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FlavBit: A GAMBIT module for computing flavour observables and likelihoods

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arxiv 1705.07933 v2 pith:5VUO2POT submitted 2017-05-22 hep-ph hep-exphysics.data-an

Florian U. Bernlochner , Marcin Chrzaszcz , Lars A. Dal , Ben Farmer , Paul Jackson , Anders Kvellestad , Farvah Mahmoudi , Antje Putze
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Christopher Rogan Pat Scott Nicola Serra Christoph Weniger Martin White (The GAMBIT Flavour Workgroup)
This is my paper · ORCID
classification hep-phhep-exphysics.data-an
keywords flavourphysicsflavbitobservablesgambitdetailmodulethen
verification ladder T0 review T1 audit T2 compute T3 formal
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Flavour physics observables are excellent probes of new physics up to very high energy scales. Here we present FlavBit, the dedicated flavour physics module of the global-fitting package GAMBIT. FlavBit includes custom implementations of various likelihood routines for a wide range of flavour observables, including detailed uncertainties and correlations associated with LHCb measurements of rare, leptonic and semileptonic decays of B and D mesons, kaons and pions. It provides a generalised interface to external theory codes such as SuperIso, allowing users to calculate flavour observables in and beyond the Standard Model, and then test them in detail against all relevant experimental data. We describe FlavBit and its constituent physics in some detail, then give examples from supersymmetry and effective field theory illustrating how it can be used both as a standalone library for flavour physics, and within GAMBIT.

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Cited by 2 Pith papers

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  1. Electroweak baryogenesis from charged current anomalies in $B$ meson decays

    hep-ph 2025-02 conditional novelty 6.0 of 10

    Complex lepton Yukawa couplings in a two Higgs doublet model that explain the R(D(*)) flavor anomalies can also source electroweak baryogenesis, yielding the observed baryon asymmetry under assumed strong first-order ...

  2. Current status and prospects of light bino-higgsino dark matter in natural SUSY

    hep-ph 2026-02 conditional novelty 4.0 of 10

    In natural SUSY with Δ_EW<30, light bino-higgsino neutralinos are always subdominant dark matter (f≤0.02), and HL-LHC can probe the surviving parameter space.

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