REVIEW 3 major objections 4 minor 2 cited by
The production and decay of $X_0(2900)$ state with different interpretation
T0 review · 3 major / 4 minor · reviewed 2026-08-11 · deepseek-v4-flash
Pith's one-line read The X0(2900) state's production and decay both match a D* K* molecule interpretation, computed from QCD sum rules and final-state rescattering.
desk verdict A useful QCD sum rule + FSI calculation of X0(2900) production that moderately favors the D*K* molecule, but the central consistency claim leans heavily on long, unvalidated vertex extrapolations. 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 object is the set of strong coupling constants $g_{ABC}(Q^2)$ at hadronic vertices, computed from three-point QCD sum rules and then extrapolated from the Euclidean momentum region where the sum rule is valid ($Q^2\sim 3.5$ to $6$ GeV$^2$) to the physical meson pole ($Q^2=-m_K^2$ or $-m_{K^*}^2$) with fitted monopole or exponential forms. These $Q^2$-dependent couplings replace the common monopole form factor, because the sum-rule results do not always follow a monopole curve; the $\bar D^* K^* X_0$ coupling in particular is better described by an exponential. The production amplitude is assembled from eight final-state-interaction rescattering diagrams, with the weak $b\to c(c\bar s)$ transition factorized into known $B\to D^{(*)}$ form factors and meson decay constants. The two largest contributions come from the $D_s^*\bar D\to DX_0$ ($K$ exchange) and $D_{s1}\bar D^*\to DX_0$ ($K^*$ exchange) rescattering processes.
What would settle it
A lattice-QCD computation of the off-shell $\bar D K X_0$ and $\bar D^* K^* X_0$ couplings at the kaon and $K^*$ poles would settle the extrapolation; alternatively, measuring the ratio of $B^0\to D^0 X_0\to D^0\bar D^0 K^0$ to $B^+\to D^+ X_0\to D^+D^-K^+$ would distinguish the molecular-rescattering prediction of equal rates from the triangle-singularity prediction of strong suppression.
Extended reading notes
Core claim
On the paper's own terms, the central result is that the $\bar D^* K^*$ molecular interpretation of $X_0(2900)$ survives a quantitative comparison with experiment. The authors build the production amplitude $B^+\to D^+X_0$ from eight rescattering diagrams in which the weakly produced $c\bar s$ pair hadronizes into $D_s$ or $D_{s1}$ and rescatters off $D$ or $D^*$ mesons by exchanging $K$, $K^*$, $K_1$, or $K_0^*$ mesons. The strong couplings at these vertices are obtained from three-point QCD sum rules, including $g_{\bar D K X_0}$ and $g_{\bar D^* K^* X_0}$. Summing the amplitudes gives $\mathrm{Br}(B^+\to D^+ X_0)=(2.47^{+2.07}_{-1.55})\times 10^{-5}$ and $\Gamma(X_0\to DK)=(64.07\pm 18.23)\,\mathrm{MeV}$ for the molecule, consistent with the measured values of roughly $(2.4\pm 1.0)\times 10^{-5}$ and $(57\pm 12\pm 4)\,\mathrm{MeV}$. The authors also state that the compact tetraquark interpretation cannot be excluded within the uncertainties.
Load-bearing premise
Everything rests on extrapolating the QCD sum-rule vertex couplings, which are computed only at positive momentum transfers around $3.5$ to $6$ GeV$^2$, down to the negative momentum transfer where the exchanged kaon or $K^*$ is on shell; if that extrapolation is not the true behaviour of the vertices, the two largest rescattering amplitudes change and the agreement with experiment is no longer guaranteed.
Editorial extensions
If this is right
- If the molecular interpretation is correct, the observed $X_0(2900)$ is a hadronic molecule rather than a compact four-quark state, and its dominant strong decay into $DK$ follows naturally from the $\bar D^* K^*$ constituents.
- The production rate in $B$ decays is set largely by long-distance rescattering, so measuring $B\to DX_0$ channels probes how the weak-produced $c\bar s$ pair hadronizes before final-state interactions.
