Title: Phenomenology of Supersymmetric GaugeHiggs Unification
1Phenomenology of Supersymmetric Gauge-Higgs
Unification
- Sylvain Fichet
- LPSC Grenoble
- Collaboration Felix Brümmer (IPPP Durham),
Arthur Hebecker (Heidelberg) and Sabine Kraml
(LPSC) - Arxiv 0906.2957
2Gauge-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
3SUSY 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.
4Theory
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
5Theory
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
-
6Theory
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
-
7Theory
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 !
8Theory
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
9Theory
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
-
10Theory
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.
-
11Theory
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.
12Phenomenology
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
13Phenomenology
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 )
14Phenomenology
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
15Scans 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
-
16RGE 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
17RGE 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
18RGE analysis
Phenomenology
14
- If large and positive
- If small or negative
19Phenomenology
RMSB parameter space
15
- RMSB parameters for the same points
-
- is , is not too large
wrt - No points for !
-
20Phenomenology
Relic density
16
- Dark matter relic density 3s WMAP measurement
-
- Assuming standard cosmology !
-
Not enough
Good
Too much
!
21Phenomenology
Mass spectrum and decays
17
- Masses
-
-
-
- 3 possible LSPs
- small
-
-
-
2
1
0
22Phenomenology
Mass spectrum and decays
17
- Masses
-
-
-
- 3 possible LSPs
- small
-
- SFOS dilepton
-
2
65
30
1
50
0
2318
- 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 26Constraint with g-2
27Examples of mass spectrum
28Fixed point vs dichotomy
29Algorithm
30A mSUGRA example
Higgs Gauginos Sparticles
Gluino dominated squark running
Radiative EWSB
31Higgs sector
- Higgs potential (after some gauge rotations)
- -potentiel bounded from below
- -non-trivial minimum
- Minimization
with
32Higgs sector
- The bilinear parameter µ
- The bilinear parameter B (susy breaking)
- Higgs masses (susy breaking)
with
33Interesting 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
34Couplings and sparticles masses
- Yukawas
- Trilinear couplings (susy breaking)
- Sparticle masses (susy breaking)