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    Fundamentals

    Page 20
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      It is standard practice for experimenters to report how many quarks and gluons are produced in the reactions they study, how they are distributed in energy and angle, and so forth. What they’ve actually observed is the corresponding jets, but the identification, after thousands of successful applications, has become routine. Quarks and gluons entered the world as weird, suspect theoretical phantoms—confined particles that, according to theory, would never be observed in isolation. Tamed by beautiful ideas, they’ve become tangible realities— not mere particles, but jets.

      GEOMETRY OF SPACE AND DENSITY OF MATTER

      General relativity predicts a striking relationship between the average curvature of space, the average density of matter within it, and the rate of expansion of the universe. If the total density of matter is equal to a certain critical density, then space will be flat; if the density is larger, it will be positively curved, like a sphere; if the density is smaller, it will be negatively curved, like a saddle.

      At present, the critical density is about 10−29 grams per cubic centimeter. This is equivalent to the mass of about six hydrogen atoms per cubic meter. Though this critical density is far below the density of the best “ultra-high vacuum” people have achieved in laboratories on Earth, it seems that it is close to the average density of the universe as a whole.

      Astronomers can measure the shape of space geometrically, using sophisticated versions of the procedures we indicated in chapter 1. They can also measure the density, by adding up contributions from ordinary matter, dark matter, and dark energy. They find that space is very nearly flat, and that the density is very nearly the critical density. This is consistent with the prediction of general relativity. That consistency encourages us to think that the dark matter and dark energy mysteries can be understood within the framework of general relativity. Certainly, they do not require its modification.

      ABCDEFGHIJKLMNOPQRSTUVWXYZ

      Index

      The page numbers in this index refer to the printed version of this book. The link provided will take you to the beginning of that print page. You may need to scroll forward from that location to find the corresponding reference on your e-reader.

      abundance, xiv–xv, 13–15

      See also energy abundance; material abundance; spatial abundance; time

      acceleration, 16, 115, 116

      excess, explaining, 193–96

      Adams, John Couch, 194

      afterglows

      of the big bang, 152, 154–55, 157–59, 163, 200, 202

      of neutron star mergers, 182

      See also dark matter

      AHUMEN (Annual Human Energy), 127

      Allegory of the Cave, 168–69

      Almagest (Ptolemy), 6

      AlphaZero, 204

      analysis and synthesis method, 8

      angular momentum, 74, 75–76

      animals, perception in, 169–70, 171

      Annual Human Energy (AHUMEN), 127

      antineutrinos, 48, 118, 119, 151

      antiquarks, 114, 151

      anyons, 89–90

      Arovas, Dan, 89

      art, visual, 217

      artificial intelligence, 54, 58, 59, 70–71, 204, 220–22

      See also information flows and processing

      astronomy and cosmology, 128

      abundance and uniformity of matter in the cosmos, 21–22, 38, 149–51, 156, 161–62

      astronomical observation, 5–6, 21, 22

      astronomical timekeeping, 45

      cosmic horizon, 28–31

      Ptolemy’s synthesis, 6–7

      Ramsey on astronomy, 42

      and spectroscopy, 109

      surveying the cosmos, 21–28

      See also big bang theory; galaxies; planets; stars; universe; entries beginning with “cosmic”

