Quantum Mechanics
Classical Results, Modern Systems, and
Visualized Examples
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Quantum
Mechanics
Classical Results, Modern
Systems, and Visualized
Examples
Second Edition
Richard W. Robinett
Pennsylvania State University
1
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3
Great Clarendon Street, Oxford OX2 6DP
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British Library Cataloguing in Publication Data
Data available
Library of Congress Cataloging in Publication Data
Robinett, Richard W. (Richard Wallace)
Quantum mechanics : classical results, modern systems, and
visualized examples / Richard W. Robinett.—2nd ed.
p. cm.
ISBN-13: 978–0–19–853097–8 (alk. paper)
ISBN-10: 0–19–853097–8 (alk. paper)
1. Quantum theory. I. Title.
QC174.12.R6 2006
530.12—dc22
2006000424
Typeset by Newgen Imaging Systems (P) Ltd., Chennai, India
Printed in Great Britain
on acid-free paper by
Biddles Ltd, King’s Lynn, Norfolk
ISBN 0–19–853097–8
978–0–19–853097–8
10 9 8 7 6 5 4 3 2 1
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Preface to the Second Edition
One of the hallmarks of science is the continual quest to refine and expand one’s
understanding and vision of the universe, seeking not only new answers to old
questions, but also proactively searching out new avenues of inquiry based on
past experience. In much the same way, teachers of science (including textbook
authors) can and should explore the pedagogy of their disciplines in a scientific
way, maintaining and streamlining what has been documented to work, but also
improving, updating, and expanding their educational materials in response to
new knowledge in their fields, in basic, applied, and educational research. For that
reason, I am very pleased to have been given the opportunity to produce a Second
Edition of this textbook on quantum mechanics at the advanced undergraduate
level.
The First Edition of Quantum Mechanics had a number of novel features,
so it may be useful to first review some aspects of that work, in the context
of this Second Edition. The descriptive subtitle of the text, Classical Results,
Modern Systems, and Visualized Examples, was, and still is, intended to suggest a
number of the inter-related approaches to the teaching and learning of quantum
mechanics which have been adopted here.
• Many of the expected familiar topics and examples (the Classical Results)
found in standard quantum texts are indeed present in both editions, but we
also continue to focus extensively on the classical–quantum connection as one
of the best ways to help students learn the subject. Topics such as momentumspace probability distributions, time-dependent wave packet solutions, and the
correspondence principle limit of large quantum numbers can all help students
use their existing intuition to make contact with new quantum ideas; classical
wave physics continues to be emphasized as well, with its own separate chapter,
for the same reason. Additional examples of quantum wave packet solutions
have been included in this new Edition, as well as a self-contained discussion
of the Wigner quasi-probability (phase-space) distribution, designed to help
make contact with related ideas in statistical mechanics, classical mechanics,
and even quantum optics.
• An even larger number of examples of the application of quantum mechanics to Modern Systems is provided, including discussions of experimental
realizations of quantum phenomena which have only appeared since the First
Edition. Advances in such areas as materials science and laser trapping/cooling
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vi
PREFACE TO THE SECOND EDITION
have meant a large number of quantum systems which have historically been
only considered as “textbook” examples have become physically realizable. For
example, the “quantum bouncer”, once discussed only in pedagogical journals, has been explored experimentally in the Quantum states of neutrons in
the Earth’s gravitational field.É The production of atomic wave packets which
exhibit the classical periodicity of Keplerian orbitsÊ is another example of a
Classical Result which has become a Modern System.
The ability to manipulate nature at the extremes of small distance (nanoand even atomic-level) and low temperatures (as with Bose–Einstein condensates) implies that a knowledge of quantum mechanics is increasingly
important in modern physical science, and a number of new discussions of
applications have been added to both the text and to the Problems, including
ones on such topics as expanding/interfering Bose–Einstein condensates, the
quantum Hall effect, and quantum wave packet revivals, all in the context of
familiar textbook level examples.
• We continue to emphasize the use of Visualized Examples (with 200 figures
included) to reinforce students’ conceptual understanding of the basic ideas
and to enhance their mathematical facility in solving problems. This includes
not only pictorial representations of stationary state wavefunctions and timedependent wave packets, but also real data. The graphical representation of
such information often provides the map of the meeting ground of the sometimes arcane formalism of a theorist, the observations of an experimentalist,
and the rest of the scientific community; the ability to “follow such maps” is
an important part of a physics education.