- The four cascade channels $B^+\to D^+X_0\to D^+(D^-K^+)$, $B^+\to D^+X_0\to D^+(\bar D^0 K^0)$, $B^0\to D^0 X_0\to D^0(\bar D^0K^0)$, and $B^0\to D^0X_0\to D^0(D^-K^+)$ are predicted to have equal branching fractions, a consequence of factorization combined with $X_0\to DK$ dominance.
- Tighter future measurements of the width and production rate would separate the three interpretations, since the molecular values sit closest to the current central data.
Reading between the lines
- The extrapolation of the sum-rule vertices from positive $Q^2$ to the meson pole is the step the numerical agreement hinges on; a lattice-QCD determination of $g_{\bar D K X_0}$ at the kaon pole would provide a direct check.
- The equal-branching prediction for the $B^+$ and $B^0$ cascade modes is a sharper discriminant between a genuine resonance and a triangle-singularity interpretation than the width alone, because the triangle model is argued in the literature to suppress some of these channels.
- The same QCD-sum-rule-plus-rescattering machinery can be applied to other open-flavor candidates near a $\bar D^{(*)}K^{(*)}$ threshold, making the approach a general test of molecular interpretations.
- A similar analysis of the companion $X_1(2900)$ state, whose larger width remains unexplained here, would show whether the molecular picture extends to the full observed doublet.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies the production and decay of the open-flavor tetraquark candidate X0(2900) using a final-state-interaction rescattering model. Strong vertices such as g_{\bar D K X_0}, g_{\bar D^* K^* X_0}, and the D_s^(**) D K^(**) vertices are computed with three-point QCD sum rules, and the resulting couplings are used in hadronic loop amplitudes for B^+ -> D^+ X_0. For the \bar D^* K^* molecular interpretation, the authors obtain Br(B^+ -> D^+ X_0) = (2.47 +2.07 -1.55) x 10^-5 and \Gamma(X_0 -> \bar D K) = 64.07 ± 18.23 MeV, both consistent with the LHCb values of about (2.4 ± 1.0) x 10^-5 and 57 ± 12 ± 4 MeV. The paper concludes that the molecular interpretation is favored but that the compact tetraquark interpretations cannot be excluded within uncertainties.
Significance. If the extrapolation procedure is robust, the paper provides a valuable comparison of three X0(2900) interpretations within one framework, replacing the ad hoc monopole cutoff of earlier FSI studies with sum-rule-derived vertex functions. It also presents a large set of three-point sum rules and on-shell couplings that can be checked against other approaches. The main significance is the claim of quantitative consistency with LHCb for the molecular scenario, together with an explicit statement that the compact tetraquark is not excluded. This claim, however, currently rests on long and untested off-shell extrapolations of the sum-rule couplings, so the significance is conditional on those extrapolations being validated.
major comments (3)
- [Sec. III A and Sec. IV, Eqs. (42)-(49), (11), (13), and Table V] The couplings g_{\bar D K X_0} and g_{\bar D^* K^* X_0} are extracted only for Q^2 ≳ 3.5-4 GeV^2 and then extrapolated to the physical pole and to the low-Q^2 region using monopole or exponential fits. The FSI loop integrals in Eqs. (11) and (13) sample exchanged momenta with Q^2 = -t ∈ [0.04, 7.98] GeV^2 for diagram (a), and the integrand is largest near Q^2 ≈ 0 where the propagator is smallest. In that region Eq. (42) contains the factor (Q^2 + m_K^2)/Q^2, so the OPE cannot be trusted. Since Table V shows that A_a, A_b, and A_d dominate the branching fraction, an unconstrained change in the low-Q^2 behavior of the vertex functions can shift Br by a large factor. The paper provides no independent check of the monopole/exponential extrapolations, no alternative functional form, and no estimate of this shape uncertainty. This is a load-bearing uncertainty for the central consistency claim.
