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Wheeler J.A. — Topics of modern physics. Vol. I. Geometrodynamics
Wheeler J.A. — Topics of modern physics. Vol. I. Geometrodynamics



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Название: Topics of modern physics. Vol. I. Geometrodynamics

Автор: Wheeler J.A.

Аннотация:

This is a collection of papers dealing with geometrodynamics. Geometrodynamics is the study of the geometry of curved empty space and the evolution of this geometry with time according to the equations of Einstein's standard 1916 general relativity.


Язык: en

Рубрика: Физика/

Статус предметного указателя: Готов указатель с номерами страниц

ed2k: ed2k stats

Год издания: 1962

Количество страниц: 334

Добавлена в каталог: 29.08.2013

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Предметный указатель
Geons, orientation-dependent forces between      171—172
Geons, physical quantities in, dependence of, upon distance (diagram)      160
Geons, refractive index barrier in, centrifugal versus coulombic      27
Geons, sample figures for physical magnitudes within      28
Geons, scaling law for      135 155 157—158
Geons, significance of for theory of motion      25—27
Geons, similarity transformation in      28
Geons, simple spherical, analysis of structure of      146—163 175
Geons, simple spherical, compared with thermal geons      192
Geons, simple spherical, energy density in      150—153
Geons, simple spherical, mass and radius as functions of action (diagram)      175
Geons, simple spherical, of different b-values, comparison of      165
Geons, simple spherical, quantitative features of, in dependence upon action      163
Geons, slow adiabatic changes of shape of      170
Geons, spherical, spontaneous transformation of into toroidal geon      147
Geons, thermal      168 186—224
Geons, thermal, analogy to blackbody container      191
Geons, thermal, compared with toroidal and simple spherical geons      192
Geons, thermal, coupled differential equations for      212—213
Geons, thermal, dependence of principal quantities in, upon distance (diagram)      194—195
Geons, thermal, eigenvalue determination for, by electronic computer      215
Geons, thermal, mass as a function of distance in      201
Geons, thermal, power series for metric coefficients in      213—214
Geons, thermal, statistical and JWKB analysis of modes in      196—200 206—212
Geons, thermal, variational principle for      216—218
Geons, tidal deformation of      172
Geons, toroidal, classical, of minimum size      138—139
Geons, toroidal, compared with thermal geons      192
Geons, toroidal, differences between, according as photons do or do not go around torus the same way      176
Geons, toroidal, mass spectrum of      146
Geons, transmutation physics of      173
Geons, two neutrino-containing, repulsion of      178
Geons, two toroidal, interaction of      170
Geons, upper limit to size of      136
Glashow, S.      130
Glass sphere, as model for geon      144
Glass, spherical block of, as model for a geon      27
Glove turned inside out one finger at a time, in connection with dynamics of universe      62
Goerss, R.      161
Gold, T.      118
Goldhaber, M.      6 117
Gottschalt, W.H.      187 n
Goudsmit, S.A.      xv
Goursat, E.      283 n
Gradient, in intrinsic notation      261
Gravitation      xii
Gravitation, geometrical description of      8
Gravitation, geometrical description of, acceptability of      234
Gravitational attraction, Newtonian      49
Gravitational attraction, of oppositely directed pencils of light      147 170—171
Gravitational bending of light      13
Gravitational contraction      4—6
Gravitational coupling, compared with Fermi coupling      110
Gravitational deflection of light, observation vs. prediction      46 47
Gravitational field, fluctuations in      71 72 75—83
Gravitational field, in geon, as wave guide for electromagnetic energy      26
Gravitational field, produced by gravitational wave      55
Gravitational forces, as feature of Rainich — Riemann geometry      253
Gravitational forces, coupling constant for, absence of      21