Motivated in this Edition (even more than before) by results appearing from
Physics Education Research (PER), we still stress concepts which PER studies have indicated can pose difficulties for many students, such as notions of
probability, reading potential energy diagrams, and the time-development of
eigenstates and wave packets.
As with any textbook revision, the opportunity to streamline the presentation
and pedagogy, based on feedback from actual classroom use, is one of the most
important aspects of a new Edition, and I have taken this opportunity to remove
some topics (moving them, however, to an accompanying Web site) and adding
new ones. New sections on The Wigner Quasi-Probability Distribution (and many
related problems), an Infinite Array of δ-functions: Periodic Potentials and the
Dirac Comb, Time-Dependent Perturbation Theory, and Timescales in Bound State
É The title of a paper by V. V. Nesvizhevsky et al. (2002). Nature 415, 297.
Ê See Yeazell et al. (1989).
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PREFACE TO THE SECOND EDITION vii
Systems: Classical Period and Quantum Revival Times reflect suggestions from
various sources on (hopefully) useful new additions. A number of new in-text
Examples and end-of-chapter Problems have been added for similar reasons, as
well as an expanded set of Appendices, on dimensions and mathematical methods.
An exciting new feature of the Second Edition is the development of a Web
siteË in support of the textbook, for use by both students and instructors, linked
from the Oxford University PressÌ web page for this text. Students will find
many additional (extended) homework problems in the form of Worksheets on
both formal and applied topics, such as “slow light”, femtosecond chemistry, and
quantum wave packet revivals. Additional material in the form of Supplementary
Chapters on such topics as neutrino oscillations, quantum Monte Carlo approximation methods, supersymmetry in quantum mechanics, periodic orbit theory
of quantum billiards, and quantum chaos are available.
For instructors, copies of a complete Solutions Manual for the textbook, as
well as Worksheet Solutions, will be provided on a more secure portion of the site,
in addition to copies of the Transparencies for the figures in the text. An 85-page
Guide to the Pedagogical Literature on Quantum Mechanics is also available there,
surveying articles from The American Journal of Physics, The European Journal
of Physics, and The Journal of Chemical Education from their earliest issues,
through the publication date of this text (with periodic updates planned.) In
addition, a quantum mechanics assessment test (the so-called Quantum Mechanics Visualization Instrument or QMVI) is available at the Instructors site, along
with detailed information on its development and sample results from earlier
educational studies. Given my long-term interest in the science, as well as the
pedagogy, of quantum mechanics, I trust that this site will continually grow in
both size and coverage as new and updated materials are added. Information on
accessing the Instructors area of the Web site is available through the publisher
at the Oxford University Press Web site describing this text.
I am very grateful to all those from whom I have had help in learning quantum
mechanics over the years, including faculty and fellow students in my undergraduate, graduate, and postdoctoral days, current faculty colleagues (here at
Penn State and elsewhere), my own undergraduate students over the years, and
numerous authors of textbooks and both research and pedagogical articles, many
of whom I have never met, but to whom I owe much. I would like to thank all
those who helped very directly in the production of the Second Edition of this
text, specifically including those who provided useful suggestions for improvement or who found corrections, namely, J. Banavar, A. Bernacchi, B. Chasan,
Ë See robinett.phys.psu.edu/qm
Ì See www.oup.co.uk
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viii
PREFACE TO THE SECOND EDITION
J. Edmonds, M. Cole, C. Patton, and J. Yeazell. I have truly enjoyed recent collaborations with both M. Belloni and M. A. Doncheski on pedagogical issues
related to quantum theory, and some of our recent work has found its way into
the Second Edition (including the cover) and I thank them for their insights, and
patience.
No work done in a professional context can be separated from one’s personal
life (nor should it be) and so I want to thank my family for all of their help
and understanding over my entire career, including during the production of
this new Edition. The First Edition of this text was thoroughly proof-read by my
mother-in-law (Nancy Malone) who graciously tried to teach me the proper use
of the English language; her recent passing has saddened us all. My own mother
(Betty Robinett) has been, and continues to be, the single most important role
model in my life—both personal and professional—and I am deeply indebted
to her far more than I can ever convey. Finally, to my wife (Sarah) and children
(James and Katherine), I give thanks everyday for the richness and joy they bring
to my life.
