CKM Fit and Model independent constraints on physics Beyond the Standard Model Achille Stocchi (LAL-Universite Paris-Sud/Orsay) On behalf of the UTFit.

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CKM Fit and Model independent constraints on physics Beyond the Standard Model Achille Stocchi (LAL-Universite Paris-Sud/Orsay) On behalf of the UTFit Collaboration 6th International Workshop on the CKM Unitarity Triangle (Physics Department of the University of Warwick 6-10 Sept. 2010)

Global Fit within the SM  = ±  = ± SM Fit CKM matrix is the dominant source of flavour mixing and CP violation Consistence on an over constrained fit of the CKM parameters

There are two statistical methods to perform these fits.The overall agreement between them is satisfactory, unless there is some important disagreement Problem on  combination are all consistent  (many ADS/GLW/Dalitz..) measurements are all consistent Most precise15 o error Most precise measurements (two Dalitz analyses) have an about 15 o error Combining the measurements with  the statistical method (frequentist) used by the Collaborations or UTfit we consistently get  (11-12) o (UTFit/stat. analysis a la Babar/Belle)  CKMfitter statistical treatment you get  (20-30) o CKMFitter These fits are continuously updated. Error on  from CKMFitter is 2-3 times larger wrt the frequentist/bayesian method give due to their particular statistical treatement

In this talk we address the question by examine : 1) Possible tensions in the present SM Fit ? 2)Fit of NP-  F=2 parameters in a Model “independent” way 3)“Scale” analysis in  F=2 Is the present picture showing a Standardissimo Model Standardissimo ? An evidence, an evidence, my kingdom for an evidence From Shakespeare's Richard III

SM predictions of  ms SM expectation Δm s = (18.3 ± 1.3 ) ps -1 agreement between the predicted values and the measurements at better than : 66 55 33 44 11 22 Legenda msms 10 Prediction “era” Monitoring “era”

   m s deviations within 1 

 -1.7  devation Three “news” ingredients 1)Buras&Guadagnoli BG&Isidori corrections  Decrease the SM prediction by 6% 2) Improved value for BK  BK=0.731±0.07 ± ) Brod&Gorbhan charm-top contribution at NNLO  enanchement of 3% (not included yet in this analysis)

sin2  +2.6  deviation You have to consider the theoretical error on the sin2  agreement ± (CPS)(2005-updated) 2.2  (FFJM)(2008) 1.6  sin2  =0.654 ± From direct measurement sin2  =0.771 ± from indirect determination

Br(B   -3.2  deviation Nota Bene  To accommodate Br(B   we need large value of V ub  To accommodate sin2  we need lower value of V ub Br(B   ) =(1.72± 0.28)10 -4 From direct measurement Br(B   =( 0.805± 0.071)10 -4 SM prediction

PredictionMeasurement Pull  (69.6 ±3.1)°(74 ±11)°-0.4  (85.4 ±3.7)°(91.4 ±6.1)°-0.8 sin2  0.771± ±  +2.2 V ub [10 3 ]3.55 ± ±0.20 *-0.9 V cb [10 3 ]42.69 ± ±0.45 *+1.6  K [10 3 ] 1.92 ± ± Br(B   ) 0.805± ±  m s (ps -1 )17.77± ± Summary Table of the Pulls * Both in V cb and V ub there is some tensions between Inclusive and Exclusive determinations. The measurements shown is the average of the two determinations

 CdCd dd C s ss CKCK  D  X V ub /V cb XX mdmd XX ACP  J  X X ACP  D  ),DK  X X A SL XX  XX A CH XXXX  s),  s  s XX msms X ASL(Bs)XX ACP  J  ~XX KK XX Tree processes 1  3 family 2  3 family 1  2 familiy  F=2 NP model independent Fit Parametrizing NP physics in  F=2 processes

 = ±  = ±  = ±  = ± SM analysis NP-  F=2 analysis  fit quite precisely in NP-  F=2 analysis and consistent with the one obtained on the SM analysis [error double] (main contributors tree-level  and V ub ) 5 new free parameters C s,  s B s mixing C d,  d B d mixing C  K K mixing Today : fit is overcontrained Possible to fit 7 free parameters (   C d,  d,C s,  s, C  K ) Please consider these numbers when you want to get CKM parameters in presence of NP in  F=2 amplitudes (all sectors 1-2,1-3,2-3)

With present data A NP /A SM 1.5  A NP /A SM prob. C Bd = 0.95± 0.14  Bd = -(3.1 ± 1.7) o [-7.0,0.1] 1.8  deviation dd 1.8  agreement takes into account the theoretical error on sin2 

C Bs = 0.95± 0.10 ss New : CDF new measurement reduces the significance of the disagreement. Likelihood not available yet for us. New : a  from D0 points to large  s, but also large  s  not standard  12 ?? ( NP in  12 / bad failure of OPE in  12.. Consider that it seems to work on  11 (lifetime) 3.1  deviation  Bs = (-20 ± 8) o U (-68 ± 8) o [-38,-6] U [-81,-51] 95% prob. New results tends to reduce the deviation

Effective Theory Analysis  F=2 L is loop factor and should be : L=1 tree/strong int. NP L=   s or   W for strong/weak perturb. NP C(  ) coefficients are extracted from data F 1 =F SM =(V tq V tb *) 2 F j=1 =0 MFV |F j | =F SM arbitrary phases NMFV |F j | =1 arbitrary phases Flavour generic Effective Hamiltonian in the mixing amplitudes

From Kaon 95% [TeV] ScenarioStrong/tree  s loop  W loop MFV (low tan  MFV (high tan  NMFV Generic~470000~47000~14000 From Bd&Bs 95% [TeV] ScenarioStrong/tree  s loop  W loop MFV (high tan  NMFV Generic Main contribution to present lower bound on NP scale come from  F=2 chirality-flipping operators ( Q 4 ) which are RG enhanced Preliminary

Conclusions CKM matrix is the dominant source of flavour mixing and CP violation  Nevertheless there are tensions here and there that should be continuously and quantitatively monitored : sin2 ,  K , Br(B   )  To render these tests more effective we need to improved the single implied measurements but also the predictions Model Independent fit show some discrepancy on the NP phase parameters  Bd = -(3.1 ± 1.7) o  Bs = (-20 ± 8) o U (-68 ± 8) o Effective Theory analysis quantify the known “flavor problem”.