lfv from susy-guts : the impact of uactive.pd.infn.it/g4/seminars/2007/files/calibbi.pdflfv from...

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LFV from SUSY-GUTs : the impact of U e3 Lorenzo Calibbi Università di Padova & INFN sez. di Padova JOURNAL CLUB DI FISICA TEORICA E ASTROPARTICELLARE PADOVA, 30/01/2007 Mainly based on: L.C., A. Faccia, A. Masiero and S. K. Vempati, Phys. Rev. D 74 (2006) 116002, arXiv:hep-ph/0605139 and arXiv:hep-ph/0610241.

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Page 1: LFV from SUSY-GUTs : the impact of Uactive.pd.infn.it/g4/seminars/2007/files/calibbi.pdfLFV from SUSY-GUTs : the impact of U e3 Lorenzo Calibbi ... LFV from SUSY GUTs Lorenzo Calibbi

LFV from SUSY-GUTs :the impact of Ue3

Lorenzo CalibbiUniversità di Padova & INFN sez. di Padova

JOURNAL CLUB DI FISICA TEORICA E ASTROPARTICELLARE

PADOVA, 30/01/2007

Mainly based on:

L.C., A. Faccia, A. Masiero and S. K. Vempati, Phys. Rev. D 74 (2006) 116002,

arXiv:hep-ph/0605139 and arXiv:hep-ph/0610241.

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LFV from SUSY GUTs Lorenzo Calibbi

Outline

• LFV sources in low-energy SUSY

• SO(10) framework and consequences on the Yukawas

• mSUGRA parameter space

• LFV processes and discovery potential of the dedicated experiments

• The Ue3 dependence of : RG vs. GUT effects

• Conclusions

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Why studying LFV in the era of the LHC?

•It exists in nature! (in the neutrinos sector…)

•It is (in general) a consequence of new physics at the TeV scale,

while in the SM is higly suppressed

•Model dependent

LFV from SUSY GUTs Lorenzo Calibbi

Running: BaBar, Belle

Upcoming: MEG (2006)

Future: SuperKEKB (2011)

PRISM/PRIME (next decade)

Super Flavour factory (?)

Experiments:

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Why studying LFV in the era of the LHC?

•It exists in nature! (in the neutrinos sector…)

•It is (in general) a consequence of new physics at the TeV scale,

while in the SM is higly suppressed

•Model dependent

LFV from SUSY GUTs Lorenzo Calibbi

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LFV from SUSY GUTs Lorenzo Calibbi

GUT effect (e.g. SU(5) ) if MX > MGUTSee-saw:

SUSY induced LFV:

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LFV from SUSY GUTs Lorenzo Calibbi

The most general renormalizable SO(10) superpotential, relevant to fermionmasses:

At least one of the eigenvalues of the neutrino Yukawa matrix in

has to be as large as the top Yukawa.

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LFV from SUSY GUTs Lorenzo Calibbi

And what about the mixing angles? We consider two benchmark cases:

“Minimal” mixing (CKM): “Maximal” mixing (PMNS):

CKM case:

PMNS case:

Just frameworks to compute the RG effects in the soft masses sector,

not complete fermion masses & mixings models!

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LFV from SUSY GUTs Lorenzo Calibbi

Scheme of the RG running and of the energy scales involved

Sketch of the running routineHow does the routine work:

•Running of the low energy fermion param.

•Definition of Yν

•MR from see-saw

•RG evolution of the soft parameters

•SUSY spectrum

•Th. & Exp. checks

•Computation of the LFV processes ratesthrough the exact SUSY masses and mixings

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LFV from SUSY GUTs Lorenzo Calibbi

Scanning the mSUGRA parameter space:

Theoretical constraints:

•REWSB

•No tachyonic particles

•Neutral LSP

Experimental constraints:

•LEP limit on Higgs mass

•Limits on SUSY particles

The region where at least one squark has mass below 2.5 TeVis ‘our’ LHC accessible region.

MSSM

tanβ = 30; A0 = 0; mt = 173 GeV

0 < m0 < 5000 GeV

0 < M1/2 < 1500 GeV

-3m0 < A0 < + 3m0

tanβ = 10, 40

μ and Bμ fixed by EWB

NO REWSB

STAU LSP

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LFV from SUSY GUTs Lorenzo Calibbi

Scanning the mSUGRA parameter space:

Theoretical constraints:

•REWSB

•No tachyonic particles

•Neutral LSP

Experimental constraints:

•LEP limit on Higgs mass

•Limits on SUSY particles

The region where at least one squark has mass below 2.5 TeVis ‘our’ LHC accessible region.

SU(5)RN

tanβ = 30; A0 = 0; mt = 173 GeV

0 < m0 < 5000 GeV

0 < M1/2 < 1500 GeV

-3m0 < A0 < + 3m0

tanβ = 10, 40

μ and Bμ fixed by EWB

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LFV from SUSY GUTs Lorenzo Calibbi

Scanning the mSUGRA parameter space:

Theoretical constraints:

•REWSB

•No tachyonic particles

•Neutral LSP

Experimental constraints:

•LEP limit on Higgs mass

•Limits on SUSY particles

The region where at least one squark has mass below 2.5 TeVis ‘our’ LHC accessible region.

REWSB:

0 < m0 < 5000 GeV

0 < M1/2 < 1500 GeV

-3m0 < A0 < + 3m0

tanβ = 10, 40

μ and Bμ fixed by EWB

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LFV from SUSY GUTs Lorenzo Calibbi

Scanning the mSUGRA parameter space:

Theoretical constraints:

•REWSB

•No tachyonic particles

•Neutral LSP

Experimental constraints:

•LEP limit on Higgs mass

•Limits on SUSY particles

The region where at least one squark has mass below 2.5 TeVis ‘our’ LHC accessible region.

