— Cosmic Structure Formation
Growth of structure from small density inhomogeneities in the early universe to the diverse structures observable today. Use of observable properties (cosmic microwave background, gravitational lensing, peculiar velocities, number density, etc.) to constrain models of structure formation and fundamental physics.
Prerequisites & course information
Course Description: Growth of structure from small density inhomogeneities in the early universe to the diverse structures observable today. Use of observable properties (cosmic microwave background, gravitational lensing, peculiar velocities, number density, etc.) to constrain models of structure formation and fundamental physics. Learning Activities: Lecture 3 hour(s). Grade Mode: Letter. Learning Activities: Lecture 3 hour(s). Grade Mode: Letter.
Sources
- Course catalogue ↗2026-2027