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SM Uncertainties in the B- -> >X_s+gamma X_s+gamma SM Uncertainties in the B Branching Fraction and Spectrum Branching Fraction and Spectrum Alexander Mitov Alexander Mitov University of Hawaii University of Hawaii Outline


  1. SM Uncertainties in the B- -> >X_s+gamma X_s+gamma SM Uncertainties in the B Branching Fraction and Spectrum Branching Fraction and Spectrum Alexander Mitov Alexander Mitov University of Hawaii University of Hawaii Outline • The process B->X_s+gamma. • Branching Fraction: application, status and future prospects. • The photon spectrum: application, status. • New NNLO results for the photon spectrum. • Conclusions. • Work in progress. In collaboration with Kirill Melnikov. A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  2. The process B- -> >X_s+gamma X_s+gamma The process B We can split the information about this process in two We can split the information about this process in two (not uncorrelated) pieces: (not uncorrelated) pieces: The Branching Fraction BR[B- -> >X_s+gamma X_s+gamma]. It is: ]. It is: The Branching Fraction BR[B @ Loop induced, @ Loop induced, @ Sensitive to Physics at the electroweak scale, @ Sensitive to Physics at the electroweak scale, @ An important constraint for many models of New Physics. @ An important constraint for many models of New Physics. The shape of the photon spectrum. It is: The shape of the photon spectrum. It is: @ Largely insensitive to New Physics, @ Largely insensitive to New Physics, @ Crucial for relating the @ Crucial for relating the “ “theory theory” ” BF to the experimental measurements. BF to the experimental measurements. @ Opens a window for determining various pert. and non @ Opens a window for determining various pert. and non- -pert. pert. parameters. parameters. A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  3. The Branching Fraction BR[B- -> >X_s+gamma X_s+gamma]. ]. The Branching Fraction BR[B Current status: Current status: Currently known to NLO: Currently known to NLO: (1998) ” (1998) ”Practically complete Practically complete” ” ( (Chetyrkin Chetyrkin, , Misiak Misiak and and Munz Munz). ). (2001) ” (2001) ”Essentially Essentially” ” known ( known (Gambino Gambino and and Misiak Misiak). ). (2002) ” (2002) ”Strictly complete Strictly complete” ” (Buras, (Buras, Czarnecki Czarnecki, , Misiak Misiak and Urban). and Urban). Current developments – – inclusion of the NNLO effects: inclusion of the NNLO effects: Current developments @ Evaluation of the anomalous dimensions and running of the Wilson @ Evaluation of the anomalous dimensions and running of the Wilson coefficients to scale ~ m_b m_b. . coefficients to scale ~ @ Evaluation of the matching conditions at a scale ~ M_W @ Evaluation of the matching conditions at a scale ~ M_W @ Evaluation of the matrix elements. @ Evaluation of the matrix elements. ! The NNLO inclusions are needed to reduce large uncertainties du ! The NNLO inclusions are needed to reduce large uncertainties due to e to charm mass effects induced from the four- charm mass effects induced from the four -fermion operators. fermion operators. A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  4. The Branching Fraction BR[B- -> >X_s+gamma X_s+gamma]. ]. The Branching Fraction BR[B M. Steinhauser Steinhauser , hep , hep- -ph/0406240. ph/0406240. M. At present very good agreement between theory and experiment! At present very good agreement between theory and experiment! A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  5. The photon spectrum in B- -> >X_s+gamma X_s+gamma. . The photon spectrum in B What is the useful information in this observable? What is the useful information in this observable? 1) It relates the values of the BF BF’ ’s s measured (or evaluated) with measured (or evaluated) with 1) It relates the values of the different cuts on the energy of the measured photon. different cuts on the energy of the measured photon. BR[E>E_cut E_cut] ] BR[E> Define the ratio: R(E_cut R(E_cut) = ) = -------------------- -------------------- Define the ratio: BR[E>m_b/20] BR[E>m_b/20] That is very important, since: That is very important, since: The experimental measurements are always with a lower cut: The experimental measurements are always with a lower cut: E_cut=1.8 =1.8-- --2.1 2.1 GeV GeV. . E_cut The theory predictions are usually needed for the fully inclusive e The theory predictions are usually needed for the fully inclusiv Branching Fraction. Branching Fraction. A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  6. The photon spectrum in B- -> >X_s+gamma X_s+gamma. . The photon spectrum in B What is the useful information in this observable (cont.)? What is the useful information in this observable (cont.)? 2) Needed for the extraction of the moments of the photon 2) Needed for the extraction of the moments of the photon spectrum. spectrum. Note: <E>=m_b(1/2+O(a_s)+O(non- -pert.) ). pert.) ). Note: <E>=m_b(1/2+O(a_s)+O(non Therefore: from a precise measurement one can extract from a precise measurement one can extract m_b m_b as as Therefore: well as non- -perturbative parameters. perturbative parameters. well as non However: such extraction such extraction However: depends very strongly depends very strongly on the value of the on the value of the imposed cut! imposed cut! Note: very strong sensitivity to Note: very strong sensitivity to m_b m_b for low for low E_cut E_cut. . for large E_cut for large E_cut – – low sensitivity to low sensitivity to m_b m_b but but sensitivity to other shape function parameters. s. sensitivity to other shape function parameter Kagan and Kagan and Neubert Neubert, hep , hep- -ph/9805303 ph/9805303 A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  7. The photon spectrum in B- -> >X_s+gamma X_s+gamma. . The photon spectrum in B Current state of the art for theory: Current state of the art for theory: @ The NLO contributions from all operators and their mixing is The NLO contributions from all operators and their mixing is @ accounted for. The dominant effect is from O_7 with small accounted for. The dominant effect is from O_7 with small contributions from O_2 and O_8. contributions from O_2 and O_8. !!! That is very different from the total rate! !!! That is very different from the total rate! � _0 ~a_s^2 � @ Some NNLO contributions (from O_2,7,8) Some NNLO contributions (from O_2,7,8) ~a_s^2 _0 @ (the so- -called BLM terms) are also accounted for: called BLM terms) are also accounted for: (the so Therefore, non- Therefore, non -O_7 operators are O_7 operators are only a few per- -cent effect! cent effect! only a few per Ligeti, Luke, , Luke, Manohar Manohar and Wise, and Wise, Ligeti Hep- -ph/9903305. ph/9903305. Hep A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

  8. The photon spectrum in B- -> >X_s+gamma X_s+gamma. . The photon spectrum in B However: However: 1) The BLM effects are not 100% genuine NNLO effect; can be 1) The BLM effects are not 100% genuine NNLO effect; can be absorbed by the choice of scale (cut dependent!) absorbed by the choice of scale (cut dependent!) 2) Recently - - large differences of the size of the perturbative large differences of the size of the perturbative 2) Recently uncertainty in observables related to the spectrum. uncertainty in observables related to the spectrum. Therefore: Therefore: To clarify this we calculate the dominant (genuinely) NNLO effect! ct! To clarify this we calculate the dominant (genuinely) NNLO effe A. Mitov A. Mitov SM Uncertainties in the b- SM Uncertainties in the b ->s gamma >s gamma SuperB SuperB Workshop Univ. of Hawaii, 21 April 2005 Workshop Univ. of Hawaii, 21 April 2005

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