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 Ω^0.6/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