Looking for the Observable SUSY Channel at ATLAS ATLAS Physics Workshop at JINR 14 April 2006 JINR Dubna - PowerPoint PPT Presentation

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Looking for the Observable SUSY Channel at ATLAS ATLAS Physics Workshop at JINR 14 April 2006 JINR Dubna

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It is locally invariance gauge theory and therefore Gravitation can be included ... Unification of gauge coupling constants into an universal one at very high ... – PowerPoint PPT presentation

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Title: Looking for the Observable SUSY Channel at ATLAS ATLAS Physics Workshop at JINR 14 April 2006 JINR Dubna


1
Looking for the Observable SUSY Channel at ATLAS
ATLAS Physics Workshop at JINR 14 April
2006JINR Dubna
  • Presented by
  • Gia Khoriauli
  • (On leave from TSU, Georgia)
  • Authors
  • V. Bedniakov, Y.Budagov, A. Gladyshev, D.
    Kazakov, G. Khoriauli, J.Khubua

2
SuperSymmetry (SUSY)
  • SUSY is the theory about a symmetry between
    bosons and fermions and it is the mostly
    believed/expected candidate theory for Grand
    Unification.
  • Motivations for SUSY
  • It is locally invariance gauge theory and
    therefore Gravitation can be included by the
    natural way
  • Unification of gauge coupling constants into an
    universal one at very high energies (1015 1016
    GeV) , what is not possible within Standard Model
  • It solves the problem of hierarchy and vanishes
    radiation corrections to boson masses, which are
    very big at large energy scale because of the
    contribution of very massive particle loops
  • Radiation breaking of electro-weak symmetry. This
    spontaneous symmetry breaking is naturally caused
    by radiation corrections to the mass parameters
    of Higgs potential
  • SUSY lightest neutral stable particle is good
    candidate for Dark Matter in the Universe

3
Minimal SuperSymmetry Model (MSSM)
  • In MSSM with using universality principle for all
    boson and fermions masses we can significantly
    reduce the number of free SUSY parameters. This
    model is called mSUGRA minimal supergravity.
    Free parameters are
  • m0 - universal mass for all bosons
  • m1/2 - universal mass for all fermions
  • A - parameter of soft supersymmetry breaking
  • sign(µ) sign of mixing parameter of two Higgs
    fields
  • tanß ratio of vacuum expectation values of
    Higgs fields
  • Plot on the right shows the mass parameters space
    with excluded regions (red and yellow dotted
    areas) due to the different experimental
    restrictions

4
gg -gt gg in ATLAS
  • Cross-section of 2gluons -gt 2gluino for s1/214
    TeV is estimated to be of the order of 10-12 barn
    1 pb
  • We selected the following values for free
    parameters (Fixed point region in allowed
    parameter space)
  • m0 1400 GeV
  • m1/2 180 GeV
  • A 0
  • sign(µ) 1
  • tanß 30
  • In this case gluino has large branching ratio for
    the decay mode shown on the right diagram giving
    2 b-jets 2 muons large missed transverse
    energy. This channel has quite good signature in
    SUSY searching.
  • For event generation we used Pythia generator
    within ATHENA framework

5
gg -gt gg gt 4 b-jets 4 muons Etmiss
  • The physical picture of the previous diagram is
    shown on the right plot. It is assumed that both
    initial gluons had Pt 0 and all beam remnants
    fly along the beam axis (z) . In this case, using
    the below formula we can calculate total missed
    transverse momentum, which is an observable
    quantity in an experiment
  • However, very often the initial gluons Pt is not
    zero (see the plot on the next slide) and for
    full kinematics one should consider Pt of other
    particles and jets

6
Pttot and Etmiss (Pythia)
  • Down plot shows distribution of Etmiss for the
    events when initial Pttot of gg system was in the
    range (-?Pt , ?Pt) , where ?Pt 10 GeV
  • Upper plot shows distribution of total Pt.
    Different from zero values correspond to the
    cases when one or both gluons in total had Pt ? 0

7
Pt of ?01 and µ-µ pair , Radius of B-meson
decay vertex (Pythia)
8
SM Background
  • Right plot shows the diagram for main Standard
    Model background process to the SUSY process
    discussed above
  • In this process there are also 4 b-jets and 4
    muons, but Etmiss is expected to be far less than
    it is in SUSY case
  • We are currently in studying of background
    processes

9
To do
  • To study the dependence of the received results
    on the variation of SUSY free parameter values at
    generator level
  • To continue a study of background processes at
    generator (Phytia, ) level and the comparison
    with the interesting SUSY process
  • and main task to simulate, reconstruct and
    analyze this SUSY process within the ATLAS
    detector
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