REVIEW 4 minor 52 references
Lattice-matched SU(3)F ratios of charmed-baryon semileptonic decays give clean, normalization-free tests of a long-standing experimental tension.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · grok-4.5
2026-07-15 11:58 UTC pith:MPURMBNN
load-bearing objection Clean lattice-to-SU(3)_F matching that produces three falsifiable, normalization-independent ratios for the Ξ_c puzzle.
Puzzles in charmed baryon semileptonic decays with SU(3)_F flavor symmetry and lattice inputs
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Matching lattice-QCD form factors for Λc → Λ, Λc → n and Ξc → Ξ onto an SU(3)F BCL z-expansion that includes first-order breaking yields the ratios B(Ξc+ → Σ0 ℓ+νℓ)/B(Ξc+ → Ξ0 ℓ+νℓ) = (2.6 ± 0.3)% and B(Ξc+ → Λ ℓ+νℓ)/B(Ξc+ → Ξ0 ℓ+νℓ) = (1.1 ± 0.1)%, together with the isospin partner RΣ− = (5.2 ± 0.6)%. These ratios are independent of the disputed normalization mode and therefore furnish direct experimental tests of the origin of the tension.
What carries the argument
The first-order SU(3)F parameterization of BCL coefficients, afn = Cf n (B†)i j Jj (Bc)i + Vf n (B†)i k Jj Sk j (Bc)i + Wf n (B†)k j Jj Si k (Bc)i, with the spurion S = diag(1,1,−2)/√6; the three parameters are fixed by lattice inputs and then used to predict the unmeasured Ξc → Σ, Λ channels.
Load-bearing premise
The assumption that first-order SU(3)F breaking is enough and that higher-order corrections stay at the percent level so they do not spoil the claimed precision of the ratios.
What would settle it
A precision measurement at Belle, Belle II or BESIII of the ratios RΣ0 and RΛ that lies many standard deviations away from the predicted (2.6 ± 0.3)% and (1.1 ± 0.1)% values would falsify the claim that first-order SU(3)F plus lattice inputs correctly describe the decays.
If this is right
- Precise measurements of RΣ0 and RΛ at current or near-future luminosities can decide whether the experimental–theory tension originates in the normalization channel Ξc0 → Ξ−π+.
- The same framework supplies absolute branching fractions and up-down asymmetries for the previously unmeasured Ξc → Σ and Ξc → Λ modes.
- If the measured ratios agree with the predictions, the lattice form factors and the first-order SU(3)F expansion are mutually consistent for these transitions.
- If the ratios disagree, either higher-order SU(3)F breaking or a genuine anomaly in the lattice or experimental inputs would be required.
Where Pith is reading between the lines
- The same matching procedure could be applied to non-leptonic Ξc decays whose absolute rates are also under experimental scrutiny, testing whether the normalization problem is universal.
- A confirmed discrepancy in the ratios would strengthen the case for re-measuring absolute Ξc branching fractions with independent methods (e.g., threshold production at BESIII or STCF).
- The size of the fitted V0f/C0f and W0f/C0f parameters (~10–20 %) already quantifies the expected first-order breaking; future lattice results for Ξc → Σ, Λ would allow a direct check of that size.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper constructs an SU(3)_F analysis of singly charmed baryon semileptonic form factors that includes first-order symmetry breaking, matching lattice-QCD BCL z-expansion coefficients for Λ_c → Λ, Λ_c → n and Ξ_c → Ξ onto the reduced amplitudes C_n^f, V_n^f and W_n^f (Eqs. 3–4 and Table I). With those parameters fixed, it predicts the previously unmeasured form factors and branching fractions for Ξ_c^+ → Λ ℓ^+ ν_ℓ and Ξ_c → Σ ℓ^+ ν_ℓ (Tables II–III, Fig. 1). The central results are the normalization-independent ratios R_Σ^{0} = (2.6 ± 0.3)%, R_Λ = (1.1 ± 0.1)% and R_Σ^{-} = (5.2 ± 0.6)% (Eq. 5), which are protected up to second-order SU(3)_F breaking and therefore provide clean experimental tests of the origin of the present tension between measured Ξ_c^{0} → Ξ^{-} e^{+} ν_e rates and both lattice and SU(3)_F expectations.
Significance. If the predicted ratios are confirmed, they cleanly isolate whether the long-standing experimental–theoretical discrepancy in Ξ_c semileptonic decays is due to an underestimated normalization mode B(Ξ_c^{0} → Ξ^{-} π^{+}) or to unexpectedly large SU(3)_F breaking. The construction is model-independent within the stated truncation, reproduces the input lattice form factors to O(10^{-3}), and yields falsifiable, percent-level predictions that can be tested at Belle/Belle II and BESIII/STCF with existing or near-term luminosities. The explicit matching of lattice BCL coefficients onto first-order SU(3)_F amplitudes (including the z-expansion convention conversion in the Appendix) is a useful technical contribution that can be reused for other charmed-baryon channels.
minor comments (4)
- After Table I the authors state that residual second-order SU(3)_F pieces are expected O(10^{-2}). A short quantitative estimate of how this residual propagates into the ratios of Eq. (5) (e.g., by varying the higher-order coefficients within a natural-size range) would make the claimed percent-level precision more transparent.