- [Sec. III A, Eqs. (42) and (47), and s0 input] The continuum threshold s0 = 10 GeV^2 for the X0 vertices is taken from Ref. [38], which shares an author with this paper. The sum-rule results for g_{\bar D K X_0} and g_{\bar D^* K^* X_0} are quoted only for this single s0 value, and no sensitivity study of s0 in the three-point sum rules is reported. Because the spectral integrals in Eqs. (42) and (47) depend explicitly on s0, the quoted uncertainties likely underestimate the model dependence. I request a variation of s0 (for example ±0.5-1 GeV^2) or a stability test showing that the extracted couplings and the final Br and width are insensitive to this choice.
- [Tables II and III, Eqs. (45), (49), and (67)] Several fit parameters are quoted with zero uncertainty, e.g., b = 57.43 ± 0.00 GeV^2 in Eq. (45), b = 0.22 ± 0.00 GeV^-2 in Eq. (49), and b = 0.22 ± 0.00 in Table III. This is not credible for fits to data points that themselves carry errors, and it hides the dominant systematic of the off-shell extrapolation. The authors should either propagate the fit-parameter covariance or assign a realistic uncertainty to the shape parameters; the present error budget for Br and \Gamma omits this uncertainty.
minor comments (4)
- [Sec. III B, Eq. (67)] Eq. (67) reads e^{-(-0.22 ± 0.01) Q^2}, which has a double negative in the exponent and would grow with Q^2. The decreasing curve in Fig. 8 indicates that e^{-0.22 Q^2} is intended; this typo should be corrected because a reader using Eq. (67) at face value would obtain the wrong sign of the slope.
- [Sec. IV, Eq. (68)] The text says the decay width is derived from Eq. (52), but Eq. (52) is the transition matrix element for \bar D_1 K_1 X_0. The correct reference for the \bar D K X_0 matrix element is Eq. (39).
- [Throughout] The manuscript contains several typographical artifacts, such as 'resoncance', 'e fforts', 'of fective', and 'compansate', which should be cleaned up in a final version.
- [Sec. I, Eq. (3)] The comparison with experimental Br(B^+ -> D^+ X_0) uses the isospin-inferred value (2.4 ± 1.0) x 10^-5. It would be helpful to state explicitly that this value inherits the LHCb uncertainty and that the quoted consistency does not include the experimental errors in the theory error budget.
Circularity Check
No circularity in the central prediction; only a minor self-cited continuum threshold enters as an auxiliary input.
full rationale
The derivation of Br(B+ -> D+ X0) and Gamma(X0 -> DK) is not circular with respect to the LHCb observables it claims to reproduce. The amplitudes in Eqs. (11)-(20) depend on strong couplings computed from QCD sum rules (Sec. III), weak form factors from Cheng-Chua-Hwang [57], and hadronic parameters from the PDG and the sum-rule literature; no parameter is fitted to Br(B+ -> D+ X0) ~ (2.4 +/- 1.0) x 10^-5 or Gamma = 57 +/- 12 +/- 4 MeV. The computed values (2.47 +2.07 -1.55) x 10^-5 and 64.07 +/- 18.23 MeV are genuine outputs, and Table III provides external cross-checks of the on-shell couplings (e.g., g_Ds*DK = 2.98 +1.90 -1.61 versus 2.84 +/- 0.31 from Ref. [77]). The only self-referential input is the continuum threshold s0 = 10 GeV^2 taken from Ref. [38], a prior two-point mass sum rule by H.-X. Chen, W. Chen, R.-R. Dong, and N. Su, where W. Chen is a co-author of the present paper. This is a standard auxiliary parameter in the sum rule for g_DKX0 and g_D*K*X0 and is not fitted to the target branching fraction or decay width, so it does not force the prediction by construction. The off-shell extrapolation from the QCD sum-rule window to the physical poles (monopole Eq. (44) and exponential Eq. (48)) introduces model-dependent shape uncertainty, especially for loop regions near Q^2 ~ 0, but this is a robustness and correctness concern rather than a circularity. Overall score 2 reflects the minor self-citation only.
