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Cluster Mergers, e.g. Bullet Cluster
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Classroom Contents
The Quest for Dark Matter
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- 1 Intro
- 2 Big Bang Nucleosynthesis
- 3 Cosmic Microwave Background
- 4 Structure Formation
- 5 Cluster Mergers, e.g. Bullet Cluster
- 6 Typical Rotation Curve: M33
- 7 Dark Matter Has Been Discovered have evidence at all time scales and vast length scales have no clue what Dark Matter is made of
- 8 Simulation: Cold or Warm?
- 9 X-Section From Astrophysics are galaxies and Dark Matter offset?
- 10 Sterile Neutrinos
- 11 3.5kV Line: 7keV vs?
- 12 ADMX Resonant Axion Search microwave cavity, up to 8T, down to 100mk cover most expected parameter space by -2016 gemeration-3 ADMX to probe fractional halo densities
- 13 Thermal Relic Particles
- 14 WIMPs at the LHC
- 15 Mono-Jet Final State
- 16 Electrons, and Positron Excess
- 17 FERMI Galactic Center
- 18 FERMI Dwarf Galaxies
- 19 Direct Recoil Search
- 20 Direct Scattering - Simplified
- 21 SuperCDMS: Ge Crystals First analysis of 577 kg days optimized for GeV WIMP
- 22 LUX: Xenon TPC
- 23 Direct Scattering - Outlook
- 24 Conclusions • Dark Matter exists no clue what it is made of
