REVIEW 2 major objections 5 minor 2 cited by
Flavor constraints from $pp\to Vh$ and $pp\to VW$ at the LHC
T0 review · 2 major / 5 minor · reviewed 2026-08-04 · deepseek-v4-flash
Pith's one-line read The paper claims that pp→Vh and pp→VW tails at the LHC are controlled by five flavor-dependent quark-coupling shifts, yielding bounds complementary to electroweak and flavor data, with HL-LHC projections probing the Cabibbo-angle anomaly re
desk verdict A solid, clearly written SMEFT paper: new general-flavor amplitudes for Vh/VW, useful per-flavor LHC bounds, with honest caveats; worth refereeing. 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 load-bearing machinery is five effective coupling shifts — δg_ZuL, δg_ZdL, δg_ZuR, δg_ZdR and δg_WqR — together with the SU(2)_L relation δg_WqL = δg_ZuL·V − V·δg_ZdL. In the high-energy limit, the helicity amplitudes of Eqs. (3.4)–(3.5) scale as s-hat/v^2; the Goldstone equivalence theorem, which identifies longitudinal W/Z amplitudes with those of the would-be Goldstone bosons at high energy, connects the Vh and WV channels, so the same operators produce correlated energy-enhanced tails in both. This five-coupling structure, with explicit CKM factors, is what makes a flavor-general fit possible with existing LHC differential data.
What would settle it
Refit the same ATLAS/CMS pp→Vh and pp→VW differential data with dipole operators ψ²XH included as free tree-level parameters. If the preferred values of δg_ZuL, δg_ZdL, δg_ZuR, δg_ZdR or δg_WqR move outside the 95% intervals of Fig. 4.1, the paper's five-coupling amplitude basis is not the right description of the tails.
Extended reading notes
Core claim
The central result is that, at high energies, the helicity amplitudes for pp→Zh, pp→Wh, pp→WW and pp→WZ with longitudinal bosons grow as s-hat/v^2, and each flavor channel is governed by one of five effective coupling shifts (δg_ZuL, δg_ZdL, δg_ZuR, δg_ZdR, δg_WqR) times explicit CKM factors. Gauge invariance ties the left-handed charged-current shift to neutral-current ones, δg_WqL = δg_ZuL·V − V·δg_ZdL, so Vh and WV probe the same operators. From Run-2 differential data the paper derives 95% CL bounds on C_Hq^(1), C_Hq^(3), C_Hu, C_Hd and C_Hud for all flavor pairs, finds Vh roughly twice as sensitive as WV, and shows LHC constraints rival electroweak precision data for light quarks and be
Load-bearing premise
The constraints assume new physics appears only through four-fermion and Higgs-current contact terms that weakly coupled ultraviolet completions generate at tree level, with loop-type dipole operators set to zero even though they would grow with energy just as fast in pp→VW; a model with sizable tree-level dipoles would shift all the quoted bounds.
Editorial extensions
If this is right
- Associated Higgs production gives the strongest LHC limits on the five Higgs-current operators, about twice as strong as the diboson channels at the same luminosity, because the Vh SM background is dominated by longitudinal modes.
- LHC Vh+WV data remove flat directions that electroweak precision data leave in the light-quark sector, superseding the constraining power of Drell-Yan forward-backward asymmetry measurements.
- Right-handed charged currents (operator C_Hud), essentially unconstrained by Z- and W-pole data, are bounded at |C_Hud_11|/Λ² ≲ 0.1 TeV⁻² by the Vh tails.
- HL-LHC projections reach the C_Hud_11 and C_Hud_12 regions preferred by low-energy fits to the Cabibbo-angle anomaly, so the high-energy LHC can test that anomaly's new-physics explanation.
- Because no flavor ansatz is imposed, the bounds hold for non-universal models such as TeV-scale vector-like quarks coupled to first- or second-generation quarks.
Reading between the lines
- One extension of this approach is to add angular observables of Vh and WV final states, which the paper notes are available and would distinguish the five couplings by their interference patterns with the Standard Model.
- The same amplitude relations could be applied to other CKM-weighted channels such as vector-boson scattering or final states with charm quarks, extending the method beyond the processes fitted here.
