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Preface | |
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Acknowledgments | |
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Homogeneity and Clustering | |
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Homogeneity and clustering | |
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Is the universe homogeneous? | |
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Physical principles | |
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How did galaxies and clusters of galaxies form? | |
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Summary | |
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Behavior of Irregularities in the Distribution of Matter: Newtonian Approximation | |
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Newtonian approximation | |
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Particle dynamics in expanding coordinates | |
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The peculiar acceleration | |
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Two models: the Vlasov equation and the ideal fluid | |
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Linear perturbation approximation for [delta] | |
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Solutions for [delta](t): p = [Lambda] = 0 | |
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Solutions for [delta](t): effect of a uniform radiation background | |
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Solutions for [delta](t): models with [Lambda not equal] 0 | |
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The peculiar velocity field | |
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Joining conditions for [delta] and [upsilon] | |
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Critical Jeans length | |
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Primeval magnetic field as a source for [delta rho] / [rho] | |
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Second order perturbation theory for [delta rho] / [rho] | |
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Spherical model | |
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Homogeneous ellipsoid model | |
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Caustics and pancakes | |
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Expansion, vorticity, and shear | |
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Origin of the rotation of galaxies | |
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Cosmic energy equation | |
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Spherical accretion model | |
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Hierarchical clustering model | |
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Fourier transform of the equations of motion | |
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Coupling of density fluctuations | |
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n-Point Correlation Functions: Descriptive Statistics | |
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Statistical measures of the galaxy distribution | |
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Fair sample hypothesis | |
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Two-point spatial correlation function [xi](r) | |
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Two-point correlation function: another definition | |
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Two-point correlation function: Poisson model | |
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Three-point correlation function | |
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Four-point correlation function | |
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Moments of counts of objects | |
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Constraints on [xi] and [zeta] | |
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Probability generating function | |
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Estimates of P[subscript N] | |
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Cluster model | |
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Power spectrum | |
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Power law model for the spectrum | |
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Bispectrum | |
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Cross correlation function | |
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Angular two-point correlation function | |
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Angular power spectrum | |
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Estimating w([theta]) | |
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Statistical uncertainty in the estimate of w([theta]) | |
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Relation between angular and spatial two-point correlation functions | |
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Small separation approximation and the scaling relation | |
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Decoupling of magnitude and position | |
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Relation between [xi] and w: some examples | |
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Inversion of the equation | |
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Angular three-point correlation function | |
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Angular four-point correlation function | |
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Correction for curvature and expansion | |
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Summary of numerical results | |
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Power spectrum of the extragalactic light | |
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Moments of the number of neighbors | |
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Model for P[subscript N] | |
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Clustering models | |
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Continuous clustering hierarchy: Mandelbrot's prescription | |
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The mass correlation functions | |
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Clustering hierarchy: continuity speculation | |
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Remarks on the observations | |
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Dynamics and Statistics | |
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Goals | |
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Definitions of variables and distribution functions | |
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BBGKY hierarchy equations | |
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Fluid limit | |
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Evolution of the integral of [xi] | |
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Particle conservation equations | |
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Relative peculiar velocity dispersion | |
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Similarity solution | |
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Cosmic energy equation | |
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Cosmic virial theorem | |
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Joint distribution in position and velocity | |
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Behavior of the halo around a cluster of galaxies | |
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Superclusters | |
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Problems and prospects | |
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Relativistic Theory of the Behavior of Irregularities in an Expanding World Model | |
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Role of the relativistic theory | |
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Time-orthogonal coordinates | |
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The field equations for h[subscript alpha beta] | |
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Gravitational waves | |
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Newtonian approximation | |
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Linear perturbation equations for the matter | |
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Behavior of density perturbations at wavelength [characters not reproducible] ct | |
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Spherical model | |
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Evolution of acoustic waves | |
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Nonlinear acoustic waves | |
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Incompressible flow | |
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Behavior of collisionless particles | |
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Linear dissipation of adiabatic perturbations | |
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Residual fluctuations in the microwave background | |
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Isothermal perturbations | |
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Scenarios | |
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Nature of the universe at high redshift | |
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Nature of protogalaxies and protoclusters | |
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Appendix | |
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Models and notation | |
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List of Abbreviations | |
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References | |
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Index | |