Assumptions & free parameters
free parameters (13)
- a coefficient of g_DKX0(Q2) monopole fit =
25.56 +/- 1.63 GeV2
- b coefficient of g_DKX0(Q2) monopole fit =
57.43 +/- 0.00 GeV2
- a coefficient of g_D*bar K* X0(Q2) exponential fit =
0.12 +0.008/-0.008 GeV2
- b coefficient of g_D*bar K* X0(Q2) exponential fit =
0.22 +/- 0.00 GeV-2
- Borel mass M_B^2 choices =
3.30, 2.56, 5.0 GeV2 etc.
- a,b coefficients for g_D*_s0 DK fit =
a=0.58+0.26/-0.13 GeV2, b=0.43+/-0.01 GeV-2
- a,b coefficients for g_Ds1 DK* fit =
a=25.81+6.60/-3.45 GeV2, b=0.51+/-0.01 GeV-2
- a,b coefficients for g_Ds DK* fit =
a=2.25+1.67/-1.41 GeV2, b=0.52+0.03/-0.02 GeV-2
- a,b coefficients for g_D*_s DK1 fit =
a=15.41+4.96/-4.06 GeV2, b=0.41+/-0.00 GeV-2
- a,b coefficients for g_Ds DK*0 fit =
a=0.58+0.32/-0.24 GeV2, b=0.42+/-0.01 GeV-2
- a,b coefficients for g_Ds1 DK*0 fit =
a=17.01+4.45/-2.50 GeV2, b=0.33+/-0.00 GeV-2
- a,b coefficients for g_D*_s0 DK1 fit =
a=1.85+0.62/-0.39 GeV2, b=0.46+/-0.01 GeV-2
- a,b coefficients for g_Dbar*0 K*0 X0 fit (molecule) =
a=13.59+5.07/-6.21 GeV2, b=46.23+/-0.00 GeV2
assumptions (8)
- domain assumption QCD sum rules give reliable couplings for these hadronic vertices.
- domain assumption The interpolating currents in Eqs. (28)-(30) couple dominantly to the X0(2900) states under study.
- domain assumption The B+ weak decay amplitudes factorize with coefficient a1.
- domain assumption The FSI is saturated by the eight triangle diagrams in Fig. 2 with K, K*, K1, K*0 exchange.
- ad hoc to paper The off-shell vertex functions can be extrapolated from the Euclidean Q2 region to the on-shell pole by monopole or exponential fits.
- domain assumption Light quark masses can be set to zero for the X0 decay, giving isospin symmetry.
- domain assumption The continuum thresholds s0 from Refs. [38] and [62] are valid for the three-point sum rules.
- domain assumption The pole contribution is at least 40% in the chosen Borel windows.
Cite this review
Pith. "Pith review of The production and decay of $X_0(2900)$ state with different interpretation." pith.science (2026). https://pith.science/paper/6WLX4JVU
@misc{pith2026241202997,
author = {Pith},
title = {Pith review of: The production and decay of $X_0(2900)$ state with different interpretation},
year = {2026},
howpublished = {\url{https://pith.science/paper/6WLX4JVU}},
note = {Machine review of arXiv:2412.02997}
}
abstract
The observation of $X_0(2900)$ in $B^+\rightarrow D^+D^-K^+$ decay process indicates the existence of open flavor tetraquark states. We study the production and decay of $X_0(2900)$ state with final state interaction mechanism, where we calculate the strong vertices such as $g_{\bar{D}KX_0}$, $g_{\bar{D}^\ast K^\ast X_0}$, $g_{D_s^{\ast}\bar{D}K}$ and $g_{D_{s1}\bar{D} K^\ast}$ in the framework of QCD sum rules method. We find that for the interpretation of the $\bar{D}^\ast K^\ast$ molecule of $X_0(2900)$, the branching fraction of the production process and the decay width are consistent with the experimental results, indicating that the observed $X_0(2900)$ could be interpreted as the $\bar{D}^\ast K^\ast$ molecule. However, we cannot exclude the possibility of a compact tetraquark interpretation within the uncertainty. Further experimental and theoretical efforts should be made to fully understand the nature of the $X_0(2900)$ state.