- A combined future fit of Vh, WV and high-pT Drell-Yan data could simultaneously constrain the full tree-level operator class and test whether the five-coupling description remains sufficient once dipole operators are included.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies pp->Vh and pp->VW production at the LHC as probes of SMEFT Higgs-current operators (psi^2 H^2 D) with a general flavor structure. In Sec. 3 the authors derive the high-energy helicity amplitudes and express the leading flavor-dependent contributions in terms of five effective couplings (delta g_ZuL, delta g_ZdL, delta g_ZuR, delta g_ZdR, delta g_WqR) with an explicit CKM-matrix dependence. They then use Run-2 differential data from ATLAS and CMS on WW, WZ, Zh, and Wh to obtain 95% CL bounds on the Wilson coefficients C_Hq^(1), C_Hq^(3), C_Hd, C_Hu, and C_Hud for different quark-flavor indices (Fig. 4.1). The LHC constraints are compared with electroweak precision observables (Sec. 5) and with low-energy flavor data relevant to the first-row CKM unitarity test (Sec. 6), including HL-LHC projections and a vector-like-quark model. The central claim is that these LHC channels provide complementary, and in some cases competitive, constraints on flavor-non-universal Higgs-current operators.
Significance. If the derived bounds are correct, this is a useful step toward a fully flavor-general SMEFT likelihood for high-energy processes. The paper's strengths include the explicit CKM factors in the amplitudes, the use of differential LHC data rather than signal strengths, the demonstration of complementarity with EWPO and low-energy flavor fits, and falsifiable HL-LHC projections. The analysis is not circular: the amplitudes follow from the gauge-invariant SMEFT Lagrangian and are then compared with independent data sets. The main caveats are the tree-level-only operator assumption and the LO treatment of the EFT signal, both of which need quantitative support before the numerical constraints in Fig. 4.1 can be taken at face value.
major comments (2)
- [Sec. 2.1 / Table 2.1 / Fig. 4.1] The restriction to operators generated at tree level in weakly coupled UV completions is load-bearing for the identification of the pp->VW observables with the five psi^2 H^2 D couplings. Table 2.1 assigns dipole operators (psi^2 X H) the same E^2/Lambda^2 amplitude growth as psi^2 H^2 D for pp->VW, and the text acknowledges that these are dropped as loop-suppressed without quantifying the loop factor against the sensitivity of the fit. Since Fig. 4.1 combines the WW and WZ data, a loop-induced dipole coefficient of size ~g y_q/(16 pi^2) times a tree-level coefficient could be non-negligible relative to the quoted intervals, which are O(0.01-0.1) TeV^-2. I request a numerical check: either include representative dipole/TGC operators in the fit and show that the five-coupling intervals in Fig. 4.1 shift negligibly, or derive upper bounds on those operators from the same data. The Vh const
- [Sec. 4.1 and Sec. 4.2] The EFT contributions (A_NP and B_NP in Eq. (4.1)) are simulated at LO QCD, while the SM predictions are taken from the experimental analyses, and the paper states without demonstration that PDF/scale uncertainties on the EFT terms have a negligible impact. Because the bounds are extracted from the high-pT tails, the scale and PDF dependence of the EFT signal can shift the inferred intervals. Please provide a quantitative estimate of this uncertainty (e.g., a scale/PDF envelope) or cite a validation specific to these final states. This is relevant to all channels and hence to the central bounds in Fig. 4.1.
minor comments (5)
- [Sec. 4.1.1, Eqs. (4.3)-(4.4)] The CMS WW recast uses hand-set pull uncertainties sigma_th, sigma_bkg in [0.1,0.2]. The authors state that the implementation was validated against CMS limits, but reporting the dependence of the WW-only bounds on these choices would improve reproducibility and robustness.
- [Sec. 1] Typo: 'illlustrate' should be 'illustrate'; 'Particle Distribution Functions' should be 'Parton Distribution Functions'.
- [Sec. 6.2.2] Typo: 'short-distand electroweak corrections' should be 'short-distance electroweak corrections'.
- [Sec. 6.3] The statement that there are other charged-current transitions for which the LHC constraints derived in this study can already supersede flavor bounds [87] refers to unpublished work. Either show this explicitly or soften the claim.
- [Sec. 5] The EWPO bounds are evaluated at mu = 1 TeV, but the LHC bounds in Fig. 4.1 are not accompanied by an explicit statement of the renormalization scale used for the LHC predictions. Please state the scale convention so the comparison in Fig. 5.1 is unambiguous.
