Contributions to the TASI-02 and TASI-03 summer schools.
Report-no: SU-GP-04/1-1
astro-ph/0401547

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TASI LECTURES: INTRODUCTION TO COSMOLOGY

Mark Trodden 1 and Sean M. Carroll 2


1 Department of Physics, Syracuse University, Syracuse, NY 13244-1130, USA
2 Enrico Fermi Institute, Department of Physics,
and Center for Cosmological Physics, University of Chicago, 5640 S. Ellis Avenue, Chicago, IL 60637, USA


Abstract. These proceedings summarize lectures that were delivered as part of the 2002 and 2003 Theoretical Advanced Study Institutes in elementary particle physics (TASI) at the University of Colorado at Boulder. They are intended to provide a pedagogical introduction to cosmology aimed at advanced graduate students in particle physics and string theory.


Table of Contents

INTRODUCTION

FUNDAMENTALS OF THE STANDARD COSMOLOGY
Homogeneity and Isotropy: The Robertson-Walker Metric
Dynamics: The Friedmann Equations
Flat Universes
Including Curvature
Horizons
Geometry, Destiny and Dark Energy

OUR UNIVERSE TODAY AND DARK ENERGY
Matter: Ordinary and Dark
Supernovae and the Accelerating Universe
The Cosmic Microwave Background
The Cosmological Constant Problem(s)
Dark Energy, or Worse?

EARLY TIMES IN THE STANDARD COSMOLOGY
Describing Matter
Particles in Equilibrium
Thermal Relics
Vacuum displacement
Primordial Nucleosynthesis
Finite Temperature Phase Transitions
Topological Defects
Baryogenesis
Baryon Number Violation

INFLATION
The Flatness Problem
The Horizon Problem
Unwanted Relics
The General Idea of Inflation
Slowly-Rolling Scalar Fields
Attractor Solutions in Inflation
Solving the Problems of the Standard Cosmology
Vacuum Fluctuations and Perturbations
Reheating and Preheating
The Beginnings of Inflation

REFERENCES

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