Figures
Figures from the paper (5 more)
Forward citations
Cited by 2 Pith papers
-
Searching for the $2^+$ partner of the $T_{cs0}(2870)$ in the $B^- \to D^- D^0 K^0_S$ reaction
The small D0 K0S mass bump near 2.73 GeV in B- -> D- D0 K0S could be a 2+ D* K* molecular state, and its angular moments should show a clear signal.
-
Strong decays of the possible $D^{*}K$ and $\bar{D}^{*}K$ molecules
An effective-Lagrangian calculation predicts the I=1 D*K molecule T^a_cs1(2470) has a D_s*pi0 width of 13 to 196 MeV, about 10^3 times the predicted D_s1(2460) molecular width.
Reference graph
Works this paper leans on
- [38]
-
[1]
off shell and D∗ sDK, Ds1DK∗, D∗ s0DK, DsDK∗, D∗ sDK1, Ds0DK∗ 1, D∗ sDK∗ 0, Ds1DK∗ 0 strong decay vertices with K(K∗, K1, K∗
-
[2]
αs(µ) αs(2GeV) # 12 33−2n f , mc(µ) = mc(mc)
off shell. Some of these strong decay vertices are studied by some previous QCD sum rule analysis. We use the following interpolating currents forX0(2900) by considering it as a ¯D∗K∗ molecule, scalar diquark-scalar antidiquark compact tetraquark and axial-vector diquark-axial-vector antidiquark compact tetraquark: JX0(mol) = ¯caγµda ¯sbγµub, (28) JX0(S−S...
-
[3]
Gell-Mann, Phys
M. Gell-Mann, Phys. Lett. 8, 214 (1964)
1964
-
[4]
Zweig, in: D.Lichtenberg, S.P.Rosen(Eds.), Developments in the Quark Theory of Hadrons, VOL
G. Zweig, in: D.Lichtenberg, S.P.Rosen(Eds.), Developments in the Quark Theory of Hadrons, VOL. 1. 1964 - 1978:pp. 22–101, 1964
1964
-
[5]
R. L. Workman et al. [Particle Data Group], PTEP 2022, 083C01 (2022)
2022
- [6]
-
[7]
H. X. Chen, W. Chen, X. Liu and S. L. Zhu, Phys. Rept. 639, 1-121 (2016)
2016
Show all 84 references
-
[8]
Richard, Few Body Syst
J.-M. Richard, Few Body Syst. 57, 1185 (2016)
2016
-
[9]
Esposito, A
A. Esposito, A. Pilloni and A. D. Polosa, Phys. Rept. 668, 1-97 (2017)
2017
-
[10]
Ali, J.S
A. Ali, J.S. Lange, and S. Stone, Prog. Part. Nucl. Phys. 97, 123 (2017)
2017
-
[11]
F. K. Guo, C. Hanhart, U. G. Meißner, Q. Wang, Q. Zhao and B. S. Zou, Rev. Mod. Phys. 90, no.1, 015004 (2018)
2018
-
[12]
Albuquerque, J.M
R.M. Albuquerque, J.M. Dias, K.P. Khemchandani, A.M. Torres, F.S. Navarra, M. Nielsen, and C.M. Zanetti, J. Phys. G 46, 093002 (2019)
2019
-
[13]
Y . R. Liu, H. X. Chen, W. Chen, X. Liu and S. L. Zhu, Prog. Part. Nucl. Phys.107, 237-320 (2019) 19
2019
-
[14]
Brambilla, S
