Contents


Abstract
.
Contents
List of Figures
List of Tables
Acknowledgements
Declaration
Introduction
Introduction to Cosmogony
The Laplace Nebula Theory: Monistic
Revival of the Laplace Model
The Roche Limit
Jeans' Tidal Theory: Dualistic
The Jeans Mass
Objections to Jeans' Tidal Theory
Further Comments on Jeans' Tidal Theory
The Capture Theory
The Solar Nebula Theory
The Capture Process
Towards a Complete Theory of Planetary Formation
The Interstellar Medium and Star Formation
Star-Star Interactions
Planetary Formation
Satellite Formation
Orbital Evolution
The Terrestrial Planets
Explained Features of the Solar System
Smoothed Particle Hydrodynamics
Motivation
The Kernel and the Smoothing Length
Variable Smoothing Lengths
Constant Number of Neighbours
Neighbour Search Algorithm
Forces
Hydrodynamical Forces
General SPH Equations and Derivatives
Artificial Viscosity
Gravitational Forces
Gravitational Softening
Consistent Representation of Matter
Sphere-Sphere Gravitational Softening
Point-Sphere Gravitational Softening
The Equation of State
Energy Equations
Time Integration
Choice of Integrator
Embedded Improved Euler Scheme
Time-Step Control
Additional Computational Techniques
Tree Gravity
Principles and Methods
Tree implementation
Tree Construction
Tree Storage in Memory
Centre of Mass Calculation
Force Calculation
TreeSPH
Tree Radiation
Motivation
Radiative Principles and Assumptions
Opacity
A First Idea
Tree Radiation Method
Defining the Tree
Interpolating the Particle Properties to the Tree
Tree Absorption Properties
Radiative Energy Transfer Process
Additional Tree Walking Considerations
Time integration
Rate of Transfer Considerations
Interpolating the Tree Energy to the Particles
Testing the Code
Gravity
Initial Configuration
Uniform Grid - Point Mass Force
Uniform Grid - Softened Force
Displaced Grid - Softened Force
Free-Fall curves
Hydrodynamics
The Structure of Polytropes
The Oscillation of Polytropes
Radiation Transport
Luminosity of an Isolated Sphere
Radiation Received from a Point Source
Equilibrium Temperatures of Illuminated Bodies
Radiation Transport in the Opaque Regime
Simulating the Capture Theory
Quasi-Static Collapse of Spherical Bodies
Low Mass Bodies
Results
Larger Mass Bodies
The Capture Mechanism
Initial Orbital Components
Quasi-Static Collapsing Protostar Interactions
Near Free-Fall Protostar Interactions: Tidal Induced Fragmentation Followed by Capture
Results
An Example Encounter: Without Solar Radiation
An Example Encounter: With Solar Radiation
Evolution of Protoplanets
Conclusion
Introduction
Smoothed Particle Hydrodynamics
Additional Computational Techniques
Testing the Code
Simulating the Capture Theory
Future Work
Conclusion
Pseudo-Code
Particle Insertion Routine During Tree Construction
Mass and Centre of Mass Calculation via $1$ Tree Traversal
Smoothing Length Calculation Routine for Particle $i$
Density Calculation for Particle $i$
Force Calculation Routine for Particle $i$
Tree Pruning via 1 Tree Traversal
Compact Tree Creation
Tree Walk for 1 Power Packet
Derivations
Free-Fall Derivation
Point Source Absorption Derivation
References
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Stephen Oxley 2002-01-19