Anomalies in (semi)-leptonic B decays B±→τ±ν, B±→Dτ± ν and B±→D∗τ± ν, and possible resolution with sterile neutrino

Gorazd Cvetič, Francis Halzen, C. S. Kim, Sechul Oh

Research output: Contribution to journalArticlepeer-review

26 Citations (Scopus)

Abstract

The universality of the weak interactions can be tested in semileptonic b→c transitions, and in particular in the ratios R(D(∗)) ≡ Γ(B→D(∗)τν)/Γ(B→D(∗)lν) (where l=μ or e). Due to the recent differences between the experimental measurements of these observables by BaBar, Belle and LHCb on the one hand and the Standard Model predicted values on the other hand, we study the predicted ratios R(D(∗))=Γ(B→D(∗)τ+"missing")/Γ(B→D(∗)lν) in scenarios with an additional sterile heavy neutrino of mass ∼1 GeV. Further, we evaluate the newly defined ratio R(0)≡Γ(B→τ+"missing")/Γ(B→μν) in such scenarios, in view of the future possibilities of measuring the quantity at Belle-II.

Original languageEnglish
Article number113102
JournalChinese Physics C
Volume41
Issue number11
DOIs
Publication statusPublished - 2017 Nov

Bibliographical note

Funding Information:
Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Article funded by SCOAP3 and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd

Funding Information:
in part by the NRF grant

Publisher Copyright:
© Article funded by SCOAP3 and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd.

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Instrumentation
  • Astronomy and Astrophysics

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