- 57 Views
- Uploaded on

Download Presentation
## PowerPoint Slideshow about ' Constrained MSSM' - joella

**An Image/Link below is provided (as is) to download presentation**

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.

- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -

Presentation Transcript

Constrained MSSM

Requirements:

- Unification of the gauge couplings
- Radiative EW Symmetry Breaking
- Heavy quark and lepton masses
- Rare decays (b -> sγ, b->μμ)
- Anomalous magnetic moment of muon
- LSP is neutral
- Amount of the Dark Matter
- Experimental limits from direct search

Allowed region

in the parameter

space of the MSSM

ConstrainedMSSM (Choiceofconstraints)

Experimental lower limits on Higgs and superparticle masses

Regions excluded by Higgs experimental limits provided by LEP2

tan β =35

tan β =50

ConstrainedMSSM(Choice of constraints)

Data on rare processes branching ratios

Regions excluded by experimental limits (for large tanβ)

tan β =50

tan β =35

Constrained MSSM (Choice of constraints)

Data on rare processes branching ratios

Regions excluded by experimental limits (for large tanβ)

tan β =50

tan β =35

Constrained MSSM (Choice of constraints)

Muon anomalous magnetic moment

Regions excluded by muon amm constraint

tan β =50

tan β =35

Constrained MSSM (Choice of constraints)

The lightest supersymmetric particle (LSP) is neutral.

This constraint is aconsequence of R-parity conservation requirement

Regions excluded by LSP constraint

tan β =35

tan β =50

Favoured regions of parameter space

Pre-WMAP allowed regions in the parameter space.

From the Higgs searches tan β>4, from aμmeasurements μ >0

tan β =35

tan β =50

Allowed regions after WMAP

In allowed region one fulfills all the constraints simultaneously and has the suitable amount of the dark matter

LSP

charged

WMAP

Narrow allowed region enables one to predict the particle spectra and the main decay patterns

Higgs

EWSB

Phenomenology essentially depends on the region of parameter space and has direct influence on the strategy of SUSY searches

tan β =50

The Lightest Superparticle

property

signature

- Gravity mediation

jets/leptons

stable

- Gauge mediation

stable

photons/jets

lepton

stable

- Anomaly mediation

lepton

stable

- R-parity violation

LSP is unstable SM particles

Rare decays

Neutrinoless double decay

- Modern limit

SUSY Dark Matter

Neutralino = SUSY candidate for the cold Dark Matter

Neutralino = the Lightest Superparticle (LSP) = WIMP

photino zino higgsino higgsino

- Superparticles are created in pairs
- The lightest superparticle is stable

Download Presentation

Connecting to Server..