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REVIEW 4 major objections 5 minor 72 references

Prospects for probing light photophobic axion-like particles via displaced vertex signals at the CEPC

T0 review · 4 major / 5 minor · reviewed 2026-08-02 · deepseek-v4-flash

Pith's one-line read At a future Z-pole electron-positron collider, long-lived 'photophobic' axion-like particles could be discovered through displaced vertices produced in Z→aγ decays, covering unexplored regions of mass and coupling.

desk verdict A useful but unvalidated CEPC sensitivity projection for photophobic ALPs via displaced vertices; the zero-background assumption is explicit and the dimuon upper edge looks off by an order of magnitude. read the letter →

arxiv 2603.13746 v3 pith:KMAOPP2V submitted 2026-03-14 hep-ph

classification hep-ph
keywords axion-likeparticlesphotophobicALPlong-liveddisplacedverticesZpoleCEPCleptoncolliderelectroweakcouplings
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper argues that a Z-pole electron-positron collider running at 91.2 GeV with very high integrated luminosity can discover light, long-lived axion-like particles that have no direct couplings to photons or fermions. Such 'photophobic' ALPs, if lighter than about 10 GeV, decay through loop-induced couplings and thus travel macroscopic distances before decaying. By focusing on the dominant production channel Z→aγ followed by a→μ+μ− or a→τ+τ−, the displaced vertex inside the inner tracker becomes a nearly background-free signature. With 100 ab−1 of data, the proposed collider could probe ALP–W couplings between roughly 10−4 and 10−1 TeV−1 for ALP masses of 1–9 GeV, a parameter region that existing collider searches do not cover.

What carries the argument

The central object is the photophobic ALP: an axion-like particle whose tree-level couplings to photons and fermions vanish, leaving only couplings to electroweak gauge bosons (W, Z, Zγ). After electroweak symmetry breaking, the scenario reduces to two parameters: the ALP mass m_a and the coupling g_aWW. The effective fermion and photon couplings are generated by one-loop renormalization-group running, which suppresses the total decay width and lengthens the proper decay length. The search exploits the observables |d_0| (transverse impact parameter), v_0 and v_z (vertex displacement), ΔR between the two leptons, and the transverse momentum of the dilepton system to separate the boosted, long

What would settle it

Run a detector-level simulation of the Z-pole environment, including pile-up and track reconstruction, and count background events passing the full cut set (|d0| > 2 mm, 0.1 m < v0 < 1.8 m, vz < 2.35 m, ΔR < 1.0, and dilepton pT > 25 GeV for muons or > 30 GeV for taus); if any background event survives, the projected 95% CL regions are optimistic.

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Extended reading notes

Core claim

At the heart of the paper is the observation that photophobic ALPs — axion-like particles with no tree-level coupling to photons or fermions — can be produced at the Z pole via Z→aγ, then decay into charged leptons through loop-induced couplings. Because those couplings are small, the ALP travels a macroscopic distance before decaying, creating a displaced vertex that is essentially background-free after moderate cuts. The authors simulate the μ+μ−γ and τh+τh− E_T^miss γ signals and derive 95% CL sensitivities: g_aWW ∈ [1.27×10−3, 0.68] TeV−1 for m_a ∈ [1,4] GeV and g_aWW ∈ [7×10−4, 9.4×10−3] TeV−1 for m_a ∈ [4,9] GeV. These regions are presented as new ground, uncovered by existing collider

Load-bearing premise

The entire sensitivity projection rests on the assumption that after the chosen cuts, pile-up, random-track crossings, and other instrumental backgrounds are negligible; if even one such event survives in 100 ab−1, the 3-event benchmark for the 95% CL limit no longer holds.

