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David Stuart, UCSB. PHENO’04 Searches for new physics at the Tevatron David Stuart, UC Santa Barbara for the CDF & D0 collaborations PHENO’04, April 26, 2004

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Page 1: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04Searches for new physicsat the Tevatron

David Stuart, UC Santa Barbara

for the CDF & D0 collaborations

PHENO’04, April 26, 2004

Page 2: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

(massabetized to avoid any indication of bias)

New physics has the same ingredients

as bread & butter physicsPhotons, MET, leptons, jets, b’s

The experimental challenge is in defining and understanding the ingredients

CDF & D0 have done that as evidenced by the SM measurements

Combine the ingredients (with some reference to cookbook) for something new.

Similar Combinations:⇒ Z or Z’

ETjets ⇒ top or LQ or SUSY or Higgs

Page 3: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

New physics has the same ingredients

as bread & butter physicsPhotons, MET, leptons, jets, b’s

Page 4: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 5: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 6: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 7: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 8: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 9: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 10: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 11: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 12: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 13: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 14: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 15: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

Page 16: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

CDF and D0 obtain Z’σ•Br limits of ≈50 fb

⇒M>750 GeV (with SM couplings)

Page 17: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass di-leptons

See talk by M.Karagoz Unel Tuesday at 3pm.

Page 18: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass e+e- and γγ

Page 19: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass e+e- and γγ

Page 20: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for high mass e+e- and γγ

= fSM + fKK η2 + fint η f = f(M,cosθ*)

η = ±πM4

S

2

Ms > 1.22 TeV (+)

Ms > 1.10 TeV (-)

Page 21: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Excited electron search (eeγγ)

Page 22: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Excited electron search (eeγγ)

See talk by H.Gerberich Tuesday at 6pm.

Page 23: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Excited electron search (eeγγ)

See talk by H.Gerberich Tuesday at 6pm.

Expect 3 ± 0.4

Observe 3

Page 24: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Excited electron search (eeγγ)

See talk by H.Gerberich Tuesday at 6pm.

Page 25: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Leptoquark Searches (eejj)

Page 26: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Leptoquark Searches (eejj)

Require Scalar Sum of eejj ET > 450 GeVσ•Br < 60 fb ⇒ M > 238 GeV/c2 if Br(LQ→eq)=1

Page 27: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Leptoquark Searches (eνjj)

Page 28: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Leptoquark Searches

Page 29: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Leptoquark Searches

Low β ⇒⇒ Jets + MET mode

Page 30: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature of<insert currently popular model name here>

Page 31: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofLarge extra dimensions

Page 32: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofLarge extra dimensions

Page 33: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofLarge extra dimensions

KK

Page 34: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofSupersymmetry

Page 35: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofSupersymmetry

Page 36: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofQuantum Chromodynamics

Page 37: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofQuantum Chromodynamics

Page 38: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofQCD or beam splash or cosmics

Page 39: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Jets+MET is a classic signature ofQCD or beam splash or cosmics

Confirm with track jets

Calorimeter timing cuts

Veto e and mu

Page 40: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Mono-Jets+MET results

KK

ET > 150 GeV

no 2nd jet with ET>50 GeV

ET > 150 GeVΔφ > 30º

Page 41: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Mono-Jets+MET results

ET > 150 GeV

no 2nd jet with ET>50 GeV

ET > 150 GeVΔφ > 30º

KK

Predictions dominated by EWK backgrounds

Z → νν + jet

W → τν + jetSignal shape is indistinguishable from background.

Page 42: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Predict 100 ± 10 Stat & δσ

Mono-Jets+MET results

Page 43: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Predict 100 ± 10 Stat & δσ

Observe 63

Mono-Jets+MET results

Page 44: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Predict 100 ± 10 Stat & δσ

Observe 63

Jet Energy scale is also a significantsystematic on background and signal.

Mono-Jets+MET results

Page 45: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Mono-Jets+MET results

Monojet

Predict 100 ± 10 Stat & δσ

Observe 63

Jet Energy scale is also a significantsystematic on background and signal.

