LARGE SCALE STRUCTURE IN THE UNIVERSE
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