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    Quantum Man: Richard Feynman's Life in Science

    Page 30
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      New York Times, 292–93

      New York Times Magazine, 287

      Nobel Committee, 170–71, 230–31

      Nobel Prize, xii, xiv, 19, 31–32, 39, 41, 74, 84, 94, 106, 124, 125, 143, 156, 159, 170–71, 186, 190, 202, 209, 218, 219–20, 222–23, 229–32, 235, 241, 265, 268, 270, 271–72, 293, 300, 305, 307, 310

      nodes, 54

      Noether, Emmy, 199–200

      Noether’s theorem, 199–200, 204

      nonzero energy, 174

      nonzero probabilities, 52, 55, 72

      nonzero spin, 120

      North Pole, 203–4

      nuclear democracy, 291–92, 305–6

      nuclear physics, 20, 46–47, 67–68, 72, 74, 76–95, 108, 122, 163–64, 178, 194, 239, 273–74, 283

      nuclei, atomic, 84, 107, 294

      nucleons, 178–79

      numbers:

      atomic, 66

      complex, 116

      as integers, 100, 175, 178–79, 291

      negative, 97, 103

      prime, 284, 285–86

      quantum, 200–201

      number theory, 9

      Oak Ridge Laboratory, 90

      Occhialini, Giuseppe, 106–7

      Oersted, Hans Christian, 28

      Olum, Paul, 68

      omega-minus particle, 290, 292, 293

      Onnes, Kamerlingh, 170–72, 174, 263

      Onsager, Lars, 186, 190–92

      Oppenheimer, J. Robert, 78–80, 90–91, 92, 105–6, 122, 148, 149, 154, 155, 156, 241

      orbital gravitation, 203–4

      O-ring failure, xv, 309

      Osheroff, Douglas, 227

      parallel processors, 276–77, 283

      parity flips, 212

      parity nonconservation, 204–5, 206, 207–8, 210–17

      particle accelerators, 154, 169, 200, 292–300, 305, 312

      particles, subatomic, 4–5, 28–35, 38, 39–42, 113–14, 120–21, 133–40, 166, 173–79, 193–94, 197–98, 200–202, 205–6, 208–11, 220, 263–64, 287–309, 315–16

      decay of, 104–5, 193–94, 200–201, 205–6, 207, 208, 210, 211–15

      paths of, 14–17, 48–50, 52–58, 65, 69–70, 73–74, 97, 99, 100–104, 107, 117–18, 126–28, 145–46, 153, 154, 176, 178–79, 185, 193–94, 210–12, 256–57, 309–10

      strange, 196, 200–201, 202, 205–6, 273, 291–92, 305

      see also specific particles

      partons, 295–96, 298, 299–300

      Pasteur, Louis, 296

      path-integral formalism, xiii, 73, 210–12, 255–57, 283–84, 309–10

      pattern recognition, 277–78

      Pauli, Wolfgang, 39–40, 100–101, 105–6, 110–11, 139–40, 209

      Pauli exclusion principle, 100–101, 105–6

      phase transitions, 116–17, 190–92

      phenomenological model, 180–82

      philosophy, 71, 276

      photons, 28–32, 114, 130–31, 134, 137, 201–2, 246–47, 249, 260, 301–2, 303

      Physical Review, 20, 98, 152–53, 200–201, 290, 292

      physical signatures, 240

      physics:

      astro-, 20, 82–85, 106–7, 239, 240, 255–61

      classical, 24, 27–28, 30–31, 37–38, 47, 48, 52–53, 56, 58, 62, 63, 71, 72–73, 100, 131, 142, 173, 224–25, 238, 239, 243, 245–46, 265, 278–81, 282

      of dense materials, 172–79, 181–82, 183, 190–91

      experimental, 19–20, 25–26, 30, 35, 38, 41, 66, 67–68, 81, 85–86, 168–69, 171–72, 193–96, 208, 209, 235–38, 245, 283, 293–300, 312–13

      formalism in, 49–50, 59–65, 73, 97, 99, 117–18, 126–28, 130–46, 150–54, 158, 176, 178–79, 185, 196, 210–12, 214–16, 219, 256–57, 299–300, 309–10

      kluges used in, 198, 210, 215–16, 301, 310

      laws of, 13–14, 30–32, 192, 193, 199–200, 209–10, 223–24, 241–42, 252, 255–57, 269–72, 278–81, 282, 293, 310–13

      nuclear, 20, 46–47, 67–68, 72, 74, 76–95, 108, 122, 163–64, 178, 194, 239, 273–74, 283

