REVIEW 3 major objections 5 minor 6 cited by
Complete dispersive evaluation of the hadronic light-by-light contribution to muon $g-2$
T0 review · 3 major / 5 minor · reviewed 2026-08-12 · deepseek-v4-flash
Pith's one-line read A complete dispersive evaluation determines the hadronic light-by-light contribution to the muon's magnetic moment as $a_\mu^\text{HLbL} = 101.9(7.9)\times 10^{-11}$.
desk verdict First complete dispersive HLbL evaluation with a realistic error budget; the U(3) axial-vector assumption is the main thing to probe, but it is handled as a transparent systematic. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central mechanism is a Bardeen–Tung–Tarrach decomposition of the four-photon HLbL tensor, which reduces the amplitude to 54 scalar coefficient functions (12 independent after the equations of motion). The master formula for $a_\mu$ integrates these functions against known kernels over the three photon virtualities. The functions are reconstructed dispersively from their discontinuities, which are saturated by a finite set of hadronic intermediate states: pseudoscalar poles ($\pi^0,\eta,\eta'$) with transition form factors from data, two-meson boxes and rescattering, and narrow-resonance approximations for axial-vector, scalar, and tensor mesons. In the deep-Euclidean region the same functions are matched to the perturbative quark loop with $\alpha_s$ corrections, and in the asymmetric region to the operator product expansion controlled by the vector-vector-axial-vector correlator $w_{L,T}$. A newly introduced effective-pole parametrization estimates the error from intermediate states that lie between the hadronic and asymptotic descriptions.
What would settle it
New data on the $f_1$ or $f_1'$ transition form factor that deviate from the U(3)-symmetric parameterization by more than the assigned 30% would move the axial-vector contribution beyond the quoted systematic error.
Extended reading notes
Core claim
The authors establish a data-driven, dispersive value for the hadronic light-by-light contribution to the muon's $g-2$, $a_\mu^\text{HLbL} = 101.9(7.9)\times 10^{-11}$, by reconstructing the HLbL tensor from its unitarity cuts and matching the sum of exclusive hadronic states to short-distance constraints. This is the first such evaluation that includes axial-vector resonances ($a_1$, $f_1$, $f_1'$), scalar and tensor resonances, the full vector-vector-axial-vector correlator for the OPE region, and a dedicated estimate of the matching uncertainty via an effective-pole ansatz. The result agrees with the 2020 phenomenological consensus, $92(19)\times 10^{-11}$, but reduces the uncertainty by more than half, meeting the precision target set for the final result of the muon g-2 experiment.
Load-bearing premise
The calculation assumes that the axial-vector meson transition form factors follow U(3) symmetry with no more than 30% deviation; if the true symmetry breaking is larger, the central value shifts outside the quoted uncertainty.
Editorial extensions
If this is right
- The uncertainty of the HLbL contribution drops from $19\times 10^{-11}$ to $7.9\times 10^{-11}$, so the hadronic light-by-light piece no longer dominates the theory error for the muon $g-2$ prediction.
- The quoted precision meets the requirement set by the final result of the muon g-2 experiment, making the comparison between the Standard-Model prediction and experiment sensitive mainly to the hadronic vacuum polarization contribution.
- The new value agrees with the 2020 phenomenological estimate but with an uncertainty reduced by more than a factor of two, strengthening the data-driven benchmark against which lattice QCD calculations are compared.
- The axial-vector resonance contribution is now the largest subleading term with an assumption-based error, so new measurements of the $f_1$ and $f_1'$ transition form factors directly test the main systematic uncertainty.
Reading between the lines
- A natural next step would be a direct dispersive calculation of the $a_1$ transition form factor from $\tau$-decay data, which could replace the U(3)-symmetry assumption with an experimental determination.
- If the effective-pole matching error is as small as quoted, then the dominant remaining model dependence in the subleading contributions sits in the tensor-meson treatment; a triangle-kinematics dispersive calculation of the $f_2$ contribution would provide a sharp cross-check.
- The small tension with two of the lattice QCD evaluations, if it persists, may point to a systematic effect in one of the methods; the present result offers a data-driven reference point for locating the difference.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper presents a data-driven dispersive evaluation of the hadronic light-by-light (HLbL) contribution to the muon anomalous magnetic moment. The HLbL tensor is reconstructed from its discontinuities using four-point dispersion relations, with contributions from pseudoscalar poles, meson boxes, rescattering, axial-vector and tensor resonances, heavy scalars, and a matching to pQCD and OPE short-distance constraints. The final result is a_mu^HLbL = 101.9(7.9) x 10^-11 (Eq. (8)), which the authors state meets the precision requirements of the final Fermilab result. The paper relies on a companion paper (Ref. [82]) for many technical details.
