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The Trouble With Physics: The Rise of String Theory, The Fall of a Science, and What Comes Next

Page 47

by Lee Smolin


  octonions, 274

  “On the Electrodynamics of Moving Bodies” (Einstein), 36

  Oppenheim, Paul, 296

  Paczuski, Maya, 342–43

  particles

  accelerator discoveries on, 54

  as composites, 73

  kinds of, 12

  mass differences/hierarchy of, 70

  in string theory, 102

  as waves, 67, 132

  See also specific types; unification of particles and forces

  Pauli, Wolfgang

  exclusion principle, 67–68

  quantum gravity, 84–85, 86

  unified theory, 49

  peer review

  affirmative action, 336–37

  African American candidates, 335–37

  bias, 334–36

  big research programs and, 337–39

  candidates who think differently, 335–36, 337–48

  comparative rankings, 334–35

  description, 332, 333

  normal science and, 339–40

  polarized responses with, 342, 353

  power and, 333–34, 336–39, 342

  status/grants and, 337–38

  string theorists and, 338–39

  women candidates, 335–37

  Penrose, Roger

  landscape of string theories, 364 n5 (ch. 12)

  on quantum theory and gravity, 319

  Sciama and, 322–23

  as seer/rebel, 294, 313, 319

  twistor theory/space, 244, 245

  perturbation theory, 179–80, 186–87, 188, 278–79

  phenomenon of length contraction, 227

  Philosophiae Naturalis Principia Mathematica (Newton), 3

  phlogiston, 19

  Phong, Duong H., 187, 280

  phonon, 132

  photinos, 74, 75

  photons

  description, 106, 183

  Einstein, quantum revolution, and, 52

  electromagnetic waves and, 55

  gamma rays and, 224

  gauge bosons and, 58, 106

  as massless particles, 106

  in quantum field theory, 55

  vibrations of strings and, 183

  Physical Review Letters, 104

  physics as

  “almost complete,” 3

  beyond string theory (overview), 238, 254–56

  breakthrough trends (before late 1970s), 66

  communication problems, 239

  division of, 5

  dominant fields and, 268

  failures (since late 1970s), viii, xi–xiii, 3–4, 66, 261–62

  fundamental principles and, 218–19

  historical overview of, viii–xi, xiii–xiv

  key problems in, 3–17, 349–50

  “missing element” and, 101–2

  need for seers, 311, 312–14

  normal science period (craftspeople), 311–12, 324

  responses to failure, 66–67

  revolutionary periods of, 3, 311, 324

  risky new research programs, 294

  style of research in, xxii–xxiii, 262–64

  theory characteristics, 256

  types of people studying, 95

  wrong assumptions and, 256–58, 316

  See also academic landscape; science; sociology of physics, string theory

  Pioneer 10/11, 213–14

  pions, 220, 221

  Planck, Max, 3, 4, 51–52

  Planck energy, 173, 221

  Planck length/paradox, 227, 228–29

  Planck mass, 70, 71

  Planck scale

  cosmic ray studies and, 220

  description, 204, 224, 225

  probing of, 224–26

  special relativity breakdown and, 224–25, 231

  Planck’s formula, ix, 3, 4

  Planck time, 168

  planets, 27–30

  Plato, 218

  Platonic solids

  description/types of, 28

  Kepler’s use of, 27–29, 28

  Polchinski, Joseph

  on alternatives to string theory, xv–xvi

  anthropic principle, 169

  inducing strings to become bigger, 171

  Maldacena conjecture, 282

  string theory, branes, 136–38, 155, 158

  politics and power over social world, 297

  Polyakov, Alexander, 110, 141–42, 249

  Popov, Victor Nicolaevich, 88

  Popper, Karl, 293, 296, 297

  predictions

  anthropic principle, 163, 168–69

  on DSR theory, 252

  general relativity, 45

  on Higgs boson/particle, 70, 76, 77

  Kaluza-Klein theory, 48

  Kepler’s work, 30

  special relativity, 219

  string theory, problems with, xiv, 69–70, 124, 128, 174–76, 180, 183, 193, 197, 199, 223, 352