      paradox and inconsistency in, 23, 30–32, 34–35, 36, 70, 71–73, 75, 88

      particle, see particles, subatomic

      theoretical, 39–42, 66, 68–69, 73–75, 85–86, 110–11, 118–19, 141–42, 168–69, 193–97, 208, 234–38, 263–64, 283, 286, 287–305, 311–13

      unitary approaches in, 145, 178–79

      see also quantum mechanics

      Physics Letters, 290

      Physics of Star Trek, The (Krauss), 265

      pions, 205, 210, 212–13

      Planck’s constant, 26–27, 63

      plutonium, 84, 86

      Pocono conference (1948), 144–46, 157

      point particles, 100–102

      Politzer, David, 306–7, 312

      polyhedra, 289

      polymers, 271

      Popov, Victor, 304

      positive energy, 102–3, 114, 174

      positive probabilities, 53–54

      positrons, 106–7, 110–11, 113–14, 131–40, 144–46, 197–98

      potential energy, 15–16, 49–50, 257–59, 309–13

      predictions, 71–72, 102–3, 118, 128–29, 138–40, 150–54, 158–59, 201–2, 246, 252–54

      prime factorization, 285–86

      prime numbers, 284, 285–86

      “primeval atom” model, 240

      Princeton University, 22–23, 30–32, 36–50, 59–65, 66, 67–68, 74, 77, 79, 81, 96, 164

      “Principle of Least Action in Quantum Mechanics, The” (Feynman), 74, 97–98

      probability, 41, 48, 52, 53, 54–58, 62–64, 69–70, 72, 97, 99, 116–17, 145–46, 183, 278–79, 280, 283–84

      probability amplitudes, 54–58, 62–64, 69–70, 99, 116–17

      probability waves, 183

      processors, computer, 276–77

      Progress in Theoretical Physics, 148–49

      proportionality, 60–61

      protons, 66, 100, 103, 104–5, 173, 178–79, 207, 291, 294–95, 297–98, 300, 302, 305, 312

      pseudoscalar (P) interaction, 212

      psychology, 14, 16, 59, 65

      Putnam score, 21–22

      Pythagorean theorem, 9

      quanta, 28

      quantized resistance, 271

      quantum bits (qubits), 283–85

      quantum chromodynamics (QCD), 305–9

      quantum electrodynamics (QED), 97–159, 169–232

      absolute zero in, 170, 174–75, 185–86

      absorption theory in, 28–32, 38, 69, 110–20 (span), 114, 121, 126, 130–31

      altered-loop configurations in, 137–39

      amplitude weight in, 63–64

      anti-electrons in, 105–7

      APS meeting on (1948), 143–44, 157

      atomic structure in, 171–79, 181–82

      axial vector (A) interaction in, 212–16, 292

      beta decay in, 194, 208, 210, 213–15

      Bethe’s finite calculations on, 122–23, 125–26, 129, 139–40, 148, 154

      Bohr’s contributions to, 61–62, 100, 112, 119–20, 145–46, 173, 186–87

      Bose-Einstein condensation in, 175–76, 180, 189

      bosons in, 102, 175, 176, 182, 184

      classical electromagnetism compared with, 47, 48, 49, 52–53, 56, 58, 62, 63, 69, 71, 72–73, 100, 131, 142, 173, 224–25, 243

      collapsed systems in, 71–72

      conference on (1947), 122–23, 124, 143

      conservation in, 199–200, 204–5, 209–10, 215–16

      Dirac’s contributions to, 59–65, 97, 102, 103–7, 108, 110–12, 114–16, 118–19, 120, 121, 124, 131, 138, 157, 158, 192, 210, 2
    11, 231

      dynamic evolution of, 23–35, 38–42, 47–75, 154–59

      Dyson’s contributions to, 148–54

      electromagnetic fields in, 48–50, 52–53, 197–98, 245–46

      electron activity in, 24–25, 54–58, 97, 100–107, 111, 113–14, 126, 127, 128–40, 137, 143–44, 154–56, 157, 173–74, 181–82, 186–88, 190, 197–98, 208–10, 212–13

      electron-positron (particle-antiparticle) pairs in, 113–14, 133–40, 137, 197–98

      energy states in, 49–50, 102–6, 113, 125, 126, 151, 170–74, 177, 181–88, 189

      experimental data on, 69, 70–73, 106–7, 118–30, 138–39, 148–59, 169, 173, 180–81, 185–86, 207–17, 222–23

      “Feynman rules” in, 153, 304

      Feynman’s contributions to, 58, 59–65, 66, 68–75, 86, 97–107, 108, 113, 115–18, 120, 121–22, 124–59, 161, 163, 164, 169–210, 229–32, 238, 246, 288–89, 300, 304, 305