Significance. If correct, this would be the most precise data-driven determination of a_mu^HLbL to date, reducing the uncertainty of the 2020 White Paper evaluation by more than a factor of two and providing a sharp benchmark for comparisons with lattice QCD. The paper is notable for its detailed error budget, separating experimental, matching, systematic, and effective-pole uncertainties, and for demonstrating stability of the integral under variation of the matching scale Q0 and the OPE parameter r (Fig. 5). The result is also falsifiable in the sense that future BESIII and Belle II measurements of axial-vector transition form factors, as well as improved lattice calculations, will directly test the assumptions that underlie the axial-vector and tensor contributions.
major comments (3)
- [Exclusive hadronic states / Table II / Eq. (7)] The axial-vector sector is the most load-bearing input for the claimed precision, yet the a1(1260) transition form factors are not extracted from direct data. The Letter fixes the f1 and f1' TFF normalizations and mixing angle from e+e- data and then defines the complete set of axial-vector TFFs using U(3) symmetry, assigning a global 30% uncertainty 'to account for possible symmetry violations.' This 30% is not derived from a spread of models, fits, or dispersion relations; the supporting comparison with the dispersive VVA calculation of Ref. [81] constrains only the singly-virtual a1 form factor, not the doubly-virtual TFFs that dominate the HLbL integral. Since the axial-vector contribution is 12.2(2.3) x 10^-11 (Table II), the largest non-pseudoscalar subleading piece, a U(3) violation of 40-50% in the a1 TFF normalizations or virtuality dependence would shift the result by more than the quoted 7.9 x 10^-11 total uncertainty and would invalidate the precision claim of Eq. (8). Please calibrate the 30% by explicit sensitivity studies (e.g., 50% variations or an alternative model spread) or soften the claim accordingly.
- [Matching to short-distance constraints / Fig. 4 / Table II] The effective-pole model (P(2200), A(1700)) is introduced to estimate the impact of missing higher intermediate states in the matching between hadronic and pQCD/OPE regions. The Letter assigns an effective-pole uncertainty larger than the entire effective-pole contribution (3.9 x 10^-11 vs. contributions of 2.0 and 1.2 x 10^-11 in Table II), which is conservative in that specific sense. However, the effective-pole amplitude is an ad-hoc construct with masses fixed at 2.2 GeV and 1.7 GeV and a TFF scale varied only over the same range as Q0; no explicit functional form is given in the Letter. A different pole structure or asymptotic behavior could shift the central value beyond the quoted eff uncertainty. Please provide the explicit effective-pole parameterization in the Letter or in a form that can be checked against Ref. [82], and demonstrate robustness to the assumed pole masses and the number of poles.
- [Tensor contributions / Table II / Eq. (7)] The tensor contribution is estimated using a quark-model-inspired TFF with a single nonvanishing form factor, with the scale set to M_rho. The Letter adds a 100% uncertainty on the total tensor contribution 'to protect against the cancellation observed between a_mu[Pi1,2] and a_mu[Pi3-12],' but this protects against the sign cancellation rather than against individual normalization or shape errors. The two tensor components in Table II are -2.6(3) and -5.1(7) x 10^-11; a 50% error in the f2(1270) TFF alone would shift the sum by roughly 3.9 x 10^-11, exceeding the quoted total sys error. Please provide a more robust estimate of the tensor uncertainty, for example by varying the TFF scale and form independently or by including a dispersive D-wave treatment as the paper itself identifies as future work.
minor comments (5)
- [Title and abstract] The phrase 'complete dispersive evaluation' overstates the treatment of axial-vector and tensor states, which are evaluated in narrow-resonance and quark-model approximations rather than fully dispersively; consider qualifying the claim as 'complete within the stated hadronic approximations' or moving the stronger claim to the conclusions.
- [Figure 4 caption] The caption refers to the effective pole P(2200) without defining its amplitude; please either define it in the text or refer explicitly to the equation in Ref. [82] where it is introduced.
- [Table II] The 'Eff.' rows list central values without uncertainties, while Eq. (7) quotes an effective-pole uncertainty; please clarify whether the quoted eff uncertainty is meant to cover these entries or is an additional assignment.
- [Exclusive hadronic states] The sentence 'all contributions but a single TFF vanish' is ambiguous; please specify which of the tensor TFFs is kept and in which basis the vanishing occurs.
- [Table I] The K± box entry is quoted as -0.5(0); please provide the actual uncertainty (even if negligible) to avoid the appearance of an exactly vanishing error.
