The Large-Scale Structure of the Universe:Princeton series in physics

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1980-11
ISBN: 9780691082400
装帧: 其他
开本: 其他
纸张: 其他
  • Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. P.J.E. Peebles argues that the evolution proceeded from a nearly uniform initial state to a progressively more irregular and  HOMOGENEITY AND CLUSTERING
    3
    Physical principles
    11
    How did galaxies and clusters of galaxies form?
    18
    Summary
    35
    NEWTONIAN APPROXIMATION
    37
    Particle dynamics in expanding coordinates
    41
    The peculiar acceleration
    43
    the Vlasov equation and the ideal fluid
    45
    Relation between t and w some examples
    195
    Inversion of the equation
    200
    Angular threepoint correlation function
    203
    Angular fourpoint correlation function
    209
    Correction for curvature and expansion
    213
    Summary of numerical results
    221
    Power spectrum of the extragalactic light
    225
    Moments of the number of neighbors
    230
    Linear perturbation approximation for 5
    49
    p A 0
    56
    models with A 0
    59
    The peculiar velocity field
    63
    Joining conditions for d and v
    66
    Critical Jeans length
    68
    Primeval magnetic field as a source for Spp
    71
    Second order perturbation theory for 5pp
    74
    Spherical model
    77
    Homogeneous ellipsoid model
    86
    Caustics and pancakes
    95
    Expansion vorticity and shear
    103
    Origin of the rotation of galaxies
    107
    Cosmic energy equation
    110
    Spherical accretion model
    115
    Hierarchical clustering model
    120
    Fourier transform of the equations of motion
    124
    Coupling of density fluctuations
    128
    DESCRIPTIVE STATISTICS
    138
    Fair sample hypothesis
    142
    Twopoint spatial correlation function tr
    143
    another definition
    145
    Poisson model
    147
    Threepoint correlation function
    148
    Fourpoint correlation function
    150
    Moments of counts of objects
    152
    Constraints on t and f
    156
    Probability generating function
    158
    Estimates of PN
    160
    Cluster model
    163
    Power spectrum
    166
    Power law model for the spectrum
    169
    Bispectrum
    171
    Cross correlation function
    172
    Angular twopoint correlation function
    174
    Angular power spectrum
    175
    Estimating w6
    183
    Statistical uncertainty in the estimate of w0
    187
    Relation between angular and spatial twopoint correlation functions
    189
    Small separation approximation and the scaling relation
    191
    Decoupling of magnitude and position
    194
    Relation between t and w some examples
    195
    Inversion of the equation
    200
    Angular threepoint correlation function
    203
    Angular fourpoint correlation function
    209
    Correction for curvature and expansion
    213
    Summary of numerical results
    221
    Power spectrum of the extragalactic light
    225
    Moments of the number of neighbors
    230
    Model for PN
    233
    Clustering models
    236
    Mandelbrots prescription
    243
    The mass correlation functions
    249
    continuity speculation
    253
    Remarks on the observations
    255
    DYNAMICS AND STATISTICS
    257
    Definitions of variables and distribution functions
    258
    BBGKY hierarchy equations
    259
    Fluid limit
    262
    Evolution of the integral of
    264
    Particle conservation equations
    266
    Relative peculiar velocity dispersion
    272
    Similarity solution
    275
    Cosmic energy equation
    278
    Cosmic virial theorem
    280
    Joint distribution in position and velocity
    285
    Behavior of the halo around a cluster of galaxies
    291
    Superclusters
    299
    Problems and prospects
    301
    RELATIVISTIC THEORY OF THE BEHAVIOR OF IRREGULARITIES IN AN EXPANDING WORLD MODEL
    304
    Timeorthogonal coordinates
    306
    The field equations for haf
    310
    Gravitational waves
    312
    Newtonian approximation
    313
    Linear perturbation equations for the matter
    317
    Behavior of density perturbations at wavelength ct
    319
    Spherical model
    324
    Evolution of acoustic waves
    330
    Nonlinear acoustic waves
    333
    Incompressible flow
    341
    Behavior of collisionless particles
    345
    Linear dissipation of adiabatic perturbations
    352
    Residual fluctuations in the microwave background
    363
    Isothermal perturbations
    373
    SCENARIOS
    379
    Nature of protogalaxies and protoclusters
    384
    APPENDIX
    395
    LIST OF ABBREVIATIONS
    401
    INDEX
    417
    Copyright
  • 内容简介:
    Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. P.J.E. Peebles argues that the evolution proceeded from a nearly uniform initial state to a progressively more irregular and 
  • 目录:
    HOMOGENEITY AND CLUSTERING
    3
    Physical principles
    11
    How did galaxies and clusters of galaxies form?
