Title: Signatures in alternative models beyond the Standard Model
1Signatures 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
3Introduction
- 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.
4Z
5Underlying 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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7Examples of U(1) extensions
E6 models breaking chain
? model ß0 ? model ßp/2 ? model
ßarctan(-v5/3)
8LR model
(WL3, WR3, B) basis
Diagonalized to give eigenvalues
9and eigenstates
where
Note that
Unknown model parameters are
MZ Z-Z mixing angle
10Z couplings to quarks and leptons
Lagrangian for a Z
The Z-Z mixing angle is given by
11Couplings for E6 inspired models and LR model
e.g.
where
12Phenomenology
Drell-Yan process
13Experimental limits
PDG 2008
14CDF collab., Phys. Rev. Lett., 95, 252001 (2005)
15Identification 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.
16S. Godfrey and T. A. W. Martin, PRL 101, 151803
(2008)
17Measuring 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.
19M. Dittmar, Phys. Rev. D 55, 161 (1997)
20Acceptance 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
21Calculation
Differential cross section
Parity symmetric couplings
Parity violating couplings
22Rewrite the differential cross section
Absorbing
We have
23Define four observables
24which are expressed in terms of observables
25We derive the Master equation
where
26e.g. If we let
Solving the Master equation to have
27Results
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34- 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.
35Exotic Z
- Generation-dependent couplings
- Leptophobic
- Hadrophobic
- Flavour-violating
- And more
36W
37Underlying 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
-
38LR model (e.g.)
(WL, WR) basis
Diagonalized to give
where
39Search for W
W ? l- ?
W ? t b
- High energy single lepton final states
- Single top production
40Transverse mass
Edges of transverse mass distribution are
crucially related to the mass of W.
D0 collaboration, PRL 100, 031804 (2008)
41Experimental limits
PDG 2008
42CDF constraints
43D0 observations
D0 collaboration, PRL 100, 031804 (2008)
44Feasibility of W at the CMS
e.g.
C. Hof, Acta Phys. Pol. B 38, 443 (2007)
Reference models same couplings as the SM
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46Exotic 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
47H
48Underlying 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
-
49Higgs 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
50Charged Higgs boson in the LR model
Mass matrix
where
Diagonalization by
Charged Higgs mass
51 relevant tbH couplings
similarly for lepton sector
52Phenomenology
Light charged Higgs from t? H??b at Tevatron
Light charged Higgs boson
Absence of observed charged Higgs boson
Constrained by
53CDF collaboration, PRL 96, 042003 (2006)
54Pair production of charged Higgs boson at LEP
ALEPH collaboration, PLB 543, 1 (2002)
55B? ? ???? and charged Higgs boson
R. Barlow, ICHEP 2006
56Experimental constraints for LR charged Higgs
57allowed
allowed
D.-W. Jung, K. Y. Lee., Phys. Rev. D 76, 095016
(2007)
58Light 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)
59Heavy charged Higgs production at the LHC
dominant channel
K-factors for the NNLO QCD corrections
considered N. Kidonakis, JHEP 05, 011 (2005).
60D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
61D.-W. Jung, K. Y. Lee., Phys. Rev. D 78, 015022
(2008)
62Decay of produced charged Higgs boson
in the LR model
in the 2HD model
63D.-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.
65H
66Underlying 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
-
67H in the LR model
Lepton number violating terms are
- Production depends on WR mass
- Phenomenology depends on neutrino structure and
see-saw mechanism.
? mWR
68Productions
69Decays
70Reconstructed pp?HH-- ?µ µ µ- µ-
CMS collab., J. Phys., G 34, N47 (2007)
71Expected discovery of pp?HH-- ?µ µ µ- µ-
CMS collab., J. Phys., G 34, N47 (2007)
72100 dilepton assumeda. 100 fb-1b. 300 fb-1
ATLAS collab., J. Phys., G 32, 73 (2006)
73q
74Underlying 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.
-
75Why 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)
76Decays
- Charged current decays
- FCNC decays
77Present bounds
PDG 2008
78Q, L
79Underlying 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
81Dark Matter
82Underlying 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
-
83Summary
- Many possibilities are open at the LHC.
-