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WIN 05

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Why SUSY is a good idea. One of the most appealing extensions ... [Branson et al, ATLAS] Warning: model dependent plot! Same-sign dileptons. Signal: Background: ... – PowerPoint PPT presentation

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Title: WIN 05


1
WIN 05
Supersymmetry searches at the LHC
Filip Moortgat, CERN
  • Inclusive signatures
  • discovery, fast but not
    unambiguous
  • Exclusive final states long term measurements
  • towards understanding
    the underlying model

2
Why SUSY is a good idea
One of the most appealing extensions of the
Standard Model
TeV-scale supersymmetry
a symmetry between fermions and bosons,
duplicates the SM particle spectrum, but not the
couplings
Solves several problems at once
  • dark matter candidate (e.g. lightest neutralino)
  • opening towards a theory of gravity
  • unification of gauge couplings
  • hierarchy problem
  • allows to explain why the Higgs mechanism works

3
SUSY models
  • In general MSSM many allowed soft SUSY breaking
    parameters (124) due to unknown nature of SUSY
    breaking mechanism
  • difficult to work with
  • ? use more constrained models
  • Most popular mSUGRA
  • Also mGMSB, AMSB

m0 , m1/2 , A0 , tan b , sign(m)
4
The Large Hadron Collider
(8 T !!)
also AA and pA collisions for PbPb 5.5
TeV/nucleon and L 1027 cm-2s-1
5
Generic SUSY signatures
  • General characteristics of R-parity conserving
    SUSY
  • sparticles pair produced and LSP stable
  • ? large amount of missing transverse energy
  • coloured sparticles are copiously produced and
    cascade down to the LSP with emission of
  • many hard jets and often leptons

Generic SUSY signatures are ETmiss multi-jets
(and multi-leptons)
6
Inclusive SUSY
  • jets ETmiss
  • 1,2,3 lepton ETmiss
  • opposite sign (OS) or
  • same sign (SS) di-leptons
  • often several topologies
  • simultaneously visible

7
Jet MET
  • Signature ETmiss jets
  • s 1 pb at 1 TeV
  • ? physics for startup
  • significant reach after 1 yr
  • with 300 fb-1, reach squarks and gluinos up to
    2.5 TeV
  • (need good understanding of
  • detector and backgrounds!)

8
Et sum
Branson et al, ATLAS
Variable that gives information on the SUSY
scale
SM background
SUSY (700 GeV)
Warning model dependent plot!
9
Same-sign dileptons
Signal
Background
_
? ask for 2 SS leptons hard jets ETmiss
Drozdetski et al, CMS
10
Exclusive final states
  • so far inclusive measurements
  • fast discovery, but does not
  • unambiguously single out
    SUSY
  • need to reconstruct sparticle decay chains and
    masses involved
  • need to be prepared for all
    possible final states
  • goal is to measure cross sections, BRs (?
    couplings)
  • and even spin of the sparticles
  • LHC can not only discover
    SUSY, but
  • also MEASURE its properties
    (if nature is kind)

11
Coloured sparticle decays
Pape, CMS
12
Neutralino2 decay signatures
Significant fraction of
Pape, CMS
13
Decay chain to dileptons
  • 2 high pt isolated leptons
  • 2 high pt jets
  • missing Et

Final state
14
Kinematic endpoints
Kinematic endpoint technique construct
lepton/quark upper/lower endpoints and relate
them to the masses in the decay chain
E.g. 4 unknown masses 4 endpoints ?
all masses can be determined
Usually non-linear relations ? all masses, not
just differences Extra endpoints, or start from
gluino ? constraints
15
Final states with dileptons (1)
  • M(ll) very sharp end point,
  • triangular shape (due to spinless
    slepton)
  • ?

Biglietti et al, ATLAS
Chiorboli et al, CMS
16
Final states with dileptons (2)
  • M(l1q)
  • M(l2q)
  • ?Can distinguish M(l1q)max from M(l2q)max
  • M(llq)

M(llq)
ATLAS
17
Gluino reconstruction
Choose dilepton pairs close to the edge then
assuming can be at
rest in the frame of
? can reconstruct and
Chiorboli et al, CMS
18
Final state with taus
  • often decays to taus instead of
    electrons/muons
  • can we use hadronic tau final states?

endpoint smeared out
Biglietti et al, ATLAS
19
Decay chain to h0 or Z0
20
Final states with h0 or Z0
Paige, ATLAS
  • Higgs peak can be reconstructed
  • from 2 b-jets
  • ? could be a h0 discovery channel !
  • (even for light H0 and A0)
  • Z0 reconstructed from di-lepton decay
  • Decay chain is shorter than for di-leptons ?
  • e.g. start from gluino
  • M(q1h0),M(q2h0),M(qq),M(qqh0)
  • to determine 4 masses

M(bb)
Moortgat, CMS
h0
A0,H0
21
GMSB signatures
  • In GMSB, the light gravitino is the LSP
  • Who is NLSP?
  • Neutralino is NLSP
  • Stau is NLSP
  • ? ETmiss ? , ? or long-lived particles

TOF measurement in the CMS muon DTs
Wrochna, CMS
? dE/dx and TOF
22
SUSY spin measurement
Make use of spin correlations in decay of squark
Barr, ATLAS
no spin correlations
23
SUSY spin measurements (2)
washes out for antisquarks, but in pp colliders
? more squarks produced than antisquarks
Barr, ATLAS
  • Visible asymmetry
  • (500 fb-1)

no spin correlations
24
Conclusions
  • If TeV-scale SUSY exists, its discovery at the
    LHC should be (relatively) fast, using inclusive
    signatures
  • The LHC can measure sparticle properties
    reconstruction of masses in sparticle decay
    chains, mainly using kinematic endpoints
  • Ultimately would like to measure spins and
    couplings
  • (WIN 05 ? WINO 5?)
  • only 750 days to startup so focusing on being
    ready for first day physics now!

25
Backup
26
Cross sections _at_ the LHC
Well knownprocesses, dont need to keep all of
them
New Physics!! This we want to keep!!
27
CMS
28
ATLAS
29
Civil Engineering
USC 55
UXC 55
30
End points and configurations
31
Higgs to sparticles
If accessible, we may exploit the sparticle decay
modes
A, H ? ?20 ?20 ? 4l ETmiss
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