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Lectures on quantum mechanics / Jean-Louis Basdevant.

Math/Physics/Astronomy Library QC174.12 .B374 2007
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Format:
Book
Author/Creator:
Basdevant, J. L. (Jean-Louis)
Language:
English
Subjects (All):
Quantum theory.
Physical Description:
xvi, 307 pages : illustrations ; 24 cm
Place of Publication:
New York : Springer, . 2007.
Summary:
Beautifully illustrated and engagingly written, Lectures on Quantum Mechanics presents theoretical physics with a breathtaking array of examples and anecdotes. Basdevant's style is clear and stimulating, in the manner of a brisk classroom lecture that students can follow with ease and enjoyment. Here is a sample of the book's style, from the opening of Chapter 1: "If one were to ask a passer-by to quote a great formula of physics, chances are that the answer would be 'E = mc[superscript 2]'. Nevertheless, the formula 'E = hv' which was written in the same year 1905 by the same Albert Einstein, and which started quantum theory, concerns their daily life considerably more. In fact, of the three watershed years for physics toward the beginning of the 20th century-1905: the Special Relativity of Einstein, Lorentz and Poincare; 1915: the General Relativity of Einstein, with its extraordinary reflections on gravitation, space and time; and 1925: the full development of Quantum Mechanics-it is surely the last which has the most profound implications for the development of science and technology. There is no way around it: all physics is quantum, from elementary particles, to stellar physics and the Big Bang, not to mention semiconductors and solar cells."
Contents:
1 Praise of physics 1
1.1 The interplay of the eye and the mind 1
1.2 Advanced technologies 5
1.3 The pillars of contemporary physics 6
1.3.1 Mysteries of light 6
1.3.2 Fundamental structure of matter 8
1.4 The infinitely complex 9
1.5 The Universe 12
2 A quantum phenomenon 13
2.1 Wave behavior of particles 16
2.1.1 Interferences 16
2.1.2 Wave behavior of matter 17
2.1.3 Analysis of the phenomenon 18
2.2 Probabilistic nature of quantum phenomena 20
2.2.1 Random behavior of particles 20
2.2.2 A nonclassical probabilistic phenomenon 20
2.4 Phenomenological description 23
3 Wave function, Schrodinger equation 25
3.1 Terminology and methodology 25
3.1.2 Methodology 26
3.2 Principles of wave mechanics 27
3.2.1 The interference experiment 27
3.2.2 Wave function 27
3.2.3 Schrodinger equation 29
3.3 Superposition principle 30
3.4 Wave packets 31
3.4.1 Free wave packets 31
3.4.2 Fourier transformation 32
3.4.3 Shape of wave packets 33
3.5 Historical landmarks 33
3.6 Momentum probability law 35
3.6.1 Free particle 35
3.6.2 General case 36
3.7 Heisenberg uncertainty relations 36
3.7.1 Size and energy of a quantum system 37
3.7.2 Stability of matter 38
3.8 Controversies and paradoxes 40
3.8.1 The 1927 Solvay Congress 40
3.8.2 The EPR paradox 41
3.8.3 Hidden variables, Bell's inequalities 41
3.8.4 The experimental test 42
4 Physical quantities 45
4.1 Statement of the problem 46
4.1.1 Physical quantities 46
4.1.2 Position and momentum 47
4.2 Observables 48
4.2.1 Position observable 49
4.2.2 Momentum observable 49
4.2.3 Correspondence principle 50
4.2.4 Historical landmarks 50
4.3 A counterexample of Einstein and its consequences 51
4.3.1 What do we know after a measurement? 53
4.3.2 Eigenstates and eigenvalues of an observable 54
4.3.3 Wave packet reduction 55
4.4 The specific role of energy 56
4.4.1 The Hamiltonian 56
4.4.2 The Schrodinger equation, time and energy 57
4.4.3 Stationary states 58
4.4.4 Motion: Interference of stationary states 59
4.5 Schrodinger's cat 60
4.5.1 The dreadful idea 60
4.5.2 The classical world 63
5 Energy quantization 65
5.1 Methodology 65
5.1.1 Bound states and scattering states 66
5.1.2 One-dimensional problems 67
5.2 The harmonic oscillator 67
5.2.1 Harmonic potential 67
5.2.2 Energy levels, eigenfunctions 68
5.3 Square well potentials 69
5.3.1 Square potentials 69
5.3.2 Symmetric square well 70