Circularity Check
No circularity: the final result is a sum of externally fitted inputs and explicitly estimated matching contributions, not a redefinition of its own input.
full rationale
The derivation chain is self-contained. Equation (8) is obtained by adding the dispersive pseudoscalar/box/rescattering contributions from Table I, the subleading hadronic and short-distance-matched contributions from Table II, and the independent charm-loop estimate. None of these inputs use a_mu^HLbL as a fit target or as a defining condition. The axial-vector TFFs are parameterized from fits to f1/f1' data in Refs. [73,74] and extended to a1 via an explicitly stated U(3) symmetry assumption with a 30% systematic uncertainty; this is a modeling input, not a quantity derived from the final result. The VVA correlator input [81] is a separate dispersive calculation used for the OPE region and as a cross-check, and the effective-pole and tensor contributions are estimates with uncertainties assigned at or above their full size. No equation in the paper defines the output in terms of its own fitted values, and no load-bearing conclusion is justified solely by a self-citation chain. The reliance on prior work by the same authors is reliance on data-driven analyses whose inputs are external experiments and dispersion relations, which does not constitute circularity.
Assumptions & free parameters
free parameters (6)
- Matching scale Q0 =
1.5 GeV (central), varied 1.2-2.0 GeV
- OPE matching parameter r =
1/4 (central), varied 1/8-1/2
- Effective pole masses M_P^eff, M_A^eff =
2.2 GeV and 1.7 GeV
- Effective pole TFF scale =
varied with Q0 in [1.2,2.0] GeV
- Tensor TFF scale =
M_rho = 0.775 GeV
- Axial-vector TFF normalizations and f1-f1' mixing angle
assumptions (7)
- domain assumption The HLbL tensor can be reconstructed from its discontinuities via dispersion relations in four-point kinematics, and the infinite sum of intermediate states can be truncated to the listed exclusive hadronic states plus pQCD/OPE matching.
- domain assumption The narrow-resonance approximation is valid for the axial-vector states a1, f1, f1' and heavy scalars/tensors.
- domain assumption U(3) symmetry determines the full set of axial-vector TFFs from the f1 data.
- ad hoc to paper The quark-model-inspired TFF with a single nonzero form and scale M_rho describes the tensor and heavy-scalar contributions.
- ad hoc to paper The effective-pole model with parameters fixed in the symmetric asymptotic limit captures the intermediate-energy matching between hadronic and pQCD/OPE regions.
- domain assumption The OPE limit relates the HLbL tensor to the VVA correlator, and the cancellation found in Ref [80] holds beyond leading order.
- standard math Standard QCD factorization and alpha_s evolution from Refs [124,125] apply in the pQCD quark-loop region.
invented entities (2)
-
Effective pole P(2200)
-
Effective pole A(1700)
Cite this review
Pith. "Pith review of Complete dispersive evaluation of the hadronic light-by-light contribution to muon $g-2$." pith.science (2026). https://pith.science/paper/AOYSNPLJ
@misc{pith2026241200190,
author = {Pith},
title = {Pith review of: Complete dispersive evaluation of the hadronic light-by-light contribution to muon $g-2$},
year = {2026},
howpublished = {\url{https://pith.science/paper/AOYSNPLJ}},
note = {Machine review of arXiv:2412.00190}
}
abstract
Hadronic light-by-light (HLbL) scattering defines one of the critical contributions in the Standard-Model prediction of the anomalous magnetic moment of the muon. In this Letter, we present a complete evaluation using a dispersive formalism, in which the HLbL tensor is reconstructed from its discontinuities, expressed in terms of simpler hadronic matrix elements that can be extracted from experiment. Profiting from recent developments in the determination of axial-vector transition form factors, short-distance constraints for the HLbL tensor, and the vector-vector-axial-vector correlator, we obtain $a_\mu^\text{HLbL}=101.9(7.9)\times 10^{-11}$, which meets the precision requirements set by the final result of the Fermilab experiment.
Figures
Figures from the paper (3 more)
Forward citations
Cited by 6 Pith papers
-
Tensor meson transition form factors in holographic QCD and the muon $g-2$
Holographic QCD predicts a positive tensor-meson contribution of about +11e-11 to the muon g-2, driven by a previously omitted doubly-virtual form factor.
-
Longitudinal short-distance constraints on hadronic light-by-light scattering and tensor meson contributions to the muon $g-2$
In hard-wall holographic QCD, the infinite tower of tensor mesons fills most of the missing symmetric longitudinal short-distance constraint and yields a total hadronic light-by-light contribution of about +11 x 10^-1...
