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Charming Penguins in B Meson Decays

Updated 8 July 2026
  • Charming penguins are non-factorizable long-distance charm-loop contributions in weak B-meson decays that exhibit helicity- and q²-dependent behavior.
  • They induce shifts in short-distance amplitudes, complicating the extraction of Wilson coefficients and the interpretation of lepton universality tests.
  • Recent data-driven fits and lattice-QCD strategies aim to quantify these nonperturbative effects, thereby refining predictions for New Physics signals.

Searching arXiv for the specified papers to ground the article in current source records. Charming penguins are long-distance charm-loop contributions in weak BB-meson decays. In exclusive bs+b\to s\ell^+\ell^- transitions they arise from the non-local matrix elements of the current–current operators Q1,2cQ_{1,2}^{c}, while in charmless two-body decays they are associated with the amplitude component AcA_c induced by internal ccˉc\bar c loops. Their common feature is that they generate non-factorizable hadronic effects that can be helicity-dependent, q2q^2-dependent, and, in some formulations, intrinsically nonperturbative. Because these effects enter precisely in channels used to test Lepton Universality Violation (LUV) and to extract short-distance Wilson coefficients, their treatment materially affects both Standard Model predictions and New Physics inference. Recent work has also formulated a lattice-QCD strategy to compute these amplitudes using spectral-density methods, including the charmonium region (Ciuchini et al., 2021, Zhu, 2010, Frezzotti et al., 5 Aug 2025).

1. Definition and conceptual scope

In charmless two-body BB decays, the decay amplitude is decomposed using CKM unitarity as

A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,

with

T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,

where q=d,sq=d,s. In this notation, bs+b\to s\ell^+\ell^-0 denotes contributions from loops with internal charm quarks. The nonleptonic operators with a bs+b\to s\ell^+\ell^-1 pair can generate long-distance effects of order bs+b\to s\ell^+\ell^-2; these are dubbed “charming penguins” (Zhu, 2010).

In exclusive bs+b\to s\ell^+\ell^-3 decays, the dominant short-distance amplitudes are generated by the local operators bs+b\to s\ell^+\ell^-4, bs+b\to s\ell^+\ell^-5, and the radiative dipole bs+b\to s\ell^+\ell^-6. However, because the charm quark in the photon-penguin loop remains “light” at scale bs+b\to s\ell^+\ell^-7, one must also account for the non-local matrix element of the current–current operators

bs+b\to s\ell^+\ell^-8

the so-called “charming penguins.” These produce an a priori unknown, helicity- and bs+b\to s\ell^+\ell^-9-dependent shift in the short-distance amplitude (Ciuchini et al., 2021).

The theoretical interpretation differs across factorization frameworks. In QCDF, the entire amplitude Q1,2cQ_{1,2}^{c}0, including the Q1,2cQ_{1,2}^{c}1 loop, is treated perturbatively in terms of factorizable form factors, LCDAs, and perturbative kernels, with modeled endpoint divergences. In SCET, by contrast, the charm-loop contribution is argued to induce nonfactorizable operators whose Wilson coefficients are dominated by the nearly on-shell Q1,2cQ_{1,2}^{c}2 region, so that the corresponding charming-penguin matrix elements are nonperturbative parameters to be fitted from data (Zhu, 2010).

2. Helicity amplitudes and general parameterization in Q1,2cQ_{1,2}^{c}3

For Q1,2cQ_{1,2}^{c}4, the full helicity amplitudes are decomposed as

Q1,2cQ_{1,2}^{c}5

Q1,2cQ_{1,2}^{c}6

Q1,2cQ_{1,2}^{c}7

The seven factorizable form factors Q1,2cQ_{1,2}^{c}8 are smooth functions of Q1,2cQ_{1,2}^{c}9, known from light-cone sum rules or lattice QCD, whereas all genuine non-factorizable QCD effects are encoded in the complex functions AcA_c0 (Ciuchini et al., 2021).

A very general parameterization models these functions as low-order Taylor expansions in AcA_c1 around zero: AcA_c2

AcA_c3

AcA_c4

In this language, AcA_c5 acts like a universal shift AcA_c6, and AcA_c7 like a lepton-universal AcA_c8, while higher-order AcA_c9 are genuine long-distance effects that cannot be absorbed into local Wilson coefficients. This structure is central to separating hadronic dynamics from short-distance semileptonic physics (Ciuchini et al., 2021).

3. Conservative hadronic treatment and fitted charm-loop structure

A conservative treatment of hadronic uncertainties adopts a data-driven fit in which fourteen real parameters,

ccˉc\bar c0

are treated as free. To account for flavor-ccˉc\bar c1 breaking in ccˉc\bar c2 relative to ccˉc\bar c3, one writes

ccˉc\bar c4

with Gaussian priors ccˉc\bar c5. All ccˉc\bar c6-parameters are assigned broad, flat priors, and the fit is driven by differential rates and angular observables. Two more model-dependent alternatives are also considered: full extrapolation of LCSR results via dispersion relations over the entire ccˉc\bar c7 range, and LCSR constraints only for ccˉc\bar c8, letting the data determine the ccˉc\bar c9 at higher q2q^20 (Ciuchini et al., 2021).

