hep-ph/0111080
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2 NASA/Fermilab Astrophysics Center
Fermi National
Accelerator Laboratory
P. O. Box 500, Batavia, IL 60510
3 Department of Astronomy & Astrophysics
The University of
Chicago
5640 S. Ellis Avenue, Chicago, IL 60637
4 Department of Physics
Syracuse University
Syracuse, NY, 13244-1130
Abstract. This is the report of the Working Group on Early Universe Cosmology and Tests of Fundamental Physics, group P4.8 of the of the Snowmass 2001 conference. Here we summarize the impressive array of advances that have taken place in this field, and identify opportunities for even greater progress in the future. Topics include Dark Energy, Cosmic Acceleration, Inflation, Phase Transitions, Baryogenesis, and String/M-theory Cosmology. The introductory section gives an executive summary with six key open questions on which we can expect to make significant progress.
Table of Contents
INTRODUCTION
DARK MATTER
DARK ENERGY AND THE ACCELERATING UNIVERSE
Inflation: Models Tests and Alternatives
Overview
The basic idea
Tests of Inflation
Density
Coherence from inflation
Gravity waves from inflation
The scalar spectral index
Further tests of inflation
Can one really test inflation?
Inflation and fundamental physics
Alternatives to inflation
PHASE TRANSITION AND THEIR RELICS
Overview
The many roles of cosmic phase transitions
BARYOGENESIS
FUNDAMENTAL PHYSICS AND COSMOLOGY
Finite Temperature String / M-Theory and
Cosmology
Extra Dimensions and Cosmology
de-Sitter Space as a Solution to M-Theory
Transplanckian Physics and Cosmology
REFERENCES