      asymptotic freedom, 112, 123–24, 149, 203, 238, 239

      ATLAS detector, 176

      atomic clocks, 17, 18–19, 55–56, 68–69

      atomic nuclei

      components and properties of, 62, 79, 84, 85, 105, 109–10

      original formation of, 155, 163

      and weak force processes, 119

      See also QCD

      atomic spectra, 106–9

      atoms

      atomic models and complementarity, 214–15

      as building blocks of complexity, 130–32

      structure of, 35–37, 62, 78–79, 83, 103, 105–6

      viewed as basic building blocks, 61–62, 72, 96

      See also atomic nuclei

      Augustine, Saint, 44, 159, 219

      axions, 122, 159, 166, 201–2

      babies. See infant development

      Barish, Barry, 180

      bats, 170

      bees, 171

      big bang theory, 29, 146, 148–55

      afterglows of the big bang, 152, 154–55, 157–59, 163, 200, 202

      assumptions and principles of, 148–52, 163

      and dark matter/dark energy, 199–201

      evidence for, 29, 152–55, 157

      potential recreation of the big bang, 166

      when the big bang occurred, 30, 37, 47, 157

      black holes, 149–50, 180, 182

      Blake, William, xviii, 169

      Bohr, Niels, 108, 207–8, 210, 211, 212

      bonus particles, 77, 119, 191, 236–37

      Borges, Jorge Luis, 166, 167

      bosons, 174, 234–35

      Brahe, Tycho, 7

      brain processes, speeds and complexity of, 52–54, 58–60, 134–35, 138

      See also human cognition; perception

      carbon dating, 48–51

      cellular biology and processes, 90–91

      Cepheid variables, 27

      change

      fundamental laws as descriptions of, 63, 65, 122–25

      and time, 46–47

      change, particles of, 77, 234–36

      charge, 73, 74, 77, 233–34

      of atoms, 79

      of specific particle types, 78, 81, 85, 235, 237

      See also color charge; electric charge

      chemistry and chemical processes

      cellular biology and processes, 90–91

      chemistry of material that emerged from the big bang, 155

      femtochemistry and the speed of biochemical processes, 52, 54, 56–57, 59

      and the fundamental laws, 120–21

      imaging through x-ray diffraction patterns, 33–34

      molecular complexity, 130–35

      and radioactive dating, 48, 50

      and spectroscopy, 109

      See also atoms; molecules and molecular processes

      chess, 204, 220

      chi, 114

      classical mechanics, 8

      the dark matter problem, 194–96

      as framework for later investigations, 94–96, 193–94

      and GPS, 18, 19

      Newtonian theory of gravity, 66–67, 94, 95, 114–15, 116, 117

      See also motion; planetary motion and arrangements

      Clay Foundation, 204

      climate change, 140–41

      clocks, 17, 18–19, 44, 47, 55–56, 68–69

      CMB. See cosmic microwave background

      cognitive processes, 52–54, 58–60

      color charge, 84, 122–23, 234

      of specific particle types, 78, 84, 85, 235, 237

      color vision, 170–71

      combinatorial explosion, 131–32

      commutation relations. See quantum conditions

      complementarity, 206–22

      basic principles of, 206, 218–19

      between human comprehensibility and accurate understanding, 220–21

      between humility and self-respect, 221–22

      and levels of description, 213–16


      as mind expanding, 206–7, 218–19

      in music and art, 216–17

      quantum complementarity, 208–13

      in science, 207–16

      complexity, 160–67

      dynamic complexity, 129–36

      factors in the emergence of, 161–66

      within simplicity, 160, 166–67, 189

      computer games, 70–71

      computer processes. See artificial intelligence; information flows and processing

      construction, particles of, 77, 78–86

      See also electrons; gluons; gravitons; photons; quarks

      Copernicus, Nicolaus, 6

      Core concept, 121–25

      cosmic background radiation, 152, 154–55, 157, 162, 163, 200–201

      cosmic distances, 42, 43

      cosmic horizon, 28–31, 37–38

      measuring, 23–28, 30–31, 198–99

      cosmic energy abundance, 126–28

      See also energy abundance

      cosmic history, 145–59

      and the cosmic horizon, 37–38

      future investigations of, 156–59

      inflation concept, 156–57, 162, 189

      role of dark matter and dark energy, 199–200

      scope and limits of, 146–48

      See also big bang theory

      cosmic microwave background (CMB), 154–55, 157, 162, 163, 200–201

      cosmic rays, 236

      cosmic strings, 166

      cosmological constant (Einstein), 195, 197–98, 200

      cosmology. See astronomy and cosmology; big bang theory; universe; entries beginning with “cosmic”

