Chapter 4. Dark Matter in the Universe
- 4.1. Overview
- 4.1.1. The Virial Theorem
- 4.2. Evidence for Dark Matter as a
Function of Scale Size
- 4.2.1. The Solar System
- 4.2.2. The Solar Neighborhood
- 4.2.3. Galactic Scales
- 4.3. Other Dark Matter Indicators
for Galaxies
- 4.3.1. Hot Halos Around Elliptical
Galaxies
- 4.3.2. Binary Galaxies
- 4.3.3. Stellar Population Effects
on Mass-to-Light Ratios
- 4.3.4. Some Measured Values for
M / L
- 4.3.5. Clusters of Galaxies
- 4.4. The Large Scale Distribution of
Dark Matter
- 4.5. The Inflationary Paradigm and
OMEGA = 1
- 4.6. Dark Matter Candidates and
Detection
- 4.6.1. Normal Baryonic Dark Matter
- 4.6.2. Exotic Baryonic Dark Matter
- 4.6.3. Nucleosynthesis Constraints
on Baryonic Matter
- 4.6.4. Non-baryonic Dark Matter
- 4.6.5. Direct Detection of Dark
Matter
- 4.6.6. The Microlensing Surveys
- 4.6.7. The Solar Neutrino Experiment
- 4.7. Further Implications of Dark
Matter
- 4.8. Summary