5.3.3 Infinite well, particle in a box 73
5.4 Double well, the ammonia molecule 74
5.4.1 The model 74
5.4.2 Stationary states, the tunnel effect 75
5.4.3 Energy levels 76
5.4.4 Wave functions 78
5.4.5 Inversion of the molecule 79
5.5 Illustrations and applications of the tunnel effect 81
5.5.1 Sensitivity to the parameters 81
5.5.2 Molecular structure 82
5.6 Tunneling microscopy, nanotechnologies 84
5.6.1 Nanotechnologies 84
5.6.2 Classical limit 85
6 Principles of quantum mechanics 87
6.1 Hilbert space 88
6.1.1 Two-dimensional space 89
6.1.2 Square integrable functions 89
6.2 Dirac formalism 92
6.2.1 Notations 92
6.2.2 Operators 93
6.2.3 Syntax rules 95
6.2.4 Projectors; decomposition of the identity 95
6.3 Measurement results 96
6.3.1 Eigenvectors and eigenvalues of an observable 96
6.3.2 Results of the measurement of a physical quantity 97
6.3.3 Probabilities 98
6.3.4 The Riesz spectral theorem 98
6.3.5 Physical meaning of various representations 100
6.4 Principles of quantum mechanics 101
6.4.1 The principles 101
6.4.2 The case of a continuous spectrum 102
6.4.3 Interest of this synthetic formulation 102
6.5 Heisenberg's matrices 103
6.5.1 Matrix representation of operators 103
6.5.2 Matrices X and P 104
6.5.3 Heisenberg's thoughts 104
6.6 The polarization of light, quantum "logic" 107
7 Two-state systems 113
7.1 The NH[subscript 3] molecule 113
7.2 "Two-state" system 114
7.3 Matrix quantum mechanics 116
7.3.1 Vectors 116
7.3.2 Hamiltonian 117
7.3.3 Observables 117
7.3.5 Basis of classical configurations 119
7.3.6 Interference and measurement 120
7.4 NH[subscript 3] in an electric field 120
7.4.1 Uniform constant field 121
7.4.2 Weak and strong field regimes 122
7.4.3 Other two-state systems 123
7.5 The ammonia molecule in an inhomogeneous field 123
7.5.1 Force on the molecule in an inhomogeneous field 124
7.5.2 Population inversion 126
7.6 Reaction to an oscillating field, the maser 126
7.7 Principle and applications of the maser 128
7.7.1 Amplifiers 129
7.7.2 Oscillators 130
7.7.3 Atomic clocks 130
7.7.4 Tests of relativity 132
7.8 Neutrino oscillations 134
7.8.1 Lepton families 134
7.8.2 Mechanism of the oscillations; reactor neutrinos 135
7.8.3 Successive hermaphroditism of neutrinos 138
8 Algebra of observables 143
8.1 Commutation of observables 143
8.1.1 Fundamental commutation relation 143
8.1.2 Other commutation relations 144
8.1.3 Dirac in the summer of 1925 145
8.2 Uncertainty relations 146
8.3 Evolution of physical quantities 147
8.3.1 Evolution of an expectation value 147
8.3.2 Particle in a potential, classical limit 148
8.3.3 Conservation laws 149
8.4 Algebraic resolution of the harmonic oscillator 150
8.4.1 Operators a, a, and N 151
8.4.2 Determination of the eigenvalues 151
8.4.3 Eigenstates 152
8.5 Commuting observables 154
8.5.1 Theorem 154
8.5.3 Tensor structure of quantum mechanics 155
8.5.4 Complete set of commuting observables (CSCO) 156
8.5.5 Completely prepared quantum state 157
8.6 Sunday, September 20, 1925 158
9 Angular momentum 161
9.1 Fundamental commutation relation 162
9.1.1 Classical angular momentum 162
9.1.2 Definition of an angular momentum observable 162
9.1.3 Results of the quantization 163
9.2 Proof of the quantization 163
9.2.1 Statement of the problem 163
9.2.2 Vectors |j, m > and eigenvalues j and m 164
9.2.3 Operators J[Characters not reproducible] = J[subscript x Characters not reproducible] iJ[subscript y] 165
9.2.4 Quantization 166
9.3 Orbital angular momenta 168
9.3.1 Formulae in spherical coordinates 168
9.3.2 Integer values of m and l 168
9.3.3 Spherical harmonics 169
9.4 Rotation energy of a diatomic molecule 170
9.4.1 Diatomic molecule 171
9.4.2 The CO molecule 172
9.5 Angular momentum and magnetic moment 173
9.5.1 Classical model 173
9.5.2 Quantum transposition 175
9.5.3 Experimental consequences 175
9.5.4 Larmor precession 176
9.5.5 What about half-integer values of j and m? 177
10 The Hydrogen Atom 179
10.1 Two-body problem; relative motion 180
10.2 Motion in a central potential 182
10.2.1 Spherical coordinates, CSCO 182
10.2.2 Eigenfunctions common to H, L[superscript 2], and L[subscript z] 182
