Phenomenology of supersymmetric TeV scale seesaw models - PowerPoint PPT Presentation

1 / 29
About This Presentation
Title:

Phenomenology of supersymmetric TeV scale seesaw models

Description:

Oct/27/2005. Gi-Chol Cho. 1. Phenomenology of ... women's university in Tokyo. Location of Ochanomizu (????) area ~ center of Tokyo. Ocha (??) = Tea ... – PowerPoint PPT presentation

Number of Views:53
Avg rating:3.0/5.0
Slides: 30
Provided by: gicho
Category:

less

Transcript and Presenter's Notes

Title: Phenomenology of supersymmetric TeV scale seesaw models


1
Phenomenology of supersymmetric TeV scale see-saw
models
  • Gi-Chol Cho
  • (Ochanomizu Univ.)
  • in collaboration with
  • Satoru Kaneko and Aya omote
  • Seminar at MSU, Oct. 27, 2005

2
Tips
  • Ochanomizu University
  • womens university in Tokyo
  • Location of Ochanomizu (????) area center of
    Tokyo
  • Ocha (??) Tea
  • mizu (?) water

3
Phenomenology of supersymmetric TeV scale see-saw
models
  • Gi-Chol Cho
  • (Ochanomizu Univ.)
  • in collaboration with
  • Satoru Kaneko and Aya omote
  • Seminar at MSU, Oct. 27, 2005

4
1. Introduction
  • Origin of neutrino mass?
  • effective operators for the lepton masses under
    the gauge group of SM
  • then, the electron and neutrino masses are given
    as

L lepton doublet E right-handed electron H
Higgs
5
1. Introduction
  • a simple model which leads to a tiny neutrino
    mass
  • mass matrix of neutrinos
  • neutrino mass

N right-handed neutrino
see-saw mechanism Yanagida (79), Gell-Mann et
al (79)
6
1. Introduction
  • the see-saw mechanism
  • neutrino Yukawa coupling O(1)
  • right-handed neutrino mass 108 GeV
  • hopeless to test the see-saw mechanism directly
  • Alternative? (testable model)
  • possible to lower the see-saw scale?

7
TeV scale see-saw mechanism associated with the
supersymmetry breaking
  • Arkani-Hamed, Hall, Murayama, Smith, Weiner,
    PRD64, 115011, 2001
  • Borzumati, Nomura, PRD64, 053005, 2001
  • March-Russell, West, PLB593, 181, 2004
  • framework hidden sector SUSY breaking scenario
    (SUGRA)
  • tool Giudice-Masiero mechanism for the
    -problem
  • scale of the right-handed neutrino is given as a
    result of SUSY breaking
  • the neutrino Yukawa is naturally suppressed

8
-problem and Giudice-Masiero mechanism
Giudice, Masiero, 1988
  • -problem in the minimal SUSY-SM
  • superpotential
  • scalar potential
  • its scale must be O(mw) for EWSB
  • however, an operator is invariant
    under the SM gauge group
  • natural scale of the -term Planck scale?

9
-problem and Giudice-Masiero mechanism
  • introduce a global symmetry G
  • Hu Hd massless via G
  • superfield X singlet under GSM, but non-trivial
    under G
  • v.e.v. of the F-comp. of X
  • the following operator leads to small mu-term
    after SUSY breaking

10
in this talk
  • gauge invariant mass (i.e. right-handed neutrino)
    can be small owing to the Giudice-Masiero
    mechanism
  • right-handed (s)neutrinos appear in the TeV (or
    EW) scale
  • we discuss some phenomenological aspects of this
    framework

11
Plan of this talk
  • Introduction
  • Model
  • corrections to the lightest Higgs boson mass
  • sneutrino production via charged Higgs decay
  • Summary

12
Model
Arkani-Hamed etal, (2001)
  • Set-up
  • a field X SM singlet, its v.e.v. breaks SUSY
  • R-charges
  • consider high. D operators in the leptonic sector

13
Model
  • If a field X develops both A- and F-component
    v.e.v.

Yukawa coupling 10-8
A-term 103 GeV
14
Model
  • right-handed neutrino mass
  • then, neutrino mass matrix is given as

