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Contents
Introduction
Objectives of the Study
Outline of the Thesis
Formation of Large-scale Structures
Matter Content of the Universe
Origin of Structures
Historical Perspective
Gravitational Instability
Generation of Perturbations
Peculiar Velocity Fields
The Local Group and the Local Neighbourhood
The Dynamics of Galaxies
Simplifying Assumptions
Hamilton's principle
Equations of Motion
The Lagrangian
The Orbits
Calculating the Equation of Motion
Numerical Methods
Introduction
Integration
Optimization
Method of Steepest Descent
Method of Conjugate Gradients
The Newton-Raphson Method
Secant Method
Orbits of Galaxies
Implementation of the AVP
The
AVP
Code
Trial Orbits
N-body Algorithm
Small-N Systems
The
NBODY1
Algorithm
N-body Solution of the Trial Orbits
First Evaluation of Optimizing Methods
Orbits of Galaxies in the LG and the LN
The System Parameters
Extended Evaluation of Optimizing Methods
A Physical Discussion
Review of the AVP
Areas of Application
Different Implementations
Conclusions
A brief Summary
Suggestions for Future Work
References
The
AVP
Sourcecode
Framework
Optimizing Methods
Modules
Input Files
Addition to the
NBODY1
Code
About this document ...
Trond Hjorteland
Mon Jul 5 02:59:28 MET DST 1999