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https://doi.org/10.1142/9789814532464Cited by:0 (Source: Crossref)
Abstract:

The Table of Contents for the full book PDF is as follows:

  • Preface

  • Photograph of Participants

  • List of Participants

  • I. Observing Large Scale Structure

    • Comparison of Large Scale Structures and Velocities

    • The Peculiar Velocity Field from Sc Galaxies

    • Estimation of Peculiar Velocity from the Inverse Tully-Fisher Relation

    • Measuring the Value of Ω0.6/b Using Redshift Space Distortions in the Stromlo-APM Survey

    • Variational Principle Analysis of Orbits in the Local Supercluster

    • Constraints on Large Scale Structure from X-Ray Surveys

    • Large Scale Structure in the Las Campanas Redshift Survey

    • Principles and Applications of Low-Resolution

    • Redshift Surveys

    • Large Scale Structure in the Durham/UKST Galaxy Redshift Survey

  • II. Formation of Large Scale Structure

    • The Formation and Evolution of Large Scale Structure

    • The Physical Measurement of Large Scale Structure

    • Formation of the Supercluster-Void Network

    • The Distribution of Rich Clusters – A Chessboard Universe?

    • Void Hierarchy in the Northern Local Supervoid

    • The Evolution of the Supercluster-Void Network

    • Constraints on the Power Spectrum of Mass Fluctuations from Galaxy Cluster Peculiar Velocities

    • Formation of Large Scale Structures and Quasars as its Tracers

    • Angular Correlation Function of Galaxies in CDM and C+HDM Models

    • On Estimating ξ(r): to Weight or not to Weight?

    • Mixed Cold-Hot Dark Matter Models with Several Massive Neutrino Types

    • Large Scale Structure from Perturbation Spectra with Broken Scale Invariance

    • Large Scale Structure of the Universe from Blue Primordial Perturbation Spectra

  • III. Measures of Large Scale Structure

    • The Largest Structures in the Universe

    • The Void Probability Function: A Severe Test for Dark Matter Models

    • Voids and Their Evolution in the Adhesion Model

    • A Two-Fluid Model for the Formation of Large Scale Structure

    • Robust Morphological Measures for Large Scale Structure

    • Weakly Nonlinear Evolution of Topology of Large Scale Structure

    • Velocity Field and Thermal Evolution of Gas for Spectra with Broken Scale Invariance

    • Redshift Distortion of Clustering: A Lagrangian Approach

    • Higher Moments of Large Scale Cosmic Fields

  • IV. Cosmological Aspects of Clusters of Galaxies

    • X-Ray Clusters of Galaxies as Cosmological Probes

    • X-Ray Temperature vs. Galaxy Velocity Dispersion in Galaxy Clusters

    • X-Ray and Radio Observations of the Bimodal Galaxy Cluster A3528

    • Cosmology with Clusters of Galaxies

    • The Cluster Distribution as a Test for Dark Matter Models

    • On the Omega-Dependence of Cluster Density Profiles

    • Substructures of Clusters and Cosmological Models

    • Cluster Abundance from Perturbation Spectra with Broken Scale Invariance

    • Evolution of the X-Ray Luminosity Function of Clusters of Galaxies

    • Microwave Background Fluctuations due to Nonlinear Structures: A Short Assessment of the Subject

    • The Morphological Types of Central Dominant Galaxies in Clusters

  • V. QSO Absorption Lines and Galaxy Formation

    • QSO Absorption Line Systems

    • Modelling of QSO Absorption Line Distribution with N-Body Simulations

    • Constraining Galaxy Formation Models by Observations of Damped Lyman Alpha Systems

    • Quasar Absorption Lines and the Parameters of the Friedmann Universe

    • Physical Mechanisms for Biased Galaxy Formation

    • Numerical Models of Galaxy Formation and Evolution

    • Faint Field Galaxies: A Population of Intrinsically Faint Objects at Low Redshift?

  • VI. Gravitational Lensing

    • Cluster Masses from Weak Lensing

    • The Correlation of 1-Jansky Sources to Zwicky Clusters

    • Determining the Mass Distribution of Clusters from Gravitational Lensed Background Galaxies

    • Studying Gravitational Lens Properties of Cosmogonic Models

    • Quadruple Lenses: A Probe for (Dark) Matter Distribution

    • Chromatic, Spectroscopic and Polarisation Effects in Microlensing Events from Stellar Sources

  • VII. Theoretical Models

    • Inhomogeneous Cosmological Models and their Homogenization

    • Decay and Production of Particles in Fluid Cosmology

    • Chiral Non-Linear Sigma Models and Problems of an Inflationary Cosmology

    • Non-Flat Primordial Power Spectra

    • Stability Properties of the Starobinsky Cosmological Model

    • Multidimensional Cosmological Models as Dynamical Systems

    • Primordial Nucleosynthesis Constraints of Conformal Weyl Gravity Cosmological Models

    • Distortion of the MWB Spectrum by the Primeval Hydrogen Recombination

    • Primordial Magnetic Fields in String Cosmology

    • Comparison of Nonlinear Approximations to Gravitational Instability

    • Optimized Lagrangian Approximations for Modelling Large Scale Structure at Non-Linear Stages

  • VIII. Summary

    • Rating Cosmological Models