- The efficiencies used for the event-yield projections (Sec. III, after Eq. 6) are taken from disparate Belle analyses; a brief remark on whether they are assumed q^{2}-independent and how that assumption affects the projected δR would strengthen the experimental discussion.
- Fig. 1 shows form-factor bands but does not display the corresponding lattice points for the input channels; overlaying those points (or stating that they lie within the bands to O(10^{-3})) would make the reproduction claim immediately visible.
- Typographical consistency: the abstract and Eq. (5) write Λ while Table III and the text sometimes write Λ^{0}; a uniform notation for the Λ hyperon would avoid minor confusion.
Circularity Check
No load-bearing circularity: lattice form factors fix C/V/W; new-channel ratios are genuine first-order SU(3)_F extrapolations, not forced by construction.
full rationale
The derivation chain is: external LQCD form-factor coefficients a_n^f for the three input channels Λ_c oΛ, Λ_c o n and Ξ_c oΞ are inverted via the linear map (4) to obtain the SU(3)_F parameters C_n^f, V_n^f, W_n^f of Table I; those parameters are then inserted into the same decomposition (3) to generate the previously unmeasured form factors of Ξ_c^+ oΣ^0 and Ξ_c^+ oΛ (Table II and Fig. 1). The ratios R_Σ^{0}, R_Λ and R_Σ^{-} of Eq. (5) are formed from the resulting branching fractions; because the overall multiplet normalizations cancel and the residual second-order breaking is estimated O(10^{-2}) from the observed size of V_0/C_0 and W_0/C_0, the ratios are protected predictions rather than tautologies. The fit reproduces the three lattice inputs to O(10^{-3}) by construction of the 3 imes3 matrix, but that is ordinary parameter determination, not a prediction of the inputs themselves. Self-citations to earlier SU(3)_F papers by overlapping authors supply only the general multiplet language and do not enter the numerical extraction or the protection argument for the ratios. No step reduces a claimed prediction to its own definition or to a fitted quantity that is statistically forced to equal the prediction.
Axiom & Free-Parameter Ledger
free parameters (2)
- Lattice BCL coefficients a_n^f for Λ_c→Λ, Λ_c→n, Ξ_c→Ξ
- CKM elements V_cd, V_cs and baryon lifetimes
axioms (3)
- domain assumption First-order SU(3)_F breaking is captured by the two independent spurion insertions V and W of S=diag(1,1,−2)/√6; higher-order terms are O((m_s/Λ_QCD)^2)≈0.01–0.04 and do not affect the quoted precision of the ratios.
- domain assumption The BCL z-expansion with the conventional D(∗)π/K poles and the end-point constraints (Eq. (2)) adequately describes the q^{2} dependence over the physical range.
- standard math Isospin symmetry relates Ξ_c^0→Σ^− to Ξ_c^+→Σ^0 by a factor √2.
read the original abstract
Recent measurements of charmed-baryon semileptonic decays signal large tensions between experiment and theory, including $SU(3)_F$ analyses and lattice-quantum chromodynamics simulations. Possible sources of the discrepancy include the experimental normalization mode $\Xi_c^0 \to \Xi^- \pi ^+$. Using lattice-QCD inputs in an $SU(3)_F$ analysis including first-order symmetry breaking, we predict ${\cal B}( \Xi_c^+ \to \Sigma^0 \ell^+ \nu_\ell ) / {\cal B}( \Xi_c^+ \to \Xi^0 \ell^+ \nu_\ell )=(2.6\pm0.3)\%, $ and ${\cal B}( \Xi_c^+ \to \Lambda \ell^+ \nu_\ell )/{\cal B}( \Xi_c^+ \to \Xi^0 \ell^+ \nu_\ell )=(1.1\pm0.1)\%, $ with $\ell^+=(e^+,\mu^+)$. These ratios provide normalization-independent tests and may help clarify the origin of the present tension.
