l. perera lpc physics meeting 11/17/2005 1 search for h/a → lalith perera rutgers university for...
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L. Perera LPC physics meeting 11/17/2005 1
Search for H/A →
Lalith PereraRutgers University
for
Rutgers CMS GroupAmit Lath, Keith Rose, Sunil Somalvar, Steve
Schnetzer, Bob Stone, Alik McPerson, Dimity Hits, (Eva Halkiadakis)
L. Perera LPC physics meeting 11/17/2005 2
Why H→ • At LHC MSSM higgs are expected to produced by
• gg →bbH , gg →H qq→ H• Dominant decay modes of H:
• B(H→ ) ~ 8% , B(H→ bb) ~90%• bb channel is affected by large dijet background
• could tag associative b to lower backgrounds
• Dominant back ground to from Z/*:• can be estimated ( # of Zs from Z→e e, ..)
channel could be equally promising
L. Perera LPC physics meeting 11/17/2005 3
→e →e 3 High DY → ee BG
→ → 3 High DY → BG
→e → 6 low QCD BG
→e →h 23 promising
→ →h 23 promising
→h →h 41 multi jet BG
mode fraction % comments
H→ Decay Modes
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CDF results on H
•Rutgers CDF group did CDF run II, Hanalysis
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• B/ group (and others) already working on this channel
• Rutgers group plan to concentrate on low mass higgs
low mass higgs search is challenging due to overlap with Z
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CMS hadronic taus• Level 1: narrow hadronic jet with ET cut
• Level2 (HLT): • Localized energy in ECAL – isolation 0.4
• Level 25: • isolation in tracker (Calo+pixel, Si)
• signal cone 0.07, isolation cone, 0.4, ET , PT
• Offline taged tau jets:• Isolation using fully reconstructed tracks
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• 1 tau jet ET > 93 GeV (104 high L)
• 2 tau jets ET > 66 GeV (76 high L) ….
• This is good at rejecting Z back ground
2 1
ET of from Z →
GeV
L1 tau trigger:
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But also rejects low mass higgs
M(H) = 120GeV M(H)= 140GeV
2 1 2 1
ET ET
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L1 efficiency for H→
1 or 2 tau bit
L1 global efficiency Any L1 tau bit
Any: tau 1, tau 2, tau+gamma
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L1 Trigger ratesData L1 Accept 1 or 2 Tau “Any” Tau
Z->ee 16.8% 0.2% 8.0%
Z-> 55.8% 0.9% 3.7%
Z-> 65.9% 0.1% 3.0%
H(120)-> 38.1% 0.8% 11%
H(140)-> 44.0% 1.0% 15%
H(180)-> 53.2% 2.8% 25%
H(250)-> 67.7% 15% 41%
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Possible ways to improve sensitivity to low mass higgs
• Understanding/estimating back grounds
• Tau reconstruction: to reject jet backgrounds, improve energy resolution
• Use tau Impact parameter
• Any other signatures of →– angular distributions. H scaler, Z-vector
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Number of tracks in tagged tau jets . (from H→ m(H) =140)
(fewer 3 prong taus likely a bug in Exroot)
Tau mass reconstruction
→ h 0 25.9%
→h 11.8%
→3h 10%
→h20 9.4%
→h30 4.5%
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Tau mass Calculation
Case study with 140GeV →
• Use tau tagged jets with a single track (→ n0)
• Add energy in ECAL and HCAL cells within 0.25 of jet axis
• exclude cells 0.04 (ECAL)/0.15 (HCAL) from track
• Calculate the momentum of photons and take the sum
• Add track momentum and energy
• Calculate invariant mass
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Angle between pion and gammas in the tau decay (from MC)
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Visible tau mass from generator e/p of tau decay particles except neutrinos.
(what is possible with an ideal detector )
Reconstructed Tagged tau jet Invariant mass
(for single track tau jets)
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Improving tau mass reconstruction• Is it track energy In ECAL MIP or more?
Can we identify?
Opposite form what is expected ?
CAL
CAL
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fraction of energy in HCAL, f <0.05 f > 0.05
Again, does not look right ?
Investigating!
Reconstructed visible tau mass single track tau jets
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Reconstructing higgs mass
Calculate energy, momentum in collinear approx.
add to to the visible e-p to get mass.
Method used by CERN (Higgs PRS) group:
L. Perera LPC physics meeting 11/17/2005 19
H/A mass generator level
Reconstructed 2 mass from MC parameters of t decay products
Use energies of s to get ET
Use e-p of tau decay particles as jet/track energyA 30% minimum loss for 140 GeV H
Testing Collinear approximation
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Alternate method (CDF)
• Use missing ET (Ex, Ey) from calorimeter and
• Take neutrino E =ET Px=Ex; Py=Ey; Pz= 0
GeV
For m(H)=140 GeV
Generater level p-E from tau decays particles
ET from neutrinos
No loss of efficiency, Lower reconstructed mass
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Future Plans
• More trigger and background studies (more MC)
• Improvements to tau mass reconstruction
• Looking at other possible parameters, …
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Back up slides
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L. Perera LPC physics meeting 11/17/2005 24
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