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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.FUNDAMENTALS OF THE STANDARD
COSMOLOGY
- 2.1.Homogeneity and Isotropy: The
Robertson-Walker Metric
- 2.2.Dynamics: The Friedmann
Equations
- 2.3.Flat Universes
- 2.4.Including Curvature
- 2.5.Horizons
- 2.6.Geometry, Destiny and Dark
Energy
- 3.OUR UNIVERSE TODAY AND DARK ENERGY
- 3.1.Matter: Ordinary and Dark
- 3.2.Supernovae and the
Accelerating Universe
- 3.3.The Cosmic Microwave
Background
- 3.4.The Cosmological Constant
Problem(s)
- 3.5.Dark Energy, or Worse?
- 4.EARLY TIMES IN THE STANDARD
COSMOLOGY
- 4.1.Describing Matter
- 4.2.Particles in Equilibrium
- 4.3.Thermal Relics
- 4.4.Vacuum displacement
- 4.5.Primordial Nucleosynthesis
- 4.6.Finite Temperature Phase
Transitions
- 4.7.Topological Defects
- 4.8.Baryogenesis
- 4.9.Baryon Number Violation
5.INFLATION
5.1.The Flatness Problem
5.2.The Horizon Problem
5.3.Unwanted Relics
5.4.The General Idea of Inflation
5.5.Slowly-Rolling Scalar Fields
5.6.Attractor Solutions in
Inflation
5.7.Solving the Problems of the
Standard Cosmology
5.8.Vacuum Fluctuations and
Perturbations
5.9.Reheating and Preheating
5.10.The Beginnings of Inflation
REFERENCES