Circularity Check
No significant circularity: the amplitudes are derived from SMEFT gauge invariance and matched to independent LHC, EWPO and flavor data; the CKM-anomaly benchmark is imported from external fits.
full rationale
The derivation chain is self-contained against external benchmarks. Section 2 defines the SMEFT operator basis and the matching relations (Eq. 2.6), with the gauge-invariance relation Eq. (2.4) taken from an independent reference [32]. Section 3 derives the high-energy helicity amplitudes for pp→Vh and pp→VW directly from those couplings, including explicit CKM factors; no fitted quantity is reused as an input to the same prediction. Section 4 builds a chi-square likelihood from published LHC Run-2 differential measurements and uses it to constrain the Higgs-current Wilson coefficients: these are fits to data, not predictions masquerading as tests. The comparison in Section 5 uses electroweak precision observables that are external to the LHC fit, and Section 6 imports the viable CKM-unitarity-anomaly benchmark from independent global fits [60,61] before applying the LHC constraints. The only assumptions that could affect the interpretation, such as the restriction to tree-level-generated operators and the neglect of loop-suppressed dipole/TGC operators noted in Sec. 2.1 and Table 2.1, are stated model assumptions rather than circular reductions; they concern robustness but do not make the LHC bounds equivalent to any input in the derivation. Self-citations [24,25,79,87] provide Drell-Yan methodology, Kℓ3 expressions, and future-work references, none of which is load-bearing for the central Vh/VW amplitude derivation or for the numerical constraints.
Assumptions & free parameters
free parameters (4)
- CMS WW pull uncertainties (σ_th, σ_bkg, σ_dat) =
σ_th, σ_bkg ∈ [0.1, 0.2]; σ_dat = 0.02
- EWPO reference scale μ = 1 TeV =
1 TeV
- Low-energy CKM fit parameters (λ, δg_VR^d, δg_VR^s) =
95% CL region in Fig. 6.1
- Vector-like quark mass m_Q =
2 TeV
assumptions (8)
- standard math SMEFT truncated at dimension six in the Warsaw basis
- standard math Gauge-invariance relation δg_W^L = δg_Zu^L·V − V·δg_Zd^L
- standard math Goldstone Boson Equivalence Theorem
- domain assumption Only tree-level-generated operators are included; dipoles (ψ^2XH) and TGCs (X^3) are neglected
- domain assumption EFT validity Λ ≫ E for the LHC processes
- domain assumption Wilson coefficients are real
- domain assumption Down-type quark Yukawas are diagonal with q_i = [(V†u)_Li, d_Li]^T
- standard math External low-energy inputs (lattice decay constants and form factors, S_EW, radiative corrections) are taken as given
Cite this review
Pith. "Pith review of Flavor constraints from $pp\to Vh$ and $pp\to VW$ at the LHC." pith.science (2026). https://pith.science/paper/5D6K5ZHB
@misc{pith2026250908437,
author = {Pith},
title = {Pith review of: Flavor constraints from $pp\to Vh$ and $pp\to VW$ at the LHC},
year = {2026},
howpublished = {\url{https://pith.science/paper/5D6K5ZHB}},
note = {Machine review of arXiv:2509.08437}
}
abstract
We investigate the potential of associated Higgs $pp\to Vh$ and diboson production $pp\to VW$ channels at the LHC (with $V=W,Z$) to constrain flavor-physics operators. Within a general Effective Field Theory (EFT) framework, we derive the helicity amplitudes for these processes at high energies and identify the leading contributions from dimension-six operators involving different quark flavors. Using available LHC data, we show that these processes are sensitive to non-trivial flavor structures and provide complementary constraints to those from low-energy observables. We illustrate this synergy through an explicit comparison between our LHC bounds with electroweak precision data, and with flavor limits derived from charged-current pion and kaon decays. In particular, we show that our HL-LHC projections can probe viable EFT scenarios proposed to accommodate the discrepancies in the extraction of the Cabibbo angle.
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Reference graph
Works this paper leans on
-
[1]
S. Chatrchyanet al.[CMS], Phys. Lett. B716(2012), 30-61 [arXiv:1207.7235 [hep- ex]]; G. Aadet al.[ATLAS], Phys. Lett. B716(2012), 1-29 [arXiv:1207.7214 [hep- ex]]
arXiv 2012
-
[2]
Hagiwara, R
K. Hagiwara, R. D. Peccei, D. Zeppenfeld and K. Hikasa, Nucl. Phys. B282(1987), 253-307
1987
-
[3]
Hagiwara, S
K. Hagiwara, S. Ishihara, R. Szalapski and D. Zeppenfeld, Phys. Rev. D48(1993), 2182-2203
1993
-
[4]
C. Degrande, N. Greiner, W. Kilian, O. Mattelaer, H. Mebane, T. Stelzer, S. Wil- lenbrock and C. Zhang, Annals Phys.335(2013), 21-32 [arXiv:1205.4231 [hep-ph]]. 28
arXiv 2013
-
[5]
Constraining anomalous Higgs interactions
T. Corbett, O. J. P. Eboli, J. Gonzalez-Fraile and M. C. Gonzalez-Garcia, Phys. Rev. D86(2012), 075013 [arXiv:1207.1344 [hep-ph]]; T. Corbett, O. J. P. ´Eboli, J. Gonzalez-Fraile and M. C. Gonzalez-Garcia, Phys. Rev. Lett.111(2013), 011801 [arXiv:1304.1151 [hep-ph]]
work page Pith review arXiv 2012
- [6]
-
[7]
J. J. Ethier, R. Gomez-Ambrosio, G. Magni and J. Rojo, Eur. Phys. J. C81(2021) no.6, 560 [arXiv:2101.03180 [hep-ph]]
arXiv 2021
-
[8]
The Gauge-Higgs Legacy of the LHC Run I
A. Butter, O. J. P. ´Eboli, J. Gonzalez-Fraile, M. C. Gonzalez-Garcia, T. Plehn and M. Rauch, JHEP07(2016), 152 [arXiv:1604.03105 [hep-ph]]; T. Corbett, O. J. P. Eboli, J. Gonzalez-Fraile and M. C. Gonzalez-Garcia, Phys. Rev. D87 (2013), 015022 [arXiv:1211.4580 [hep-ph]]; E. d. Almeida, A. Alves, O. J. P. ´Eboli and M. C. Gonzalez-Garcia, Phys. Rev. D105(...