    18
    Summary
    35
    NEWTONIAN APPROXIMATION
    37
    Particle dynamics in expanding coordinates
    41
    The peculiar acceleration
    43
    the Vlasov equation and the ideal fluid
    45
    Relation between t and w some examples
    195
    Inversion of the equation
    200
    Angular threepoint correlation function
    203
    Angular fourpoint correlation function
    209
    Correction for curvature and expansion
    213
    Summary of numerical results
    221
    Power spectrum of the extragalactic light
    225
    Moments of the number of neighbors
    230
    Linear perturbation approximation for 5
    49
    p A 0
    56
    models with A 0
    59
    The peculiar velocity field
    63
    Joining conditions for d and v
    66
    Critical Jeans length
    68
    Primeval magnetic field as a source for Spp
    71
    Second order perturbation theory for 5pp
    74
    Spherical model
    77
    Homogeneous ellipsoid model
    86
    Caustics and pancakes
    95
    Expansion vorticity and shear
    103
    Origin of the rotation of galaxies
    107
    Cosmic energy equation
    110
    Spherical accretion model
    115
    Hierarchical clustering model
    120
    Fourier transform of the equations of motion
    124
    Coupling of density fluctuations
    128
    DESCRIPTIVE STATISTICS
    138
    Fair sample hypothesis
    142
    Twopoint spatial correlation function tr
    143
    another definition
    145
    Poisson model
    147
    Threepoint correlation function
    148
    Fourpoint correlation function
    150
    Moments of counts of objects
    152
    Constraints on t and f
    156
    Probability generating function
    158
    Estimates of PN
    160
    Cluster model
    163
    Power spectrum
    166
    Power law model for the spectrum
    169
    Bispectrum
    171
    Cross correlation function
    172
    Angular twopoint correlation function
    174
    Angular power spectrum
    175
    Estimating w6
    183
    Statistical uncertainty in the estimate of w0
    187
    Relation between angular and spatial twopoint correlation functions
    189
    Small separation approximation and the scaling relation
    191
    Decoupling of magnitude and position
    194
    Relation between t and w some examples
    195
    Inversion of the equation
    200
    Angular threepoint correlation function
    203
    Angular fourpoint correlation function
    209
    Correction for curvature and expansion
    213
    Summary of numerical results
    221
    Power spectrum of the extragalactic light
    225
    Moments of the number of neighbors
    230
    Model for PN
    233
    Clustering models
    236
    Mandelbrots prescription
    243
    The mass correlation functions
    249
    continuity speculation
    253
    Remarks on the observations
    255
    DYNAMICS AND STATISTICS
    257
    Definitions of variables and distribution functions
    258
    BBGKY hierarchy equations
    259
    Fluid limit
    262
    Evolution of the integral of
    264
    Particle conservation equations
    266
    Relative peculiar velocity dispersion
    272
    Similarity solution
    275
    Cosmic energy equation
    278
    Cosmic virial theorem
    280
    Joint distribution in position and velocity
    285
    Behavior of the halo around a cluster of galaxies
    291
    Superclusters
    299
    Problems and prospects
    301
    RELATIVISTIC THEORY OF THE BEHAVIOR OF IRREGULARITIES IN AN EXPANDING WORLD MODEL
    304
    Timeorthogonal coordinates
    306
    The field equations for haf
    310
    Gravitational waves
    312
    Newtonian approximation
    313
    Linear perturbation equations for the matter
    317
    Behavior of density perturbations at wavelength ct
    319
    Spherical model
    324
    Evolution of acoustic waves
    330
    Nonlinear acoustic waves
    333
    Incompressible flow
    341
    Behavior of collisionless particles
    345
    Linear dissipation of adiabatic perturbations
    352
    Residual fluctuations in the microwave background
    363
    Isothermal perturbations
    373
    SCENARIOS
    379
    Nature of protogalaxies and protoclusters
    384
    APPENDIX
    395
    LIST OF ABBREVIATIONS
    401
    INDEX
    417
    Copyright
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