives a set of line spectra in the save position, sodium another set, iron still another and so on the line structure of the spectrum extends into both the ultraviolet and infrared regions. It is impossible to explain such a line spectrum phenomenon without using quantum theory. For many years, unsuccessful attempts were made to correlate the observed frequencies with those of a fundamental and its overtones (denoting other lines here). Finally, in 1885, Balmer

Page 51: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

found a simple formula which gave the frequencies of a group lines emitted by atomic hydrogen. Since the spectrum of this element is relatively simple, and fairly typical of a number of others, we shall consider it in more detail.

Under the proper conditions of excitation, atomic hydrogen may be made to emit the sequence of lines illustrated in Fig. 8.5. This sequence is called series.

(nm)

H H H

H H

656.3 486.1

434.1

410.2

364.6

Fig. 8.5 the Balmer series of atomic hydrogen.

There is evidently a certain order in this spectrum, the lines becoming crowded more and more closely together as the limit of the series is approached. The line of

longest wavelength or lowest frequency, in the red, is known as H, the next, in the blue-green, as H, the third as H, and so on.

Page 52: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Balmer found that the wavelength of these lines were given accurately by the simple formula

,1

2

1122

nR

where is the wavelength, R is a constant called the Rydberg constant, and n may have the integral values 3, 4, 5, etc.* if is in meters,

1710097.1 mR

Substituting R and n = 3 into the above formula, one obtains the wavelength of the H-line:

nm3.656For n = 4, one obtains the wavelength of the H-line, etc. for n= , one obtains the limit of the series, at = 364.6nm –shortest wavelength in the series.

(9.4.1)

(9.4.2)

Page 53: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Other series spectra for hydrogen have since been discovered. These are known, after their discoveries, as Lymann, Paschen, Brackett and Pfund series. The formulas for these are

Lymann series: ,4,3,2,1

1

1122

n

nR

Paschen series: ,6,5,4,1

3

1122

n

nR

,6,5,4,1

4

1122

n

nR

Brackett series:

,6,5,4,1

5

1122

n

nR

Pfund series:

(9.4.3)

Page 54: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

The Lymann series is in the ultraviolet, and the Paschen, Brackett, and Pfund series are in the infrared. All these formulas can be generalized into one formula which is called the general Balmer series.

,3,2,1,111

22

kkkn

nkR

All the spectra of atomic hydrogen can be described by this simple formula. As no one can explain this formula, it was ever called Balmer formula puzzle.

9.4.2 Bohr’s atomic theory

Bohr’s was not by any means the first attempt to understand the internal structure of atoms. Starting in 1906, Rutherford and his co-workers had performed experiments on the scattering of alpha

(9.4.4)

Page 55: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

Particles by thin metallic. These experiments showed that each atom contains a massive nucleus whose size is much smaller than overall size of the atom. The nucleus is surrounded by a swarm (一大群 ) of electrons. To account for the fact, Rutherford postulated that the electrons revolve about the nucleus in orbits, more or less as the planets in the solar system revolve around the sun, but with electrical attraction providing the necessary centripetal force.

This assumption, however, has an unfortunate consequence . A body moving in a circle is continuously accelerated toward the center of the circle and, according to classical electromagnetic theory, an accelerated electron radiates energy. The total energy of the electrons would therefore gradually decrease, their orbits would become smaller and smaller, and eventually they would spiral into the nucleus and come to rest. Furthermore, according to classical theory, the frequency of the electromagnetic waves emitted by a revolving electron is equal to the frequency of revolution. Their angular velocities would change continuously

Page 56: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

and they would emit a continuous spectrum (a mixture of frequencies), in contradiction to the line spectrum actually observed.

Faced with the dilemma, Bohr concluded that , in spite of the success of electromagnetic theory in explaining large scale phenomenon, it could not be applied to the processes on an atomic scale. He therefore postulated that an electron in an atom can revolve in certain stable orbits, each having a definite associated energy, without emitting radiation. The momentum mvr of the electron on the stable orbits is supposed to be equal to the integer multiple of h/2π. This condition may be stated as

,3,2,12

nh

nmvr

where n is quantum number, this is the hypothesis of stable state And it is called the quantization condition of orbital angularmomentum.

(9.4.5)

Page 57: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

For the transition hypothesis, Bohr postulated that the radiation happens only at the transition of electron from one stable state to another stable state. The radiation frequency or the energy of the photon is equal to the difference of the energies corresponding to the two stable states.

h

EE

EEh

kn

kn

(9.4.6)

Another equation can be obtained by the electrostatic force of attraction between two charges and Newton’s law:

r

vm

r

e 2

2

2

04

1

(9.4.7)

Solving the simultaneous equation of (8.4.5) and (8.4.7), we have

Page 58: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

),3,2,1(2

,0

22

2

20 n

hn

evn

me

hr nn

So the total energy of the electron on the nth orbit is

220

4

0

22

842

1

nh

me

r

emvEEE

nnpkn

It is easy to see that all the energy in atoms should be discrete not continuous. When the electron transits from nth orbit to kth orbit, the frequency and wavelength can be calculated as

2222320

4

22320

4

1111

8

1

11

8

nkR

nkch

me

c

knnkh

me

h

EE kn

(9.4.8)

(9.4.9)

Page 59: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

where ch

meR

320

4

8 is Rydberg constant. It is found that

the value of R is matched with experimental data very well. Till then, the 30-years puzzle of line spectra of atoms was solved by Bohr since equation (8.4.9) is exactly the general Balmer formula.

