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Signatures in alternative models beyond the Standard Model

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Title: Signatures in alternative models beyond the Standard Model


1
Signatures in alternative models beyond the
Standard Model
  • ??? (?????)

_at_ Korean CMS group workshop 2008. 12. 19.
2
Contents
  • Introduction
  • Z
  • W
  • H
  • H
  • t, b
  • Q, L
  • Dark matter
  • Summary

3
Introduction
  • LHC will explore for the first time a relevant
    energy range, well above the Fermi scale.
  • LHC is the Energy frontier machine best to search
    for the new (heavy) particles.
  • We concentrate on the new particles discovery.
  • The detailed phenomenology depends upon the
    model.

4
Z
5
Underlying Physics
  • Z Extra neutral gauge boson
  • Exists when there is extra gauge symmetries.
  • U(1) extensions of the SM
  • LR model
  • Other gauge extended models
  • Other species excited states of Z
  • Little Higgs model
  • Extra dimensional models

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Examples of U(1) extensions
E6 models breaking chain
? model ß0 ? model ßp/2 ? model
ßarctan(-v5/3)
8
LR model
(WL3, WR3, B) basis
Diagonalized to give eigenvalues
9
and eigenstates
where
Note that
Unknown model parameters are
MZ Z-Z mixing angle
10
Z couplings to quarks and leptons
Lagrangian for a Z
The Z-Z mixing angle is given by
11
Couplings for E6 inspired models and LR model
e.g.
where
12
Phenomenology
Drell-Yan process
13
Experimental limits
PDG 2008
14
CDF collab., Phys. Rev. Lett., 95, 252001 (2005)
15
Identification of Z using t and b
e.g.
S. Godfrey and T. A. W. Martin, Phys. Rev.
Lett., 101, 151803 (2008)
Kq depends on QCD and EW corrections.
16
S. Godfrey and T. A. W. Martin, PRL 101, 151803
(2008)
17
Measuring Z couplings at the LHC
e.g.
F. Petriello and S. Quackenbush, Phys. Rev. D 77,
115004 (2008).
Basic Observables
  • Z mass and total width
  • Cross section to
  • Forward-backward asymmetry
  • Rapidity ratio
  • Off-peak asymmetry

18
  • Forward-backward asymmetry

where
y1 is introduced to exclude low Z rapidity
events.
  • Rapidity ratio

19
M. Dittmar, Phys. Rev. D 55, 161 (1997)
20
Acceptance Cuts
  • Detector resolution effects are ignored.
  • Reconstruction efficiency of Z production is
    near 90 from CMS simulation.
  • CTEQ 6.5 NLO PDF used.
  • Integrated luminosity 100fb-1 unless stated
    otherwise.
  • Factorization and renormalization scale MZ

21
Calculation
Differential cross section
Parity symmetric couplings
Parity violating couplings
22
Rewrite the differential cross section
Absorbing
We have
23
Define four observables
24
which are expressed in terms of observables
25
We derive the Master equation
where
26
e.g. If we let
Solving the Master equation to have
27
Results
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  • If MZ 1.5 TeV, 100 fb-1 luminosity and y10.8
    can discriminate the example models with 90 C.L.
    and 1 ab-1 luminosity (SLHC) will provide precise
    determination.
  • If MZ 3 TeV, 100 fb-1 luminosity and y10.4 can
    discriminate some models.
  • For MZ 3 TeV, 1 ab-1 luminosity (SLHC) will
    provide reasonable determination.

35
Exotic Z
  • Generation-dependent couplings
  • Leptophobic
  • Hadrophobic
  • Flavour-violating
  • And more

36
W
37
Underlying Physics
  • W Extra charged gauge boson
  • Exists when there are extra gauge symmetries more
    than U(1).
  • LR model
  • Other gauge extended models
  • Other species excited states of W
  • Little Higgs model
  • Extra dimensional models

38
LR model (e.g.)
(WL, WR) basis
Diagonalized to give
where
39
Search for W
W ? l- ?
W ? t b
  • High energy single lepton final states
  • Single top production

40
Transverse mass
Edges of transverse mass distribution are
crucially related to the mass of W.
D0 collaboration, PRL 100, 031804 (2008)
41
Experimental limits
PDG 2008
42
CDF constraints
43
D0 observations
D0 collaboration, PRL 100, 031804 (2008)
44
Feasibility of W at the CMS
e.g.
C. Hof, Acta Phys. Pol. B 38, 443 (2007)
Reference models same couplings as the SM
45
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46
Exotic W
  • Left-right asymmetric coupling constants and
    CKM
  • Leptophobic
  • Hadrophobic
  • Flavour-dependent SU(2)
  • Exotic gauge self-couplings W-W-Z, W-W-Z
  • And more