Richard Robinett
December, 2005
State College, PA
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Contents
Part I The Quantum Paradigm
1
2
A First Look at Quantum Physics
3
1.1
How this Book Approaches Quantum Mechanics
3
1.2
Essential Relativity
1.3
Quantum Physics:
1.4
Semiclassical Model of the Hydrogen Atom
17
1.5
Dimensional Analysis
21
1.6
Questions and Problems
23
8
as a Fundamental Constant
10
Classical Waves
34
2.1
The Classical Wave Equation
34
2.2
Wave Packets and Periodic Solutions
36
2.2.1
General Wave Packet Solutions
36
2.2.2
Fourier Series
38
2.3
Fourier Transforms
43
2.4
Inverting the Fourier transform: the Dirac δ-function
46
2.5
Dispersion and Tunneling
51
2.5.1
Velocities for Wave Packets
51
2.5.2
Dispersion
53
2.5.3
Tunneling
56
2.6
3
1
Questions and Problems
57
The Schrödinger Wave Equation
65
3.1
The Schrödinger Equation
65
3.2
Plane Waves and Wave Packet Solutions
67
3.2.1
Plane Waves and Wave Packets
67
3.2.2
The Gaussian Wave Packet
70
3.3
“Bouncing” Wave Packets
75
3.4
Numerical Calculation of Wave Packets
77
3.5
Questions and Problems
79
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CONTENTS
4
Interpreting the Schrödinger Equation
84
4.1
84
Introduction to Probability
4.1.1
Discrete Probability Distributions
84
4.1.2
Continuous Probability Distributions
87
4.2
Probability Interpretation of the Schrödinger Wavefunction
91
4.3
Average Values
96
4.3.1
Average Values of Position
96
4.3.2
Average Values of Momentum
4.3.3
Average Values of Other Operators
4.4
Real Average Values and Hermitian Operators
102
4.5
The Physical Interpretation of φ(p)
104
4.6
Energy Eigenstates, Stationary States, and the Hamiltonian Operator
107
4.7
The Schrödinger Equation in Momentum Space
111
4.7.1
Transforming the Schrödinger Equation Into Momentum
Space
4.7.2
4.8
5
111
Uniformly Accelerating Particle
Commutators
114
116
4.9
The Wigner Quasi-Probability Distribution
118
4.10
Questions and Problems
121
The Infinite Well: Physical Aspects
5.1
5.2
134
The Infinite Well in Classical Mechanics: Classical Probability
Distributions
134
Stationary States for the Infinite Well
137
5.2.1
137
5.2.2
Position-Space Wavefunctions for the Standard Infinite Well
Expectation Values and Momentum-Space Wavefunctions for
the Standard Infinite Well
5.2.3
The Symmetric Infinite Well
140
144
5.3
The Asymmetric Infinite Well
146
5.4
Time-Dependence of General Solutions
151
5.4.1
Two-State Systems
151
5.4.2
Wave Packets in the Infinite Well
154
5.4.3
Wave Packets Versus Stationary States
157
5.5
6
98
100
Questions and Problems
157
The Infinite Well: Formal Aspects
166
6.1
Dirac Bracket Notation
166
6.2
Eigenvalues of Hermitian Operators
167
6.3
Orthogonality of Energy Eigenfunctions
168
6.4
Expansions in Eigenstates
171
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CONTENTS xi
7
6.5
Expansion Postulate and Time-Dependence
175
6.6
Parity
181
6.7
Simultaneous Eigenfunctions
183
6.8
Questions and Problems
185
Many Particles in the Infinite Well: The Role of Spin and
Indistinguishability
192
7.1
The Exclusion Principle
192
7.2
One-Dimensional Systems
193
7.3
Three-Dimensional Infinite Well
195
7.4
Applications
198
7.4.1
Conduction Electrons in a Metal
198
7.4.2
Neutrons and Protons in Atomic Nuclei
200
7.4.3
White Dwarf and Neutron Stars
200
7.5
8
Questions and Problems
Other One-Dimensional Potentials
210
8.1
210
8.2
Singular Potentials
8.1.1
Continuity of ψ (x)
210
8.1.2
Single δ-function Potential
212
8.1.3
Twin δ-function Potential
213
8.1.4
Infinite Array of δ-functions: Periodic Potentials and the Dirac
Comb
216
The Finite Well
221
8.2.1
Formal Solutions
221
8.2.2
Physical Implications and the Large x Behavior of
Wavefunctions
8.3
8.4
9
206
Applications to Three-Dimensional Problems
225
230
8.3.1
The Schrödinger Equation in Three Dimensions
230
8.3.2
Model of the Deuteron
231
Questions and Problems
234
The Harmonic Oscillator
239
9.1
The Importance of the Simple Harmonic Oscillator
239
9.2