  supersymmetry, problems with, 69–70, 174–76

  theory and, xvi with unification proposals, 20, 40–41

  of vacuum (ground-state) energy, 152, 158

  Weinberg-Salam model of electroweak force, 62

  preons, 73–74, 253–54

  Preskill, John, xi–xii

  “protected” masses, 72

  proton decay

  probing the Planck scale and, 225

  standard model and, 63–65

  protons

  cosmic rays and, 219, 220–21

  mass description, 70

  quarks and, 56, 63–64

  radioactive decay and, 63–65, 103

  Ptolemy

  epicycles, xvii, 21, 24, 196, 218

  unification proposals, 20–21, 23, 24

  Pynchon, Thomas, 233

  QCD (quantum chromodynamics), 62, 110

  QED (quantum electrodynamics)

  as finite, 278

  quantum field theory and, 55–56

  quantum gravity and, 84, 86–87

  quantum chromodynamics, 62, 110

  quantum computers, 317–18, 325

  quantum electrodynamics. See QED

  quantum field theory

  approximation procedures and, 182–83

  description, 55, 182–83

  difficulties in determining, 55

  QED, 55–56

  renormalization, 292

  special relativity and, 55

  strong/weak nuclear forces and, 55–56

  unification of electromagnetism, quantum theory, 55

  quantum geometry, 248, 249, 250

  quantum gravity approaches (after string theory)

  atmosphere of, 239–40, 262–64

  background-independence requirement, 239, 247, 249, 251–52, 253, 255, 317

  basic ideas of, 241

  causal dynamical triangulation, 242–43, 242

  causality and, 240–41

  causal set theory, 243–44

  condensed-matter models, 247

  Connes’s noncommutative geometry, 245–47

  loop quantum gravity and, 249–54

  overview, 254–56

  reformulation of general relativity equations, 239

  space as emergent in, 240, 241

  string theorists’ ignoring of, 239

  twistor theory/space, 244–45

  quantum gravity theory

  answers needed from, 145–46

  approaches to (summary), 83, 98

  background dependence, 85, 86–87, 88–89, 98

  background independence, 83, 85, 86

  black hole information paradox, 91

  cosmological constant problem, 153

  difficulties of, 83–84

  Einstein’s statement of problem, 83

  failure of work in, 87, 88–89

  gravity effects on quantum phenomena studies, 89–91

  key question of, 83

  loop quantum gravity, 229

  pioneers of, 80, 85–86

  Planck length, 227

  Planck scale, 220

  probabilities and, 88


  problem of, 5–8, 12, 13

  string theory problems with, 83, 184–92, 197–98

  supergravity and, 91–98

  Yang-Mills theories and, 88–89

  quantum language, 7

  quantum mechanics

  domain of, 6

  field theories and, 55, 84

  new theory for, 9–11

  observed system/observers division and, 7–8

  problem-solving need, 8–11

  realism and, 7, 8–10

  quantum spacetime, 248, 249

  quantum theory

  as (possibly) wrong, 316–26

  conceptual paradoxes of, 6

  debates over, 7, 323–24

  description, ix, 67

  development of, 4

  Einstein’s view of, 52

  infinities problem with, 5–6

  invention of string theory, 104–5, 107–8

  reality/formalism and, 6–8

  unified field theory, 51–52

  quarks

  “colors”/versions, 62

  discovery of, 56

  force between, 104

  overview, x, 12

  particles made from, 63–64, 103

  unification of forces and, 56

  Ramond, Pierre, 105, 111

  Randall, Lisa, xvi, 173–74

  random dynamics, 316

  realism

  quantum mechanics and, 7, 8–10

  quantum theory and, 6–8

  “real world out there” (RWOT), 7, 9

  Rechel-Cohn, Amelia, 290

  Rees, Martin, 322–23

  relativity community, 262–63, 341

  religion, 297, 303

  rest

  definition/description, 21–22

  unification of motion and, 21, 22, 24, 39, 203, 219

  Riemann hypothesis, 282

  risk and science, xvi, xxi, 294, 330–31, 342–44, 353

  Rocek, Martin, 93, 95

  Roots of Civilization, The (Marshack), 297

  Rovelli, Carlo

  career of, 340–41

  relational quantum theories, 317

  as seer, 313

  string theorists’ criticism of, 281

  Royal Society, United Kingdom, 353

  S-duality (strong-weak duality)

