Abstract
We present a model-independent anatomy of the ∆F = 2 transitions K0− {overline{K}}^0 , Bs,d− {overline{B}}_{s,d} and D0− {overline{D}}^0 in the context of the Standard Model Effective Field Theory (SMEFT). We present two master formulae for the mixing amplitude [M12]BSM. One in terms of the Wilson coefficients (WCs) of the Low-Energy Effective Theory (LEFT) operators evaluated at the electroweak scale μew and one in terms of the WCs of the SMEFT operators evaluated at the BSM scale Λ. The coefficients {P}_a^{ij} entering these formulae contain all the information below the scales μew and Λ, respectively. Renormalization group effects from the top-quark Yukawa coupling play the most important role. The collection of the individual contributions of the SMEFT operators to [M12]BSM can be considered as the SMEFT atlas of ∆F = 2 transitions and constitutes a travel guide to such transitions far beyond the scales explored by the LHC. We emphasize that this atlas depends on whether the down-basis or the up-basis for SMEFT operators is considered. We illustrate this technology with tree-level exchanges of heavy gauge bosons (Z′, G′) and corresponding heavy scalars.
Highlights
K0−K 0, Bs,d−Bs,d and D0−D 0 mixings have been already for many years the stars among the flavour-changing neutral-current processes (FCNC) [1, 2]
We present a model-independent anatomy of the ∆F = 2 transitions K0 − K 0, Bs,d − Bs,d and D0 − D 0 in the context of the Standard Model Effective Field Theory (SMEFT)
One in terms of the Wilson coefficients (WCs) of the Low-Energy Effective Theory (LEFT) operators evaluated at the electroweak scale μew and one in terms of the WCs of the SMEFT operators evaluated at the beyond the SM (BSM) scale Λ
Summary
K0−K 0, Bs,d−Bs,d and D0−D 0 mixings have been already for many years the stars among the flavour-changing neutral-current processes (FCNC) [1, 2]. It depends on the model-independent matrix elements evaluated at μew = 160 GeV and on Wilson coefficients of these operators evaluated at the same scale. In this context we stress the importance of the Yukawa RG effects in the evolution from Λ down to μew.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.