Gravitational radiation, as part of environment for two-body problem      49
Gravitational radiation, curving universe to closure      62
Gravitational radiation, detection of      7
Gravitational radiation, energy density of, in cosmos      7
Gravitational radiation, mass-energy density of, in universe      115—117 130
Gravitational radiation, possibilities to detect      113—114
Gravitational radius      141
Gravitational waves, as members of geometrodynamical zoo      50
Gravitational waves, generation of      7
Gravitational waves, gravitational field produced by      55
Gravitational waves, mass-energy of      57
Gravitational waves, plane      63
Gravitational waves, response of test particles to      58
Gravitational waves, symmetric in time and asymptotically Schwarzschildean, as example of geometry which is always free of singularity      54
Gravitational waves, time symmetric      63
Gravitational waves, time symmetric, strength of, measured by a parameter      55
Gravitational waves, weak, polarization      32 33
Graviton      6
Graviton-induced processes      109
Green's theorem      281—282
Griffin, J.J.      93 n
Grommer, J.      24 n
Gross, F.      115 n
Ground state, of electromagnetic field      8
Guggenheim, J.S.      xvi
Gulmanelli, P.      90 n
Gurney, R.W.      143
Hamermesh, M.      xiv 153 207 294
Hamilton — Cayley — Klein description of a rotation      92
Hamilton's canonical formalism      xv
Hamilton, W., R.      222
Hamiltonian, and evolution of quantum system in time      85
Handle, topological      see "Wormhole"
Hard core repulsion, ineffectiveness of, in big A problem      123
Harmonic integrals      xv
Harmonic oscillator, as illustrative of method of sum over histories      84—87
Harmonic vector fields      xv 289—293
Harris, A.      130 n
Harris, C.      115 n
Harrison, B.K.      5 121 122 123 125 128
Harrison, F.B.      1 n 106
Hausdorff, character of a manifold      256
Hedlund, G.A.      187 n
Heisenberg, W.      80 n 89 140 176 181 219
Helium, liquid, in connection with collective disturbances      79
Helmer, O.      73 n 231
Helmholtz instability      69 189
Histories, Feynman's method of sum over, extended to Fermi field      97—102
Histories, number of distinct, for source-free electromagnetism and geometrodynamics      37—40
Histories, number of, for source-free metric      43 44
Histories, sum over, topological aspects of      83—87
Histories, unruly, and Klauder's action option      101—102
History, of 3-geometry, as described by 4-geometry      35—40
Hodge, W.V.D.      xv 260 278 290
Hoffmann, B.      24 n 49 133 237 302
Homeomorphism, defined      255
Homeomorphism, orientation-preserving      265
Homology groups      xii 272
Homology theory      267—279
Hoyle, F.      118
Hubble constant, implications of for density of mass-energy      116
Hubble, E.P., and red shift      59
Hydrodynamical analogue to expansion and recontraction of universe      61—63
Hydrodynamics, analogies to geometrodynamics, in equation of motion of concentration of energy      25
Hydrodynamics, compared and contrasted with geometrodynamics (table)      187—189
Hydrodynamics, eventual singularity of wave in      67 68 72
Hydrogen spectrum      9
Hydrogen, density of, in space      116
Hydrostatic equilibrium, general relativity equation for      123 124
Imaeda, K.      91 n
Images, multiple, in an irregularly curved space      115 130
Imbedding of 3-space in 4-space, or of 2-space in 3-space      34
Impact parameter, for light rays in simple spherical geons      166—167
Impact parameter, in analysis of geodesies      191 196—200 205
Implosion of universe, maximum      63
Imposition of gravitational wave      56 57
Impulsive radiation, electromagnetic and gravitational      113—114
Incoherence, of modes in simple spherical geon      146—147
Indices, raised, defined      15
Inertia, origin of      58 59
Infeld, L.      xv 24 49 133 234 237 302
Ingard, U.      115 n
Initial value data, contrasted with data required in two-surface formulation      42
Initial value data, for electromagnet ism      31 283—289
Initial value data, for electromagnetism in curved space, via Fourier analysis      289—294