10.2.3 Quantum numbers 183
10.3 The hydrogen atom 186
10.3.1 Atomic units; fine structure constant 186
10.3.2 The dimensionless radial equation 188
10.3.3 Spectrum of hydrogen 191
10.3.4 Stationary states of the hydrogen atom 191
10.3.5 Dimensions and orders of magnitude 193
10.3.6 Historical landmarks 194
10.4 Muonic atoms 195
11 Spin 1/2 199
11.1 Experimental results 199
11.2 Spin 1/2 formalism 200
11.2.1 Representation in a particular basis 201
11.2.2 Matrix representation 201
11.3 Complete description of a spin 1/2 particle 202
11.3.1 Observables 203
11.4 Physical spin effects 204
11.5 Spin magnetic moment 205
11.5.1 Hamiltonian of a one-electron atom 205
11.6 The Stern-Gerlach experiment 206
11.6.1 Principle of the experiment 206
11.6.2 Semi-classical analysis 207
11.6.3 Experimental results 208
11.6.4 Explanation of the Stern-Gerlach experiment 208
11.6.5 Successive Stern-Gerlach setups 211
11.6.6 Measurement along an arbitrary axis 211
11.7 The discovery of spin 213
11.7.1 The hidden sides of the Stern-Gerlach experiment 213
11.7.2 Einstein and Ehrenfest's objections 215
11.7.3 Anomalous Zeeman effect 216
11.7.4 Bohr's challenge to Pauli 217
11.7.5 The spin hypothesis 217
11.7.6 The fine structure of atomic lines 218
11.8 Magnetism, magnetic resonance 219
11.8.1 Spin effects, Larmor precession 220
11.8.2 Larmor precession in a fixed magnetic field 221
11.8.3 Rabi's calculation and experiment 221
11.8.4 Nuclear magnetic resonance 225
11.8.5 Magnetic moments of elementary particles 227
11.9 Entertainment: Rotation by 2[pi] of a spin 1/2 228
12 The Pauli Principle 229
12.1 Indistinguishability of two identical particles 230
12.1.1 Identical particles in classical physics 230
12.1.2 The quantum problem 230
12.1.3 Example of ambiguities 231
12.2 Systems of two spin 1/2 particles, total spin 232
12.2.1 The Hilbert space of the problem 232
12.2.2 Hilbert space of spin variables 232
12.2.3 Matrix representation 233
12.2.4 Total spin states 233
12.3 Two-particle system; the exchange operator 235
12.3.1 The Hilbert space for the two-particle system 235
12.3.2 The exchange operator between identical particles 236
12.3.3 Symmetry of the states 237
12.4 The Pauli principle 238
12.4.1 The case of two particles 238
12.4.2 Independent fermions and exclusion principle 239
12.4.3 The case of N identical particles 239
12.5 Physical consequences of the Pauli principle 241
12.5.1 Exchange force between two fermions 241
12.5.2 The ground state of N identical independent particles 241
12.5.3 Behavior of fermion and boson systems at low temperatures 243
13 Entangled states: The way of paradoxes 247
13.1 The EPR paradox 247
13.2 The version of David Bohm 249
13.2.1 Bell's inequality 251
13.2.2 Experimental tests 254
13.3 Quantum cryptography; how to enjoy a nuisance 256
13.3.1 The communication between Alice and Bob 256
13.3.2 Present experimental setups 258
13.4 Quantum teleportation 260
13.4.1 Bell states 260
13.4.2 Teleportation 261
14 Quantum mechanics in the Universe 263
14.1 Quantum mechanics and astronomy 265
14.1.1 Life and death of stars 265
14.1.2 Spectroscopy 268
14.2 Radioastronomy, the interstellar medium 268
14.2.1 The interstellar medium 269
14.3 Cosmic background radiation: Birth of the Universe 273
14.4 The 21-cm line of hydrogen 275
14.4.1 Hyperfine structure of hydrogen 276
14.4.2 Hydrogen maser 278
14.4.3 Importance of the 21-cm line 279
14.5 The Milky Way 280
14.6 The intergalactic medium; star wars 281
14.6.1 Spiral arms, birthplaces of stars 285
14.7 Interstellar molecules, the origin of life 287
14.7.1 Rotation spectra of molecules 287
14.7.2 Interstellar molecules 288
14.7.3 The origin of life 289
14.8 Where are they? Quantum mechanics, the universal cosmic language 291
14.8.1 Life, intelligence, and thought 291
14.8.2 Listening to extraterrestrials 293
14.8.3 Quantum mechanics, the universal cosmic language 295.
Notes:
Includes bibliographical references and index.
ISBN:
0387377425
9780387377421
0387377441
9780387377445
OCLC:
123410782

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