When fitted to the latest LHCb and Belle measurements, the extracted helicity combinations q2q^21, q2q^22, and q2q^23 exhibit a non-trivial q2q^24 shape, comparable in magnitude to the short-distance q2q^25 rather than to the q2q^26 QCDF corrections. In the fully data-driven fit, the 68% highest-posterior-density intervals include

q2q^27

so that q2q^28, q2q^29, and BB0 deviate from zero at the BB1 level. The reported 95% contours for BB2 lie above the purely perturbative expectation throughout the low-BB3 region. This suggests that long-distance charm effects are neither small nor reducible to a universal local shift (Ciuchini et al., 2021).

4. Consequences for LUV observables and New Physics interpretation

In the pure Standard Model, where BB4 and BB5 matrix elements are lepton-universal, non-local charm effects cancel out almost exactly in the ratios

BB6

leading to the predictions

BB7

Once New Physics enters through a shift in BB8 or BB9, the interference with the hadronic term A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,0 reintroduces a residual uncertainty (Ciuchini et al., 2021).

The numerical impact depends strongly on how charming penguins are modeled. In a scenario with only A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,1 (“scenario A”), the prediction for A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,2 is

A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,3

in the data-driven hadronic fit,

A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,4

in the intermediate LCSR fit, and

A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,5

in the full Khodjamirian LCSR fit. The more optimistic hadronic model therefore enhances the NP-induced deviation in A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,6 by approximately A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,7. Similarly, A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,8 and A(BM1M2)=VubVuqT+VtbVtqP,A(B\to M_1M_2)=V_{ub}V_{uq}^*\,T+V_{tb}V_{tq}^*\,P,9 undergo shifts of T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,0 in their central values and of order T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,1 in their uncertainties when moving from the conservative to the optimistic hadronic treatment (Ciuchini et al., 2021).

Under the most conservative data-driven treatment, two NP patterns are singled out as most economical. A pure axial coupling, T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,2 (“scenario C”), gives

T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,3

with T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,4. A pure left-handed coupling through the SMEFT operator T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,5, corresponding at low energy to T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,6 (“scenario B”), gives

T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,7

with T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,8. By contrast, a pure vector shift T=AuAc,P=AtAc,T=A_u-A_c,\qquad P=A_t-A_c,9 is less favored once the q=d,sq=d,s0 are allowed to float, and can admit two disconnected solutions, one with q=d,sq=d,s1 and q=d,sq=d,s2, the other with q=d,sq=d,s3. The reported conclusion is that long-distance effects reduce the need for a vector-like NP contribution q=d,sq=d,s4, while the most robust emerging NP patterns feature either q=d,sq=d,s5 or q=d,sq=d,s6, with best-fit Wilson coefficients of order unity at q=d,sq=d,s7 (Ciuchini et al., 2021).

5. Charming penguins in charmless q=d,sq=d,s8 decays: QCDF, SCET, and the ratio q=d,sq=d,s9

For bs+b\to s\ell^+\ell^-00, the amplitude is written as

bs+b\to s\ell^+\ell^-01

with

bs+b\to s\ell^+\ell^-02

In QCDF the tree coefficient is

bs+b\to s\ell^+\ell^-03

where the brackets are free of endpoint singularities except in bs+b\to s\ell^+\ell^-04, whose hard-spectator uncertainty is parameterized by

bs+b\to s\ell^+\ell^-05

Using Beneke–Neubert inputs and bs+b\to s\ell^+\ell^-06, the numerical result is

bs+b\to s\ell^+\ell^-07

with the quoted error dominated by bs+b\to s\ell^+\ell^-08 and bs+b\to s\ell^+\ell^-09. On this basis, bs+b\to s\ell^+\ell^-10 is described as reliably predicted at the few-percent level (Zhu, 2010).

Using this QCDF value together with flavor-bs+b\to s\ell^+\ell^-11, one predicts

bs+b\to s\ell^+\ell^-12

to be compared with the CDF measurement bs+b\to s\ell^+\ell^-13. Two explanations are identified. One is that the form-factor ratio is smaller than in light-cone sum rules, bs+b\to s\ell^+\ell^-14. The other is that the QCDF estimate of bs+b\to s\ell^+\ell^-15 is too large because the charming penguin bs+b\to s\ell^+\ell^-16 is nonperturbative and gives a sizable shift in bs+b\to s\ell^+\ell^-17; in SCET, this can reduce bs+b\to s\ell^+\ell^-18 by bs+b\to s\ell^+\ell^-19–bs+b\to s\ell^+\ell^-20 (Zhu, 2010).