work page Pith review arXiv 2016
Show all 90 references
-
[9]
Falkowski, M
A. Falkowski, M. Gonzalez-Alonso, A. Greljo and D. Marzocca, Phys. Rev. Lett.116 (2016) no.1, 011801 [arXiv:1508.00581 [hep-ph]]; A. Falkowski, M. Gonzalez-Alonso, A. Greljo, D. Marzocca and M. Son, JHEP02(2017), 115 [arXiv:1609.06312 [hep- ph]]
2016 arXiv
-
[10]
Baglio, S
J. Baglio, S. Dawson and I. M. Lewis, Phys. Rev. D96(2017) no.7, 073003 [arXiv:1708.03332 [hep-ph]]
2017 arXiv
-
[11]
Franceschini, G
R. Franceschini, G. Panico, A. Pomarol, F. Riva and A. Wulzer, JHEP02(2018), 111 [arXiv:1712.01310 [hep-ph]]
2018 arXiv
-
[12]
Grojean, M
C. Grojean, M. Montull and M. Riembau, JHEP03(2019), 020 [arXiv:1810.05149 [hep-ph]]
2019 arXiv
-
[13]
Banerjee, C
S. Banerjee, C. Englert, R. S. Gupta and M. Spannowsky, Phys. Rev. D98(2018) no.9, 095012 [arXiv:1807.01796 [hep-ph]]; S. Banerjee, D. Reichelt and M. Span- nowsky, Phys. Rev. D110(2024) no.11, 11 [arXiv:2406.15640 [hep-ph]]
2018 arXiv
-
[14]
Biek¨ otter, A
A. Biek¨ otter, A. Knochel, M. Kr¨ amer, D. Liu and F. Riva, Phys. Rev. D91(2015), 055029 [arXiv:1406.7320 [hep-ph]]
2015 arXiv
-
[15]
Liu and L
D. Liu and L. T. Wang, Phys. Rev. D99(2019) no.5, 055001 [arXiv:1804.08688 [hep-ph]]
2019 arXiv
-
[16]
de Blas, A
J. de Blas, A. Goncalves, V. Miralles, L. Reina, L. Silvestrini and M. Valli, [arXiv:2507.06191 [hep-ph]]; J. de Blas, M. Ciuchini, E. Franco, S. Mishima, M. Pierini, L. Reina and L. Silvestrini, JHEP12(2016), 135 [arXiv:1608.01509 [hep-ph]]
2016
-
[17]
Corbett, O
T. Corbett, O. J. P. ´Eboli and M. C. Gonzalez-Garcia, Phys. Rev. D96(2017) no.3, 035006 [arXiv:1705.09294 [hep-ph]]. 29
2017 arXiv
-
[18]
J. M. Cornwall, D. N. Levin and G. Tiktopoulos, Phys. Rev. D10(1974), 1145 [erratum: Phys. Rev. D11(1975), 972]
1974
-
[19]
D’Ambrosio, G
G. D’Ambrosio, G. F. Giudice, G. Isidori and A. Strumia, Nucl. Phys. B645(2002), 155-187 [arXiv:hep-ph/0207036 [hep-ph]]
2002 arXiv
-
[20]
Barbieri, G
R. Barbieri, G. Isidori, J. Jones-Perez, P. Lodone and D. M. Straub, Eur. Phys. J. C71(2011), 1725 [arXiv:1105.2296 [hep-ph]]
2011 arXiv
-
[21]
D. A. Faroughy, G. Isidori, F. Wilsch and K. Yamamoto, JHEP08(2020), 166 [arXiv:2005.05366 [hep-ph]]; A. Greljo, A. Palavri´ c and A. E. Thomsen, JHEP10 (2022), 010 [arXiv:2203.09561 [hep-ph]]
2020 arXiv
-
[22]
Buchmuller and D
W. Buchmuller and D. Wyler, Nucl. Phys. B268(1986), 621-653
1986
-
[23]
Grzadkowski, M
B. Grzadkowski, M. Iskrzynski, M. Misiak and J. Rosiek, JHEP10(2010), 085 [arXiv:1008.4884 [hep-ph]]
2010 arXiv
-
[24]
Allwicher, D
L. Allwicher, D. A. Faroughy, F. Jaffredo, O. Sumensari and F. Wilsch, JHEP03 (2023), 064 [arXiv:2207.10714 [hep-ph]]
2023 arXiv
-