      Feynman space-time diagrams for, 107, 129–40, 132, 133, 134, 135, 137, 144–46, 148–54, 169, 173, 193

      finite calculations in, 138–40, 150–51, 158–59, 246

      formalism in approach to, 49–50, 59–65, 73, 97, 99, 117–18, 126–28, 130–46, 150–54, 158, 176, 178–79, 185, 196, 210–12, 214–16, 219, 256–57, 299–300, 309–10

      free particles in, 176–78

      frequency shifts in, 119–23, 124, 126

      gaseous states in, 170–76

      Gell-Mann’s contributions to, 195–208, 212, 214–17, 218, 288–89

      ground state configuration in, 183–84, 185, 186, 189

      Hamiltonian approach to, 158

      Heisenberg’s contributions to, 26–30, 65, 105–6, 111, 112, 115–16, 133, 182

      helium properties in, 101, 170–76, 178, 180, 182, 184, 186, 189–90, 288, 294–95

      hydrogen properties in, 81, 84–85, 119–23, 126, 174, 201–2

      infinite higher-order corrections in, 118, 121–22, 124–29, 131, 139–40, 150–51, 154, 158–59, 197, 231, 302

      “integrating out” process in, 73–74, 110, 127–28

      interference patterns in, 25–26, 54–55, 71, 174, 175

      irrationality of, 51–58

      irrotational states in, 186–87, 289

      kinetic vs. potential energy in, 49–50

      K-mesons (Kaons) in, 205–6, 207, 210

      Kosterlitz-Thouless transition in, 191–92

      K-zero particles in, 201–2

      Lagrangian formalism in, 59–65, 97, 117–18, 157

      Lamb shift in, 119–23, 124, 125, 128, 129, 139, 140, 148

      Landau’s contributions to, 181–82, 184, 187–88, 190

      least action principle in, 14–17, 49–50, 56–57, 62, 69, 73–75, 97–98, 126–27

      least time principle in, 11–14, 18, 57–58

      lowest-order predictions in, 128–29, 150–54, 246

      for low temperature states, 170–74, 181–85, 187–88

      macro-vs. microscopic levels of, 40–41, 71, 171–79, 180, 181–82

      magnetic field lines in, 190–91

      magnetic moment of electrons in, 128–29, 143–44

      mass-energy conversion in, 102, 103–6, 113, 125, 126, 151, 177

      mathematical analysis of, 48, 49, 69, 74–75, 86, 112, 122–23, 125–26, 129–30, 131, 138–40, 145, 148–59, 169, 185–86, 188, 199–200, 211–12, 246

      measurement theory in, 70–73

      mesons in, 154–55, 169, 178, 193, 200, 205–6, 207, 210

      negative energy in, 102–3

      neutrinos in, 154–56, 194, 210–11, 213, 214–16, 219–20, 222–23

      neutron-electron interactions in, 154–56

      neutrons in, 86, 100, 154–56, 194, 201, 210, 213

      Noether’s theorem for, 199–200, 204

      nonrelativistic approach to, 122–23, 125–26

      nucleons in, 178–79

      observer problem in, 71–73

      odd vs. even (left-right or weak-strong) parities in, 204–5, 206, 207–8, 210–17

      orbital angular momentum in, 186–88, 190

      parity flips in, 212

      particle decay in, 104–5, 193–94, 200–201, 205–6, 207, 208, 210, 211–15

      particle paths in, 48–50, 52–58, 65, 69–70, 73–74, 97, 99, 100–104, 107, 117–18, 126–28, 145–46, 153, 154, 176, 178–79, 185, 193–94, 210–12, 256–57, 309–10

      path-integral formalism in, 73, 210–12, 309–10

      Pauli exclusion principle in, 100–101, 145–46

      phase transitions in, 116–17, 190–92

      phenomenological model for, 180–82

      photons in, 28–32, 114, 130–31, 134, 137, 201–2, 246, 301

      pions in, 205, 210, 212–13

      point particles in, 100–102

      polarities in, 128–29, 143–44, 203–4, 207–8, 212

      positrons in (anti-particles), 106–7, 110–11, 113–14, 131–32, 144–46

      predictions of reality based on, 71–72, 102–3, 118, 128–29, 138–40, 150–54, 158–59, 201–2, 246

      probabilities in, 48, 52, 53, 54–58, 62–64, 69–70, 97, 99, 116–17, 145–46, 183

      probability amplitudes in, 54–58, 62–64, 69–70, 99, 116–17

      proportionality in, 60–61

      protons in, 66, 100, 103, 104–5, 173, 178–79, 207

      pseudoscalar (P) interaction in, 212

      quantum coherence in, 180, 285

      quantum number in, 200–201

      quantum state in, 65, 100–104, 183–84, 186–87, 188

      quantum theory compared with, 180, 200–201, 243, 246–47, 249, 280, 285, 288–89, 300, 301, 302–3, 312

      relativity theory and, 69, 97, 99–100, 102, 110–12, 114, 117, 118, 119, 122–23, 125–26, 130, 131, 148, 159, 246–47, 249

      renormalization in, 125, 138–39, 150–51, 197–98, 231

      rest mass in, 125, 126, 151

      scalar (S) interaction in, 212, 213, 215

      Schrödinger equation for, 19, 51–52, 63, 65, 69, 97, 119–20, 121, 158, 161, 173, 188

