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Acknowledgments | p. xi |
Prelude: The Mystery of the Missing Antimatter | p. 1 |
Constant Physics in an Evolving Universe | p. 7 |
Universal Laws | p. 7 |
Hubble and the Expanding Universe | p. 8 |
Red-shifts: Evidence for an Expanding Universe | p. 12 |
Numbers Large and Small | p. 17 |
What Do We Mean by "Universe"? | p. 19 |
As the Universe Expands | p. 21 |
Running the Clock Forward: Radiation | p. 21 |
Running the Clock Forward: Dark Matter | p. 26 |
Running the Clock Forward: Light Nuclei | p. 29 |
Running the Clock Forward: Matter and Antimatter | p. 32 |
What Is Antimatter? | p. 36 |
What Is Matter? | p. 36 |
Dirac Introduces Antimatter | p. 42 |
Experiments Confirm That Antimatter Exists | p. 45 |
Radioactive Decays of Nuclei | p. 48 |
Enter Neutrinos | p. 51 |
Pauli: The Beta Decay Puzzle | p. 51 |
Fermi: The Theory of Neutrinos Develops | p. 53 |
Cowan and Reines: Neutrinos Detected | p. 55 |
Mesons | p. 57 |
Yukawa and the Pi-Meson | p. 57 |
Strange Mesons, Strange Quantum Concepts | p. 61 |
Through the Looking Glass | p. 63 |
What Physicists Mean by the Term Symmetry | p. 63 |
A Gedanken Experiment | p. 64 |
The Actual Experiment | p. 67 |
Through the Looking Antiglass | p. 73 |
Another Gedanken Experiment | p. 73 |
Cronin and Fitch: Matter and Antimatter Do Not Follow the Same Laws | p. 75 |
The Survival of Matter | p. 80 |
Pauli's Other Letter: Initial Conditions on the Universe | p. 80 |
Sakharov: The Conditions Needed to Develop an Imbalance | p. 84 |
Cosmology with Sakharov's Conditions Met: Baryogenesis | p. 88 |
Enter Quarks | p. 91 |
Quarks | p. 91 |
Why Don't We See the Quarks? | p. 96 |
What about Dark Matter? | p. 100 |
The Missing Charm, the Surprising Tau | p. 101 |
The Standard Model: Particles and Interactions | p. 107 |
Energy Rules | p. 111 |
Stored Energy, Forces, and Energy Conservation | p. 111 |
Force Fields Permeating Space | p. 114 |
Field Theory and the Energy Function | p. 116 |
Symmetry Rules | p. 121 |
Symmetries as Answers to the Question "Why?" | p. 121 |
Symmetries and Conservation Laws | p. 123 |
Space-Time Symmetries | p. 124 |
Gauge Symmetries | p. 126 |
Discrete Symmetries | p. 128 |
Baryon and Lepton Number Conservation? | p. 130 |
Standard Model Gauge Symmetries | p. 132 |
The Symmetry behind the Electromagnetic Interaction | p. 132 |
The Symmetry behind the Strong Interaction | p. 134 |
The Symmetry behind the Weak Interaction | p. 137 |
A Missing Piece | p. 140 |
The Puzzle of Particle Masses | p. 140 |
How Do We Describe Nothing? | p. 146 |
At Last, CP Violated in the Standard Model | p. 153 |
It Still Doesn't Work! | p. 159 |
Running the Clock Forward: The Standard Model | p. 159 |
Now What? | p. 163 |
Tools of the Trade | p. 168 |
Accelerators | p. 168 |
Detectors | p. 172 |
Data Handling and Analysis | p. 177 |
How Projects Develop | p. 178 |
Searching for Clues | p. 180 |
Where Are We Now? | p. 180 |
Testing the Standard Model in B-Meson Decays | p. 182 |
Oddone: How to Build B Factories? | p. 184 |
Running the B Factories: The First Test | p. 190 |
Speculations | p. 194 |
Why Are We Never Satisfied? | p. 194 |
Grand Unified Theories | p. 195 |
Supersymmetry | p. 201 |
Way beyond the Standard Model | p. 204 |
Neutrino Surprises | p. 206 |
Davis, Bahcall, Koshiba: Solar Neutrinos | p. 206 |
Quantum Neutrino Properties | p. 214 |
Following the New Clues | p. 222 |
Some Things We Know | p. 222 |
Some Things We Speculate About | p. 225 |
Fitting It All Together | p. 227 |
Finale | p. 231 |
Appendix: A Timeline of Particle Physics and Cosmology | p. 233 |
Perspective | p. 233 |
Relevant Nineteenth-Century Developments | p. 234 |
1900-1930: Development of Quantum Ideas, Beginnings of Scientific Cosmology | p. 238 |
1930-1950: New Particles, New Ideas | p. 245 |
1930-1960s: The Advent of Accelerator Experiments--The Particle Explosion; Implications of Expanding Universe Explored | p. 249 |
1964-1973: Formulation of the Modern View of Particles and the Universe | p. 256 |
Two Standard Models Emerge--Particles and Cosmology | p. 263 |
Index | p. 273 |
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