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Dark Matter @ Colliders David-fest 2011 Roni Harnik, Fermilab Bai, - PowerPoint PPT Presentation

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Dark Matter @ Colliders David-fest 2011 Roni Harnik, Fermilab Bai, Fox, RH - 1005.3797 Fox, RH, Kopp, Tsai -1103.0240 Fox, RH, Kopp, Tsai - 1109.4389 Very related work by the Irvine Clan: Goodman, Ibe, Rajaraman, Shepherd, Tait and

  1. Dark Matter @ Colliders David-fest 2011 Roni Harnik, Fermilab Bai, Fox, RH - 1005.3797 Fox, RH, Kopp, Tsai -1103.0240 Fox, RH, Kopp, Tsai - 1109.4389 Very related work by the “Irvine Clan”: Goodman, Ibe, Rajaraman, Shepherd, Tait and Haibo Yu -1005.1286 Goodman, Ibe, Rajaraman, Shepherd, Tait and Haibo Yu - 1008.1783 Fortin and Tait - 1103.3289 Rajaraman, Shepherd,Tait and Wijangco - 1108.1196 Shepherd and Goodman - 1111.2359

  2. Dark Matter needs no introduction.

  3. But it has a lot to answer for: What sets its abundance? Does it interact with matter apart from gravity? How strong/weak are these interactions? Does it fit into a larger framework? What is the particle mediating this interaction?

  4. But it has a lot to answer for: What sets its abundance? Does it interact with matter apart from gravity? How strong/weak are these interactions? Answers (and limits) come from direct & indirect searches . Directly complemented by past and present colliders. Does it fit into a larger framework? What is the particle mediating this interaction?

  5. But it has a lot to answer for: What sets its abundance? Does it interact with matter apart from gravity? How strong/weak are these interactions? Answers (and limits) come from direct & indirect searches . Directly complemented by past and present colliders. Does it fit into a larger framework? What is the particle mediating this interaction? LHC (e.g. Higgs mediated interactions)

  6. Outline Motivation: Colliders as direct detection experiments. Tevatron & LHC mono-jets: Rough estimates. Operators Results LEP mono-photons. Scattering via the Higgs & LHC Higgs searches. Coffee.

  7. The WIMP Hint Does DM have interactions with matter? If we throw a weakly interacting particle with weak scale mass into the primordial hot soup, , the DM abundance comes out roughly right. DM SM Hint: There is an interaction. Leads to pb-ish cross sections DM SM

  8. Probes of DM Interactions We hope to probe dark matter in several ways: DM-nucleus scattering DM annihilation DM DM DM q DM ¯ q q q direct indirect Focus on direct detection in this talk. (a similar game can be played for indirect)

  9. Direct detection DM DM Direct detection places limits on . q q Heroic effort with remarkable results. DD has some weaknesses. -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  10. Direct detection DM DM Direct detection places limits on . q q Heroic effort with remarkable results. DD has some weaknesses. -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 low mass XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  11. Direct detection DM DM Direct detection places limits on . q q Heroic effort with remarkable results. DD has some weaknesses. spin dependent -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 low mass XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  12. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  13. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  14. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na XENON100 -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ]

  15. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na XENON100 -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ] tri-leptons+ jets + MET

  16. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na XENON100 -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ] tri-leptons+ jets + MET jets + MET

  17. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na XENON100 -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) { Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ] tri-leptons+ same-sign jets + MET jets + MET di-leptons +MET

  18. Collider Connections? DM experiments and colliders are often said to be related in a specific framework (SUSY) . -39 -39 10 10 DAMA/Na XENON100 -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) { Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 100 100 200 200 300 400 300 400 1000 1000 2 2 WIMP Mass [GeV/c WIMP Mass [GeV/c ] ] tri-leptons+ same-sign jets + MET jets + MET di-leptons +MET “XENON100 is starting to probe the MSSM’s pseudopod, LHC killed the Membrane, but the ectoplasm is still safe.” [submitted to nature]

  19. A Simple Point In order to get a particular DM-nucleon cross -39 -39 10 10 DAMA/Na -40 -40 10 10 ] ] 2 2 WIMP-Nucleon Cross Section [cm WIMP-Nucleon Cross Section [cm CoGeNT DAMA/I section, , we assume the existence of -41 -41 10 10 CDMS -42 -42 10 10 EDELWEISS -43 -43 10 10 XENON100 (2010) -44 -44 10 10 XENON100 (2011) Buchmueller et al. -45 -45 10 10 6 7 8 910 6 7 8 910 20 20 30 30 40 50 40 50 200 200 300 400 300 400 100 100 1000 1000 DM 2 2 DM WIMP Mass [GeV/c WIMP Mass [GeV/c ] ] a DM-hadron interaction, . q q The same interaction can lead to DM production at a hadron machine. DM q p ¯ p → nothing ¯ q DM

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