Initial value data, for geometrodynamics      36—39 294—301
Initial value data, for geometrodynamics, compared in tabular form with case of electrodynamics      38—39
Initial value data, for time-symmetric gravitational waves      54—57
Initial value data, in two body problem      49
Initial value equations, applied to expansion and recontraction of universe      60
Initial value equations, for electromagnetism      32
Initial value equations, for geometrodynamics      33—40
Initial value equations, of hydrodynamics and geometrodynamics, parallelism of      187
Initial value problem of geometrodynamics and question of superpotential      306
Integrals, harmonic      xv
Interactions, gravitational      2
Interactions, neutrino      2
Interactions, weak      2
Interference, constructive, of wave trains, as determining geodesic      221—224
Intergalactic space, particle density in, relevant to geon losses      29
Interval, invariant relativistic, measurement of      10—12
Intrinsic 3-geometry, for time symmetric gravitational wave      54
Intrinsic curvature invariant, equations relative to a 3-surface      51 52
Intrinsic curvature, and initial value condition      41—43
Intrinsic curvature, for spherical universe      60—62
Intrinsic curvature, infinity of in Schwarzschild geometry      63—65
Intrinsic curvature, vanishing of, at moment of time symmetry for source-free gravitational wave      54
Intrinsic curvature, vanishing of, spelled out for 3-geometry of axial symmetry      55
Intrinsic description of vectors and tensors, contrasted with tensor analysis      259—260
Intrinsic geometry, Euclidean, of a, bent piece of paper      48
Invariants of electromagnetic field      229 238 240—242
IVANENKO, D.      6 79 80 91 96 109
Ivanenko, D. and Fock, V., coefficients      95
Jacobi, K.G.J.      222
Jacoby, K.      xv
Jauch, J.      227 n
Jehle, H.      96 n
Jordan, P.      89 n 181
JWKB, Jeffreys — Wentzel — Kramers — Bril-louin approximation, for modes of electromagnetic oscillation in geon      196 199 224
Kaellen, G.      78 n
Karplus, R.      140 n
Kawaguchi, M.      90 n
Kay, W.C.      xvi
Kelley, J.L.      255 n
Khalatnikov, I.M.      79 n
Kinetic energy, analog of, in dynamics of universe      60 61 64
Kircher, C.E.      xvi
Klauder, J.R.      96 n 97—101 102
Klauder, L., Jr.      117 n
Klein bottle      231
Klein, O.      105 n
Kockel, B.      140 n 219
Kofoed-Hansen, O.      105 n
Komar, A.      53 n 66 161 187 286
Kompaneyets, A.S.      63
Kramers, H.A.      70 n 89 103 181
Kronig, R. de L.      89 n 103 181
Kruse, H.W.      1 n 6 106 127
Kruskal's coordinates for Schwarzschild geometry, used to bring out intrinsic singularity at r = 0      45 53 65
Kruskal, M.      45 47 48
Kuiper, Gr.      46 n
Kutta      215
Lagrange density, in variational principle for Rainich — Riemann geometry, not known      253
Lagrange function, and evolution of quantum system in time      85
Lagrange or two-surface formulation of electromagnetism contrasted with initial surface formulation      283
Lamb — Retherford, shift      69
Lamb, W., shift of level of hydrogen      66
Lanczos, C.      305 n
Landau, L.      xiv 60 79 121 123 124 153 189 222 227 256 294 297
Laplace's equation, analogy to equation for minimal surface and to field equations of general relativity      52
Laurent, B.E.      93 n
Leakage of energy from geon      see "Geon leakage
Lee, T.D.      104 n 105 106 107
Lee, T.D., and C.N. Yang, their 2-component equation for neutrino      95
Lefshetz, S.      xiv 268
Lemaitre, G.      297 n
Lengths, as central concepts in the description of physics      13
Lens, for concentration of electromagnetic radiation      57
Lepton number, conservation of      6
Leptonic charge, wormhole picture not appropriate for      102
Lichnerowicz, A.      xiv 31 33 62 187 260 295 297 301
Lie groups and question of solutions of equations of geometrodynamics      306
Lie, S.      306
Lifshitz, E.      xiv 60 153 188 207 222 227 256 294 297
Light ray, as one of tools for measuring interval      10—12
Light ray, in thermal geon (diagram)      191 196—200
Light, deflection of, by gravitational field, in geon      141