N. Brambilla, S. Eidelman, C. Hanhart, A. Nefediev, C. P. Shen, C. E. Thomas, A. Vairo and C. Z. Yuan, Phys. Rept.873, 1-154 (2020)
2020
-
[15]
Richard, A
J.-M. Richard, A. Valcarce, and J. Vijande, Annals Phys. 412, 168009 (2020)
2020
-
[16]
Faustov, V .O
R.N. Faustov, V .O. Galkin, and E.M. Savchenko, Universe 7, 94 (2021)
2021
-
[17]
H. X. Chen, W. Chen, X. Liu, Y . R. Liu and S. L. Zhu, Rept. Prog. Phys.86, 026201 (2023)
2023
-
[18]
L. Meng, B. Wang, G. J. Wang and S. L. Zhu, Phys.Rept. 1019 ,1-149 (2023)
2023
-
[19]
V . M. Abazovet al.[D0], Phys. Rev. Lett. 117, no.2, 022003 (2016)
2016
-
[20]
Aaij et al.[LHCb], Phys
R. Aaij et al.[LHCb], Phys. Rev. Lett. 117 no.15, 152003 (2016)[Addendum: Phys. Rev. Lett. 118, no.10, 109904 (2017)]
2016
-
[21]
A. M. Sirunyan et al.[CMS], Phys. Rev. Lett. 120, no.20, 202005 (2018)
2018
-
[22]
Aaltonen et al.[CDF], Phys
T. Aaltonen et al.[CDF], Phys. Rev. Lett. 120, no.20, 202006 (2018)
2018
-
[23]
M.Aaboud et al.[ATLAS], Phys. Rev. Lett.120, no.20, 202007 (2018)
2018
-
[24]
Aaij et al.[LHCb], Phys
R. Aaij et al.[LHCb], Phys. Rev. Lett. 125, 242001 (2020)
2020
-
[25]
Aaij et al.[LHCb], Phys
R. Aaij et al.[LHCb], Phys. Rev. D 102, 112003 (2020)
2020
-
[26]
Z. Yu, Q. Wu, and D.-Y . Chen, arXiv: 2310.12398 [hep-ph]
-
[27]
Cheng, S.-Y
J.-B. Cheng, S.-Y . Li, Y .-R. Liu, Y .-N. Liu, Z.-G. Si, and T. Yao, Phys. Rev. D101, no.11, 114017 (2020)
2020
-
[28]
T. Guo, J. Li, J. Zhao, and L. He, Phys. Rev. D 105, 054018 (2022)
2022
-
[29]
X.-G. He, W. Wang, and R. Zhu, Eur. Phys. J. C 80, no.11, 1026 (2020)
2020
-
[30]
G.-J. Wang, L. Meng, L.-Y . Xiao, M. Oka, and S.-L. Zhu, Eur. Phys. J. C81, no.2, 188 (2021)
2021
-
[31]
Zhang, Phys
J.-R. Zhang, Phys. Rev. D 103, no.5, 054019 (2021)
2021
-
[32]
Wang, Int
Z.-G. Wang, Int. J. Mod. Phys. A 35, no.30, 2050187 (2020)
2020
-
[33]
L ¨u, D.-Y
Q.-F. L ¨u, D.-Y . Chen, and Y .-B. Dong, Phys. Rev. D102, no.7, 074021 (2020)
2020
-
[34]
Agaev, K
S.S. Agaev, K. Azizi, and H. Sundu, Phys. Rev. D 106, no.1, 014019 (2022)
2022
-
[35]
Hu, X.-Y
M.-W. Hu, X.-Y . Lao, P. Ling, and Q. Wang, Chin. Phys. C45, no.2, 021003 (2021)
2021
-
[36]
Kong, J.-T
S.-Y . Kong, J.-T. Zhu, D. Song, and J. He, Phys. Rev. D104 no.9, 094012 (2021)
2021
-
[37]
Ke, Y .-F
H.-W. Ke, Y .-F. Shi, X.-H. Liu, and X.-Q. Li, Phys. Rev. D106, no.11, 114032 (2022)
2022
-
[39]
Wang, and S.-L
B. Wang, and S.-L. Zhu, Eur. Phys. J. C 82, no.5, 419 (2022)
2022
-
[40]
