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Astronomical Unit, 7

Atkins, Peter, 168

atomic clocks, 24–25

Bardeen, Carter and Hawking, ‘The Four Laws of Black Hole Mechanics’, 187–90

Barish, Barry, 7

beginning of universe, 2, 5, 155, 177

Bekenstein, Jacob, 163–4, 179

Bekenstein(–Hawking) entropy, 179, 183–6, 232

Bell Burnell, Jocelyn, 4

Bell state, 212

Bell, John, 212

Bertschinger, Edmund, 22, 29

bets

Hawking and Thorne vs. Preskill, 18–19, 238

Hawking vs. Thorne and Preskill, 144

Big Bang, 2, 5, 177

Birkhoff, George David, 157

bit, 179–83

black hole

complementarity, 197–207, 225–31

distorting space and time, 1, 11, 104

early scepticism, 3, 11–15, 149

18th-century ideas, 9–10

energy extraction, 145–8, 195

entanglement with Hawking radiation, 218–25, 229–32, 246–51

entropy, 179–86, 188–90

evaporation, 17, 201–5, 218–25, 247–50

event horizon, 1–2, 9, 11

formation, 2, 7, 14–15, 149–59

geometry, 46, 99, 122, 128–9, 135

hair, 150, 161

inevitability of formation, 14–16, 152–6

information paradox, 17–19, 201–8, 218–53

Kerr, 131–148, 189

observation, 5–8

Penrose diagram, 91–5, 136–9, 157–61

river model, 107–10, 133–4

rotating, see Kerr

Schwarzschild, 88–95, 115–18

shadow, 5–6

supermassive, 1, 5–7, 93, 156

temperature, 17, 186–90, 195–6

thermodynamics, 163, 179–91

‘Black Hole Explosions?’ (Hawking), 16, 186, 201

Black Hole War, The (Susskind), 18, 203

Blandford, Roger, 29

Boltzmann, Ludwig, 171, 175–6

Boltzmann’s equation, 175, 178

brewing, 165–6

bridge, Einstein–Rosen, 114–16, 125, 245–6; see also wormhole

Brief History of Time, A (Hawking), 18

Brownian motion, 167

Buckminster Fuller, R., 76

‘Building up spacetime …’ (Van Raamsdonk), 243–4

caloric, 166

Carter–Penrose diagram, 49

Carter, Brandon, 49, 140, 187

causal influence, 30–1, 37–40, 51–2, 69

cause and effect, 37–40, 45, 215

Chandrasekhar limit, 13

Chandrasekhar, Subrahmanyan, 13–14, 149–50, 156

Character of Physical Law, The (Feynman), 173

Christmas in spacetime, 35–40, 57

chronology protection conjecture, 141

Clausius, Rudolph, 169

clocks and rulers, 37, 55–63

closed timelike curves, 140–41

collapse of stars, 2–4, 15, 149–61

halting, 11–14

inevitability of black hole formation, 14–16, 152–6

realistic black holes, 149–61

spherically symmetric, 151, 157–8

compact object, see black hole, neutron star

complementarity, 197–207, 225–31

conformal field theory (CFT), 236, 240

conformal projection, 49, 51, 235

conformal spacetime diagram, 49, 51

conservation

of energy, 146–7, 168–9, 189

of information, 17–19, 203–7, 219–20, 223–5, 237–8

of momentum, 146

coordinates, 54, 81–3, 96

Kruskal–Szekeres, 115, 117–18

Schwarzschild, 84–90, 93

cosmic censorship conjecture, 142–5, 161

cosmic microwave background radiation temperature, 17

curvature, 80, 84, 120–22

curved spacetime, constructing from flat pieces, 77–80

curved surfaces, constructing from flat pieces, 76–8, 81–3, 96; see also non–Euclidean geometry