-
Dispersive analysis of the pion vector form factor without zeros
Imposing the absence of complex zeros in the pion vector form factor reduces the dominant systematic uncertainty and makes the tensions between CMD-3 and other e+e- data sets appear sharper, including in the pion char...
-
Hadronic vacuum polarization for the muon $g-2$ from lattice QCD: Long-distance and full light-quark connected contribution
The light-quark connected hadronic vacuum polarization contribution to muon g-2 is determined to 0.69% precision, 655.2(4.5) x 10^-10, from lattice QCD.
-
Dispersion relation for hadronic light-by-light scattering: $\eta$ and $\eta'$ poles
A dispersive analysis of the eta and eta' transition form factors yields data-driven pole contributions to the muon g-2 of 14.7(9) x 10^-11 and 13.5(7) x 10^-11.
-
Dispersion relation for hadronic light-by-light scattering: subleading contributions
A dispersive evaluation gives a_mu^HLbL subleading = 33.2(7.2) x 10^-11 and total = 101.9(7.9) x 10^-11.
Reference graph
Works this paper leans on
- [82]
-
[81]
J. Bijnens, N. Hermansson-Truedsson, and A. Rodr ´ ıguez-S´ anchez, JHEP 02, 167 (2023), 2211.17183
arXiv 2023
-
[1]
J. S. Schwinger, Phys. Rev. 73, 416 (1948)
1948
-
[2]
Kusch and H
P. Kusch and H. M. Foley, Phys. Rev. 74, 250 (1948)
1948
-
[3]
exp”) errors already shown in Table II, we include the following uncertainty esti- mates: (ii) matching (“match
derive from the orig- inal 54 Π i and represent the dynamical content of the theory. In this Letter, we follow the original approach from Refs. [21, 71] and consider dispersion relations in four-point kinematics, i.e., for the Mandelstam variables of the scattering process (3) with fixed photon virtual- ities, in contrast to an alternative approach in tri...
2024
-
[4]
D. P. Aguillard et al. (Muon g − 2), Phys. Rev. D 110, 032009 (2024), 2402.15410
arXiv 2024
-
[5]
D. P. Aguillard et al. (Muon g − 2), Phys. Rev. Lett. 131, 161802 (2023), 2308.06230
arXiv 2023
- [6]
Show all 138 references
- [7]
-
[8]
Aoyama, T
T. Aoyama, T. Kinoshita, and M. Nio, Atoms 7, 28 (2019)
2019
-
[9]
Aoyama, M
T. Aoyama, M. Hayakawa, T. Kinoshita, and M. Nio, Phys. Rev. Lett. 109, 111808 (2012), 1205.5370
2012 arXiv
-
[10]
Gnendiger, D
C. Gnendiger, D. St¨ ockinger, and H. St¨ ockinger-Kim, Phys. Rev. D 88, 053005 (2013), 1306.5546
2013 arXiv
-
[11]
Czarnecki, W
A. Czarnecki, W. J. Marciano, and A. Vainshtein, Phys. Rev. D 67, 073006 (2003), [Erratum: Phys. Rev. D 73, 119901 (2006)], hep-ph/0212229
2003 arXiv
-
[12]
Keshavarzi, D
A. Keshavarzi, D. Nomura, and T. Teubner, Phys. Rev. D 97, 114025 (2018), 1802.02995
2018 arXiv
-
[13]
Davier, A
M. Davier, A. Hoecker, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 77, 827 (2017), 1706.09436
2017 arXiv
-
[14]
Hoferichter, B.-L
M. Hoferichter, B.-L. Hoid, and B. Kubis, JHEP 08, 137 (2019), 1907.01556
2019 arXiv
-
[15]
Colangelo, M
G. Colangelo, M. Hoferichter, and P. Stoffer, JHEP 02, 006 (2019), 1810.00007
2019 arXiv
-
[16]
Keshavarzi, D