Solutions for the SHO
243
9.2.1
Differential Equation Approach
243
9.2.2
Properties of the Solutions
247
9.3
Experimental Realizations of the SHO
249
9.4
Classical Limits and Probability Distributions
251
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CONTENTS
9.5
Unstable Equilibrium: Classical and Quantum Distributions
254
9.6
Questions and Problems
255
10 Alternative Methods of Solution and Approximation
Methods
260
10.1
Numerical Integration
261
10.2
The Variational or Rayleigh–Ritz Method
266
10.3
The WKB method
273
10.3.1 WKB Wavefunctions
274
10.3.2 WKB Quantized Energy Levels
277
10.4
Matrix Methods
278
10.5
Perturbation Theory
286
10.5.1 Nondegenerate States
286
10.5.2 Degenerate Perturbation Theory
293
10.5.3 Time-Dependent Perturbation Theory
295
Questions and Problems
299
10.6
11 Scattering
11.1
307
Scattering in One-Dimensional Systems
307
11.1.1 Bound and Unbound States
307
11.1.2 Plane Wave Solutions
310
11.2
Scattering from a Step Potential
310
11.3
Scattering from the Finite Square Well
315
11.3.1 Attractive Well
315
11.4
11.5
11.3.2 Repulsive Barrier
319
Applications of Quantum Tunneling
321
11.4.1 Field Emission
321
11.4.2 Scanning Tunneling Microscopy
324
11.4.3 α-Particle Decay of Nuclei
325
11.4.4 Nuclear Fusion Reactions
328
Questions and Problems
330
12 More Formal Topics
333
12.1
Hermitian Operators
333
12.2
Quantum Mechanics, Linear Algebra, and Vector Spaces
337
12.3
Commutators
341
12.4
Uncertainty Principles
343
12.5
Time-Dependence and Conservation Laws in Quantum Mechanics
346
12.6
Propagators
352
12.6.1 General Case and Free Particles
352
12.6.2 Propagator and Wave Packets for the Harmonic Oscillator
353
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CONTENTS xiii
12.7
12.8
Timescales in Bound State Systems: Classical Period and Quantum
Revival Times
357
Questions and Problems
360
13 Operator and Factorization Methods for the Schrödinger
370
Equation
13.1
Factorization Methods
370
13.2
Factorization of the Harmonic Oscillator
371
13.3
Creation and Annihilation Operators
377
13.4
Questions and Problems
380
14 Multiparticle Systems
384
14.1
Generalities
384
14.2
Separable Systems
387
14.3
Two-Body Systems
389
14.3.1 Classical Systems
390
14.3.2 Quantum Case
391
14.4
Spin Wavefunctions
394
14.5
Indistinguishable Particles
396
14.6
Questions and Problems
407
Part II The Quantum World
413
15 Two-Dimensional Quantum Mechanics
15.1
15.2
15.3
15.4
415
2D Cartesian Systems
417
15.1.1 2D Infinite Well
418
15.1.2 2D Harmonic Oscillator
422
Central Forces and Angular Momentum
423
15.2.1 Classical Case
423
15.2.2 Quantum Angular Momentum in 2D
425
Quantum Systems with Circular Symmetry
429
15.3.1 Free Particle
429
15.3.2 Circular Infinite Well
432
15.3.3 Isotropic Harmonic Oscillator
435
Questions and Problems
437
16 The Schrödinger Equation in Three Dimensions
448
16.1
Spherical Coordinates and Angular Momentum
449
16.2
Eigenfunctions of Angular Momentum
454
16.2.1 Methods of Derivation
454
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xiv
CONTENTS
16.3
16.2.2 Visualization and Applications
463
16.2.3 Classical Limit of Rotational Motion
465
Diatomic Molecules
467
16.3.1 Rigid Rotators
467
16.3.2 Molecular Energy Levels
469
16.3.3 Selection Rules
472
16.4
Spin and Angular Momentum
475
16.5
Addition of Angular Momentum
482
16.6
Free Particle in Spherical Coordinates
491
16.7
Questions and Problems
492
17 The Hydrogen Atom
501
17.1
Hydrogen Atom Wavefunctions and Energies
501
17.2
The Classical Limit of the Quantum Kepler Problem
507
17.3
Other “Hydrogenic” Atoms
513
17.3.1 Rydberg Atoms
513
17.3.2 Muonic Atoms
515
Multielectron Atoms
517
17.4.1 Helium-Like Atoms
519
17.4.2 Lithium-Like Atoms
524
17.4.3 The Periodic Table
527
Questions and Problems
529
17.4
17.5
18 Gravity and Electromagnetism in Quantum Mechanics
540
18.1
Classical Gravity and Quantum Mechanics
540
18.2
Electromagnetic Fields
543
18.2.1 Classical Electric and Magnetic Fields
543
