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Direct Detection Signals from Absorption of Fermionic Dark Matter J. A. Dror, G. Elor, Robert McGehee 1905.12635, 1908.XXXXX DPF 2019, 8/1/2019 Disclaimer Youre probably tiredits Day 4, after Lunch My promises to you: This


  1. Direct Detection Signals from Absorption of Fermionic Dark Matter J. A. Dror, G. Elor, Robert McGehee 1905.12635, 1908.XXXXX DPF 2019, 8/1/2019

  2. Disclaimer You’re probably tired…it’s Day 4, after Lunch… My promises to you: • This slide has by far the most text (besides the summary). • I’ll start my talk with story time! • There’s not a single equation! • I’ve hidden a picture of Einstein! Robert McGehee

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  11. Fermionic “Absorption” χ ν N, 𝑓 − N, 𝑓 − Robert McGehee

  12. Fermionic “Absorption” 𝑓 ± χ ν χ N, 𝑓 − N, 𝑓 − N’ N Robert McGehee

  13. Fermionic “Absorption” 𝑓 − χ ν χ N’ N N N Robert McGehee

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  16. “Neutral Current” Kinematics χ ν N N Robert McGehee

  17. Preliminary 1908.XXXXX Robert McGehee

  18. Preliminary 1908.XXXXX Robert McGehee

  19. 1905.12635 Robert McGehee

  20. 1905.12635 Robert McGehee

  21. 1905.12635 Robert McGehee

  22. 1905.12635 Robert McGehee

  23. 1905.12635 Robert McGehee

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  25. 1905.12635 Robert McGehee

  26. “Charged Current” Induced β − Decays 𝑓 − χ N’ N • 𝑓 − ! • NR! • γ ! • N’ Decay! Robert McGehee

  27. 1905.12635 Robert McGehee

  28. Summary Relaxing DM stability assumptions allows for novel signals and operators. Neutral current operators yield peaked, correlated nuclear recoil (NR) signals. Charged current operators yield β − , NR, and γ signals. New searches at existing experiments can probe both neutral and charged current operators. Fermionic DM absorption is an exciting playground for both experiments and model building! Robert McGehee

  29. Backup Slides Robert McGehee

  30. Preliminary 1908.XXXXX Robert McGehee

  31. Preliminary 1908.XXXXX Robert McGehee

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