Dark Matter Freeze-out During SU(2)L Confinement

Dark Matter Freeze-out During SU(2)L Confinement

Harvard CMSA via YouTube Direct link

Deriving pion interactions

10 of 15

10 of 15

Deriving pion interactions

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Classroom Contents

Dark Matter Freeze-out During SU(2)L Confinement

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

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