• Open Access

Imprint of SUSY in radiative B-meson decays

Helmut Eberl, Keisho Hidaka, Elena Ginina, and Akimasa Ishikawa
Phys. Rev. D 104, 075025 – Published 19 October 2021

Abstract

We study supersymmetric (SUSY) effects on C7(μb) and C7(μb) which are the Wilson coefficients (WCs) for bsγ at b-quark mass scale μb and are closely related to radiative B-meson decays. The SUSY-loop contributions to C7(μb) and C7(μb) are calculated at leading order (LO) in the Minimal Supersymmetric Standard Model (MSSM) with general quark-flavor violation (QFV). For the first time we perform a systematic MSSM parameter scan for the WCs C7(μb) and C7(μb) respecting all the relevant constraints, i.e., the theoretical constraints from vacuum stability conditions and the experimental constraints, such as those from K- and B-meson data and electroweak precision data, as well as recent limits on SUSY particle masses and the 125 GeV Higgs boson data from LHC experiments. From the parameter scan we find the following: (1) The MSSM contribution to Re(C7(μb)) can be as large as ±0.05, which could correspond to about 3σ significance of New Physics (NP) signal in the future LHCb and Belle II experiments. (2) The MSSM contribution to Re(C7(μb)) can be as large as 0.08, which could correspond to about 4σ significance of NP signal in the future LHCb and Belle II experiments. (3) These large MSSM contributions to the WCs are mainly due to (i) large scharm-stop mixing and large scharm/stop involved trilinear couplings TU23, TU32 and TU33, (ii) large sstrange-sbottom mixing and large sstrange-sbottom involved trilinear couplings TD23, TD32 and TD33 and (iii) large bottom Yukawa coupling Yb for large tanβ and large top Yukawa coupling Yt. In case such large NP contributions to the WCs are really observed in the future experiments at Belle II and the LHCb Upgrade, this could be the imprint of QFV SUSY (the MSSM with general QFV) and would encourage to perform further studies of the WCs C7(μb) and C7MSSM(μb) at higher order (NLO/NNLO) level in this model.

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  • Received 1 July 2021
  • Accepted 16 September 2021

DOI:https://doi.org/10.1103/PhysRevD.104.075025

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Helmut Eberl1, Keisho Hidaka2, Elena Ginina1,3, and Akimasa Ishikawa4,5,6

  • 1Institut für Hochenergiephysik der Österreichischen Akademie der Wissenschaften, A-1050 Vienna, Austria
  • 2Department of Physics, Tokyo Gakugei University, Koganei, Tokyo 184-8501, Japan
  • 3VRVis Zentrum für Virtual Reality und Visualisierung Forschungs-GmbH, A-1220 Vienna, Austria
  • 4Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Ibaraki 305-0801, Japan
  • 5The Graduate University for Advanced Studies (SOKENDAI), Hayama 240-0193, Japan
  • 6International Center for Elementary Particle Physics, University of Tokyo, Tokyo 113-0033, Japan

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Issue

Vol. 104, Iss. 7 — 1 October 2021

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