A particularly clean discriminator is

bs+b\to s\ell^+\ell^-21

Because the penguin-over-tree ratios are below bs+b\to s\ell^+\ell^-22, their squared effects largely cancel, leading to

bs+b\to s\ell^+\ell^-23

With bs+b\to s\ell^+\ell^-24, bs+b\to s\ell^+\ell^-25, and bs+b\to s\ell^+\ell^-26, QCDF predicts

bs+b\to s\ell^+\ell^-27

independent of the form factor. If charming penguins are important, a global SCET fit gives, for example,

bs+b\to s\ell^+\ell^-28

so that bs+b\to s\ell^+\ell^-29, or in another solution bs+b\to s\ell^+\ell^-30, both well below the QCDF value. A measured value near bs+b\to s\ell^+\ell^-31 would support small, perturbative charming penguins as in QCDF, whereas bs+b\to s\ell^+\ell^-32 would signal sizable nonperturbative charming-penguin contributions beyond QCDF expectations. The proposed experimental sensitivity is at the bs+b\to s\ell^+\ell^-33 level with LHCb and Belle II (Zhu, 2010).

6. First-principles lattice-QCD framework

A lattice-QCD framework has been developed for bs+b\to s\ell^+\ell^-34 and bs+b\to s\ell^+\ell^-35 that targets precisely the complex contributions generated by on-shell intermediate states between the weak operator and electromagnetic current(s), including charming penguins and the chromomagnetic operator bs+b\to s\ell^+\ell^-36 (Frezzotti et al., 5 Aug 2025).

The relevant four-quark operators are

bs+b\to s\ell^+\ell^-37

with bs+b\to s\ell^+\ell^-38, together with

bs+b\to s\ell^+\ell^-39

The time-ordered amplitude

bs+b\to s\ell^+\ell^-40

is split into bs+b\to s\ell^+\ell^-41 and bs+b\to s\ell^+\ell^-42 pieces, where the latter admits a spectral representation

bs+b\to s\ell^+\ell^-43

On the lattice one computes the Euclidean correlator

bs+b\to s\ell^+\ell^-44

and reconstructs the Minkowski integral using the Hansen–Lupo–Tantalo expansion

bs+b\to s\ell^+\ell^-45

so that

bs+b\to s\ell^+\ell^-46

The connected charming-penguin diagram in which the virtual photon is emitted from the bs+b\to s\ell^+\ell^-47 loop is isolated through a four-point correlator with smeared bs+b\to s\ell^+\ell^-48- and bs+b\to s\ell^+\ell^-49-interpolating fields. On-shell charmonium resonances such as bs+b\to s\ell^+\ell^-50 and bs+b\to s\ell^+\ell^-51 appear as plateaux in the effective mass

bs+b\to s\ell^+\ell^-52

Renormalization is nontrivial. Each time ordering is individually UV-divergent as bs+b\to s\ell^+\ell^-53, although the sum is only logarithmic; a three-term subtraction of the kernel separates a UV-finite part from a divergent part without an bs+b\to s\ell^+\ell^-54 pole. In addition, bs+b\to s\ell^+\ell^-55 mix with lower-dimension operators such as bs+b\to s\ell^+\ell^-56 and bs+b\to s\ell^+\ell^-57 with coefficients of order bs+b\to s\ell^+\ell^-58 or bs+b\to s\ell^+\ell^-59. With Wilson–Clover twisted-mass fermions at maximal twist, spurionic symmetries and nonperturbative subtraction conditions are used to remove these mixings (Frezzotti et al., 5 Aug 2025).

The full charm-loop amplitude is then

bs+b\to s\ell^+\ell^-60

and contracting with the lepton current and photon propagator shows that charming penguins shift the effective Wilson coefficient, bs+b\to s\ell^+\ell^-61. In an exploratory calculation on a single ETMC bs+b\to s\ell^+\ell^-62 ensemble with bs+b\to s\ell^+\ell^-63, bs+b\to s\ell^+\ell^-64, bs+b\to s\ell^+\ell^-65, and a lighter-than-physical heavy mass bs+b\to s\ell^+\ell^-66, the bs+b\to s\ell^+\ell^-67 signal is very clean and the bs+b\to s\ell^+\ell^-68 signal is about an order of magnitude smaller. A stability analysis in the trade-off parameter bs+b\to s\ell^+\ell^-69 yields a robust reconstruction for a range of bs+b\to s\ell^+\ell^-70, and comparison with a “VSA + Breit–Wigner + perturbative continuum” model shows qualitative agreement in the shape and size of the real and imaginary parts of bs+b\to s\ell^+\ell^-71 after a global bs+b\to s\ell^+\ell^-72 renormalization. The stated long-term goal is a first-principles Standard Model prediction for bs+b\to s\ell^+\ell^-73 and bs+b\to s\ell^+\ell^-74 over the full bs+b\to s\ell^+\ell^-75 range, including the charmonium region, once the charming-penguin and bs+b\to s\ell^+\ell^-76 contributions are determined to bs+b\to s\ell^+\ell^-77 accuracy (Frezzotti et al., 5 Aug 2025).

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