A. Keshavarzi, D. Nomura, and T. Teubner, Phys. Rev. D 101, 014029 (2020), 1911.00367
2020 arXiv
-
[17]
Davier, A
M. Davier, A. Hoecker, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 80, 241 (2020), [Erratum: Eur. Phys. J. C 80, 410 (2020)], 1908.00921
2020 arXiv
-
[18]
Melnikov and A
K. Melnikov and A. Vainshtein, Phys. Rev. D 70, 113006 (2004), hep-ph/0312226
2004 arXiv
-
[19]
B.-L. Hoid, M. Hoferichter, and B. Kubis, Eur. Phys. J. C 80, 988 (2020), 2007.12696
2020 arXiv
-
[20]
Colangelo, M
G. Colangelo, M. Hoferichter, M. Procura, and P. Stof- fer, Phys. Rev. Lett. 118, 232001 (2017), 1701.06554
2017 arXiv
-
[21]
Masjuan and P
P. Masjuan and P. S´ anchez-Puertas, Phys. Rev. D 95, 054026 (2017), 1701.05829
2017 arXiv
-
[22]
Hoferichter, B.-L
M. Hoferichter, B.-L. Hoid, B. Kubis, S. Leupold, and S. P. Schneider, Phys. Rev. Lett. 121, 112002 (2018), 1805.01471
2018 arXiv
-
[23]
Colangelo, M
G. Colangelo, M. Hoferichter, M. Procura, and P. Stof- fer, JHEP 04, 161 (2017), 1702.07347
2017 arXiv
-
[24]
G´ erardin, H
A. G´ erardin, H. B. Meyer, and A. Nyffeler, Phys. Rev. D 100, 034520 (2019), 1903.09471
2019 arXiv
-
[25]
Hoferichter, B.-L
M. Hoferichter, B.-L. Hoid, B. Kubis, S. Leupold, and S. P. Schneider, JHEP 10, 141 (2018), 1808.04823
2018 arXiv
-
[26]
Colangelo, F
G. Colangelo, F. Hagelstein, M. Hoferichter, L. Laub, and P. Stoffer, Phys. Rev. D 101, 051501 (2020), 1910.11881
2020 arXiv
-
[27]
Bijnens, N
J. Bijnens, N. Hermansson-Truedsson, and A. Rodr ´ ıguez-S´ anchez, Phys. Lett. B 798, 134994 (2019), 1908.03331
2019 arXiv
- [28]
-
[29]
Colangelo, F
G. Colangelo, F. Hagelstein, M. Hoferichter, L. Laub, and P. Stoffer, JHEP 03, 101 (2020), 1910.13432
2020 arXiv
-
[30]
Jegerlehner, The Anomalous Magnetic Moment of the Muon, vol
F. Jegerlehner, The Anomalous Magnetic Moment of the Muon, vol. 274 (Springer, Cham, 2017)
2017
-
[31]
Danilkin and M
I. Danilkin and M. Vanderhaeghen, Phys. Rev. D 95, 014019 (2017), 1611.04646
2017 arXiv
-
[32]
Eichmann, C
G. Eichmann, C. S. Fischer, and R. Williams, Phys. Rev. D 101, 054015 (2020), 1910.06795
2020 arXiv
-
[33]
Knecht, S
M. Knecht, S. Narison, A. Rabemananjara, and D. Ra- betiarivony, Phys. Lett. B 787, 111 (2018), 1808.03848
2018 arXiv
-
[34]
Calmet, S
J. Calmet, S. Narison, M. Perrottet, and E. de Rafael, Phys. Lett. B 61, 283 (1976). 6
1976
- [35]
-
[36]
Colangelo, M
G. Colangelo, M. Hoferichter, A. Nyffeler, M. Passera, and P. Stoffer, Phys. Lett. B 735, 90 (2014), 1403.7512
2014 arXiv
-
[37]
A. Kurz, T. Liu, P. Marquard, and M. Steinhauser, Phys. Lett. B 734, 144 (2014), 1403.6400
2014 arXiv
-
[38]
Crivellin, M
A. Crivellin, M. Hoferichter, C. A. Manzari, and M. Montull, Phys. Rev. Lett. 125, 091801 (2020), 2003.04886
2020 arXiv
-
[39]
Hoferichter and T
M. Hoferichter and T. Teubner, Phys. Rev. Lett. 128, 112002 (2022), 2112.06929
2022 arXiv
- [40]
-
[41]
Keshavarzi, W
A. Keshavarzi, W. J. Marciano, M. Passera, and A. Sir- lin, Phys. Rev. D 102, 033002 (2020), 2006.12666
2020 arXiv
-
[42]
Stamen, D