Light, deflection of, by sun, observation vs. prediction      13 46 47
Light, scattering of, by light, in small dense geon      140 174—178
Lighthill, M.J.      188 n
Lindquist, R.W.      188 n 300
Lines of force, trapped in topology      232
Local linearity of gravitational field equations      80
Longitudinal field      289—291
Lorentz, force law, from field theory      301—302
Lorentz, force law, not given by non-Riemannian type of unified field theory      234
Lorentz, H.A.      70 n
Lorentz, reference system      11
Lorentz, reference system, chosen to simplify discussion of complexion      18 19
Lorentz, reference system, chosen to simplify Maxwell stress tensor      17
Lorentz, reference system, reducing Poynting flux to zero      16 17 see
Lorentz, reference system, used to discuss initial value equations of electromagnetism      40
Lorentz, reference system, view of wormhole mouth in      304—305
Lorentz, transformation, compared and contrasted with duality rotation      240 241
Luyten, W.J.      46 n
Mach, E., his principle      58 59 63 94 231
Mach, E., triple point      188
Maehly, H.J.      123 124
Magnetic charge associated with a given homology class      274
Magnetic field, as coordinate in field theory      42 44
Magnetic field, as projection or trace      285
Magnetic field, contribution of, to density of mass-energy in universe      116—117
Magnetic poles, absence of      304—305
Majorana equation for neutrino      108
Malkus, W.V.R.      305 n
Manifolds      xv
Manifolds, defined      255—256
Manifolds, examples of      256—259
Manifolds, properly closed in space, eventual singularity of geometry of      58 61
Manifolds, Riemannian, enormous physical content of this hypothesis      12 13
Manifolds, Riemannian, subclass of, consistent with Einstein — Maxwell theory      21
MARIOT, L.      17 n
Markus, L.      228 n 244
Mars, perihelion precession of      46
Marshak, R.E.      105 n
Marzke, R.F.      10 n
Mass spectrum, of simple toroidal geons      146
Mass, alternative models for      25
Mass, as a length      13
Mass, as function of distance, in thermal geon      201
Mass, classical models for      234
Mass, geometrodynamical description of      8
Mass, geon as a model of      25—31
Mass-energy, effective density of, in source-free gravitational wave      55
Mass-energy, effective density of, in universe      46 60 61 116
Mass-energy, effective density of, of gravitational radiation, in universe      115—117 130
Mass-energy, of geon      26
Masses, nuclear, semiempirical formula for      122
Matter at high density, opacity of      4
Matter, nature of      68—71 76
Maxwell energy density, in initial value equation of geometrodynamics      33 295
Maxwell field, 2-form representation of, connected with vector representation of      275
Maxwell field, as a 2-form      261 263
Maxwell stress-energy tensor      15 16 21 132—133 237
Maxwell stress-energy tensor, in diagonal form      229
Maxwell stress-energy tensor, physical significance of individual components of      238
Maxwell stress-energy tensor, table of components of, in special reference system      17
Maxwell stresses, as aspect of Rainich — Riemann geometry      253
Maxwell's equations      14 15 20 21 91 178 234
Maxwell's equations, basic non-linearity in, when coupled with Einstein's equations      254
Maxwell's equations, consequences of, in a multiply connected space      49 50
Maxwell's equations, derived from condition lines of force never end      41
Maxwell's equations, derived from initial value conditions plus covariance      40—41
Maxwell's equations, for a non-null field, demand existence of complexion      249—253
Maxwell's equations, in a multiply connected space      233
Maxwell's equations, in curved space      227
Maxwell's equations, in curved space time, in (3+1)-dimensional notation      31
Maxwell's equations, in curved space, briefly summarized      132—133
Maxwell's equations, metric free half of      255
Maxwell's equations, metric-dependent part of      280
Maxwell's equations, number of solutions of      37—40
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