A Selection of Exotics with ATLAS - PowerPoint PPT Presentation

1 / 31
About This Presentation
Title:

A Selection of Exotics with ATLAS

Description:

North American Physics Workshop. K. Benslama. 1. A Selection of ... Other models: VF, Chiral F, Singlets F. Final state llZZ. Analysis. gg & DY. 2l, 2Z (4jets) ... – PowerPoint PPT presentation

Number of Views:42
Avg rating:3.0/5.0
Slides: 32
Provided by: pog7
Category:

less

Transcript and Presenter's Notes

Title: A Selection of Exotics with ATLAS


1
A Selection of Exotics with ATLAS
Kamal Benslama Columbia University
  • Strong Symmetry Breaking
  • Extra Dimensions
  • Little Higgs
  • Compositeness
  • New particles
  • Plans for the Rome Workshop

2
Introduction
  • Hierarchy problem
  • SUSY Elegant, not discussed here
  • Technicolor
  • . New strong interactions 1 TeV
  • Extra Dimensions
  • Gravity scale brought down to 1 TeV
  • Little Higgs
  • Higgs is pseudo-Goldstone boson ? 10TeV
  • Possible new physics
  • Excited fermions, contact interactions
  • Extension of EW gauge group
  • New gauge Bosons
  • Unexpected

3
Strong Symmetry Breaking
Technicolor
4
Technicolor (1)
  • TC
  • - New strong interaction O(TeV) with
    Techniquarks condensates -gt EWSB
  • no elementary scalar boson
  • ETC w/walking coupling
  • account for fermion masses
  • Supress FCNC
  • Predictions
  • Technimesons resonances in WLWL and WLZL
    scattering

Ruled out by EW precision data
5
Technicolor (2)
Rome
  • ?T?

6
Extra Dimensions
  • Large Extra Dimensions
  • TeV-1-sized Extra Dimensions
  • Warped Extra Dimensions

Talk by V. Vassilakopoulos
7
Large Extra Dimensions
  • Large extra dimensions (gtgt 1/TeV)
  • ADD model (Arkani, Dimopoulos, Dvali)
  • SM particules in brane
  • Gravity propagates in bulk (Xtra Ds)
  • Hence new gravity scale MPL2 MD2? R?
  • KK graviton excitations MD TeV for R lt mm

KK mode separation is very small e.g.
MD 1 TeV, n 2 ? R 0.08 mm ? R-1 2.6 x
10-3 eV n
4 ? R 1600 fm ? R-1 120 keV
? continuous spectrum
? high density of states compensates low
coupling (1/MPl ) ? chance
to observe effects at LHC
8
ADD Graviton Emission
Rome
  • Process
  • Reach
  • gG
  • ?G

L. Vacavant and I. Hinchliffe, J. Phys. G
Nucl. Part. Phys. 27 (2001) 1839
Background calibrated by Z j -gt ll j
9
TeV-1 Extra-Dimensions
  • One extra dimension compactified on a S1/Z2
    orbifold
  • radius of compactification small enough ? gauge
    bosons in the bulk
  • fermions localized on
  • a fixed point (M1 model) invariance under y ?
    -y
  • opposite fixed points (M2 model) under y ? y
    2?R
  • Kaluza-Klein spectra for Z(k), W(k) mk2 m02
    k2MC2
  • for MC 4 TeV m1 4 TeV, m2 8 TeV
  • ? look for pp ? ?(1)/Z(1) ? ll- on top of SM
    Drell-Yan

10
TeV-1 Direct ?(1)/Z (1)
  • Look at resonance in ll spectrum
  • Observation up to 5.8 TeV with 100 fb-1

11
Little Higgs
  • Motivation
  • Signatures

12
Introduction
  • Motivation
  • H is Goldstone boson of larger group
  • Cut-off ? introduced 10 TeV
  • Divergences canceled by
  • dm2Htop New colored fermion T
  • dm2Hgauge New bosons WH, ZH, AH
  • dm2HHiggs Higgs triplet
  • Constraints
  • T M lt 2TeV
  • A, W, Z M lt 6TeV
  • Higgs Triplet M lt 10GeV

13
Heavy T
Rome
L 3105 pb-1
  • Decay
  • bW (50), tZ (25), th (25)
  • tZ mode
  • 3 leptons 1 b-jet
  • th mode
  • Confirmation mode
  • 3 b-jets 1 lepton
  • The heavy quark T can be observed for a mass up
    to 2TeV

L 3105 pb-1 ?1 ?2 S 12 M 1 TeV
ATLAS
tZ
wb
14
New Higgs ?
Rome
  • Production
  • Via WW fusion
  • Forward jet tag essential
  • Decay
  • WW to l?l?

