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New Physics at the LHC in the first year

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Title: New Physics at the LHC in the first year


1
New Physics at the LHC in the first year
Orin Harris UW Physics Grad Student
2
Talk Outline
  • The LHC Enormous Potential
  • New Physics
  • New Gauge Boson(s)
  • SM Higgs Particle
  • SUSY Particles
  • Summary

3
The LHC Enormous Potential
  • Design Luminosity Should reach 100 fb-1 per year
    after 3 years of operation.
  • Initial Luminosity 10 fb-1 in the first year
    (10x Tevatron)
  • Energy 14 TeV (7x Tevatron)
  • Only 1 day at 1 design luminsoty would produce
    8000 t quarks, 100 QCD Jets beyond kinematic
    limit of Tevatron

4
New Gauge Boson(s)
  • New massive electrically neutral Gauge Bosons Z
    are a common feature in most extensions of the SM
    gauge group. They also arise in theories
    postulating extra dimensions.
  • Dominant decay channels Z? ee-, µµ-, jj
  • Discovery potential as a function of mz depends
    on how strongly Z couples to quarks/leptons
    compared to Z, ie how ?(Z) and BR(Z?) compares
    to ?(Z) and BR(Z?).

5
Z ? ee-, ??-, jj
If the Zs BR into leptons is similar to Zs, can
expect about 10 events for an integrated
luminosity as low as 300 pb-1 (3 days _at_ initial
luminosity) for a particle mass of 1.5 TeV
100 fb-1
Shown is the ratio of coupling strengths, as a
fucntion of mZ needed for a 5? confidence level
signal
6
Signal will be resonant peak on top of smooth
Drell-Yan background. Should be very clear signal
if ECAL response understood to a few
100 fb-1
(SM-like)
7
SM Higgs ParticleThe last undetected particle
predicted by SM
  • Discovery potential depends highly on the Higgs
    mass
  • SM perturbative validity mH lt 1 TeV
  • LEP program 114 GeV lt mH lt 186 GeV, with 95
    confidence
  • For any assumed value of mH, SM predicts Higgs
    production cross-section and relative rate of
    various decay channels

8
Dominant Higgs Production mechanisms and Cross
Sections
9
Low mass region mH lt 130 GeV
  • Dominant Channel H ? has large cross section
    BR 90, but a prohibitve QCD 2-jet background.
  • Background too high for direct -fusion
    production channel. Must resort to observing
    leptonic decays for triggering from the
    associated production with W or Z boson or
    pair
  • Requires excellent b-tagging, HCAL performance,
    and jet reconstruction probably not realistic in
    first year

10
H ? ??
  • H ? ?? is a rare decay channel BR10-3
  • large background S/B 120.
  • Demands excellent ECAL performance, angular
    resolution
  • to observe the narrow mass peak above ??
    background

Expected signal for mH 120 GeV with 100 fb-1
11
Outlook much better for larger Higgs mass 130
GeV lt mH lt 180 GeV
  • Most promising channel H ? ZZ ? 4l until 180
    Gev when H ? ZZ ? 4l channel opens up
  • Requires good identification, reconstruction, and
    measurement of high pT leptons, in each (4e,
    2e2?, 4?) decay channel.
  • Detector performance should be good enough to
    ensure high significance discovery in this mass
    range in a year or two

12
4? channel (muon spectrometer)
13
180 GeV lt mH lt 800 GeV
  • Dominant channel H ? ZZ ? 4l
  • Background lt Signal
  • Detector performance not crucial
  • Signal broadens at high mass. In the unlikely
    case mH gt 800 GeV, the more difficult ZZ ? ll??,
    lljj, and WW ? l?jj decay modes cover that rest
    of the mass range

14
Overall Sensitivity to SM Higgs Theoretically
(but not realistically) entire Higgs mass range
accesible at LHC in first year
15
SUSY ParticlesSolves Hierarchy Problem,
candidate for dark matter
  • Expect huge squark and gluino production cross
    sections, even for masses as large as a few TeV
  • If R-parity is conserved (no proton decay), clear
    model-independent signature of several high-pT
    jets and large Etmiss
  • But reliable reconstruction of Etmiss events is
    crucial
  • And unlike Higgs, SUSY complicated by many free
    parameters.
  • The best we can do is investigate in detail the
    signatures for particular points in the parameter
    space

16
Constraining SUSY
  • But even the most minimal SUSY extension of the
    SM (MSSM) has 105 new parameters. The space of
    free parameters is too large to meaningfully
    compare predictions with data.
  • The most minimal gravity-mediated or
    gauge-mediated SUSY-breaking extensions of MSSM
    reduce the number of free parameters to 5 and 6,
    respectively.

17
The minimal supergravity (mSUGRA) extension
  • mSUGRA assumes that at the GUT scale all scalars
    have a common mass m0, all gauginos and Higgsinos
    have a common mass m1/2 (there are 3 other free
    parameters also)
  • Though probably overly constraining, this model
    has a small enough parameter space that its
    predicted signatures can be studied with some
    thoroughness

18
One point in the parameter space
5? isolines for squarks and gluinos, parametrized
in terms of m0 and m1/2, as a function of
integrated luminosity
19
Another point (A0 300, tan? 2.1, ? gt 0)
More recent matrix-element techniques predict
higher backgrounds in this region (up to yellow
line)
meff ? Etmiss PT,1 PT,2 PT,3 PT,4
20
In Summary
  • If a Z of a few TeV exists whose BR into leptons
    is near Zs, it will be discovered in first year
  • SM Higgs gt 180 GeV will likely produce a
    significant signal in the first year, but current
    data suggests SM Higgs lt 186 Gev
  • Squarks and Gluinos up to a few TeV could
    produce a convincing signal in first year

21
References
  • ATLAS TDR pp673-952
  • azrXiv hep-ph/050422 v1 25 Apr 2005
  • LHC physics the first one-two years(s),
    Gianotti and Mangano
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