Abstract

The Wilson coefficient C7 governing the radiative electromagnetic decays of B meson has been calculated toa very high accuracy in the Standard Model, but experimental bounds on either the magnitude or the sign of C7 are often model-dependent. In the present paper, we attempt at constraining both the magnitude and sign of C7 using a systematic approach. We consider already measured observables like the branching ratios of B → Xsμ+μ and B → Xsγ, the isospin and CP asymmetries in B → Kγ, as well as AFB and FL in B → K+. We also discuss the transverse observable AT(2) which, once measured, may help to disentangle some of the scenarios considered. We explore the constraints on C7, C9, C10 as well as their chirality-flipped counterparts. Within our framework, we find that we need to extend the constraints up to 1.6σ to allow for the “flipped-sign solution” of C7. The SM solution for C7 exhibits a very mild tension if New Physics is allowed in dipole operators only. We provide semi-numerical expressions for all these observables as functions of the relevant Wilson coefficients at the low scale.

Details

Title
Exploring new physics in the C7-C7′ plane
Author
Descotes-Genon Sébastien 1 ; Ghosh Diptimoy 2 ; Matias Joaquim 3 ; Ramon, Marc 3 

 CNRS/Univ. Paris-Sud 11 (UMR 8627), Laboratoire de Physique Théorique, Orsay Cedex, France (GRID:grid.5842.b) (ISNI:0000 0001 2171 2558) 
 Homi Bhabha Road, Tata Institute of Fundamental Research, Mumbai, India (GRID:grid.22401.35) (ISNI:0000 0004 0502 9283) 
 Universitat Autonoma de Barcelona, Bellaterra, Barcelona, Spain (GRID:grid.7080.f) 
Publication year
2011
Publication date
Jun 2011
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2398240369
Copyright
© The Author(s) 2011. Open Access This article is distributed under the terms of the Creative Commons Attribution License which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. This work is published under https://creativecommons.org/licenses/by-nc/2.0 (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.