Editorial extensions

If this is right

  • A Z-pole electron-positron collider with 100 ab−1 can probe photophobic ALP couplings down to about 10−4 TeV−1 for masses 4–9 GeV and about 10−3 TeV−1 for masses 1–4 GeV.
  • The dimuon and ditau channels together give continuous mass coverage from 1 to 9 GeV, with no branching-ratio gaps below the b-quark threshold.
  • The sensitivity is achieved using only inner-tracker information, so the search does not rely on calorimeter or muon-system capabilities.
  • The projected regions extend into parameter space that is complementary to existing hadron-collider and rare-meson-decay searches, so a positive signal would be a new discovery rather than a confirmation.
  • The same production and displacement logic applies to any proposed Z-pole lepton collider, so the method provides a blueprint for comparable facilities.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • A full detector-level simulation including pile-up and random-track crossings is the natural next step; any surviving background would shrink the quoted regions, especially at the weak-coupling (long-lifetime) boundary where the signal is diluted across larger volumes.
  • Because the effective fermion couplings are computed at a fixed cutoff scale f_a = 10 TeV, the sensitivity bands are tied to that choice; scanning over f_a would show how the boundaries move as the lifetime changes.
  • Extending the vertex search from the inner tracker to the calorimeters or muon system would add sensitivity to shorter and longer lifetimes, respectively; the paper explicitly leaves those options open.
  • The results suggest that a dedicated displaced-vertex search at the Z pole could be mounted with relatively modest detector requirements, which may influence design choices for future electron-positron colliders.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

4 major / 5 minor

Summary. This paper studies the discovery potential of the CEPC (a 91.2 GeV electron-positron collider with 100 ab^-1) for light, long-lived photophobic axion-like particles (ALPs). The authors adopt the photophobic ALP EFT in which the ALP couples only to electroweak gauge bosons at tree level, with loop-induced couplings to fermions and photons. They compare single-production channels, identify e+e- -> Z -> a gamma as dominant, and simulate the displaced-vertex signals from a -> mu+ mu- and a -> tau+ tau- (with hadronic tau decays), using MadGraph5_aMC@NLO, PYTHIA8, and a simplified fast simulation. Optimized cuts on displacement variables, angular separation, and the reconstructed ALP transverse momentum are applied. With the assumption that SM and instrumental backgrounds are negligible after all cuts, the authors use a 3-event benchmark for 95% C.L. sensitivity and report reachable regions: g_aWW in [1.27e-3, 6.80e-1] TeV^-1 for m_a in [1,4] GeV from the dimuon channel, and g_aWW in [7.00e-4, 9.40e-3] TeV^-1 for m_a in [4,9] GeV from the ditau channel. The paper argues these regions complement existing LEP, LHC, LHCb, and CHARM bounds and the projected HL-LHC sensitivity.

Significance. If the projected reach is correct, this would be a useful and nontrivial result: the CEPC would probe photophobic ALP parameter space not covered by current experiments, and the analysis demonstrates a concrete DV search strategy for a future Z-factory. The study uses state-of-the-art Monte Carlo tools (FeynRules/MadGraph/PYTHIA/MadAnalysis5), presents production cross sections and cut-flow efficiencies, and compares with a broad set of existing constraints. The main weakness is that the central sensitivity claim rests on an unvalidated zero-background assumption: after the displacement cuts, the SM prompt background is eliminated by construction, and the paper explicitly assumes instrumental backgrounds are negligible without a detector-level study. The projected low-edge couplings are therefore conditional on this assumption and cannot be taken as demonstrated without further quantification. This is a correctable issue, but it is load-bearing for the headline numbers.

