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Phenomenology of Supersymmetric GaugeHiggs Unification

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Extra dimensions motivated by doublet-triplet problem, GUT group breaking, proton decay ... SUSY GUTs with Gauge-Higgs Unification and RMSB generically implies : ... – PowerPoint PPT presentation

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Title: Phenomenology of Supersymmetric GaugeHiggs Unification


1
Phenomenology of Supersymmetric Gauge-Higgs
Unification
  • Sylvain Fichet
  • LPSC Grenoble
  • Collaboration Felix Brümmer (IPPP Durham),
    Arthur Hebecker (Heidelberg) and Sabine Kraml
    (LPSC)
  • Arxiv 0906.2957

2
Gauge-Higgs Unification
Theory
2
  • What is Gauge-Higgs Unification ?
  • And with supersymmetry ?

4D spin 1 gauge
4D spin 0 Higgs
Review 0704.0833
5D vector superfield 4D
vector superfield 4D chiral superfield
4D spin 1 gauge
4D spin 0 Higgs
3
SUSY GUTs with Gauge-Higgs Unification
Theory
3
  • Where SUSY GHU can appear ?
  • In orbifold SUSY GUTs
  • SUSY GUTs motivated by couplings unification
  • Extra dimensions motivated by doublet-triplet
    problem, GUT group breaking, proton decay
  • (5D SU(6) GHU Burdman, Nomura hep-ph/0210257
    )
  • A top-down motivation SUSY GUT with GHU can
    naturally come from classes of heterotic strings
    model.

4
Theory
SUSY GUTs with Gauge-Higgs Unification
4
  • Natural way to break SUSY ?
  • With Radion Mediated SUSY breaking (RMSB)
  • Chacko, Luty hep-ph/0008103
  • Radion T field associated to extra dimension
    fluctuation
  • Compactification
    implies SUSY breaking
  • (radion )
  • (chiral compensator gravity effect)
  • with
  • Anomaly Mediation contributions are generated at
    one-loop

5
Theory
SUSY GUTs with Gauge-Higgs Unification
5
  • SUSY GUTs with Gauge-Higgs Unification and RMSB
    generically implies
  • at the
    SUSY breaking scale.
  • Solves the mu-problem
  • Giudice-Masiero mechanism Giudice, Masiero 88
    Phys.Lett.B206480-484
  • Reminder

6
Theory
5D complete realization gauge-Higgs sector
6
  • 5D SUSY GUT with SU(6) GHU Burdman, Nomura
    hep-ph/0210257
  • Radius T of the 5th dimension stabilized by an
    unknown mechanism
  • and break the SU(6) adjoint
  • 2 Higgs doublets

7
Theory
5D complete realization gauge-Higgs sector
6
  • 5D SUSY GUT with SU(6) GHU Burdman, Nomura 03
    hep-ph/0210257
  • Radius T of the 5th dimension stabilized by an
    unknown mechanism
  • and break the SU(6) adjoint
  • 2 Higgs doublets
  • It implies the high-scale relations

  • Negative conclusions
  • no EWSB
  • Choi et al. hep-ph/0312178
  • But one contribution was not taken into account !

8
Theory
5D complete realization gauge-Higgs sector
7
  • In odd number of dimension, a new term in the
    Lagangian is allowed
  • the Chern-Simons term
  • e.g. in 5D non-susy
    Review 0805.1778
  • Fixed in a full theory, but here parametrized
    with free coefficient .
  • The high-scale relations become
  • Hebecker et al. 0801.4101, Brümmer et al.
    0906.2957
  • For theory consistency and
  • Sign ambiguity

9
Theory
5D complete realization matter sector
8
  • What about matter fields ?
  • Matter in the bulk, but can be confined if
    massive
  • 4D yukawas come from the overlap with Higgs
    field.
  • can generate mass hierarchy
  • for matter fermions

10
Theory
5D complete realization matter sector
8
  • What about matter fields ?
  • Matter in the bulk, but can be confined if
    massive
  • 4D yukawas come from the overlap with Higgs
    field.
  • can generate mass hierarchy
  • for matter fermions
  • What about soft scalar parameters ?
  • Only bulk matter couples
  • to SuSy breaking fields.
  • similar hierarchy for soft scalars
  • ,
    large,
  • others negligible.

11
Theory
Summary
9
  • To sum up
  • Orbifold SUSY GUT with GHU RMSB
  • Model with 5D SU(6) GHU and Chern Simons term
  • Confinement of matter fields controls
  • mass hierarchies (yukawas couplings) and
  • soft scalar parameters.