D. Stamen, D. Hariharan, M. Hoferichter, B. Kubis, and P. Stoffer, Eur. Phys. J. C 82, 432 (2022), 2202.11106
2022 arXiv
-
[43]
Colangelo, M
G. Colangelo, M. Hoferichter, and P. Stoffer, Phys. Lett. B 814, 136073 (2021), 2010.07943
2021 arXiv
-
[44]
Colangelo, M
G. Colangelo, M. Hoferichter, B. Kubis, and P. Stoffer, JHEP 10, 032 (2022), 2208.08993
2022 arXiv
-
[45]
Colangelo, A
G. Colangelo, A. X. El-Khadra, M. Hoferichter, A. Ke- shavarzi, C. Lehner, P. Stoffer, and T. Teubner, Phys. Lett. B 833, 137313 (2022), 2205.12963
2022 arXiv
-
[46]
Hoferichter, B.-L
M. Hoferichter, B.-L. Hoid, B. Kubis, and D. Schuh, JHEP 08, 208 (2023), 2307.02546
2023 arXiv
-
[47]
Hoferichter, G
M. Hoferichter, G. Colangelo, B.-L. Hoid, B. Kubis, J. Ruiz de Elvira, D. Schuh, D. Stamen, and P. Stof- fer, Phys. Rev. Lett. 131, 161905 (2023), 2307.02532
2023 arXiv
-
[48]
Davier, A
M. Davier, A. Hoecker, A.-M. Lutz, B. Malaescu, and Z. Zhang, Eur. Phys. J. C 84, 721 (2024), 2312.02053
2024 arXiv
-
[49]
Stoffer, G
P. Stoffer, G. Colangelo, and M. Hoferichter, JINST 18, C10021 (2023), 2308.04217
2023 arXiv
-
[50]
F. V. Ignatov et al. (CMD-3), Phys. Rev. Lett. 132, 231903 (2024), 2309.12910
2024
-
[51]
F. V. Ignatov et al. (CMD-3), Phys. Rev. D 109, 112002 (2024), 2302.08834
2024
- [52]
-
[53]
T. P. Leplumey and P. Stoffer (2025), 2501.09643
2025 arXiv
- [54]
- [55]
- [56]
-
[57]
Bazavov et al
A. Bazavov et al. (Fermilab Lattice, HPQCD, MILC), Phys. Rev. D 107, 114514 (2023), 2301.08274
2023 arXiv
- [58]
- [59]
- [60]
-
[61]
Djukanovic, G
D. Djukanovic, G. von Hippel, S. Kuberski, H. B. Meyer, N. Miller, K. Ottnad, J. Parrino, A. Risch, and H. Wit- tig (2024), 2411.07969
2024 arXiv
-
[62]
Campanario, H
F. Campanario, H. Czy˙ z, J. Gluza, T. Jeli´ nski, G. Ro- drigo, S. Tracz, and D. Zhuridov, Phys. Rev. D 100, 076004 (2019), 1903.10197
2019 arXiv
- [63]
-
[64]
Colangelo, M
G. Colangelo, M. Hoferichter, J. Monnard, and J. Ruiz de Elvira, JHEP 08, 295 (2022), [Erratum: JHEP 09, 177 (2024)], 2207.03495
2022 arXiv
- [65]
- [66]
-
[67]
Monnard, Ph.D
J. Monnard, Ph.D. thesis, Universit¨ at Bern (2021), URL https://boristheses.unibe.ch/2825/
2021
- [68]
-
[69]
J. P. Lees et al. (BaBar), Phys. Rev. D 108, L111103 (2023), 2308.05233
2023 arXiv
-
[70]
Colangelo, M
G. Colangelo, M. Hoferichter, B. Kubis, M. Procura, and P. Stoffer, Phys. Lett. B 738, 6 (2014), 1408.2517
2014 arXiv
-
[71]
Colangelo, M
G. Colangelo, M. Hoferichter, M. Procura, and P. Stof- fer, JHEP 09, 091 (2014), 1402.7081
2014 arXiv
-
[72]
Hoferichter, G
M. Hoferichter, G. Colangelo, M. Procura, and P. Stof- fer, Int. J. Mod. Phys. Conf. Ser. 35, 1460400 (2014), 1309.6877
2014 arXiv
-
[73]
Colangelo, M
G. Colangelo, M. Hoferichter, M. Procura, and P. Stof- fer, JHEP 09, 074 (2015), 1506.01386
2015 arXiv
- [74]
- [75]
-
[76]
Hoferichter, P
M. Hoferichter, P. Stoffer, and M. Zillinger, JHEP 04, 092 (2024), 2402.14060
2024 arXiv
- [77]
-
[78]
Bijnens, N
J. Bijnens, N. Hermansson-Truedsson, L. Laub, and A. Rodr ´ ıguez-S´ anchez, JHEP 04, 240 (2021), 2101.09169