Page 46: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Mono-Jets+MET results

Obtain limits of ≈700 GeV

Monojet

Predict 100 ± 10 Stat & δσ

Observe 63

Jet Energy scale is also a significantsystematic on background and signal.

Page 47: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Jets+MET results

ET1 > 60 GeV, ET2 > 50 GeVVeto e and µ

30º < Δφ < 165º

HT > 275

ET > 175

Page 48: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Jets+MET results

Background predictions dominated by EWK not QCD

Z → νν + 2jets

W → τν + jetExpect 2.67 ± 0.95 events

Observe 4

L = 85/pb

ET1 > 60 GeV, ET2 > 50 GeVVeto e and µ

30º < Δφ < 165º

HT > 275

ET > 175

Page 49: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Jets+MET results

Background predictions dominated by EWK not QCD

Z → νν + 2jets

W → τν + jetExpect 2.67 ± 0.95 events

Observe 4

L = 85/pb

Page 50: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Jets+MET results

Prediction and acceptance for M0 = 25 GeV/c2, A0=0, tan β = 3, µ<0, varying M1/2

L = 85/pb

Page 51: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Photons+MET

In GMSB models, gravitino is LSP ⇒

Page 52: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Photons+MET

In GMSB models, gravitino is LSP ⇒

⇒γγ+ET is a broadly sensitive signature for GMSB

Page 53: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Photons+MET

ET > 13 GeVη<1.1

ET > 45 GeV10º <Δφ(ET,j)<170º

Calorimeter timing

Page 54: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Photons+MET

ET > 20 GeVη<1.1

ET > 40 GeVΔφ(ET,γ)>30º

Δφ(ET,j)<145º

L=185/pb

Page 55: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-Photons+MET

Neutralino mass limits

≈ 105 GeV

L=185/pb

Page 56: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-leptons+MET

In MSUGRA models, neutralino LSP is stable

⇒trileptons+ET and di-leptons+ET

D0 has searched in both modes.

Page 57: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Like-sign µ±µ± +MET

Like-sign µµ

Predict 0.13 ± 0.06

Observe 1 event

Like-sign µ±µ±

pT1>11 GeV/c

pT2>5 GeV/c Δφ(ET,j)<145º

30º<Δφ(ET,µ)<145º

ET > 40 GeVMµµ < 80 GeV/c2

Page 58: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-lepton +MET + Track

Select eµ or ee + ET. Look for a 3rd, isolated track with pT > 3

Expect 1.2 ± 0.4, see 1Expect 0.5 ± 0.2, see 0

Page 59: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-lepton +MET SUSY Limits

Page 60: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-lepton +MET Higgs Limits

See talks by P.Jonsson and S.Chuang Tuesday at 2pm.

eµDilepton mass

cuts tightened

at larger MH

Page 61: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Di-lepton +MET Higgs Limits

See talks by P.Jonsson and S.Chuang Tuesday at 2pm.

Page 62: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Lepton +MET + bb Higgs Limits

See talks by H.Kim and A.Metnitchouk Tuesday at 2pm.

Page 63: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Lepton +MET + bb Higgs Limits

See talks by H.Kim and A.Metnitchouk Tuesday at 2pm.

Page 64: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

bbbb Higgs Search

At least 3 tagged jets

Page 65: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

bbbb Higgs Search

Page 66: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for h→γγ

Limits on BR(h→γγ) < ≈60%

Page 67: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Search for Doubly Charged Higgs

H++

H--

Predicted e.g., in LR symmetric models

W

W

H++

Same-sign dilepton

signature

No events observed

Page 68: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Summary

Many recent preliminary results

with twice the Run 1 sample

Page 69: David Stuart, UC Santa Barbara for the CDF & D0 collaborationsstuart.physics.ucsb.edu/Presentations/stuart_Pheno04.pdfDavid Stuart, UCSB. PHENO’04Searches for new physics at the

David Stuart, UCSB. PHENO’04

Summary

Many recent preliminary results

with twice the Run 1 sample

Cooking up another batch