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THE COSMIC MICROWAVE BACKGROUND (CMB)
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Classroom Contents
Simulating Universes
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- 1 Intro
- 2 CRASH COURSE COSMOLOGY
- 3 THE COSMIC MICROWAVE BACKGROUND (CMB)
- 4 DISCRETIZATION
- 5 N-BODY SIMULATION IN TWO DIMENSIONS
- 6 1977: SOVIET TECHNOLOGY
- 7 2005: MILLENNIUM SIMULATION
- 8 2017: EUCLID FLAGSHIP SIMULATION
- 9 DARK MATTER HALOES: FINDING AND TRACKING THEM
- 10 THE NFW-PROFILE
- 11 COMPARING WITH GALAXY SURVEYS
- 12 (QUASI-) LAGRANGIAN HYDRODYNAMICS
- 13 EXAMPLE: KELVIN-HELMHOLTZ INSTABILITY WITH AREPO
- 14 SUB-GRID MODELS: SUPERNOVAE IN A DWARF GALAXY
- 15 SUB-GRID MODELS: BLACK HOLES IN MERGING MASSIVE GALAXIES
- 16 HALO MASS TO STELLAR MASS RATIO
- 17 FASTER
- 18 CONSTRAINED N-BODY SIMULATIONS
- 19 OPENING THE VAULTS
- 20 TAKE HOME MESSAGES