H.-X. Chen, W. Chen, R.-R. Dong, and N. Su, Chin. Phys. Lett. 37, no.10, 101201 (2020)
2020
-
[41]
Agaev, K
S.S. Agaev, K. Azizi, and H. Sundu, J. Phys. G 48, no.8, 085012 (2021)
2021
-
[42]
Chen, Phys
H.-X. Chen, Phys. Rev. D 105, no.9, 094003 (2022)
2022
-
[43]
Mutuk, J
H. Mutuk, J. Phys. G 48, no.5, 055007 (2021)
2021
-
[44]
Molina, T
R. Molina, T. Branz, and E. Oset, Phys. Rev. D 82, 014010 (2010)
2010
-
[45]
Molina and E
R. Molina and E. Oset, Phys. Lett. B 811, 135870 (2020) [Erratum: Phys. Lett. B 837, 137645 (2023)]
2020
-
[46]
Huang, J.-X
Y . Huang, J.-X. Lu, J.-J. Xie, and L.-S. Geng, Eur. Phys. J. C80, no.10, 973 (2020)
2020
-
[47]
Xiao, D.-Y
C.-J. Xiao, D.-Y . Chen, Y .-B. Dong, and G.-W. Meng, Phys. Rev. D103, no.3, 034004 (2021)
2021
-
[48]
T. J. Burns, and E. S. Swanson, Phys. Rev. D 103, no.1, 014004 (2021)
2021
-
[49]
T. J. Burns, and E. S. Swanson, Phys. Lett. B 813, 136057 (2021)
2021
-
[50]
Chen, J.-J
Y .-K. Chen, J.-J. Han, Q.-F. L¨u, J.-P. Wang, and F.-S. Yu, Eur. Phys. J. C81, no.1, 71 (2021)
2021
-
[51]
Hsiao, and Y
Y .-K. Hsiao, and Y . Yu, Phys. Rev. D104, no.3, 034008 (2021)
2021
-
[52]
Li, M.-Z
J.-W. Li, M.-Z. Yang, and D.-S. Du, HEPNP 27, 665-672 (2003)
2003
-
[53]
Cheng, C.-K
H.-Y . Cheng, C.-K. Chua, and A. Soni, Phys. Rev. D71, 014030 (2005)
2005
-
[54]
L ¨u, Y .-L
C.-D. L ¨u, Y .-L. Shen, and W. Wang, Phys. Rev. D73, 034005 (2006)
2006
-
[55]
Wirbel, B
M. Wirbel, B. Stech, and M. Bauer, Z. Phys. C 29, 637 (1985)
1985
-
[56]
Bauer, B
M. Bauer, B. Stech, and M. Wirbel, Z. Phys. C 34, 103 (1987)
1987
-
[57]
Buchalla, A.J
G. Buchalla, A.J. Buras, and M.E. Lautenbacher, Rev. Mod. Phys. 68, 1125-1144 (1996)
1996
-
[58]
Gortchakov, M.P
O. Gortchakov, M.P. Locher, V .E. Markushin, and S. von Rotz, Z. Phys. A353, 447 (1996)
1996
-
[59]
Cheng, C.-K
H.-Y . Cheng, C.-K. Chua, and C.-W. Hwang, Phys. Rev. D69, 074025 (2004)
2004
-
[60]
L. J. Reinders, H. Rubinstein, and S. Yazaki, Phys. Rep. 127, 1 (1985)
1985
-
[61]
M. A. Shifman, A. I. Vainshtein, and V . I. Zakharov, Nucl. Phys.B147, 385 (1979)
1979
-
[62]
Colangelo and A
P. Colangelo and A. Khodjamirian, At the Frontier of Particle Physics, edited by M. Shifman (World Scientific, Singapore, 2001), V ol.3, pp. 1495–1576
2001
-
[63]
Narison, Camb
S. Narison, Camb. Monogr. Part. Phys. Nucl. Phys. Cosmol.17, 1-812 (2007) Cambridge University Press, 2022, ISBN 978-1-00-929029- 6, 978-1-00-929031-9, 978-1-00-929033-3, 978-0-521-03731-0, 978-0-521-81164-4, 978-0-511-18948-7
