Abstract
We compute the Darwin operator contribution ( 1/{m}_b^3 correction) to the width of the inclusive non-leptonic decay of a B meson (B+, Bd or Bs), stemming from the quark flavour-changing transition b → {q}_1{overline{q}}_2{q}_3 , where q1, q2 = u, c and q3 = d, s. The key ideas of the computation are the local expansion of the quark propagator in the external gluon field including terms with a covariant derivative of the gluon field strength tensor and the standard technique of the Heavy Quark Expansion (HQE). We confirm the previously known expressions of the 1/{m}_b^3 contributions to the semi-leptonic decay b → {q}_1mathrm{ell}{overline{nu}}_{mathrm{ell}} , with ℓ = e, μ, τ and of the 1/{m}_b^2 contributions to the non-leptonic modes. We find that this new term can give a sizeable correction of about −4 % to the non-leptonic decay width of a B meson. For Bd and Bs mesons this turns out to be the dominant correction to the free b-quark decay, while for the B+ meson the Darwin term gives the second most important correction — roughly 1/2 to 1/3 of the phase space enhanced Pauli interference contribution. Due to the tiny experimental uncertainties in lifetime measurements the incorporation of the Darwin term contribution is crucial for precision tests of the Standard Model.
Highlights
There has been considerably progress on the theory side
We confirm the previously known expressions of the 1/m3b contributions to the semi-leptonic decay b → q1 ν, with = e, μ, τ and of the 1/m2b contributions to the non-leptonic modes. We find that this new term can give a sizeable correction of about −4 % to the non-leptonic decay width of a B meson
The dependence on the spectator quark is only due to different values of the matrix elements and the coefficients Γ3,5,6 are independent of the quark content of the B meson
Summary
We limit ourselves to state that for the computation of most of the diagrams of interest it is always possible to set one mass to zero and obtain an analytic expression for all the master integrals This is not the case only for the gluon emission from the s quark in the b → ccs transition, where we need to keep all masses finite in order to regularise the infrared divergence.
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