18.2.2 E and B Fields in Quantum Mechanics
548
18.3
Constant Electric Fields
550
18.4
Atoms in Electric Fields: The Stark Effect
552
18.4.1 Classical Case
552
18.4.2 Quantum Stark Effect
555
18.5
Constant Magnetic Fields
561
18.6
Atoms in Magnetic Fields
564
18.6.1 The Zeeman Effect: External B Fields
564
18.6.2 Spin-Orbit Splittings: Internal B Fields
569
18.6.3 Hyperfine Splittings: Magnetic Dipole–Dipole Interactions
574
Spins in Magnetic Fields
576
18.7.1 Measuring the Spinor Nature of the Neutron Wavefunction
576
18.7.2 Spin Resonance
578
18.7
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CONTENTS xv
18.8
The Aharonov–Bohm Effect
583
18.9
Questions and Problems
586
19 Scattering in Three Dimensions
Classical Trajectories and Cross-Sections
597
19.2
Quantum Scattering
603
19.2.1 Cross-Section and Flux
603
19.2.2 Wave Equation for Scattering and the Born Approximation
606
19.3
Electromagnetic Scattering
612
19.4
Partial Wave Expansions
619
19.5
Scattering of Particles
624
19.5.1 Frames of Reference
625
19.6
A
C
D
E
19.5.2 Identical Particle Effects
631
Questions and Problems
635
Dimensions and MKS-type Units for Mechanics, Electricity
641
and Magnetism, and Thermal Physics
A.1
B
596
19.1
Problems
642
Physical Constants, Gaussian Integrals, and the Greek
Alphabet
644
B.1
Physical Constants
644
B.2
The Greek Alphabet
646
B.3
Gaussian Probability Distribution
646
B.4
Problems
648
Complex Numbers and Functions
649
C.1
651
Problems
Integrals, Summations, and Calculus Results
653
D.1
Integrals
653
D.2
Summations and Series Expansions
658
D.3
Assorted Calculus Results
661
D.4
Real Integrals by Contour Integration
661
D.5
Plotting
664
D.6
Problems
665
Special Functions
666
E.1
Trigonometric and Exponential Functions
666
E.2
Airy Functions
667
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xvi
F
G
CONTENTS
E.3
Hermite Polynomials
668
E.4
Cylindrical Bessel Functions
669
E.5
Spherical Bessel Functions
669
E.6
Legendre Polynomials
669
E.7
Generalized Laguerre Polynomials
670
E.8
The Dirac δ-Function
671
E.9
The Euler Gamma Function
672
E.10
Problems
672
Vectors, Matrices, and Group Theory
674
F.1
Vectors and Matrices
674
F.2
Group Theory
679
F.3
Problems
679
Hamiltonian Formulation of Classical Mechanics
680
G.1
685
Problems
REFERENCES
687
INDEX
695
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PART I
The Quantum Paradigm
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ONE
A First Look at Quantum
Physics
1.1 How This Book Approaches Quantum
Mechanics
It can easily be argued that a fully mature and complete knowledge of quantum
mechanics should include historical, axiomatic, formal mathematical, and even
philosophical background to the subject. However, for a student approaching
quantum theory for the first time in a serious way, it can be the case that an
approach utilizing his or her existing knowledge of, and intuition for, classical
physics (including mechanics, wave physics, and electricity and magnetism) as
well as emphasizing connections to experimental results can be the most productive. That, at least, is the point of view adopted in this text and can be
illustrated by a focus on the following general topics:
(1) The incorporation of a wave property description of matter into a consistent
wave equation, via the Schrödinger equation;
(2) The statistical interpretation of the Schrödinger wavefunction in terms of
a probability density (in both position- and momentum-space);
(3) The study of single-particle solutions of the Schrödinger equation, for both
time-independent energy eigenstates as well as time-dependent systems, for
many model systems, in a variety of spatial dimensions, and finally;
(4) The influence of both quantum mechanical effects and the constraints
arising from the indistinguishability of particles (and how that depends
on their spin) on the properties of multiparticle systems, and the resulting
implications for the structure of different forms of matter.