2007
-
[64]
Gelhausen, A
P. Gelhausen, A. Khodjamirian, A.A. Pivovarov, and D. Rosenthal, Phys. Rev. D 88, 014015 (2013) [Erratum: Phys. Rev. D 91, 099901 (2015)]
2013
-
[65]
Gubernari, A
N. Gubernari, A. Khodjamirian, R. Mandal, and T. Mannel, JHEP 12, 015 (2023)
2023
-
[66]
’t Hooft, G
G. ’t Hooft, G. Isidori, L. Maiani, A. D. Polosa, and V . Riquer, Phys. Lett. B662, 424 (2008)
2008
-
[67]
Narison, QCD spectral sum rules, volume 26 (1989)
S. Narison, QCD spectral sum rules, volume 26 (1989)
1989
-
[68]
Jamin, J
M. Jamin, J. A. Oller, and A. Pich, Eur. Phys. J. C 24, 237 (2002)
2002
-
[69]
Jamin and A
M. Jamin and A. Pich, Nucl. Phys. B Proc. Suppl. 74, 300 (1999)
1999
-
[70]
B. L. Io ffe, Nucl. Phys. B188, 317 (1981), [Erratum: Nucl.Phys.B 191, 591–592 (1981)]
1981
-
[71]
Chung, H
Y . Chung, H. G. Dosch, M. Kremer, and D. Schall, Z. Phys. C25, 151 (1984)
1984
-
[72]
H. G. Dosch, M. Jamin, and S. Narison, Phys. Lett. B 220, 251 (1989)
1989
-
[73]
Khodjamirian, T
A. Khodjamirian, T. Mannel, N. Offen, and Y . M. Wang, Phys. Rev. D83, 094031 (2011)
2011
-
[74]
Francis, R
A. Francis, R. J. Hudspith, R. Lewis, and K. Maltman, Phys. Rev. D 99, 054505 (2019) 20
2019
-
[75]
Casalbuoni, A
R. Casalbuoni, A. Deandrea, N. Di Bartolomeo, R. Gatto, F. Feruglio and G. Nardulli, Phys. Rept. 281, 145 (1997)
1997
-
[76]
Casalbuoni, A
R. Casalbuoni, A. Deandrea, N. Di Bartolomeo, R. Gatto, F. Feruglio and G. Nardulli, Phys. Lett. B 292, 371 (1992)
1992
-
[77]
Casalbuoni, A
R. Casalbuoni, A. Deandrea, N. Di Bartolomeo, R. Gatto, F. Feruglio and G. Nardulli, Phys. Lett. B 299, 139 (1993)
1993
-
[78]
Navarra, M
F.S. Navarra, M. Nielsen, M.E. Bracco, M. Chiapparini, and C.L. Schat, Phys. Lett. B 489, 319 (2000)
2000
-
[79]
Bracco, A
M.E. Bracco, A. Cerqueira Jr., M. Chiapparini, A. Loz ´ea, and M. Nielsen, Phys. Lett. B 641, 286 (2006)
2006
-
[80]
Colangelo, F
P. Colangelo, F. De Fazio, G. Nardulli, N. Di Bartolomeo, and R. Gatto, Phys. Rev. D 52, 6422 (1995)
1995
-
[81]
Lin, H.-X
J.-X. Lin, H.-X. Chen, W.-H. Liang, C.-W. Xiao, and E. Oset, Eur. Phys. J. C 84, no.4, 439 (2024)
2024
-
[82]
Janbazi and R
M. Janbazi and R. Khosravi, Eur. Phys. J. C 78, no.7, 606 (2018)
2018
- [83]
-
[84]
Sundu, J.Y
H. Sundu, J.Y . Sungu, S. Sahin, N. Yinelek, and K. Azizi, Phys. Rev. D83, 114009 (2011)
2011
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