[25]
Allwicher, D
L. Allwicher, D. A. Faroughy, F. Jaffredo, O. Sumensari and F. Wilsch, high-p T Drell-Yan tails beyond the standard model,” Comput. Phys. Commun.289(2023), 108749 [arXiv:2207.10756 [hep-ph]]
2023 arXiv
-
[26]
Grunwald, G
C. Grunwald, G. Hiller, K. Kr¨ oninger and L. Nollen, JHEP11(2023), 110 [arXiv:2304.12837 [hep-ph]]; S. Bißmann, C. Grunwald, G. Hiller and K. Kr¨ oninger, JHEP06(2021), 010 [arXiv:2012.10456 [hep-ph]]; A. Greljo, J. Salko, A. Smolkoviˇ c and P. Stangl, JHEP05(2023), 087 [arXi...
2023 arXiv
-
[27]
Gabrielli, L
E. Gabrielli, L. Marzola and K. M¨ u¨ ursepp, Phys. Lett. B859(2024), 139106 [arXiv:2405.14585 [hep-ph]]
2024
-
[28]
Cirigliano, A
V. Cirigliano, A. Crivellin, M. Hoferichter and M. Moulson, Phys. Lett. B838(2023), 137748 [arXiv:2208.11707 [hep-ph]]
2023 arXiv
-
[29]
Alioli, V
S. Alioli, V. Cirigliano, W. Dekens, J. de Vries and E. Mereghetti, JHEP05(2017), 086 [arXiv:1703.04751 [hep-ph]]
2017 arXiv
-
[30]
Aadet al.[ATLAS], [arXiv:2410.19611 [hep-ex]]
G. Aadet al.[ATLAS], [arXiv:2410.19611 [hep-ex]]
-
[31]
Tumasyanet al.[CMS], Phys
A. Tumasyanet al.[CMS], Phys. Rev. D109(2024) no.9, 092011 [arXiv:2312.07562 [hep-ex]]
2024 arXiv
-
[32]
Efrati, A
A. Efrati, A. Falkowski and Y. Soreq, JHEP07(2015), 018 [arXiv:1503.07872 [hep- ph]]
2015 arXiv
-
[33]
C. Arzt, M. B. Einhorn and J. Wudka, Nucl. Phys. B433(1995), 41-66 [arXiv:hep- ph/9405214 [hep-ph]]
1995
-
[34]
de Blas, J
J. de Blas, J. C. Criado, M. Perez-Victoria and J. Santiago, JHEP03(2018), 109 [arXiv:1711.10391 [hep-ph]]. 30
2018 arXiv
- [35]
-
[36]
Bordone, A
M. Bordone, A. Greljo and D. Marzocca, JHEP08(2021), 036 [arXiv:2103.10332 [hep-ph]]
2021 arXiv
-
[37]
B. W. Lee, C. Quigg and H. B. Thacker, Phys. Rev. D16(1977), 1519
1977
-
[38]
G. J. Gounaris, R. Kogerler and H. Neufeld, Phys. Rev. D34(1986), 3257
1986
-
[39]
M. S. Chanowitz, M. Golden and H. Georgi, Phys. Rev. D36(1987), 1490; M. S. Chanowitz and M. K. Gaillard, Nucl. Phys. B261(1985), 379-431
1987
- [40]
-
[41]
Aadet al.[ATLAS], [arXiv:2505.11310 [hep-ex]]
G. Aadet al.[ATLAS], [arXiv:2505.11310 [hep-ex]]
-
[42]
Aaboudet al.[ATLAS], Eur
M. Aaboudet al.[ATLAS], Eur. Phys. J. C79(2019) no.10, 884 [arXiv:1905.04242 [hep-ex]]
2019 arXiv
-
[43]
A. M. Sirunyanet al.[CMS], Phys. Rev. D102(2020) no.9, 092001 [arXiv:2009.00119 [hep-ex]]
2020 arXiv
-
[44]
Aadet al.[ATLAS], [arXiv:2507.03500 [hep-ex]]
G. Aadet al.[ATLAS], [arXiv:2507.03500 [hep-ex]]
-
[45]
Tumasyanet al.[CMS], JHEP07(2022), 032 [arXiv:2110.11231 [hep-ex]]
A. Tumasyanet al.[CMS], JHEP07(2022), 032 [arXiv:2110.11231 [hep-ex]]
2022 arXiv
-
[46]
Frederix, S