By way of example of our approach, we first note that Fig. 1.1 illustrates
an example of a precision measurement of the wave properties of ultracold
neutrons, exhibiting a Fresnel diffraction pattern arising from scattering from
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4
CHAPTER 1 A FIRST LOOK AT QUANTUM PHYSICS
1500
1000
500
100 µm
Scanning slit position
Figure 1.1. Fresnel diffraction pattern obtained from scattering at a sharp edge, obtained using ultracold
neutrons by Gähler and Zeilinger (1991).
a sharp edge, nicely explained by classical optical analogies. We devote Chapter 2
to a discussion of classical wave physics and Chapter 3 to the description of
such wave effects for material particles, via the Schrödinger equation. Figure 1.2
demonstrates an interference pattern using electron beams, built up “electron by
electron,” with the obvious fringes resulting only from a large number of individual measurements. The important statistical aspect of quantum mechanics,
simply illustrated by this experiment, is discussed in Chapter 4 and beyond.
It can be argued that much of the early success of quantum theory can be traced
to the fact that many exactly soluble quantum models are surprisingly coincident with naturally occurring physical systems, such as the hydrogen atom and
the rotational/vibrational states of molecules and such systems are, of course,
discussed here. The standing wave patterns obtained from scanning tunneling microscopy of “electron waves” in a circular corral geometry constructed
from arrays of iron atoms on a copper surface, seen in Fig. 1.3, reminds us of
the continuing progress in such areas as materials science and atom trapping
in developing artificial systems (and devices) for which quantum mechanics
is applicable. In that context, many exemplary quantum mechanical models,
which have historically been considered as only textbook idealizations, have also
recently found experimental realizations. Examples include “designer” potential
wells approximating square and parabolic shapes made using molecular beam
techniques, as well as magnetic or optical traps. The solution of the Schrödinger
equation, in a wide variety of standard (and not-so-standard) one-, two-, and
three-dimensional applications, is therefore emphasized here, in Chapters 5, 8, 9,
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1.1 HOW THIS BOOK APPROACHES QUANTUM MECHANICS 5
Figure 1.2. Interference patterns obtained by using an electron microscope showing the fringes being
“built up” from an increasingly large number of measurements of individual events. From Merli, Missiroli,
and Pozzi (1976). (Photo reproduced by permission of the American Institute of Physics.)
and 15–17. In parallel to these examples, more formal aspects of quantum theory
are outlined in Chapters 7, 10, 12, 13, and 14.
The quantum in quantum mechanics is often associated with the discrete
energy levels observed in bound-state systems, most famously for atomic systems
such as the hydrogen atom, which we discuss in Chapter 17, emphasizing that this
is the quantum version of the classical Kepler problem. We also show, in Fig. 1.4,
experimental measurements leading to a map of the momentum-space probability density for the 1S state of hydrogen and the emphasis on momentum-space
methods suggested by this result is stressed throughout the text. The influence of
additional“real-life”effects, such as gravity and electromagnetism, on atomic and
other systems are then discussed in Chapter 18. We note that the data in Fig. 1.4
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6
CHAPTER 1 A FIRST LOOK AT QUANTUM PHYSICS
Figure 1.3. Standing wave patterns obtained using scanning tunneling microscopy from a circular “corral”
of radius ∼70 Å, constructed from 48 iron atoms on a copper surface. (Photo courtesy of IBM Almaden.)