major comments (4)
  1. [Sec. III A, Tables II and III] The paper states that after all optimized cuts 'the SM background is expected to be suppressed to a negligible level,' but no background event counts or cross sections after each cut are reported. Only signal cross sections and efficiencies are given in Tables II and III. This matters quantitatively: with L = 100 ab^-1, a background cross section of 10^-11 pb gives O(1) background events, so the 3-event 95% C.L. benchmark requires that the residual background is below roughly 10^-11 pb. The authors must report the expected number of SM background events (for e+e- -> mu+mu- gamma and e+e- -> tau+tau- gamma) at each cut step, or at least give the final background count, to justify the zero-background assumption.
  2. [Sec. III A, paragraph on instrumental backgrounds] The manuscript explicitly states that instrumental backgrounds such as pile-up interactions, vertices from dense detector regions, and random-track crossings are 'beyond the scope of this study' and are assumed negligible. This is a load-bearing assumption for the quoted sensitivity: the displacement cuts reject prompt SM background by construction, so the only remaining protection against fake displaced vertices is the assumed negligible instrumental rate. With O(10^12) Z decays and 100 ab^-1, even a fractional fake rate of ~10^-9 yields O(1) events. The authors need a quantitative estimate based on CEPC occupancy, vertexing efficiency, and track-fake probabilities, or a conservative background uncertainty, before the 3-event sensitivity can be considered robust.
  3. [Sec. II, Eq. (5) and Eq. (9); Fig. 9] The sensitivity boundaries in Fig. 9 depend on the ALP lifetime, but the paper never gives the explicit formula for the total ALP width Gamma_a entering Eq. (9). The branching fractions shown in Fig. 1 are insufficient to reproduce the results; the reader needs the sum of the loop-induced partial widths (a -> f fbar, a -> gamma gamma, etc.). In addition, the effective fermion couplings in Eq. (5) depend on the assumed cutoff scale Lambda = 4 pi f_a with f_a fixed to 10 TeV. Since the sensitivity regions are quoted as functions of (m_a, g_aWW) only, the dependence of the lifetime and hence of the projected boundaries on the choice of f_a should be stated explicitly.
  4. [Sec. III, simplified fast simulation (SFS)] The SFS framework does not include full detector-level reconstruction of displaced vertices: there is no material interaction model, no vertex-fitter efficiency, and no track-fake reconstruction. The signal efficiencies in Tables II and III are obtained by applying geometric cuts on generator-level quantities (|d0|, v0, vz). Since the signal is concentrated near the tracker boundaries (e.g., 0.1 m < v0 < 1.8 m, vz < 2.35 m), detector resolution, material effects, and reconstruction inefficiencies can significantly modify these efficiencies. The authors should validate the key efficiencies with a more realistic detector simulation, or at least provide an efficiency correction/uncertainty estimate.
minor comments (5)
  1. [Sec. I] 'owning to' should be 'owing to' in the sentence about the clean experimental environment.
  2. [Eq. (4)] The second relation in Eq. (4) appears typeset incorrectly ('c2W/c2W'); if intended, it should be gaZZ = (c_W^2 / s_W^2) g_aWW. Please correct the rendering.
  3. [Sec. III A] The phrase 'with the number cuts being taken as the first step filter' is unclear; rephrase.
  4. [Figs. 1 and 9] The arXiv rendering of Figs. 1 and 9 is badly garbled (e.g., the legend text in Fig. 9 is scrambled). The published-quality figures need to be readable, with all curves and regions clearly labeled.
  5. [Sec. III B and IV] The statement that for m_a above the b bbar threshold 'no accessible parameter space' remains for long-lived ALPs is asserted without a quantitative lifetime/cut-efficiency demonstration. A short quantitative explanation would strengthen the argument.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the CEPC sensitivity is a forward Monte Carlo projection from an EFT, with no data fitting and no load-bearing self-citation.

full rationale

The paper's central derivation is self-contained: it takes the photophobic ALP effective Lagrangian (Eq. (1)), obtains loop-induced couplings via standard RGE and one-loop formulas (Eqs. (5)-(6)), computes production cross sections and decay lengths from those couplings, and then uses MadGraph/PYTHIA/fast simulation to obtain signal efficiencies and cross sections. The projected 95% C.L. regions are obtained by counting signal events after cuts with N_sig = 3, with no parameter fitted to any data subset and no 'prediction' that is equivalent to a fitted input by construction. The only self-citation is Ref. [72], the authors' own HL-LHC projection, which is used solely as a comparison region in Fig. 9 and in the concluding claim of complementarity; it is not an input to the CEPC signal or background calculation, so it is not load-bearing. The paper explicitly states two assumptions that limit the numeric reach but do not make the derivation circular: instrumental backgrounds (pile-up, random-track crossings, dense-detector-region vertices) are assumed negligible and deferred to future detector-level simulation (Sec. III A), and the cutoff is fixed at f_a = 10 TeV (Sec. II). These are stated modeling assumptions, not hidden redefinitions or fitted results. The SM backgrounds e+e- -> mu+mu- gamma and e+e- -> tau+tau- gamma are simulated and removed by the displacement cuts, which is a standard cut-and-count procedure rather than a circular reduction. Overall, no circular step is exhibited.

