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Conclusion
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Classroom Contents
Dark Matter Freeze-out During SU(2)L Confinement
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- 1 Intro
- 2 Particle physics and cosmological history
- 3 Why consider alternate cosmological histories
- 4 How to modify cosmological history?
- 5 WIMP dark matter (DM) freeze-out
- 6 Schematic outline of calculation
- 7 WIMP dark matter in this scenario
- 8 Confinement details
- 9 Pion masses and remaining gauge symmetries
- 10 Deriving pion interactions
- 11 WIMP freeze-out in this scenario
- 12 Experimental constraints: Direct detection
- 13 Other experimental constraints
- 14 Main takeaway
- 15 Conclusion
