DARK MATTER. Seen making gravitational interactions: rotational curves, CMB, gravitational lensing. BBN, bullet. Multimedia: Images

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DARK MATTER Seen making gravitational interactions: rotational curves, CMB, gravitational lensing. BBN, bullet Multimedia: Images Aliases: Wimp, Neutralino.. Age: approximately 14 billions years Weight: approximately 0.01-1 TeV Interaction: gravitational, weak Distinctive features: tendency to escape

χ SM χ SM dark matter searches of all kinds put constraints on different observables Without some kind of theoretical structure, we can t compare them. VERY Important to asses if searched topologies are exhaustive

The Inner Detector provides around 3 pixel, 8 SCT and 30 TRT measurements per charged track at η = 0. Coverage: η < 2.5 (2.0 for TRT) Resolution goal: σ pt /p T = 0.05% p T 1% η=-ln(tan(θ/2))

CONTAT INTERACTION

DM Searches: MONO-X

DM Searches: MONO-jet

MONO-Z/W

Dark matter searches interplay: EFT

EFT signal in direct detection

EFT results from all searches: 2013 Snomass Report example S.arXiv:1310.8621v1 σ σσ

χ ν

βμ

χ χ ±

χ χ ± χ Δ χχ Δ χ Δ χχ

bwχ, χ, χ Δ

EW SUSY production χ ± χχχ

EW SUSY production χ ± χχχ

χ ± /χ

MONO-X and SUSY Searches get together

pmssm scan S.arXiv:1310.8621v1

Conclusion

Higgs decay to DM: MONO-Z

Search for resonances in dilepton

Z Searches: resonances in dilepton

N events t = Lσ L = N 1 N 2 4πσ x σ y F

Neutral MSSM higgs: Φ(h,H,A) ττ High sensitivity at large tan(β) Enhanced coupling to down type fermions Address specifically associated production with b No additional signal observed in ττ final state Result interpretation (limits) within specific models m h max scenario: stop mixing term determined form maximization of lightest higgs boson mass

Neutral MSSM higgs: Φ(hHA) bb High sensitivity at large tan(β) Enhanced coupling to down type fermions No signal observed m h max scenario: stop mixing term determined form maximization of lightest higgs boson mass

Charged higgs: th ± b, th ± b (H ± τν) Two searches: MH<m t MH>m t No excess found upper limits assuming B(H ± τν)=1

Charged higgs: th ± b, th ± b (H ± τν) Two searches: MH<m t MH>m t Interpretation in the m h max scenario

Gauge Mediated SUSY Breaking models χ γ χ

GMSB searches: χ NLSP small lifetime χγ χ

χ ± χ 2 production trilepton signature

GMSB searches: χ NLSP medium lifetime χγ

MONO-W

GMSB : τ NLSP short and long lifetime ττ τ

Squarks/gluinos with long lifetime Δχ

Exotics searches

What will be reported What will not be reported CMS EXOTICA 95% CL EXCLUSION LIMITS (TEV) q* (qg), dijet q* (qw) q* (qz) q*, dijet pair q*, boosted Z e*, Λ = 2 TeV μ*, Λ = 2 TeV Z SSM (ee, μμ) Z SSM (ττ) Z (tt hadronic) width=1.2% Z (dijet) Z (tt lep+jet) width=1.2% Z SSM (ll) fbb=0.2 G (dijet) G (ttbar hadronic) G (jet+met) k/m = 0.2 G (γγ) k/m = 0.1 G (Z(ll)Z(qq)) k/m = 0.1 W (lν) W (dijet) W (td) W WZ(leptonic) WR (tb) WR, MNR=MWR/2 WKK μ = 10 TeV ρtc, πtc > 700 GeV String Resonances (qg) s8 Resonance (gg) E6 diquarks (qq) Axigluon/Coloron (qqbar) gluino, 3jet, RPV gluino, Stopped Gluino stop, HSCP stop, Stopped Gluino stau, HSCP, GMSB hyper-k, hyper-ρ=1.2 TeV neutralino, cτ<50cm 0 1 2 3 4 5 6 0 1 2 3 4 5 6 Long Lived Compositeness Heavy Resonances LQ1, β=0.5 LQ1, β=1.0 LQ2, β=0.5 LQ2, β=1.0 LQ3 (bν), Q=±1/3, β=0.0 LeptoQuarks LQ3 (bτ), Q=±2/3 or ±4/3, β=1.0 stop (bτ) 0 1 2 3 4 5 b tw, (3l, 2l) + b-jet q, b /t degenerate, Vtb=1 b tw, l+jets B bz (100%) T tz (100%) t bw (100%), l+jets t bw (100%), l+l 0 1 2 C.I. Λ, Χ analysis, Λ+ LL/RR C.I. Λ, Χ analysis, Λ- LL/RR C.I., μμ, destructve LLIM C.I., μμ, constructive LLIM C.I., single e (HnCM) C.I., single μ (HnCM) C.I., incl. jet, destructive C.I., incl. jet, constructive 0 5 10 15 Ms, γγ, HLZ, ned = 3 Ms, γγ, HLZ, ned = 6 Ms, ll, HLZ, ned = 3 Ms, ll, HLZ, ned = 6 MD, monojet, ned = 3 MD, monojet, ned = 6 MD, mono-γ, ned = 3 MD, mono-γ, ned = 6 MBH, rotating, MD=3TeV, ned = 2 MBH, non-rot, MD=3TeV, ned = 2 MBH, boil. remn., MD=3TeV, ned = 2 MBH, stable remn., MD=3TeV, ned = 2 MBH, Quantum BH, MD=3TeV, ned = 2 4th Generation 0 1 2 3 4 5 Contact Interactions Extra Dimensions & Black Holes Sh. Rahatlou 0 1 2 3 4 5 6 0 1 2 3 4 51

bwχ, χ Δ