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B physics and supersymmetry with general flavor mixing Ken-ichi Okumura (Tohoku University) In collaboration with John Foster and Leszek Roszkowski hep-ph/0604121, hep-ph/0510422, hep-ph/0506146, hep-ph/0410323 Based on 特特特特 特特特特特特特特特特特特特特特2009 「」 @ 特特

B physics and supersymmetry with general flavor mixing

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特定領域「フレーバー物理の新展開」研究会2009 @ 蒲郡. B physics and supersymmetry with general flavor mixing. Ken-ichi Okumura (Tohoku University) In collaboration with John Foster and Leszek Roszkowski. Based on. hep-ph/0604121, hep-ph/0510422, hep-ph/0506146, hep-ph/0410323. Plan of talk. Introduction - PowerPoint PPT Presentation

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Page 1: B physics and supersymmetry with general flavor mixing

B physics and supersymmetry with general flavor mixing

Ken-ichi Okumura (Tohoku University)

In collaboration with

John Foster and Leszek Roszkowski

hep-ph/0604121, hep-ph/0510422, hep-ph/0506146, hep-ph/0410323

Based on

特定領域「フレーバー物理の新展開」研究会2009 @ 蒲郡

Page 2: B physics and supersymmetry with general flavor mixing

Plan of talk

Introduction Supersymmetry with general flavor mixing b-s transitions Conclusion

Page 3: B physics and supersymmetry with general flavor mixing

The SM: CKM paradigm

Page 4: B physics and supersymmetry with general flavor mixing

Why Supersymmetry ?SM

S.P.Martin (1997)

MSSM

Page 5: B physics and supersymmetry with general flavor mixing

Supersymmetry doubles flavor

Soft mass

Tri-linear termGaugino mass

Page 6: B physics and supersymmetry with general flavor mixing

Minimal flavor violation (MFV)

Super CKM basis

Page 7: B physics and supersymmetry with general flavor mixing

General Flavor Mixing

Page 8: B physics and supersymmetry with general flavor mixing

Origin of flavor mixing

SUSY

GUT

Large flavor mixing( MSN matrix)

S.Baek, T.Goto Y.Okada KO (2000)

Ex) Seesaw mechanism

“Probe of GUT scale int.”

Radiative correction

Page 9: B physics and supersymmetry with general flavor mixing

Collider vs flavor physics

mixing

Mass

sp

ect

rum

LHC

Flavor Physics !

Complementary each other

SUSY Lagragian

Page 10: B physics and supersymmetry with general flavor mixing

b →s transitions

Page 11: B physics and supersymmetry with general flavor mixing

NP effects interfere with the SM

Add

MFV

GFM

M.Misiak&M.Steinhauser (2006)

Page 12: B physics and supersymmetry with general flavor mixing

MFV

Page 13: B physics and supersymmetry with general flavor mixing
Page 14: B physics and supersymmetry with general flavor mixing

KO and L.Roszkowski (2001)

Not diagonal !

SUSY

Page 15: B physics and supersymmetry with general flavor mixing

Higgs mediated FCNCNon-holomorphicIntegrate out SUSY particles

:Flavor diagonal

NG

Page 16: B physics and supersymmetry with general flavor mixing
Page 17: B physics and supersymmetry with general flavor mixing

J.Foster, KO, L.Roszkowski (2005)

Page 18: B physics and supersymmetry with general flavor mixing
Page 19: B physics and supersymmetry with general flavor mixing

 

P.Ball and R.Fleischer (2006)

Lattice

CKM angle & side

Page 20: B physics and supersymmetry with general flavor mixing
Page 21: B physics and supersymmetry with general flavor mixing

MFV

Page 22: B physics and supersymmetry with general flavor mixing
Page 23: B physics and supersymmetry with general flavor mixing
Page 24: B physics and supersymmetry with general flavor mixing

All combined : single insertion

Page 25: B physics and supersymmetry with general flavor mixing
Page 26: B physics and supersymmetry with general flavor mixing

CP violation in

CKMfitter UTfit

Page 27: B physics and supersymmetry with general flavor mixing
Page 28: B physics and supersymmetry with general flavor mixing

Conclusion We reported current limits on flavor mixing in b-s

transitions in minimal supersymmetry (beyond leading order+Higgs mediated).

Constraint from Bs mixing is quite severe for RR and RL mixing at moderate-large tanβ (~30) despite relatively large theoretical uncertainty.  

Precision measurement of Φ3 + Bs mixing can improve the bound (or find NP) as well as BR(Bs→μμ).

Low tanβ region can be covered by tCPV in radiative decay.

Combined with the spectrum measurement, such a measurement provides a clue to high energy scale.