R. Frederix, S. Frixione, V. Hirschi, D. Pagani, H. S. Shao and M. Zaro, JHEP07 (2018), 185 [erratum: JHEP11(2021), 085] [arXiv:1804.10017 [hep-ph]]
2018 arXiv
-
[47]
N. D. Christensen and C. Duhr, Comput. Phys. Commun.180(2009), 1614-1641 [arXiv:0806.4194 [hep-ph]]; A. Alloul, N. D. Christensen, C. Degrande, C. Duhr and B. Fuks, Comput. Phys. Commun.185(2014), 2250-2300 [arXiv:1310.1921 [hep-ph]]
2009 arXiv
-
[48]
Sjostrand, S
T. Sjostrand, S. Mrenna and P. Z. Skands, Comput. Phys. Commun.178(2008), 852-867 [arXiv:0710.3820 [hep-ph]]
2008 arXiv
-
[49]
de Favereauet al.[DELPHES 3], JHEP02(2014), 057 [arXiv:1307.6346 [hep-ex]]
J. de Favereauet al.[DELPHES 3], JHEP02(2014), 057 [arXiv:1307.6346 [hep-ex]]
2014 arXiv
-
[50]
de Florianet al.[LHC Higgs Cross Section Working Group], CERN Yellow Rep
D. de Florianet al.[LHC Higgs Cross Section Working Group], CERN Yellow Rep. Monogr.2(2017), 1-869 [arXiv:1610.07922 [hep-ph]]
2017 arXiv
-
[51]
R. Coy, M. Frigerio, F. Mescia and O. Sumensari, Eur. Phys. J. C80(2020) no.1, 52 [arXiv:1909.08567 [hep-ph]]; C. Cornella, F. Feruglio and P. Paradisi, JHEP11 (2018), 012 [arXiv:1803.00945 [hep-ph]]
2020 arXiv
-
[52]
E. E. Jenkins, A. V. Manohar and M. Trott, JHEP10(2013), 087 [arXiv:1308.2627 [hep-ph]]; E. E. Jenkins, A. V. Manohar and M. Trott, JHEP01(2014), 035 [arXiv:1310.4838 [hep-ph]]; R. Alonso, E. E. Jenkins, A. V. Manohar and M. Trott, JHEP04(2014), 159 [arXiv:1312.2014 [hep-ph]]
2013 arXiv
-
[53]
Fuentes-Martin, P
J. Fuentes-Martin, P. Ruiz-Femenia, A. Vicente and J. Virto, Eur. Phys. J. C81 (2021) no.2, 167 [arXiv:2010.16341 [hep-ph]]; A. Celis, J. Fuentes-Martin, A. Vicente and J. Virto, Eur. Phys. J. C77(2017) no.6, 405 [arXiv:1704.04504 [hep-ph]]. 31
2021 arXiv
-
[54]
Janot and S
P. Janot and S. Jadach, Phys. Lett. B803(2020), 135319 [arXiv:1912.02067 [hep- ph]]
2020 arXiv
-
[55]
Bres´ o-Pla, A
V. Bres´ o-Pla, A. Falkowski and M. Gonz´ alez-Alonso, JHEP08(2021), 021 [arXiv:2103.12074 [hep-ph]]
2021 arXiv
-
[56]
de Blas, M
J. de Blas, M. Pierini, L. Reina and L. Silvestrini, Phys. Rev. Lett.129(2022) no.27, 271801 [arXiv:2204.04204 [hep-ph]]
2022 arXiv
-
[57]
Schaelet al.[ALEPH, DELPHI, L3, OPAL, SLD, LEP Electroweak Working Group, SLD Electroweak Group and SLD Heavy Flavour Group], Phys
S. Schaelet al.[ALEPH, DELPHI, L3, OPAL, SLD, LEP Electroweak Working Group, SLD Electroweak Group and SLD Heavy Flavour Group], Phys. Rept.427 (2006), 257-454 [arXiv:hep-ex/0509008 [hep-ex]]
2006 arXiv
-
[58]
Navaset al.[Particle Data Group], Phys
S. Navaset al.[Particle Data Group], Phys. Rev. D110(2024) no.3, 030001
2024
-
[59]
Schaelet al.[ALEPH, DELPHI, L3, OPAL and LEP Electroweak], Phys
S. Schaelet al.[ALEPH, DELPHI, L3, OPAL and LEP Electroweak], Phys. Rept. 532(2013), 119-244 [arXiv:1302.3415 [hep-ex]]