Differential cross section
1.0
H(1s)
1200 eV
0.8
800 eV
400 eV
0.6
(1+q2)–4
0.4
0.2
0
0.2
0.4
0.5
0.8
1.0
Momentum q (a.u.)
1.2
1.4
Figure 1.4. Electron probability density obtained by scattering with three different energy probes, compared
with the theoretically calculated momentum-space probability density for the hydrogen-atom ground state,
from Lohmann and Weigold (1981). The data are plotted again the scaled momentum in atomic units (a.u.),
q = a0 p/ .
was obtained via scattering processes, and the importance of scattering methods
in quantum mechanics is emphasized in both one-dimension (Chapter 11) and
three-dimensions (Chapter 19). The fact that spin-1/2 particles must satisfy the
Pauli principle has profound implications for the way that matter can arrange
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Rn
Xe
Kr
Ar
Ne
He
1.1 HOW THIS BOOK APPROACHES QUANTUM MECHANICS 7
30
40
20
20
10
0
0
10
20
30
40
50
60
70
80
90
Polarizability (10–24 cm3) (dashed)
Ionizational potential (eV) (solid)
60
0
100
Nuclear charge (Z)
Figure 1.5. Plots of the ionization energy (solid) and atomic polarizability (dashed) versus nuclear charge,
showing the shell structure characterized by the noble gas atoms, arising from the filling of atomic energy
levels as mandated by the Pauli principle for spin-1/2 electrons.
itself, as shown in the highly correlated values of physical parameters shown in
Fig. 1.5 for atoms of increasing size and complexity. While it is illustrated here in
a numerical way, this should also be reminiscent of the familiar periodic table of
the elements, and the Pauli principle has similar implications for nuclear structure. We discuss the role of spin in multiparticle systems described by quantum
mechanics in Chapters 7, 14, and 17.
We remind the reader that similar dramatic manifestations of quantum phenomena (including all of the effects mentioned above) are still being discovered,
as illustrated in Fig. 1.6. In a justly famous experiment,É two highly localized
and well-separated samples of sodium atoms are cooled to sufficiently low temperatures so that they are in the ground states of their respective potential wells
(produced by laser trapping.) The trapping potential is removed and the resulting coherent Bose–Einstein condensates are allowed to expand and overlap,
exhibiting the quantum interference shown in Fig. 1.6 (the solid curve, showing
É From the paper entitled Observation of interference between two Bose condensates by Andrews et al.
(1997).
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8
CHAPTER 1 A FIRST LOOK AT QUANTUM PHYSICS
Absorpition (%)
60
30
0
200
0
400
Position (µm)
Figure 1.6. Data (from Andrews et al. (1997)) illustrating the interference of two Bose condensates as
they expand and overlap (solid curve), compared to a single expanding Bose condensate (dotted curve).
regular absorption variations across the central overlap region), while no such
interference is observed for a single expanding quantum sample (dotted data.)
Many of the salient features of this experiment can be understood using relatively
simple ideas outlined in Chapters 3, 4, and 9.
The ability to use the concepts and mathematical techniques of quantum
mechanics to confront the wide array of experimental realizations that have
come to characterize modern physical science will be one of the focuses of this
text. Before proceeding, however, we reserve the remainder of this chapter for
brief reviews of some of the essential aspects of both relativity and standard
results from quantum theory.
1.2 Essential Relativity
While we will consider nonrelativistic quantum mechanics almost exclusively,
it is useful to briefly review some of the rudiments of special relativity and the
fundamental role played by the speed of light, c.
For a free particle of rest mass m moving at speed v, the total energy (E),
momentum (p), and kinetic energy (T ) can be written in the relativistically
correct forms
E = γ mc 2 ,
p = γ mv,
and
T ≡ E − mc 2 = (γ − 1)mc 2
1
= 1−
(1.1)
where
γ ≡
1 − v 2 /c 2
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v2
c2
−1/2
(1.2)