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Lp2005

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Promising and a 2s fluctuation where LEP fluctuated and Veltman Condition satisfied. ... Lep Fluctuation. W higgstrallung fluctuation. What can we do. Improve ... – PowerPoint PPT presentation

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Title: Lp2005


1
Lp2005
2
lp2005
3
Top Mass Measurements
dilepton new
MtopCDF 172.2 3.7 GeV (2 accuracy)
2 papers submitted, 3 papers in preparation
4
Top Mass and Production Cross-section
5
new high energy effects with scale L must control
the higgs mass
  • scale of new physics from the requirement that
    the radiative corrections to the higgs mass are
    small

d

tension with accuracy of the Standard Model
Mh115 GeV
Veltman condition (I get 311)
6
Higgs
  • Promising and a 2s fluctuation where LEP
    fluctuated and Veltman Condition satisfied.
  • MSSM? NMSSM speculation?
  • HARD to measure because need to do the b jet
    energy scale right.

7
Need z-gtbbbar, clustering
8
W Jets 2 jet bin is the Signal, 1,3,4 measured
9
Single Tag
10
Double tag
11
Set limits
12
Future
13
All channels as they are, 0.36 fb-1
14
For all higgstrallung at Tev
Service work
15
H-gtWW and VBF
16
Diboson Production
  • WW production is the dominant background
  • Compulsory to first measure the WW production
    cross-section
  • Select a large WW sample to check
  • Simulation modelling of the data (PYTHIA,
    ALPGEN), ex Df(l,l)
  • Trigger, lepton identification efficiencies,
    everything comes into the mix
  • Still statistically limited

PRL 94, 211801 (2005) (CDF)
S/B 2
17
Event Selection
  • Optimized for the best a-priori 95 C.L. on
    sxBR(H?WW)
  • Two leptons
  • pT trigger, non-triggergt(20,10) GeV
  • Muons hlt1.0 electrons (hlt1.0, hlt2.0)
  • Mll gt 16 GeV
  • Jet veto (signal can only have soft ISR jets)
  • 0jet 15ltET1jetlt55 GeV 15ltET2jetlt40 GeV
  • jets ?lt2.5
  • ET gt ¼MH
  • ET gt50 GeV ??(met, closest lep/jet)gt20º
  • Opposite sign
  • Mll lt (½MH 5) GeV
  • pT1lep1pT2lep2 ET lt MH
  • Backgrounds
  • rejected







Removes VBF

18
H?WW contribution to the Tevatron Higgs search
x12
HWW channel is important for a MHgt130 GeV SM
Higgs discovery. Tune on Tom Junks talk for more.
19
1/fb projections summary
  • Assume the current analysis as starting point
  • Below are just few ways we think we can use to
    improve our sensitivity

Potential Improvement
S/sqrt(B)
  • Using a NN                                        
       1.42 
  • Including hadronic taus                        1.1
    5
  • Include associated VH and VV fusion  1.15
  • Estimate performed in hep-ph/0010338
  • Loose leptons                                     
       1.10

Overall
2.07
Equivalent to 4x more luminosity
  • There is still potential to do better
  • Not all these improvements might be ready for
    Winter conferences

20
NMSSM
h-gt aa
21
Claim to see signal at 110-115 (h-gtaa)
22
Future
23
1 fb-1 Physics Challenge (Spring-Summer 06)
Data taking Period Total Lum. (pb-1) Data processed Ntuples made Physics results
2/2002 - 8/2004 320-550 2004 2004 Spring 2005
12/2004 - 3/2005 430-680 7/2005 9/2005
3/2005 - 5/2005 540-810 8/2005 9/2005
5/2005 - 7/2005 640-910 9/2005 9/2005
7/2005 - 8/2005 700-960 10/2005 10/2005 Spring 2006
9/2005 750-1010 11/2005 11/2005
10/2005 800-1060 12/2005 12/2005
11/2005 850-1110 1/2006 1/2006
12/2005 900-1160 2/2006 2/2006
1/2006 950-1210 3/2006 3/2006
2/2006 1000-1260 4/2006 4/2006 Summer 2006
24
Observations/Conclusions
  • The Tevatron is coming within striking distance
    of the Higgs
  • A factor of 10-20 with present data is possible
  • Expect x3 or so data for winter and next summer
    (on tape, need to analyze, need to tune analysis)
  • 115 GeV higgs is the hot spot
  • Veltman bound
  • Lep Fluctuation
  • W higgstrallung fluctuation
  • What can we do
  • Improve bbbar resolution
  • Do VBF analysis at CDF we are invited
  • We learn to deal with top, underlying event, WW
    production cross section
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