REWSB:

0 < m0 < 5000 GeV

0 < M1/2 < 1500 GeV

-3m0 < A0 < + 3m0

tanβ = 10, 40

μ and Bμ fixed by EWB

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LFV from SUSY GUTs Lorenzo Calibbi

Scanning the mSUGRA parameter space:

0 < m0 < 5000 GeV

0 < M1/2 < 1500 GeV

-3m0 < A0 < + 3m0

tanβ = 10, 40

μ and Bμ fixed by EWB

Theoretical constraints:

•REWSB

•No tachyonic particles

•Neutral LSP

Experimental constraints:

•LEP limit on Higgs mass

•Limits on SUSY particles

The region where at least one squark has mass below 2.5 TeVis ‘our’ LHC accessible region.

LSP:

(right stau mass for m0 = 0 )

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LFV from SUSY GUTs Lorenzo Calibbi

and MEG sensitivity reach

But in the PMNS case, the rate depends on Ue3 …

• Maximal mixing (PMNS), high tanβ case, already ruled out in the LHC accessible region.

MEG will test it well beyond the LHC.

• Minmal case (CKM) presently unconstrained.

MEG will test, for high values of tanβ, the region

10-14

10-13

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LFV from SUSY GUTs Lorenzo Calibbi

and MEG sensitivity reach

But in the PMNS case, the rate depends on Ue3 …

• Maximal mixing (PMNS), high tanβ case, already ruled out in the LHC accessible region.

MEG will test it well beyond the LHC.

• Minmal case (CKM) presently unconstrained.

MEG will test, for high values of tanβ, the region

CHOOZ limit:

These scatter plots:

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LFV from SUSY GUTs Lorenzo Calibbi

and the Super B (and Flavour) factories

10-10

10-9

10-810-9

10-10

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LFV from SUSY GUTs Lorenzo Calibbi

and PRISM/PRIME conversion experiment

10-1610-17

10-18

10-17

10-16

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LFV from SUSY GUTs Lorenzo Calibbi

“Running” Ue3 and

PMNS case:

“CKM” case

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LFV from SUSY GUTs Lorenzo Calibbi

in the Ue3 = 0 PMNS case

• The PMNS Ue3 = 0 scenario is currentlybetter costrained by

• For high values of tanβ, MEG will probe almost all the LHC accessible parameterspace

• In the case of small tanβ, MEG will test up to

The observed enhancement is due to the interplay of different effects:

• The running of Ue3 from low energy up tothe high scale where the PMNS condition isimposed

• The dominance in some regions of the paramater space of SU(5) generatedcontributions

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LFV from SUSY GUTs Lorenzo Calibbi

The Ue3 evolution gives, for hierarchical neutrinos (phases set to 0):

RG evolution

Indipendent of Ue3 !

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LFV from SUSY GUTs Lorenzo Calibbi

The Ue3 evolution gives, for hierarchical neutrinos (phases set to 0):

RG evolution

Indipendent of Ue3 !

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LFV from SUSY GUTs Lorenzo Calibbi

“Pure” SU(5) effects

Let’s turn on the SU(5) running

double MI indipendent of Ue3 (usually subdominant):

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LFV from SUSY GUTs Lorenzo Calibbi

Region I: Region II:

SPS 3

m0 = 90 GeV , M1/2 =400 GeV,

A0 = 0, tanβ = 10

SPS 2

m0 = 1450 GeV , M1/2 =300 GeV,

A0 = 0, tanβ = 10

Contour plot

Ue3 = 0

tanβ = 10

A0 = 0 10-14

10-15

10-13

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LFV from SUSY GUTs Lorenzo Calibbi

Region I: Region II:

SPS 3

m0 = 90 GeV , M1/2 =400 GeV,

A0 = 0, tanβ = 10

SPS 2

m0 = 1450 GeV , M1/2 =300 GeV,

A0 = 0, tanβ = 10

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LFV from SUSY GUTs Lorenzo Calibbi

Region I: Region II:

SPS 3

m0 = 90 GeV , M1/2 =400 GeV,

A0 = 0, tanβ = 10

SPS 2

m0 = 1450 GeV , M1/2 =300 GeV,

A0 = 0, tanβ = 10

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LFV from SUSY GUTs Lorenzo Calibbi

Dependence on tanβ

Region I:

Region II:

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LFV from SUSY GUTs Lorenzo Calibbi

Dependence on tanβ

Region I:

Region II:

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LFV from SUSY GUTs Lorenzo Calibbi

Conclusions• LFV experiments are able to constrain/discriminate among different SUSY-GUTs scenarios, thus resulting highly complementary to the LHC.

Supposing that LHC does find evidences of SUSY:

• If they detect LFV processes, considering the interplay between different experiments, we should be able to get a deep insight into the structure of Yν

• If MEG (and Super Flavour) happens not to see LFV, only two possibilitiesshould be left:

a) minimal mixing, low tanβ scenario

b) mSUGRA-SO(10) see-saw without fine-tuned Yν is not a viable framework of new physics.

• If the planned high sensitivity of PRISM/PRIME doesn’t manage to find LFV evidences, the latter conclusion should be the most feasible one.

Moreover:

• LFV experiments will be able to test some scenarios even in the region of the mSUGRA parameter space beyond the LHC sensitivity reach

•The correlation of Ue3 and LFV can be important in the context of SUSY-GUTs and any measurement of LFV at MEG could shed some light on eitherUe3 or on the parameter space of SUSY-GUTs.