47
H
48
Underlying Physics
  • H Charged scalar
  • Exists when there is extra Higgs sector more than
    SM singlet.
  • 2HD model
  • MSSM and more extensions (NMSSM etc.)
  • LR model
  • Other GUT-based model

49
Higgs sector in the LR model
Two triplets
breaking of SU(2)R and its L-R partner
a bidoublet
electroweak symmetry breaking and fermion masses
with VEVs
Note that
define
50
Charged Higgs boson in the LR model
Mass matrix
where
Diagonalization by
Charged Higgs mass
51
relevant tbH couplings
similarly for lepton sector
52
Phenomenology
Light charged Higgs from t? H??b at Tevatron
Light charged Higgs boson
Absence of observed charged Higgs boson
Constrained by
53
CDF collaboration, PRL 96, 042003 (2006)
54
Pair production of charged Higgs boson at LEP
ALEPH collaboration, PLB 543, 1 (2002)
55
B? ? ???? and charged Higgs boson
R. Barlow, ICHEP 2006
56
Experimental constraints for LR charged Higgs
57
allowed
allowed
D.-W. Jung, K. Y. Lee., Phys. Rev. D 76, 095016
(2007)
58
Light charged Higgs production at the LHC
sequential decay
after tt pair production
108 top quarks produced
More than 105 charged Higgs expected
D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
59
Heavy charged Higgs production at the LHC
dominant channel
K-factors for the NNLO QCD corrections
considered N. Kidonakis, JHEP 05, 011 (2005).
60
D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
61
D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
62
Decay of produced charged Higgs boson
in the LR model
in the 2HD model
63
D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
64
  • Different structure of the Yukawa couplings in
    the LR model leads to different phenomenology of
    the Higgs bosons from those of the 2HD model.
  • Production cross section of the charged Higgs in
    the LR model is generically larger than that of
    the 2HD model at the LHC.
  • Decays of the heavy charged Higgs boson in the LR
    model combined with the production cross section
    might discriminate the LR charged Higgs from the
    2HD charged Higgs boson.

65
H
66
Underlying Physics
  • H Doubly charged scalar
  • appears when there exist Higgs triplets or higher
    multiplets.
  • LR model
  • 3-3-1 model
  • Little Higgs model
  • Higgs triplet model for neutrinos

67
H in the LR model
Lepton number violating terms are
  • Production depends on WR mass
  • Phenomenology depends on neutrino structure and
    see-saw mechanism.

? mWR
68
Productions
69
Decays
70
Reconstructed pp?HH-- ?µ µ µ- µ-
CMS collab., J. Phys., G 34, N47 (2007)
71
Expected discovery of pp?HH-- ?µ µ µ- µ-
CMS collab., J. Phys., G 34, N47 (2007)
72
100 dilepton assumeda. 100 fb-1b. 300 fb-1
ATLAS collab., J. Phys., G 32, 73 (2006)
73
q
74
Underlying Physics
  • t, b Fourth generation quarks
  • Generically heavier than t and b since they are
    not observed yet.
  • Why not even in the SM?
  • LEP data on invisible decay of Z boson restricts
    the number of generations 3
  • 4th neutrino should be heavier than mZ/2.

75
Why 3 generations?
LEP data on invisible decays n
Astrophysical data of He production
D.N. Schramm and M.S. Turner., Rev. of Mod.
Phys. 70, 303 (1998)
76
Decays
  • Charged current decays
  • FCNC decays


77
Present bounds
PDG 2008
78
Q, L
79
Underlying Physics
  • Excited quarks and leptons Heavy states of
    quarks and leptons sharing quantum numbers with
    ordinary quarks and leptons.
  • Appear in the composite models.
  • Quarks and leptons are bound states of some
    constituents. (Preon)
  • Experimentally similar to 4th generations.

80
  • Excited fermions can be pair-produced via gauge
    couplings.
  • If the compositeness scale is high enough, the
    compositeness manifests through effective
    4-fermion contact interactions

PDG 2008
81
Dark Matter
82
Underlying Physics
  • Dark matter (Large) missing energy at the
    collider
  • Appears in various models
  • LSP in the MSSM
  • Lightest heavy states in the Little Higgs model
  • Lightest KK states in the extra dimensional model
  • And many other models

83
Summary
  • Many possibilities are open at the LHC.
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