12
Phenomenology
Spectrum calculation
10
  • How to calculate the spectrum of such models ?
  • Use a spectrum calculator (SuSpect)
    hep-ph/0211331
  • but the pattern of input and constraints is
    different from other models
  • Usually and calculated from the
    2 equations of Higgs potential minization, at
    each iteration.
  • But in our model
    fixed from high scale relation

13
Phenomenology
Spectrum calculation
10
  • How to calculate the spectrum of such models ?
  • Use a spectrum calculator (SuSpect)
    hep-ph/0211331
  • but the pattern of input and constraints is
    different from other models
  • Usually and calculated from the
    2 equations of Higgs potential minization, at
    each iteration.
  • But in our model
    fixed from high scale relation
  • First solution compute and
    at each iteration.
  • But unstable for !
    (Potential fix fixed point gt dichotomy)
  • Second solution Simply impose
    at high energy.
  • input parameters
  • matter sector parameters (in the 5D model 2
    mixing angles and )

14
Phenomenology
Scans and constraints
11
  • Scans over
  • with 4 sign combination
    and
  • Constraints
  • Theoretical (verified in Suspect) EWSB, CCB,
    tachyons
  • Collider experiments
  • Mass bounds from LEP http//lepsusy.web.
    cern.ch/lepsusy/
  • B-physics (2s)
  • CDF 0712.1708 hep-ex
  • HFAG hep-ex/0603003
  • Dark matter (3s)
  • WMAP 0803.0586 astro-ph

15
Scans and constraints
Phenomenology
12
Scan with
  • LSP
  • red
  • blue
  • green
  • Points excluded by B-physics or too light
  • similar result with
  • No points for the 2 other combinations

16
RGE analysis
Phenomenology
13
  • Why such sign combinations ?
  • We have
  • And dominated by
  • The overall sign is fixed by
  • For a given ,
    only one is allowed.

GHU
RGE
EWSB
gt 0
17
RGE analysis
Phenomenology
13
  • Why such sign combinations ?
  • We have
  • And dominated by
  • The overall sign is fixed by
  • For a given ,
    only one is allowed.
  • Which sign is selected depends on
    running.
  • is dominated by the gluino mass
  • Roughly universal running
  • Only the initial value
    matters.

GHU
RGE
EWSB
gt 0
18
RGE analysis
Phenomenology
14
  • If large and positive
  • If small or negative

19
Phenomenology
RMSB parameter space
15
  • RMSB parameters for the same points
  • is , is not too large
    wrt
  • No points for !

20
Phenomenology
Relic density
16
  • Dark matter relic density 3s WMAP measurement
  • Assuming standard cosmology !

Not enough
Good
Too much
!
21
Phenomenology
Mass spectrum and decays
17
  • Masses
  • 3 possible LSPs
  • small

2
1
0
22
Phenomenology
Mass spectrum and decays
17
  • Masses
  • 3 possible LSPs
  • small
  • SFOS dilepton

2
65
30
1
50
0
23
18
  • CONCLUSION
  • SUSY GHU works,
  • has a particular mass spectrum,
  • and has a good potential of discovery at LHC
  • TO-DO LIST
  • Discrimination among other models
  • See what happens in warped geometry (holographic
    models)
  • Include a massive right-handed neutrino

24
  • Thanks for your attention !

25
  • EXTRAS

26
Constraint with g-2

27
Examples of mass spectrum
28
Fixed point vs dichotomy

29
Algorithm
30
A mSUGRA example
Higgs Gauginos Sparticles
Gluino dominated squark running
Radiative EWSB
31
Higgs sector
  • Higgs potential (after some gauge rotations)
  • -potentiel bounded from below
  • -non-trivial minimum
  • Minimization

with
32
Higgs sector
  • The bilinear parameter µ
  • The bilinear parameter B (susy breaking)
  • Higgs masses (susy breaking)

with
33
Interesting features of other RGES
  • Superpotential parameter corrections are
    proportional to the parameters themselves
  • All susy-breaking parameters depend on gaugino
    masses .
  • Squark masses receive large negative corrections
    from the gluino mass
  • mass receives large positive corrections from
    the top yukawa

with
34
Couplings and sparticles masses
  • Yukawas
  • Trilinear couplings (susy breaking)
  • Sparticle masses (susy breaking)
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