A window for New Physics in Bs?KK decays - PowerPoint PPT Presentation

About This Presentation
Title:

A window for New Physics in Bs?KK decays

Description:

But Fd from Amix(BdJ/YKs) and from QCD sum rules. From Adir(Bd pp), Amix(Bd pp), BR(Bdpp), Amix(BdJ/YKs) and CKM fit. BABAR BELLE. Table of results ... – PowerPoint PPT presentation

Number of Views:17
Avg rating:3.0/5.0
Slides: 20
Provided by: lnfI
Category:
Tags: decays | new | physics | window | yks

less

Transcript and Presenter's Notes

Title: A window for New Physics in Bs?KK decays


1
A window for New Physics in Bs?KK decays
  • Joaquim Matias
  • Universitat Autònoma de Barcelona
  • David London JM, PRD (2004)
  • David London JM Javier Virto, PRD (2005)
  • February 2005

2
  • Search for New Physics

Precision Flavour Physics Era
B Physics ExperimentTheory
3
  • How do we prove for NP in CP violation ?
  • Overdetermining the Unitarity Triangle
  • Determination of sides

4
  • CKM fit
  • Compare with the determination of angles from
    CP-asymmetries and ltBRgt.
  • Two strategies a) consistency check
  • b) measure NP

5
  • CP violation in non-leptonic B decays
  • Several channels
  • Fundamental role in determining b and g but
    also New Physics
  • Main problem How to deal with Hadronic Matrix
    Elements
  • Construct clean observable with small QCD
    Polution.
  • Evaluation of hadronic parameters from QCD.
  • Flavour Symmetries to extract maximal
    information from data.
  • -Main hypothesis based on experimental data
  • There are NO sizeable New Physics effects in b?d
    penguin amplitudes.
  • If there is Physics beyond the SM will affect
    b?s penguin amplitudes.

6
  • Anatomy of Bs?KK- decay
  • STANDARD MODEL DESCRIPTION
  • It is governed by the quark-level process
  • T Tree colour allowed, P gluonic penguins,
    PCEW colour suppressed EW penguins, E exchange
    and PA Penguin Annihilation topologies.
  • Two types of contributions charged-current
    VubVus AuCC

  • penguin VubVus(Pu-Pt)VcbVcs(Pc-Pt)

7
  • The SM amplitude can be written
  • Hadronic parameters
  • Remarks
  • - ?C is irrelevant in the
    Standard Model but not
  • in presence of New
    Physics.
  • - All factorizable
    corrections to d drop out.

8
  • BEYOND STANDARD MODEL
    DESCRIPTION
  • In presence of New Physics in the b?s penguin
  • NP operators assumed same size as SM b?s penguin.
  • There are many
    (qu,d,s,c)
  • All New Physics strong phases are negligible
  • - Aq and Fq are process
    dependent.
  • The amplitude is now

9
  • There are 3 measurements in Bs?KK- decay
  • From the time-dependent CP asymmetry (Adir
    and Amix)
  • In the SM these CP asymmetries are
  • AdirSM(Bs?KK-)f(d,?,g) and
    AmixSM(Bs?KK-)g(d, ?,g, Fs)
  • CP Averaged Branching Ratio in the SM

10
  • In presence of New Physics the SM CP asymmetries
    and CP-averaged branching ratio are modified
  • Total number of parameters
  • BNP, DNP and MNP are complicated functions of
    ALL these parameters.


11
  • Parameter determination
  • Weak parameters measured independently
  • CKM angle g
  • B?DK
    unaffected by New Physics
  • a from
    B?pp, B??p, B???
  • ß from
    Amix(Bd(t)?J/?Ks)
  • CKM fit.
  • Weak mixing phase Fs from CP violating Bs?J/?F
  • NP contributions to the mixing Fs FsSMdFs
  • contribution controlled
    by Bd(t)?J/?Ks lt20

12
  • Hadronic Parameters
  • Keypoint U-spin (interchange d?s) related
    process Bd?pp-
  • quark level transition
    available to B Factories.
  • no New Physics
    contribution.
  • Amplitude in SM
  • Wolfenstein parametrization in SM

  • Same functional dependence

13
  • Can we determine d, q and C?
  • Present Experimental Situation
  • Babar and Belle are inconsistent
  • If we average naïvely the asymmetries
  • A large direct CP asymmetry from Belle (large
    strong phases) would be troublesome for QCD-NLO
    factorization.
  • Three measurements Adir(Bd? pp), Amix(Bd? pp)
    and BR(Bd?pp)
  • Total parameters in SM

  • - 3 hadronic parameters

  • - 2 weak parameters


14
From Adir(Bd? pp), Amix(Bd? pp), BR(Bd?pp),
Amix(Bd?J/YKs) and CKM fit











BABAR
BELLE


15
Table of results From U-spin
breaking effects
Our predictions for Amix, Adir of Bs?KK and Rds
in SM Also from the Bd?pp and BR(Bs?KK)
we can give a prediction for g in SM
350 g
740 In the
NEAR FUTURE we will MEASURE NEW PHYSICS
Adir(Bs? KK), Amix(Bs?
KK),
BR(Bs?KK), Amix(Bs?J/YF)

Observable (SM) Babar Belle
Adir(Bs? KK-) (-1 , 1) (-.02 , .18)
Amix(Bs? KK-) (-1 , 1) (-.19 , .05)
Rds (0.1 , 13.9) (3.6 , 85.5)


16
In the meanwhile Consistency check for the
PRESENCE of NEW PHYSICS In the SU(3)
limit depend on four theoretical parameters -
Penguin parameters - Weak mixing angle
- CKM angle
CKM fit (Rb and Rt) Including all
theoretical uncertainties And
experimental errors at 1s
17
Alternative in the future DETERMINE
GAMMA/PRESENCE OF NP Once the CP asymmetries of
Bs?KK- are measured SM range strongly
restricted Sensitivity to U-spin breaking is
very reduced Allowed region to the SM


18
  • Conclusions
  • Non-leptonic B decays are playing a
    fundamental role in the exploration of CP
    violation.
  • Recent measurement of BR(Bs?KK-) together
    with the future data on the CP asymmetries
    Adir(Bs?KK-) and Amix(Bs?KK-) will open
    exciting new perspectives and strategies
  • To search for New Physics signals in B decays
  • To determine CKM angle gamma

19
  • Present experimental situation is quite
    uncertain
  • Babar and Belle are inconsistent
  • If we average naïvely
  • A large direct CP asymmetry from Belle (large
    strong phases) would be troublesome for QCD-NLO
    factorization.
  • Deviation from U-spin
  • Only non-factorizable effects in
  • Explored dependence of the predictions on U-spin
    deviations
  • for
  • 3. Prediction 350 ? 740

Write a Comment
User Comments (0)
About PowerShow.com