      Coulomb’s law, 95, 105

      Crick, Francis, 34, 225–26

      Cronin, James, 190–91

      Cubists, 217

      Cummings, Ray, 44

      dark energy, 188, 193, 195–96, 197–201

      dark matter, 158–59, 166, 188, 193–97, 199–201, 237, 241

      decay processes

      and atomic spectra, 107

      neutron decay, 118–19, 135

      proton decay, 123, 166

      radioactive dating, 47–51

      Democritus, 72–73, 77

      dendrochronology, 50

      digital photography, 138

      digital processes. See artificial intelligence; information flows and processing

      Dirac, Paul, 100, 119–20, 122, 184

      disequilibrium. See instability/disequilibrium

      distances and distance measurement

      cosmic horizon, 28–31, 37–38

      distance and the strengths of the fundamental forces, 112, 123–24

      measuring cosmic distances, 23–28, 30–31, 198–99

      quantum distance fluctuations, 40

      subatomic and interatomic distances, 33, 39–40, 56

      and time, 20, 30

      See also asymptotic freedom; size and scale

      DNA and DNA sequences, 34, 131–32

      dogs, 169

      Doppler effect, 28

      Dragon’s Egg (Forward), 59

      dynamic complexity, 129–36

      and combinatorial explosion, 131–32

      examples of, 129–30

      of human brain processes, 134–35, 138

      nonchemical platforms for, 137–39

      and provisional stability, 132–34

      solar energy as fuel for, 127–28, 133–34, 135–36, 163

      Dyson spheres, 127, 165

      Earth

      age of, 50–51, 52

      and the cosmic distance ladder, 23–24, 25

      size of, 23, 24

      surface temperature of, 133–34, 140–41

      economic growth. See human activities and purposes

      Einstein, Albert, 44, 210

      Bohr-Einstein debates, 212

      on Bohr’s work, 108, 208

      on human exceptionalism, 226–27, 228

      light-quanta hypothesis, 82–83, 99, 100–101, 107

      on scientific understanding, xii

      on simplicity, 148

      and unified field theory, 123–24

      views on complementarity, 211–12

      See also general relativity; special relativity

      electric charge, 84, 95, 233–34

      of atomic nuclei, 79

      of holes, 87–88

      of specific particle types, 78, 81–82, 84, 85, 112, 235, 237

      electric force and field, 95, 99–100, 105

      electromagnetic force and field, 84, 95–102, 103, 233

      Maxwell’s equations, 97–98, 99–100, 178, 189, 234

      and time reversal, 189

      See also QED

      electromagnetic waves, 178–79

      electrons

      and atomic structure, 62, 78–79, 83, 105–7, 108–9

      behavior and properties of, 75, 78–82, 84, 101–2

      in digital processes, 54, 59, 138–39

      as products of decay processes, 48, 49, 118, 119

      and quasiparticles, 87, 89

      elementary particles

      axions, 122, 159, 166, 201–2

      basic influences of the fundamental forces on, 103–4, 121–22

      bonus particles, 77, 119, 191, 236–37

      dark matter constituents, 200, 201–2

      designer particles and smart materials, 87–92

      Higgs particle, 57, 175–78, 234–35, 236

      particles of change, 77, 234–36

      particles of construction, 77, 78–86

      properties of, 72–76, 77, 231–34

      See also specific particle types

      Eliot, T. S., 53–54

      emergent properties, 214–15

      empathy, and scientific understanding, 227–28

      End of Science, 216

      energy

      dark energy, 188, 193, 195–96, 197–201

      and the existence of fields, 97

      human energy use and sources, 126–27, 140–41, 165–66

      and inertia and gravity, 117, 232

      latent energy, 113, 166

      and mass, 85, 113–14, 115, 117, 231, 232

      powering of stars, 113, 135–36, 163, 165, 166, 235

      related properties of quasiparticles, 90

      energy abundance, xiv, 126–30, 136, 165–66

      energy loss, 111, 113, 135–36

      equilibrium/disequilibrium

      gravitational instability, 149–51, 156, 161–62, 164, 189

      thermal equilibrium, 151, 163

      See also provisional stability

      Euclid, 39

      Euclidean geometry, 15–21, 39, 40

      geometry of space, 38, 151, 156–57, 240–41

      space-time as geometric object, 116, 151, 156

      Faraday, Michael, xiii, 95–96, 97, 98–99, 178

      femtochemistry, 56–57, 59

      Feynman, Richard, xiv, 61–62, 184

      fields, 67, 95–102

      nineteenth-century work on, 95–99, 105, 178

      quantum fields, 99–102

      See also specific field types

      Fitch, Val, 190–91, 203

      forces. See fundamental forces; specific forces

      Forward, Robert, 59

      fossil fuels, 140

      FQHE (fractional quantum Hall effect), 89

      Franklin, Benjamin, 81–82

      Franklin, Rosalind, 34

      free will, 217, 218

      Freund, Peter, 75–76

      fundamental forces, 102, 103–5, 120–21

      Core concept and unified field theory, 121–25

      and dynamic complexity, 136

      See also specific forces

      fundamental laws

      and co
    mplementarity, 213–14, 216

      Core concept, 121–25

      envisioning universes in which they do not hold, 70–72

      as foundation of practical physics, 119–22

      vs. human laws, 93–94

      locality principle, 63–64, 65, 66–67, 68–69, 96, 102, 191

      Newton’s work, 8, 66–67

      principles of, 63–66

      spectroscopy’s confirmation of, 109

      and time reversal, 148–49, 188–92

      universality of, 21, 38–39, 63, 65

      See also classical mechanics; specific laws

      fundamental properties of matter, 72–77, 86, 231–34

      See also charge; mass; spin

      galaxies

      galactic motion as evidence of the universe’s expansion, 28–31, 145–46, 149–50, 153–54, 165

      gravitational lensing of light from, 196–97

      properties and distribution of, 22, 27, 30, 150, 196

      Galilei, Galileo, xiii, 7, 8, 55

      Galois, Évariste, 52

      gamma rays, 83, 98, 182

      Gauss, Carl Friedrich, 16, 21

      GDP, 3

      Geiger, Hans, 35–37, 56

      Gell-Mann, Murray, 111

      general laws. See fundamental laws

      general relativity, 20, 57, 86, 195

      basic principles of, 115–17

      and the character of space, 39–40, 57, 116–17, 240–41

      cosmological constant, 195, 197–98, 200

      and gravitational lensing, 197

      and Mercury’s motion, 195

      See also gravitational waves; gravity

      genetic engineering, 222

      geometry. See Euclidean geometry

      Global Positioning System (GPS), 16–19

      gluons, 62, 121, 151

      behavior and properties of, 78, 83–84, 85, 114, 238, 239

      and color charge, 84, 234

      jets as avatars of, 238–40

      Go, 220

      GPS (Global Positioning System), 16–19

      gravitational wave detectors, 21

      gravitational waves, 178–82

      gravitons, 85–86, 157–58

      gravity, 114–17

      and complexity, 136, 161–62

      as fundamental force, 103

      gravitational instability, 149–51, 156, 161–62, 164, 189

      gravitational lensing, 196–97

      Newtonian theory of, 66–67, 94, 95, 114–15, 116, 117

      and the origins of the universe, 149–51, 152, 153, 156, 200

     


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