(v mSUSY )
15
Model
  • consequences of the model
  • typical see-saw scale is O(TeV)
  • neutrino Yukawa is naturally suppressed
  • sneutrino A-term (SUSY breaking scalar trilinear
    coupling) is unsuppressed by the Yukawa coupling

16
3. corrections to the lightest Higgs boson mass
  • note that the lightest Higgs mass is determined
    by the Higgs quartic coupling
  • since the scalar tri-linear coupling for
    , it may affect the lightest Higgs mass via
    1-loop correction

17
destructively interferes with the corrections in
the MSSM (top quark, etc)
however, the correction is suppressed O(10-3) for

18
4. sneutrino production via charged Higgs decay
  • a typical process by a large (unsuppressed)
    A-term
  • MSSM suppressed by lepton Yukawa couplings
  • if slepton is ligter than chargino, it decays
    into charged lepton neutralino
  • excess of charged lepton via charged Higgs decay
    can be expected as compared to MSSM/2HDM

19
Interactions
  • sources
  • D-term int.
  • scalar tri-linear int.
  • in the MSSM, it is suppressed by charged lepton
    Yukawa coupling

20
Interaction of TeV sneutrino
  • sneutrino A-term is not suppressed by the Yukawa
    coupling
  • decay rate could be increased for large A?

21
decay modes of charged Higgs
  • possible decay modes in SUSY-SM
  • top bottom
  • tau neutrino
  • slepton sneutrino
  • chargino neutralino
  • hadronic decay squark quark
  • squarks are assumed to be heavier than charged
    Higgs
  • decay into gauge bosons
    is forbidden at the tree level because of the
    custodial symmetry

22
Numerical study
  • charged Higgs mass 250 or 350 GeV
  • chargino neutralino mass
  • chargino mass matrix
  • inputs
  • neutralino mass GUT relation
  • slepton mass input ? sneutrino in MSSM is fixed
    through the SU(2) relation

23
mH 250GeV
slepton mode in MSSM is kinematically forbidden
24
mH 350GeV
slepton mode in MSSM is kinematically forbidden
25
  • therefore,
  • is smaller than 56
  • on the other hand,
  • is 10
  • therefore, excess of the number of charged lepton
    in the final state is expected
  • decay to sleptonsneutrino overwhelms or is
    comparable with the tau mode because of large
    A-term for small tanß(3)
  • when slepton is lighter than chargino, it
    dominantly decays into leptonneutralino
  • chargino mode even if it has leptonic decay mode
    only, BR is 30 per each lepton flavor.

26
discussion detectability
  • measurement of the charged Higgs pair production
  • a linear collider can do it at its threshold
  • one of them can be confirmed through tb decay
  • then we know that there is another charged Higgs
  • typical size of production cross section of
    charged Higgs pair is O(fb)

27
excess of charged leptons
  • when the integrated luminocity is 100 fb-1,
    100-1000 charged Higgs pair is produced
  • when tanß3, 1000 charged Higgs leads to
  • 30 electrons (MSSM)
  • 130 electrons (TeV seesaw)
  • However we never see any excess if tanßgt10

28
Recipe
  • after discovery of charged Higgs, chargino,
    slepton
  • in principle, MSSM prediction on of charged
    lepton can be made as a function of tanbeta and
    µ/M2
  • determine tanbeta and µ/M2 from some hadronic
    processes
  • if excess of leptons on (tanß,µ/M2) plan is
    found, it gives constraint on (A?, MR)

29
Summary
  • a possibility of TeV scale see-saw induced by
    SUSY breaking
  • some phenomenological aspects have been discussed
  • lightest Higgs boson mass is not affected (could
    not be a source to rise it)
  • collider phenomenology charged Higgs decay
  • signal could be an excess of charged leptons for
    small tanß
  • how to test the model in the case of large tanß?
  • flavor structure (neutrino mixing)?
  • RGE with universal SUSY breaking terms?
Write a Comment
User Comments (0)
About PowerShow.com