300fb-1
At 1 TeV Significance 5 s if v gt 29 GeV
15
Compositeness
  • Excited quarks and leptons

16
Introduction
Rome
  • Motivation
  • Fermionic generation explained by compositeness
  • Quarks leptons have an underlying substructure
    characterized by a compositeness scale ?
  • Interaction
  • Contact interactions Scale ?
  • Spectrum of excited states

17
Excited Quarks Leptons
  • Excited quarks
  • Reach limit for q -gt q ? 6.5TeV
  • - Reach for qw 7 TeV
  • - Reach for qz 4.5 TeV
  • ff1
  • Excited electrons
  • Reach 3 4 TeV for ? 6 TeV, 300fb-1

L 300 fb-1, L m
300fb-1
18
New particles
  • Heavy leptons
  • New gauge bosons
  • Leptoquarks

19
Heavy Leptons
Rome
  • Basics
  • Look at sequential leptons 4th family
  • Other models VF, Chiral F, Singlets F
  • Final state llZZ
  • Analysis
  • gg DY
  • 2l, 2Z (4jets)
  • Bdg tt, VVjets

(e ??)
Reach 1 TeV
Depends on Z
Significance
20
New Gauge Bosons
Atlas note in preparation
Rome
Full simulation, DC1 Z -gt ll
  • Discriminating between models
  • Look at ?x?, Asymmetry F-B
  • Look at Z rapidity

Assuming SM coupling and Accounting for
interference
Reach for 100 fb-1 5 TeV
21
Leptoquarks
Rome
  • Motivation
  • SM extension lepton-quark symmetry
  • Study Scalar LQ

30 fb-1
Preliminary
- 2jets 2 leptons 1st and 2nd generation

Sensitivity M(LQ)1.3 TeV
Beta 1
- 2 jets Et 3rd generation
Sensitivity M(LQ) 1 TeV
Beta 0.5
1st generation
22
Others
  • Models with singlet neutrino
  • Doubly Charged Higgs in LRSM
  • Heavy Majorana Neutrinos
  • Talk by V. Savinov
  • Lepton Flavor Violation

23
Plans for the Rome Workshop

It is the right time to ask ourselves the
following question What exotics can we do for
Rome? How are we going to proceed ?
24
Plans for Rome Workshop
  • Most of the exotics topics have already been done
    with ATLFAST
  • Our goal is to to redo most of them with full
    simulation using Rome-Layout
  • Study reconstruction with Rome-Layout, including
    noise and pile-up
  • Develop tools for TeV scale analyses
  • Also detector studies at the TeV scale
  • - Energy Calibration
  • - Reconstruction efficiency
  • - Refining energy resolution
  • - PID
  • - b-tagging
  • - Forward-jets tagging

25
What Exotics for Rome?
di-leptons channels

Z, G, H.
di-jets channels
  • Signal of W, Z, excited quarks,..ect
  • Signals of heavy scalar Higgs,
  • Strong Dynamics VV, G, Z,

WW, WZ, ZZ
Wb, Zb, Hb
  • Little Higgs Model, technipions

?jets, l? lZ

Excited fermions
  • Leptoquarks

ljets
MET jets
  • LED, leptoquarks

  • Non resonante excess of events

ll, ??, jj, tt
  • Black Holes

all SM particles
26
Detector Studies
  • No Physics without good understanding of the
    detector

For High Energy Particles
energy Calibration Reconstruction
efficiency Refining energy resolution Charge
misidentification for electrons and
muons PID b-tagging
DC1
Z
recalibrated
27
Preliminary Studies with Rome-Layout
q
q
  • Two High Pt leptons
  • two forward jets
  • Small MEt
  • Main background from qqww

q
28
Rome
DC2 vs Rome-Layout
Pt Lepton
E Jet1
DC2 Rome-Layout
DC2 Rome-Layout
DC2 Rome-Layout
DC2 Rome-Layout
MET
29
N. American Contributions
  • To the best of my knowledge

Physics Studies
Institution
Contact Person
H in LRSM and LHM RS Graviton H.E. e, gamma, PID
Columbia
Kamal
Hampton
K. Baker
RS Graviton
Pittsburg
Vladimir
W,Z , LFV
Z, excited e, quarks Leptoquarks,
Technicolor Jets reconsruction
G.Azuelos
Montreal
K. Loureiro
Wisconsin
Black Holes
Ian
(Litte Higgs, LED),UED?
LBL
Not for Rome
30
Roadmap for Rome
  • In order to ensure a high US contribution to the
    Exotics Physics in Rome, more people need to get
    involved in the analyses.
  • People with the same physics interests are
    encouraged to work together.
  • Studies of the detector response at the TeV scale
    is needed not only for Rome, but beyond.
  • Calibration, PID and tools development for TeV
    scale analyses should get the same priority as
    physics analyses.
  • People already involved in the Exotics group will
    be happy to
  • help new members Analyses, Software, MC
    samples,etc
  • The Rome Workshop will be a golden opportunity to
    test the software and the computing model and
    also to test the
  • US Physicists Compatibility model
  • Our Success in Rome and beyond will depend
    on how well we will work together.

31
Invitation
Compositeness
Technicolor
Little Higgs
Extra Dimensions
LFV
New particles
SERVE YOURSELF
Write a Comment
User Comments (0)
About PowerShow.com