      Schwinger’s contributions to, 122, 123, 125, 128–29, 141–45, 149, 152, 158–59, 229–30, 231, 304

      “sea of negative-energy” electrons (“Dirac sea”) in, 104–7, 114, 126, 127, 131, 157

      self-energy in, 23–24, 30, 41–42, 111–12, 115–23, 124, 136–39, 137, 150–51, 159

      speed of light in, 133

      spin as factor in, 24–25, 100–102, 116, 120–21, 128–29, 174–75, 186–88, 190, 209, 210–11

      strong vs. weak interactions in, 194, 201, 204–17, 219, 222–23

      “sum over paths” approach in, 65, 73–74, 97, 99, 117–18, 126–28, 145–46, 153, 176, 178–79, 185, 256–57

      superconductivity in, 170–72, 179, 188–89, 190, 271

      superfluidity in, 171–92

      symmetries in, 198–200, 202–11, 215–16, 302–3

      system states in, 48

      tensor (T) interaction in, 212, 213, 215

      test wave functions in, 188–89

      theory of, xii, 23–35, 38–42, 47–75, 154–59

      time direction in, xii, 34–35, 38–42, 47–48, 107, 129–40, 144–46, 148–54, 169, 173, 193

      Tomonaga’s contributions to, 148–49, 152, 229–30, 231, 304

      two-component neutrino formalism in, 215–16

      two-dimensional systems in, 192

      “two fluid” model in, 185–86

      V-A (vector-axial vector interaction in, 212–16, 292

      vacuum polarization in, 113–15, 136–40, 137, 150–51, 156–57, 159

      variational method for, 188–89

     
    vector (V) interaction in, 212–16, 292

      vortex lines in, 187–88, 189–90

      wave functions in, 52–56, 70, 117–20, 173, 182–84, 185, 188–89

      Wheeler’s contributions to, 48–50

      zero-order predictions in, 102–3, 118

      quantum mechanics, 23–35, 51–75, 238–313

      algorithms for, 273, 278–79, 283, 284, 286

      antimatter in, xii, 41

      asymptomatic freedom in, 306–7, 309, 312, 319

      attractive vs. repulsive forces in, 259–60

      black holes in, 249–51, 252

      bosons in, 102, 175, 176, 182, 184, 303–5

      branes (higher dimensional objects) in, 253–54

      classical physics and, 238, 239, 243, 245–46, 265, 278–81, 282

      computer analysis of, 308–9

      computers based on, 273–86

      consistency of, 251–52

      cosmological interpretation of, 255–61

      decouplets in, 290

      deep inelastic scattering in, 298–99

      dimensions of universe in, 251–54

      eightfold way in, 289–91

      Einstein’s contributions to, 6–7, 19, 22, 27, 39–42, 60, 93, 95, 97, 102, 175, 238, 239–40, 248, 251, 280–81

      electron-proton collisions in, 297–98

      electrons in, 294, 297–98, 301

      electroweak unification in, 304–6, 312

      energy dissipation in, 247–48 281–282, 295–300, 310

      energy v. matter in, 238–39, 250–51, 257–60, 306–7, 309–13

      event horizons in, 249–50

      in expanding universe, 239–40, 257–60

      experimental results in, 240, 252–54, 257, 260–61, 290–300, 304–9, 310, 312–13

      Faddev-Popov ghost bosons in, 304

      Feynman’s contributions to, 18, 19–20, 243–62, 273–86, 288, 289, 300, 304–5, 306, 307–13, 319

      Feynman space-time diagrams for, 252–53

      Feynman test for, 309–13

      field theory and, 238–39, 247, 252–53, 261–62, 287–88, 311–13

      finite theory (effective theory) in, 310–12

      flat space in, 258–60

      formalism in approach to, 299–300

      gauge bosons in, 303–5

      gauge invariance in, 301–5

      Gell-Mann’s contributions to, 243–44, 256–57, 287–305, 312

      geometry of, 244–45, 255–56, 258–59

      Glashow-Weinberg theory of, 304–5, 310

      gravitational contraction in, 83, 238–62, 288–89, 303–4

     


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