  definition/description, 131, 144

  eleven-dimensional theory and, 136

  unification of string theory and, 133, 188–89

  Salam, Abdus

  anthropic principle, 165

  Weinberg-Salam model of electroweak force, 61

  Yang-Mills theories and, 88

  See also Weinberg-Salam model of electroweak force

  Scherk, Joël, 106

  Schrödinger, Erwin

  debate over quantum theory, 7

  hidden-variables theory, 323

  as seer, 311

  unified theory, 49, 52–53

  Schwarz, John, string theory and, 106, 111, 112, 113, 114–15, 339

  Schwinger, Julian, 55, 87

  Sciama, Dennis, 322–23

  science

  consensus and, 300, 302, 304–5, 306–7

  as correction mechanism, 300–301

  diversity of views in, 294–95, 304–5

  democracy and, 295, 300–301

  as ethical community, 302–3, 307

  ethics violations, 305

  evolution of, 297–98

  fashion/fads and, 306

  funding reforms, 352–53, 354

  as imaginative community, 303–4, 306–7

  need for definition, 295

  need for innovation, 308–9

  need for revolutions, 311, 312–14

  normal, and craftspeople, 310, 311–12, 314, 324

  normal, and peer review, 339–40

  normal vs. revolutionary, x, xxii–xxiii, 294–95, 296–97, 300, 310, 311, 324, 348, 351

  and other belief systems, 297

  power over physical world and, 297, 298

  repeatable experiments and, 298–99, 365 n1 (ch. 13)

  responsibility of public, 353–54

  responsibility of scientists, xxi–xxii, 354–55

  revolutionary periods in physics, 3, 311, 324

  revolutions, description of, 115, 116

  role in human culture, 297–301

  seers, 310, 311, 312–14

  shared ethic of, 301–3, 350–51

  social constructivists–scientists debate, xix–xx

  solving problems in, 294, 349–55

  time and, 305–6

  wrong assumptions, 308–9

  See also academic landscape; craftspeople; physics; seers

  Science in a Free Society (Feyerabend), 291

  scientific methods, 295–98

  Scuola Internationale Superiore di Studi Avanzati (SISSA), 323

  second law of thermodynamics, 90

  seers

  background-independent approaches and, 313

  characteristics of, vii–viii, 309, 314, 321–22, 326–27, 328–30, 343, 351

  examples of, 309, 313, 314–29, 342–43

  historical/philosophical context of science and, 310–11

  need for, 311, 312–14

  recognizing, 329, 353

  revolutionary periods in science and, 310, 311, 312

  scientific/academic careers and, 265–67, 314, 315–16, 318–19, 320–25, 326–31, 344–48, 350, 351–53, 370 n14

  Seiberg, Nathan, 270

  selectrons, 68–69, 74, 75

  Shenker, Stephen, 147, 274

  Shor, Peter, 325

  Singer, Isador, 346

  SISSA (Scuola Internationale Superiore di Studi Avanzati), 323

  sleptons, 75

  Smolin, Lee

  career vs. thinking for oneself, 339–40

  cosmological natural selection, 167

  “Did the Universe Evolve?” 127

  DSR/DSR II, 231–37

  evolution and, 25–26

  Feyerabend and, 290–93

  graduate school crisis, 289–94

  Life of the Cosmos, The, 127, 167

  loop quantum gravity and relativity, 229, 271, 314–15

  “On the Relations Between Quantum and Thermal Fluctuations,” 320, 355

  as seer/craftsperson, 311, 312, 319–20

  string finiteness and, 279–82, 285

  string theory work, xviii–xix, xx–xxi, 271, 274, 279, 285

  threats to academic freedom (article), 345

  Valentini and, 326

  views on quantum theory, 319–20, 326

  VSL cosmology/relativity, 230–33

  Wheeler-DeWitt equation, 314–15

  sneutrinos, 75

  social constructivists–scientists debate, xix–xx

  sociology of physics, string theory

  belief in unproved conjectures, 278–83, 284

  confidence/arrogance and, 268–70, 284, 367 n4 (ch. 16)

  disregard for alternate approaches, xv–xvi, 270–71, 284, 351

  exaggeration of claims, 276–77, 283–84

  fads in, 271–72

  finiteness as believed/unproved, 278–82

  groupthink, 286–88, 350, 354

  ignoring/reviving work, 273–74

  inefficient use of talents, 272

  lack of assessment, 281

  lack of knowledge of key string results, 277–82

  lack of originality and innovation, xxiii, 273–74, 284

 

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