2021 arXiv
-
[79]
Bijnens, N
J. Bijnens, N. Hermansson-Truedsson, L. Laub, and A. Rodr ´ ıguez-S´ anchez, JHEP 10, 203 (2020), 2008.13487
2020 arXiv
-
[80]
Bijnens, N
J. Bijnens, N. Hermansson-Truedsson, and A. Rodr ´ ıguez-S´ anchez (2024), 2411.09578
2024 arXiv
- [83]
-
[84]
Tarrach, Nuovo Cim
R. Tarrach, Nuovo Cim. A 28, 409 (1975)
1975
-
[85]
W. A. Bardeen and W. K. Tung, Phys. Rev. 173, 1423 (1968), [Erratum: Phys. Rev. D 4, 3229 (1971)]
1968
- [86]
-
[87]
Eichmann, C
G. Eichmann, C. S. Fischer, and W. Heupel, Phys. Rev. D 92, 056006 (2015), 1505.06336
2015 arXiv
-
[88]
Hoferichter, B
M. Hoferichter, B. Kubis, and D. Sakkas, Phys. Rev. D 86, 116009 (2012), 1210.6793
2012 arXiv
-
[89]
S. P. Schneider, B. Kubis, and F. Niecknig, Phys. Rev. D 86, 054013 (2012), 1206.3098
2012 arXiv
-
[90]
Hoferichter, B.-L
M. Hoferichter, B.-L. Hoid, B. Kubis, and J. L¨ udtke, Phys. Rev. Lett. 128, 172004 (2022), 2105.04563
2022 arXiv
-
[91]
Hoferichter, B
M. Hoferichter, B. Kubis, S. Leupold, F. Niecknig, and S. P. Schneider, Eur. Phys. J. C 74, 3180 (2014), 1410.4691
2014 arXiv
-
[92]
Hanhart, A
C. Hanhart, A. Kup´ s´ c, U.-G. Meißner, F. Stollenwerk, and A. Wirzba, Eur. Phys. J. C 73, 2668 (2013), [Erra- tum: Eur. Phys. J. C 75, 242 (2015)], 1307.5654
2013 arXiv
-
[93]
Stollenwerk, C
F. Stollenwerk, C. Hanhart, A. Kup´ s´ c, U.-G. Meißner, and A. Wirzba, Phys. Lett. B 707, 184 (2012), 1108.2419
2012 arXiv
-
[94]
S. Holz, J. Plenter, C.-W. Xiao, T. Dato, C. Hanhart, B. Kubis, U.-G. Meißner, and A. Wirzba, Eur. Phys. J. C 81, 1002 (2021), 1509.02194
2021 arXiv
- [95]
-
[96]
Holz, Ph.D
S. Holz, Ph.D. thesis, University of Bonn (2022), URL https://nbn-resolving.org/urn:nbn:de:hbz: 5-67976
2022
-
[97]
S. Holz, C. Hanhart, M. Hoferichter, and B. Kubis, Eur. 7 Phys. J. C 82, 434 (2022), [Addendum: Eur. Phys. J. C 82, 1159 (2022)], 2202.05846
2022 arXiv
-
[98]
S. Holz, M. Hoferichter, B.-L. Hoid, and B. Kubis (2024), 2412.16281
2024 arXiv
-
[99]
S. Holz, M. Hoferichter, B.-L. Hoid, and B. Kubis (2024), 2411.08098
2024 arXiv
-
[100]
Hoferichter, D
M. Hoferichter, D. R. Phillips, and C. Schat, Eur. Phys. J. C 71, 1743 (2011), 1106.4147
2011 arXiv
-
[101]
Garc ´ ıa-Mart ´ ın and B
R. Garc ´ ıa-Mart ´ ın and B. Moussallam, Eur. Phys. J. C 70, 155 (2010), 1006.5373
2010 arXiv
-
[102]
Danilkin and M
I. Danilkin and M. Vanderhaeghen, Phys. Lett. B 789, 366 (2019), 1810.03669
2019 arXiv
- [103]
-
[104]
Danilkin, O
I. Danilkin, O. Deineka, and M. Vanderhaeghen, Phys. Rev. D 101, 054008 (2020), 1909.04158
2020 arXiv
- [105]
-
[106]
Sch¨ afer, M
H. Sch¨ afer, M. Zanke, Y. Korte, and B. Kubis, Phys. Rev. D 108, 074025 (2023), 2307.10357
2023 arXiv
- [107]
-
[108]
Danilkin, M
I. Danilkin, M. Hoferichter, and P. Stoffer, Phys. Lett. B 820, 136502 (2021), 2105.01666
2021 arXiv
- [109]
-
[110]
Achard et al
P. Achard et al. (L3), JHEP 03, 018 (2007)
2007
- [111]
-
[112]
J. P. Lees et al. (BaBar), Phys. Rev. D 107, 072001 (2023), 2207.10340
2023 arXiv
-
[113]
Aubert et al