Assumptions & free parameters 2 free parameters · 6 assumptions · 0 invented entities

The central claim rests on the photophobic ALP model plus a set of loop-induced coupling formulas taken from the literature, a chosen f_a, a fast detector simulation, and the assumption of negligible non-irreducible backgrounds. The main free input is f_a=10 TeV; the sensitivity is nominally a function of g_aWW and m_a only.

free parameters (2)
  • f_a (ALP decay constant) = 10 TeV
    Chosen by hand; sets the UV scale Λ=4π f_a in the RGE logs of Eq. (5) and therefore the loop-induced ALP-fermion couplings and lifetime. The quoted sensitivity ranges are not mapped in f_a.
  • Optimized cut thresholds = |d0|>2 mm; 0.1 m<v0<1.8 m; vz<2.35 m; ΔR<1; pT>25 GeV (muon), pT>30 GeV (tau)
    Hand-chosen using the signal/background distributions in Figs. 6 and 8; not validated on a separate sample and directly affect which couplings pass the displaced-vertex requirement.
assumptions (6)
  • domain assumption Photophobic boundary conditions: no tree-level couplings of the ALP to photons, fermions, or gluons
    Taken from the photophobic ALP scenario (Ref. [49]); defines the model. Entered in Sec. II after Eq. (1).
  • domain assumption The one-loop RGE formula of Eq. (5) correctly gives the low-energy ALP-fermion couplings
    Imported from Refs. [57,58] for Λ=4π f_a with f_a=10 TeV; not derived in this paper and not validated by an independent calculation here.
  • domain assumption The ALP decays only into SM final states; no invisible or exotic decays
    Total width Γ_a is computed from SM loop channels; if additional ALP decay modes exist, the lifetime changes and the sensitivity regions shrink.
  • domain assumption CEPC inner tracker geometry and performance as implemented in the SFS fast simulation are adequate
    No full Geant4 simulation; vertex reconstruction efficiency, material effects, and track reconstruction efficiency are taken from the simplified framework.
  • ad hoc to paper Instrumental backgrounds are negligible after the optimized cuts
    The paper states that a quantitative assessment requires dedicated detector simulation, which is beyond scope; the results assume these backgrounds are negligible (Sec. III A).
  • ad hoc to paper The SM backgrounds considered (μ+μ−γ and τ+τ−γ) are the only relevant ones
    Other processes at the Z pole (e.g., multi-jets, WW, ZZ) are not evaluated.

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Pith. "Pith review of Prospects for probing light photophobic axion-like particles via displaced vertex signals at the CEPC." pith.science (2026). https://pith.science/paper/KMAOPP2V

@misc{pith2026260313746,
  author       = {Pith},
  title        = {Pith review of: Prospects for probing light photophobic axion-like particles via displaced vertex signals at the CEPC},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/KMAOPP2V}},
  note         = {Machine review of arXiv:2603.13746}
}
abstract

In recent years, long-lived particles (LLPs) have attracted increasing attention in searches for physics beyond the Standard Model (SM). In this paper, we investigate the discovery prospects for light, long-lived ALPs predicted by the photophobic ALP scenario through displaced-vertex signals at the CEPC, with a center-of-mass energy of $\sqrt{s}=91.2 $ GeV and an integrated luminosity of $\mathcal{L}=$ $100$ ab$^{-1}$. After comparing several possible single-production processes for the photophobic ALP, we focus on the dominant process $e^+ e^- \to Z \to a \gamma $, in which the ALP $a$ subsequently decays into a pair of charged leptons at a displaced vertex. Dedicated Monte Carlo simulations are performed for the $\mu^+ \mu^- \gamma$ and $\tau_h^+ \tau_h^- E\mkern-10.5 mu/_T \gamma$ signals. For the $\mu^+\mu^-\gamma$ signal, the CEPC is sensitive to the parameter region $g_{aWW} \in [1.27\times10^{-3},6.80\times10^{-1}]~\mathrm{TeV}^{-1}$ for $m_a \in [1,4]~\mathrm{GeV}$. For the $\tau_h^+\tau_h^- E\mkern-10.5 mu/_T \gamma$ signal, the accessible region is $g_{aWW} \in [7.00\times10^{-4},9.40\times10^{-3}]~\mathrm{TeV}^{-1}$ for $m_a \in [4,9]~\mathrm{GeV}$. These results demonstrate the substantial potential of the CEPC to explore light, long-lived ALPs through displaced-vertex signals, providing complementary coverage to existing searches at LEP and the LHC, as well as to the projected reach of the HL-LHC.