2013 arXiv
-
[60]
Crivellin, M
A. Crivellin, M. Kirk, T. Kitahara and F. Mescia, JHEP03(2023), 234 [arXiv:2212.06862 [hep-ph]]; M. Kirk, Phys. Rev. D103(2021) no.3, 035004 [arXiv:2008.03261 [hep-ph]]
2023 arXiv
-
[61]
Cirigliano, W
V. Cirigliano, W. Dekens, J. de Vries, E. Mereghetti and T. Tong, JHEP03(2024), 033 [arXiv:2311.00021 [hep-ph]]
2024 arXiv
-
[62]
A. M. Coutinho, A. Crivellin and C. A. Manzari, Phys. Rev. Lett.125(2020) no.7, 071802 [arXiv:1912.08823 [hep-ph]]; A. Crivellin, F. Kirk, C. A. Manzari and M. Montull, JHEP12(2020), 166 [arXiv:2008.01113 [hep-ph]]
2020 arXiv
-
[63]
Belfatto and Z
B. Belfatto and Z. Berezhiani, JHEP10(2021), 079 [arXiv:2103.05549 [hep-ph]]; G. C. Branco, J. T. Penedo, P. M. F. Pereira, M. N. Rebelo and J. I. Silva- Marcos, JHEP07(2021), 099 [arXiv:2103.13409 [hep-ph]]; K. Cheung, W. Y. Keung, C. T. Lu and P. Y. Tseng, JHEP05(2020), 117 ...
2021 arXiv
-
[64]
Aokiet al.[Flavour Lattice Averaging Group (FLAG)], Eur
Y. Aokiet al.[Flavour Lattice Averaging Group (FLAG)], Eur. Phys. J. C82(2022) no.10, 869 [arXiv:2111.09849 [hep-lat]]
2022 arXiv
-
[65]
Di Carlo, D
M. Di Carlo, D. Giusti, V. Lubicz, G. Martinelli, C. T. Sachrajda, F. Sanfilippo, S. Simula and N. Tantalo, Phys. Rev. D100(2019) no.3, 034514 [arXiv:1904.08731 [hep-lat]]
2019 arXiv
-
[66]
Giusti, V
D. Giusti, V. Lubicz, G. Martinelli, C. T. Sachrajda, F. Sanfilippo, S. Simula, N. Tan- talo and C. Tarantino, Phys. Rev. Lett.120(2018) no.7, 072001 [arXiv:1711.06537 [hep-lat]]; A. Desiderio, R. Frezzotti, M. Garofalo, D. Giusti, M. Hansen, V. Lubicz, G. Martinelli, C. T. Sa...
2018 arXiv
-
[67]
R. J. Dowdall, C. T. H. Davies, G. P. Lepage and C. McNeile, Phys. Rev. D 88(2013), 074504 [arXiv:1303.1670 [hep-lat]]; A. Bazavov, C. Bernard, N. Brown, C. Detar, A. X. El-Khadra, E. G´ amiz, S. Gottlieb, U. M. Heller, J. Komijani and A. S. Kronfeld,et al.Phys. Rev. D98(2018)...
2013 arXiv
-
[68]
Bonaet al.[UTfit], Rend
M. Bonaet al.[UTfit], Rend. Lincei Sci. Fis. Nat.34(2023), 37-57 [arXiv:2212.03894 [hep-ph]]
2023 arXiv
-
[69]
Charleset al.[CKMfitter Group], Eur
J. Charleset al.[CKMfitter Group], Eur. Phys. J. C41(2005) no.1, 1-131 [arXiv:hep- ph/0406184 [hep-ph]]
2005
-
[70]
Bryman, W
D. Bryman, W. J. Marciano, R. Tschirhart and T. Yamanaka, Ann. Rev. Nucl. Part. Sci.61(2011), 331-354
2011
-
[71]
Cirigliano, A
V. Cirigliano, A. Falkowski, M. Gonz´ alez-Alonso and A. Rodr ´ ıguez-S´ anchez, Phys. Rev. Lett.122(2019) no.22, 221801 [arXiv:1809.01161 [hep-ph]]; V. Cirigliano, D. D ´ ıaz-Calder´ on, A. Falkowski, M. Gonz´ alez-Alonso and A. Rodr ´ ıguez-S´ anchez, JHEP04(2022), 152 [arXi...