Dalton, John, 166

dark star, 9–10

Darwin, Charles, 19

Davies–Unruh effect, 198

Davies, Paul, 198

de Kremer, Gerard, 48

degeneracy pressure

electron, 12–14

neutron, 13

determinism, 18, 203, 220

dimensions, higher, 41–4, 119–22, 234–5

Dirac, Paul, 211

distance between events, see interval

distortion of representation of spacetime, 51–3, 59–60

distortion of spacetime by matter and energy, 40–41, 51, 46

Dong, Xi, 258

Doppler effect, 61–2

E = mc2, 27, 183

Eddington, Arthur, 3, 12–13, 46, 164

on thermodynamics, 164

scepticism of black holes, 3, 13

Einstein–Rosen bridge, 114–16, 125, 245–6; see also wormhole

Einstein, Albert

1905 work on molecular motion, 167

1905 work on photons, 180, 183

1905 work on relativity, 24–8, 40, 183

1915 work on gravity, 2, 22–3, 40–41, 70–72, 78–82

1935 scepticism of quantum theory, 209, 245–6

1935 work on wormholes, 114, 125

1939 scepticism of black holes, 3, 11, 14–15, 149

Einstein’s equations, see General Theory of Relativity

electromagnetic wave, electromagnetic, 25, 104–5, 180

electromagnetism, 19, 25, 171

Maxwell’s theory, 25–6

electron degeneracy pressure, 12–14

electrons, 4, 12–13, 17, 194

Ellis, George, 2

embedding diagram, 119–28

emergence of spacetime and gravity from quantum theory, 20, 191, 236, 244–5, 261

energy extraction from black hole, 145–8, 195

entanglement, 20, 208–18, 254–5

between Hawking radiation and black hole, 218–25, 229–32, 246–51

entropy, 222–4, 242–3, 247–51

in quantum computing, 254–61

monogamy of, 230

vacuum, 218, 230–31, 244–5

entropy

black hole, 179–86, 188–90

classical, 164–5, 169–71

entanglement, 222–4, 242–3, 247–51

information-theoretic, 177–9

statistical, 171–7

thermal, 171–7, 221–4

‘EPR’ paper, 245

Equivalence Principle, 71, 89, 198

contradiction, 181, 200, 228

resolution, 231

ER = EPR, 130, 245, 247, 251–2

ergosphere, 132–5, 145–9

escape velocity, 9

Escher, M. C., 47, 235

Euclidean geometry, 43, 81, 121

event, spacetime, 28–40, 51–7

event horizon, 1–2, 9, 11

in river model, 107–8

increasing area rule, 148, 164, 188–9

inner and outer, 132, 135–6, 148

Event Horizon Telescope Collaboration, 5–6

Exclusion Principle, Pauli, 12

Exploring Black Holes (Taylor, Wheeler, Bertschinger), 22, 29

extra dimensions, 41–4, 119–22, 234–5

Feynman, Richard, 150, 173

firewall, 228–32

First Law of Thermodynamics, 168–9, 189

Flamm, Ludwig, 114

Flat Albert, see flatland

Flat Eric, 42

flat rulers on curved surfaces, 76–80, 96; see also metric

flat spacetime, 49–51, 67, 77, 157–8

flatland, 41–4, 76

wormholes in, 119–26

Flatland: A Romance of Many Dimensions (Abbott), 42

floating, 67, 70, 94, 103

fluctuations, vacuum, 16–17, 193–200

‘Four Laws of Black Hole Mechanics, the’ (Bardeen, Carter, Hawking), 187–90

Fowler, R. H., 11–13

free will, 140, 215

freefall, 70–71, 80, 89

fridge, 169–70, 189

Fuller, Robert, 16

Fulling, Stephen, 198

fusion, thermonuclear, 3, 12, 15

General Theory of Relativity, 2, 40–41, 75–83

equivalence principle, 70–71; see also Equivalence Principle

gravitational waves, 7, 151, 156

Kerr solution, 131–3, 149–51

Schwarzschild solution, 75–7, 80, 83–7

Wheeler’s maxim, 46, 75

Genzel, Reinhard, 7

geodesic, greedy, 260–61

geodesic dome, see Montreal Biosphere

geometry

distortion by matter and energy, 40–41, 51, 46

Euclidean, 43, 81, 121

Kerr, 131–9, 142–5, 149–51

non-Euclidean, 44, 67, 76–7, 119, 235

Schwarzschild, 75–7, 80, 83–95

Geons, Black Holes and Quantum Foam (Wheeler), 150