When Bohr’s theory met problems in explaining a little bit more complex atoms (He) or molecules (H2), Bohr realized that his theory is full of contradictions as he used both quantum and classical theories. The problem was solved completely after De Broglie proposed that electron also had the wave-particle duality. Since then, the proper theory describing the motion of the micro-particles , quantum mechanics, have been gradually established by many scientists.

Page 60: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.6 De Broglie Wave

9.6.1 De Broglie

In the previous sections we traced the development of the quantum character of electromagnetic waves. Now we will turn to the consequences of the discovery that particles of classical physics also possess a wave nature. The first person to propose this idea was the French scientist Louis De Broglie.

De Broglie’s result came from the study of relativity. He noted that the formula for the photon momentum can also be written in terms of wavelength

h

c

hc

c

hcmP p

2(9.5.1)

Page 61: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

If the relationship is true for massive particles as well as for photons, the view of matter and light would be much more unified.

In certain circumstances each could behave as a wave, and in other instances each could behave as a particles.

De Broglie’s point was the assumption that momentum-wavelength relation is true for both photons and massive particles.

So De Broglie wave equations are

hEmv

h

p

hhP (9.5.2)

Where P is the momentum of particles, λis the wavelength of particles. At first sight, to claim that a particle such as an electron has a wavelength seems somewhat absurd. The classical concept

Page 62: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

of an electron is a point particle of definite mass and charge, but De Broglie argued that the wavelength of the wave associated with an electron might be so small that it had not been previously noticed. If we wish to prove that an electron has a wave nature, we must perform an experiment in which electrons behave as waves.

Electron diffractions

In order to show the wave nature of electrons, we must demonstrate interference and diffraction for beams of electrons. At this point, recall that interference and diffraction of light become noticeable when light travels through slits whose width and separation are comparable with the wavelength of the light. So let us first look at an example to determine the magnitude of the expected wavelength for some representative objects. Therefore, we use de Broglie wavelength for an electron whose kinetic energy is 600 eV is 0.0501nm. The de Broglie wavelength for a golf ball of mass 45g traveling at 40m/s is: 3.68 ×10-34 m. Such a short wave is hardly observed.

Page 63: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

We recall that diffraction of light waves is obvious when the slit width is about the same as or smaller than the wavelength. We must mow consider whether we could observe diffraction of electrons whose wavelength is a small fraction of a nanometer. For a grating to show observable diffraction, the slit separation should be comparable to the wavelength, but we cannot rule a series of lines that are only a small fraction of a nanometer apart, as such a length is less than the separation of the atoms in solid materials.

When electrons pass through a thin gold or other metal foils (箔 ), we can get diffraction patterns. So it indicates the wave nature of electrons. Look at the pictures on page 265 and 231 in your Chinese and English text book respectively.

Introduce: Electron single and double slits experiments; electronic microscope, nuclear reactor etc. (see Ch. book)

Page 64: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

9.7 The Heisenberg Uncertainty principle

Heisenberg proposed a principle that has come to be regarded as basic to the theory of quantum mechanics. It is called "uncertainty principle", and it limits the extent to which we can possess accurate knowledge about certain pairs of dynamical variables.

Both momentum and position are vectors. When dealing with a real three dimensional situation, we take the uncertainties of the components of each vector in the same direction.

Our sample calculation is restricted to the simplest interpretation of what we mean by uncertainty. A more elaborate (详细阐述的 ) statistical interpretation gives the lower

Page 65: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

limit of the uncertainty product as:

Δx Δpx

x

h

x

hppx

sin

Consider other order diffractions, we have:

hpx x But precise derivation is

4h

px x

Page 66: Chapter 9 Introduction to Quantum Mechanics (May. 20, 2005)

We can briefly review how quantum dynamics differs from classical dynamics. Classically, both the momentum and position of a point particle can determined to whatever degree of accuracy that the measuring apparatus permits. However, from the quantum viewpoint, the product of the momentum and position uncertainties must be at least as great as h/4/π.

See the examples in our Ch. Text book on page 266.

Another pair of important uncertainty is the time and energy. It is found by E = p^2/2m + Ep that

hxE From these examples and Heisenberg principle, we know that classical theory is still useful in the macro-cases. However you have to use quantum theory in the micro-world.