Figures

Figures reproduced from arXiv: 2603.13746 by the authors.

Figure 1
Figure 1. FIG. 1: The branching ratios of different photophobic ALP decay modes as functions of its [PITH_FULL_IMAGE:figures/full_fig_p006_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2: The proper decay length of the ALP as functions of its mass [PITH_FULL_IMAGE:figures/full_fig_p007_2.png] view at source ↗
Figure 3
Figure 3. FIG. 3: The Feynman diagrams for the single-production processes of the photophobic ALP, [PITH_FULL_IMAGE:figures/full_fig_p009_3.png] view at source ↗
Figures from the paper (6 more)
Figure 4
Figure 4. Figure 4: FIG. 4: The production cross sections of the processes [PITH_FULL_IMAGE:figures/full_fig_p009_4.png]
Figure 5
Figure 5. Figure 5: FIG. 5: The production cross sections of the [PITH_FULL_IMAGE:figures/full_fig_p011_5.png]
Figure 6
Figure 6. Figure 6: FIG. 6: The normalized distributions of [PITH_FULL_IMAGE:figures/full_fig_p012_6.png]
Figure 7
Figure 7. Figure 7: FIG. 7: Same as Fig. 5 but for the [PITH_FULL_IMAGE:figures/full_fig_p015_7.png]
Figure 8
Figure 8. Figure 8: FIG. 8: Same as Fig. 6 but for the observables [PITH_FULL_IMAGE:figures/full_fig_p016_8.png]
Figure 9
Figure 9. Figure 9: FIG. 9: Our projected [PITH_FULL_IMAGE:figures/full_fig_p018_9.png]

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Works this paper leans on

72 extracted references · 51 linked inside Pith

  1. [55]

    Wang, Y .-P

    S.-Y . Wang, Y .-P. Jiao, H.-H. Zhang, and G. Cacciapaglia (2025), 2509.17718

  2. [1]

    M. C. Gonzalez-Garcia and M. Maltoni, Phys. Rept. 460, 1 (2008), 0704.1800

  3. [2]

    Bertone, D

    G. Bertone, D. Hooper, and J. Silk, Phys. Rept. 405, 279 (2005), hep-ph/0404175

  4. [3]

    K. R. Dienes and B. Thomas, Phys. Rev. D 85, 083523 (2012), 1106.4546

  5. [4]

    R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38, 1440 (1977)

  6. [5]

    R. D. Peccei and H. R. Quinn, Phys. Rev. D 16, 1791 (1977)

  7. [6]

    Wilczek, Phys

    F. Wilczek, Phys. Rev. Lett. 40, 279 (1978)

  8. [7]

    J. L. Feng, Ann. Rev. Nucl. Part. Sci. 63, 351 (2013), 1302.6587

Show all 72 references
  1. [8]

    Lanfranchi, M

    G. Lanfranchi, M. Pospelov, and P. Schuster, Ann. Rev. Nucl. Part. Sci.71, 279 (2021), 2011.02157

  2. [9]

    Antel et al., Eur

    C. Antel et al., Eur. Phys. J. C 83, 1122 (2023), 2305.01715

  3. [10]

    Jeanty and B

    L. Jeanty and B. Shuve (2025), 2511.17934

  4. [11]

    Aaboud et al

    M. Aaboud et al. (ATLAS), Phys. Rev. D 99, 012001 (2019), 1808.03057

  5. [12]

    Aad et al

    G. Aad et al. (ATLAS), Phys. Lett. B 801, 135114 (2020), 1907.10037

  6. [13]

    Aad et al

    G. Aad et al. (ATLAS), JHEP 06, 200 (2023), 2301.13866

  7. [14]

    Aad et al

    G. Aad et al. (ATLAS), Phys. Rev. D 102, 032006 (2020), 2003.11956

  8. [15]

    Aad et al

    G. Aad et al. (ATLAS), Eur. Phys. J. C 80, 450 (2020), 1909.01246

  9. [16]

    Aaboud et al

    M. Aaboud et al. (ATLAS), Phys. Rev. D 99, 052005 (2019), 1811.07370

  10. [17]

    Aad et al

    G. Aad et al. (ATLAS), Phys. Rev. D 101, 052013 (2020), 1911.12575

  11. [18]