B. Aubert et al. (BaBar), Phys. Rev. D 76, 092005 (2007), [Erratum: Phys. Rev. D 77, 119902 (2008)], 0708.2461
2007 arXiv
-
[114]
Leutgeb, J
J. Leutgeb, J. Mager, and A. Rebhan, Phys. Rev. D 107, 054021 (2023), 2211.16562
2023 arXiv
-
[115]
Navas et al
S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024)
2024
-
[116]
G. A. Schuler, F. A. Berends, and R. van Gulik, Nucl. Phys. B 523, 423 (1998), hep-ph/9710462
1998 arXiv
- [117]
-
[118]
Cappiello, O
L. Cappiello, O. Cat` a, G. D’Ambrosio, D. Greynat, and A. Iyer, Phys. Rev. D 102, 016009 (2020), 1912.02779
2020 arXiv
- [119]
-
[120]
Masjuan, P
P. Masjuan, P. Roig, and P. S´ anchez-Puertas, J. Phys. G 49, 015002 (2022), 2005.11761
2022 arXiv
- [121]
-
[122]
Colangelo, F
G. Colangelo, F. Hagelstein, M. Hoferichter, L. Laub, and P. Stoffer, Eur. Phys. J. C 81, 702 (2021), 2106.13222
2021 arXiv
- [123]
-
[124]
Herren and M
F. Herren and M. Steinhauser, Comput. Phys. Com- mun. 224, 333 (2018), 1703.03751
2018 arXiv
-
[125]
Eichmann, C
G. Eichmann, C. S. Fischer, T. Haeuser, and O. Regen- felder (2024), 2411.05652
2024 arXiv
-
[126]
Vainshtein, Phys
A. Vainshtein, Phys. Lett. B 569, 187 (2003), hep- ph/0212231
2003
-
[127]
K. G. Chetyrkin, J. H. K¨ uhn, and M. Steinhauser, Com- put. Phys. Commun. 133, 43 (2000), hep-ph/0004189
2000 arXiv
-
[128]
T. Blum, N. Christ, M. Hayakawa, T. Izubuchi, L. Jin, C. Jung, and C. Lehner (RBC, UKQCD), Phys. Rev. Lett. 124, 132002 (2020), 1911.08123
2020 arXiv
-
[129]
Knecht, S
M. Knecht, S. Peris, M. Perrottet, and E. de Rafael, JHEP 03, 035 (2004), hep-ph/0311100
2004 arXiv
-
[130]
E.-H. Chao, R. J. Hudspith, A. G´ erardin, J. R. Green, and H. B. Meyer, Eur. Phys. J. C 82, 664 (2022), 2204.08844
2022 arXiv
-
[131]
E.-H. Chao, R. J. Hudspith, A. G´ erardin, J. R. Green, H. B. Meyer, and K. Ottnad, Eur. Phys. J. C 81, 651 (2021), 2104.02632
2021 arXiv
-
[132]
Fodor, A
Z. Fodor, A. G´ erardin, L. Lellouch, K. K. Szab´ o, B. C. Toth, and C. Zimmermann (BMWc) (2024), 2411.11719
2024 arXiv
-
[133]
T. Blum, N. Christ, M. Hayakawa, T. Izubuchi, L. Jin, C. Jung, C. Lehner, and C. Tu (RBC, UKQCD), Phys. Rev. D 111, 014501 (2025), 2304.04423
2025 arXiv
-
[134]
C. F. Redmer, Nuovo Cim. C 47, 247 (2024)
2024
-
[135]
Prades, E
J. Prades, E. de Rafael, and A. Vainshtein, Adv. Ser. Direct. High Energy Phys. 20, 303 (2009), 0901.0306
2009 arXiv
-
[136]
Altmannshofer et al
W. Altmannshofer et al. (Belle-II), PTEP 2019, 123C01 (2019), [Erratum: PTEP 2020, 029201 (2020)], 1808.10567
2019
-
[137]
Ablikim et al
M. Ablikim et al. (BESIII), Chin. Phys. C 44, 040001 (2020), 1912.05983
2020
-
[2020]
Glasgow consensus
and the “Glasgow consensus” [133] (PdR V 2009), as well as the lattice-QCD calculations by RBC/UKQCD [128, 131] (including the charm loop from Ref. [130]), Mainz [129, 130], and BMWc [132]. vinced that Eq. (8) represents a realistic and conservative estimate of the current unc...
2009
Reviewed August 12, 2026 · model on record in the stance chip above.
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