2019 arXiv
-
[72]
Antonelliet al.[FlaviaNet Working Group on Kaon Decays], Eur
M. Antonelliet al.[FlaviaNet Working Group on Kaon Decays], Eur. Phys. J. C69 (2010), 399-424 [arXiv:1005.2323 [hep-ph]]
2010 arXiv
-
[73]
W. J. Marciano and A. Sirlin, Phys. Rev. Lett.71(1993), 3629-3632; A. Sirlin, Rev. Mod. Phys.50(1978), 573 [erratum: Rev. Mod. Phys.50(1978) no.4, 905]
1993
-
[74]
C. Y. Seng, D. Galviz, M. Gorchtein and U. G. Meißner, JHEP07(2022), 071 [arXiv:2203.05217 [hep-ph]]; C. Y. Seng, D. Galviz, W. J. Marciano and U. G. Meißner, Phys. Rev. D105(2022) no.1, 013005 [arXiv:2107.14708 [hep-ph]]
2022 arXiv
-
[75]
Carrasco, P
N. Carrasco, P. Lami, V. Lubicz, L. Riggio, S. Simula and C. Tarantino, Phys. Rev. D93(2016) no.11, 114512 [arXiv:1602.04113 [hep-lat]]
2016 arXiv
-
[76]
Aokiet al.[Flavour Lattice Averaging Group (FLAG)], [arXiv:2411.04268 [hep- lat]]
Y. Aokiet al.[Flavour Lattice Averaging Group (FLAG)], [arXiv:2411.04268 [hep- lat]]
-
[77]
Bazavovet al.[Fermilab Lattice and MILC], Phys
A. Bazavovet al.[Fermilab Lattice and MILC], Phys. Rev. D99(2019) no.11, 114509 [arXiv:1809.02827 [hep-lat]]
2019 arXiv
-
[78]
Moulson, PoSCKM2016(2017), 033 [arXiv:1704.04104 [hep-ex]]
M. Moulson, PoSCKM2016(2017), 033 [arXiv:1704.04104 [hep-ex]]
2017 arXiv
-
[79]
Beˇ cirevi´ c, F
D. Beˇ cirevi´ c, F. Jaffredo, A. Pe˜ nuelas and O. Sumensari, JHEP05(2021), 175 [arXiv:2012.09872 [hep-ph]]
2021 arXiv
-
[80]
Falkowski, M
A. Falkowski, M. Gonz´ alez-Alonso and O. Naviliat-Cuncic, JHEP04(2021), 126 [arXiv:2010.13797 [hep-ph]]
2021 arXiv
-
[81]
Czarnecki, W
A. Czarnecki, W. J. Marciano and A. Sirlin, Phys. Rev. Lett.120(2018) no.20, 202002 [arXiv:1802.01804 [hep-ph]]
2018 arXiv
-
[82]
C. Y. Seng, M. Gorchtein, H. H. Patel and M. J. Ramsey-Musolf, Phys. Rev. Lett. 121(2018) no.24, 241804 [arXiv:1807.10197 [hep-ph]]. 33
2018 arXiv
-
[83]
Gorchtein and C
M. Gorchtein and C. Y. Seng, JHEP10(2021), 053 [arXiv:2106.09185 [hep-ph]]
2021 arXiv
-
[84]
I. S. Towner and J. C. Hardy, Rept. Prog. Phys.73(2010), 046301
2010
-
[85]
F. M. Gonzalezet al.[UCNτ], Phys. Rev. Lett.127(2021) no.16, 162501 [arXiv:2106.10375 [nucl-ex]]
2021 arXiv
-
[86]
J. C. Hardy and I. S. Towner, Phys. Rev. C102(2020) no.4, 045501
2020
-
[87]
Becirevic, M
D. Becirevic, M. Martines, O. Sumensari, S. Rosauro-Alcaraz,In preparation
-
[88]
[ATLAS], ATL-PHYS-PUB-2025-012
2025
-
[89]
Aadet al.[ATLAS], Phys
G. Aadet al.[ATLAS], Phys. Rev. D110(2024) no.5, 052009 [arXiv:2405.19862 [hep-ex]]; A. Hayrapetyanet al.[CMS], Phys. Rept.1115(2025), 570-677 [arXiv:2405.17605 [hep-ex]]
2024 arXiv
-
[90]
I. Baum, V. Lubicz, G. Martinelli, L. Orifici and S. Simula, Phys. Rev. D84(2011), 074503 [arXiv:1108.1021 [hep-lat]]. 34
2011 arXiv
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