    Aad et al

    G. Aad et al. (ATLAS), Phys. Rev. D 106, 032005 (2022), 2203.00587

  12. [19]

    Aad et al

    G. Aad et al. (ATLAS), JHEP 06, 005 (2022), 2203.01009

  13. [20]

    Aad et al

    G. Aad et al. (ATLAS), JHEP 11, 229 (2021), 2107.06092

  14. [21]

    Aaboud et al

    M. Aaboud et al. (ATLAS), JHEP 10, 031 (2018), 1806.07355

  15. [22]

    Tumasyan et al

    A. Tumasyan et al. (CMS), JHEP 05, 228 (2023), 2205.08582

  16. [23]

    Tumasyan et al

    A. Tumasyan et al. (CMS), JHEP 04, 062 (2022), 2112.13769

  17. [24]

    A. M. Sirunyan et al. (CMS), Phys. Rev. D 104, 052011 (2021), 2104.13474

  18. [25]

    A. M. Sirunyan et al. (CMS), Phys. Rev. D 104, 012015 (2021), 2012.01581

  19. [26]

    Tumasyan et al

    A. Tumasyan et al. (CMS), JHEP 03, 160 (2022), 2110.13218

  20. [27]

    Aaij et al

    R. Aaij et al. (LHCb), Eur. Phys. J. C 77, 812 (2017), 1705.07332. 20

  21. [28]

    Aaij et al

    R. Aaij et al. (LHCb), Eur. Phys. J. C 76, 664 (2016), 1609.03124

  22. [29]

    Dong et al

    M. Dong et al. (CEPC Study Group) (2018), 1811.10545

  23. [30]

    Abdallah et al

    W. Abdallah et al. (CEPC Study Group), Radiat. Detect. Technol. Methods 8, 1 (2024), [Erratum: Radiat.Detect.Technol.Methods 9, 184–192 (2025)], 2312.14363

  24. [31]

    Abada et al

    A. Abada et al. (FCC), Eur. Phys. J. ST 228, 261 (2019)

  25. [32]

    Benedikt et al

    M. Benedikt et al. (FCC), Eur. Phys. J. C 85, 1468 (2025), 2505.00272

  26. [33]

    Gao (CEPC Accelerator Study Group) (2022), 2203.09451

    J. Gao (CEPC Accelerator Study Group) (2022), 2203.09451

  27. [34]

    Cheung and Z

    K. Cheung and Z. S. Wang, Phys. Rev. D 101, 035003 (2020), 1911.08721

  28. [35]

    Z. S. Wang and K. Wang, Phys. Rev. D 101, 115018 (2020), 1904.10661

  29. [36]

    Alipour-Fard, N

    S. Alipour-Fard, N. Craig, M. Jiang, and S. Koren, Chin. Phys. C 43, 053101 (2019), 1812.05588

  30. [37]

    Q.-H. Cao, J. Guo, J. Liu, Y . Luo, and X.-P. Wang, Phys. Rev. D110, 015029 (2024), 2311.12934

  31. [38]

    R. G. Suarez, Acta Phys. Polon. B 52, 953 (2021), 2102.07597

  32. [39]

    Zhang, C

    Y . Zhang, C. Mo, X. Chen, B. Li, H. Chen, J. Hu, and L. Li, Front. Phys. (Beijing) 21, 056202 (2026), 2401.05094

  33. [40]

    Blondel et al., Front

    A. Blondel et al., Front. in Phys. 10, 967881 (2022), 2203.05502

  34. [41]

    K. A. Urqu ´ıa-Calder´on, Phys. Rev. D 109, 055002 (2024), 2310.17406

  35. [42]

    Chrzaszcz, R

    M. Chrzaszcz, R. G. Suarez, and S. Monteil, Eur. Phys. J. Plus 136, 1056 (2021), 2106.15459

  36. [43]

    J. E. Kim, Phys. Rev. Lett. 43, 103 (1979)

  37. [44]

    M. A. Shifman, A. I. Vainshtein, and V . I. Zakharov, Nucl. Phys. B166, 493 (1980)

  38. [45]

    M. Dine, W. Fischler, and M. Srednicki, Phys. Lett. B 104, 199 (1981)

  39. [46]

    A. R. Zhitnitsky, Sov. J. Nucl. Phys. 31, 260 (1980)

  40. [47]

