Rare B decays and B-B mixing in NMFV SUSY

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Rare B decays and B-B mixing in NMFV SUSY

Miguel Arana Catania

Higgs Boson masses and B-Physics Constraints in Non-Minimal Flavor Violating SUSY scenarios

http://arxiv.org/hep-ph/1109.6232

Published on JHEP, vol 2012, issue 5

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Hunting the NMFV

1. SUSY scenarios with NMFV 2. Constraints from B-Physics

3. Radiative corrections to Higgs masses

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SUSY scenarios with NMFV

Quark sector: Interaction basis Mass basis

Squark sector: Interaction basis SCKM basis

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We consider all

possible deltas

parameterizing 2

and 3 generation

mixing.

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LHC constraints

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LHC constraints

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Heavy SUSY scenarios in order to avoid LHC constraints. All SUSY Other points with <0 and ≠ 0 also considered

Lightests

sparticles

masses

(in GeV):

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Constraints from B-Physics

We choose the following observables:

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Constraints from B-Physics

and prime operators exchanging L by R

We consider MSSM contributions from:

Loops with Higgs bosons Loops with charginos

Loops with gluinos

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Box diagrams with charginos Z-penguin diagrams with charginos

Neutral Higgs penguin diagrams with charginos and gluinos and prime operators

exchanging L by R

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Box diagrams (charginos and gluinos) Z-penguin diagrams (charginos)

Neutral Higgs double penguin diagrams

(charginos and gluinos)

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sets strict bounds on

sets bounds for large and low General larger sensitivity to the sb sector.

ct sector less constrained

sets also strong bounds on

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Large allowed if heavy SUSY at large also restricts

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Results changing the sign of ( <0)

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also set If is low,

restrictions even at low =5

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Excluded MFV points can be recovered in NMFV

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CMSSM-30

Constraints from B-Physics (two-dimensional constraints)

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CMSSM-30

We found large allowed space in the RRct

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CMSSM-30

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CMSSM-5

The allowed space grows for low

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CMSSM-5

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CMSSM-5

And also large LR/RLct deltas allowed.

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NUHM-30

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NUHM-30

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NUHM-30

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NUHM-5

In low scenarios if is small,

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NUHM-5

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NUHM-5

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Radiative corrections to Higgs masses

We computed the NMFV contributions to Higgs masses since this contributions could be relevant.

Feynman diagrammatic approach

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Radiative corrections to Higgs masses

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In general, larger corrections for the light Higgs coming

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CMSSM-5

Constraints from B-Physics and radiative corrections to Higgs masses

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CMSSM-30

Very large Higgs

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NUHM-30

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CMSSM-5

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NUHM-5

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Conclusions

We found bounds for flavor from B physics, and large corrections to the Higgs boson masses compatible with these bounds, up to several tens GeV for the lightest boson.

These corrections are two orders of magnitude larger than the LHC precission, and three orders than the ILC.

Mainly coming from the ct sector (which is less constrained by B- Physics) and from scenarios with low . Also from high if SUSY is very heavy (order 1 TeV or larger).

These corrections can be used to set further bounds on flavour

Rare B decays and B-B mixing in NMFV SUSY