    A. A. Anselm and N. G. Uraltsev, Phys. Lett. B 114, 39 (1982)

  41. [48]

    Ringwald, in 49th Rencontres de Moriond on Electroweak Interactions and Unified Theories (2014), pp

    A. Ringwald, in 49th Rencontres de Moriond on Electroweak Interactions and Unified Theories (2014), pp. 223–230, 1407.0546

  42. [49]

    Craig, A

    N. Craig, A. Hook, and S. Kasko, JHEP 09, 028 (2018), 1805.06538

  43. [50]

    M. Aiko, M. Endo, and K. Fridell, JHEP 06, 194 (2024), 2401.13323

  44. [51]

    Ding, Y .-n

    Z. Ding, Y .-n. Mao, and K. Wang, JHEP06, 087 (2025), 2411.08660

  45. [52]

    Y .-n. Mao, K. Wang, and Y . Xiong, Chin. Phys. C49, 083106 (2025), 2411.14041

  46. [53]

    Feng, Y .-n

    J. Feng, Y .-n. Mao, and K. Wang (2025), 2511.21003

  47. [54]

    Z. Ding, J. Feng, Y .-n. Mao, K. Wang, and Y . Xiong (2025), 2512.23155. 21

  48. [56]

    Georgi, D

    H. Georgi, D. B. Kaplan, and L. Randall, Phys. Lett. B 169, 73 (1986)

  49. [57]

    Bauer, M

    M. Bauer, M. Neubert, and A. Thamm, JHEP 12, 044 (2017), 1708.00443

  50. [58]

    Bauer, M

    M. Bauer, M. Neubert, S. Renner, M. Schnubel, and A. Thamm, JHEP04, 063 (2021), 2012.12272

  51. [59]

    Bonilla, I

    J. Bonilla, I. Brivio, M. B. Gavela, and V . Sanz, JHEP 11, 168 (2021), 2107.11392

  52. [60]

    Alloul, N

    A. Alloul, N. D. Christensen, C. Degrande, C. Duhr, and B. Fuks, Comput. Phys. Commun. 185, 2250 (2014), 1310.1921

  53. [61]

    Alwall, R

    J. Alwall, R. Frederix, S. Frixione, V . Hirschi, F. Maltoni, O. Mattelaer, H. S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, JHEP07, 079 (2014), 1405.0301

  54. [62]

    Sj ¨ostrand, S

    T. Sj ¨ostrand, S. Ask, J. R. Christiansen, R. Corke, N. Desai, P. Ilten, S. Mrenna, S. Prestel, C. O. Rasmussen, and P. Z. Skands, Comput. Phys. Commun. 191, 159 (2015), 1410.3012

  55. [63]

    J. Y . Araz, B. Fuks, and G. Polykratis, Eur. Phys. J. C 81, 329 (2021), 2006.09387

  56. [64]

    Conte, B

    E. Conte, B. Fuks, and G. Serret, Comput. Phys. Commun. 184, 222 (2013), 1206.1599

  57. [65]

    Conte, B

    E. Conte, B. Dumont, B. Fuks, and C. Wymant, Eur. Phys. J. C 74, 3103 (2014), 1405.3982

  58. [66]

    Conte and B

    E. Conte and B. Fuks, Int. J. Mod. Phys. A 33, 1830027 (2018), 1808.00480

  59. [67]

    Aaij et al

    R. Aaij et al. (LHCb), Phys. Rev. D 95, 071101 (2017), 1612.07818

  60. [68]

    Aaij et al

    R. Aaij et al. (LHCb), Phys. Rev. Lett. 115, 161802 (2015), 1508.04094

  61. [69]

    Bergsma et al

    F. Bergsma et al. (CHARM), Phys. Lett. B 157, 458 (1985)

  62. [70]

    P. D. Acton et al. (OPAL), Phys. Lett. B 311, 391 (1993)

  63. [71]

    Adriani et al

    O. Adriani et al. (L3), Phys. Lett. B 292, 472 (1992)

  64. [72]

    Yue, X.-Y

    C.-X. Yue, X.-Y . Li, S. Yang, and M.-S.-Y . Wang, Eur. Phys. J. C85, 1442 (2025), 2510.24097. 22

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Reviewed August 2, 2026 · model on record in the stance chip above.