Figures
Reference graph
Works this paper leans on
-
[1]
Y. B. Liet al.[Belle], Phys. Rev. Lett.127, no.12, 121803 (2021)
2021
-
[2]
Acharyaet al.[ALICE], Phys
S. Acharyaet al.[ALICE], Phys. Rev. Lett.127, no.27, 272001 (2021) [erratum: Phys. Rev. Lett.134, no.17, 179902 (2025)]
2021
-
[3]
I. J. Abualrobet al.[ALICE], JHEP12, 038 (2025)
2025
-
[4]
Navaset al.[Particle Data Group], Phys
S. Navaset al.[Particle Data Group], Phys. Rev. D110, no.3, 030001 (2024)
2024
-
[5]
Q. A. Zhang, J. Hua, F. Huang, R. Li, Y. Li, C. Lü, C. D. Lu, P. Sun, W. Sun and W. Wang,et al.Chin. Phys. C46, no.1, 011002 (2022)
2022
-
[6]
C.FarrellandS.Meinel, Phys.Rev.D111, no.11, 114521 (2025)
2025
-
[7]
X. G. He, F. Huang, W. Wang and Z. P. Xing, Phys. Lett. B823, 136765 (2021). 5
2021
-
[8]
C. Q. Geng, X. G. He, X. N. Jin, C. W. Liu and C. Yang, Phys. Rev. D109, no.7, L071302 (2024)
2024
-
[9]
H. Y. Cheng, F. Xu and H. Zhong, Phys. Rev. D111, no.3, 034011 (2025)
2025
-
[10]
C. Q. Geng, C. W. Liu and S. L. Liu, Phys. Rev. D109, no.9, 093002 (2024)
2024
-
[11]
C. Yang, X. G. He and C. W. Liu, JHEP09, 193 (2025)
2025
- [12]
-
[13]
M. J. Savage and R. P. Springer, Phys. Rev. D42, 1527- 1543 (1990)
1990
-
[14]
M. J. Savage, Phys. Lett. B257, 414-418 (1991)
1991
-
[15]
Pirtskhalava and P
D. Pirtskhalava and P. Uttayarat, Phys. Lett. B712, 81-86 (2012)
2012
-
[16]
Grossman and D
Y. Grossman and D. J. Robinson, JHEP04, 067 (2013)
2013
-
[17]
C. D. Lü, W. Wang and F. S. Yu, Phys. Rev. D93, no.5, 056008 (2016)
2016
-
[18]
C. Q. Geng, Y. K. Hsiao, Y. H. Lin and L. L. Liu, Phys. Lett. B776, 265-269 (2018)
2018
-
[19]
C. Q. Geng, Y. K. Hsiao, C. W. Liu and T. H. Tsai, JHEP11, 147 (2017)
2017
-
[20]
D. Wang, P. F. Guo, W. H. Long and F. S. Yu, JHEP 03, 066 (2018)
2018
-
[21]
C. Q. Geng, Y. K. Hsiao, C. W. Liu and T. H. Tsai, Phys. Rev. D97, no.7, 073006 (2018)
2018
-
[22]
C. Q. Geng, Y. K. Hsiao, C. W. Liu and T. H. Tsai, Eur. Phys. J. C78, no.7, 593 (2018)
2018
-
[23]
C. Q. Geng, C. W. Liu and T. H. Tsai, Phys. Lett. B 790, 225-228 (2019)
2019
-
[24]
C. Q. Geng, Y. K. Hsiao, C. W. Liu and T. H. Tsai, Phys. Rev. D99, no.7, 073003 (2019)
2019
-
[25]
J. Y. Cen, C. Q. Geng, C. W. Liu and T. H. Tsai, Eur. Phys. J. C79, no.11, 946 (2019)
2019
-
[26]
Y. K. Hsiao, Y. Yao and H. J. Zhao, Phys. Lett. B792, 35-39 (2019)
2019
-
[27]
C. Q. Geng, C. W. Liu, T. H. Tsai and Y. Yu, Phys. Rev. D99, no.11, 114022 (2019)
2019
-
[28]
C. Q. Geng, C. W. Liu, T. H. Tsai and S. W. Yeh, Phys. Lett. B792, 214-218 (2019)
2019
-
[29]
C. P. Jia, D. Wang and F. S. Yu, Nucl. Phys. B956, 115048 (2020)
2020
-
[30]
C. Q. Geng, C. W. Liu and T. H. Tsai, Phys. Lett. B 794, 19-28 (2019)
2019
-
[31]
C. W. Liu, Phys. Rev. D109, no.3, 033004 (2024)
2024
-
[32]
Y. K. Hsiao, JHEP11, 117 (2023)
2023
- [33]
-
[34]
Zhong, F
H. Zhong, F. Xu and H. Y. Cheng, Phys. Rev. D109, no.11, 114027 (2024)
2024
-
[35]
X. G. He and C. W. Liu, Sci. Bull.70, 2598-2603 (2025)
2025
-
[36]
J. Sun, Z. P. Xing and R. Zhu, Eur. Phys. J. C85, no.3, 262 (2025)
2025
-
[37]
Z. P. Xing, Y. J. Shi, J. Sun and Y. Xing, Eur. Phys. J. C84, no.10, 1014 (2024)
2024
-
[38]
C. Q. Geng, C. W. Liu and S. L. Liu, JHEP07, 151 (2025)
2025
-
[39]
X. Wu, Q. Chen, Y. Xing, Z. P. Xing and R. Zhu, Chin. Phys.49, no.12, 123101 (2025)
2025
-
[40]
H. Y. Cheng, F. Xu and H. Zhong, Phys. Rev. D112, no.5, 054022 (2025)
2025
-
[41]
Bourrely, I
C. Bourrely, I. Caprini and L. Lellouch, Phys. Rev. D 79, 013008 (2009) [erratum: Phys. Rev. D82, 099902 (2010)]
2009
-
[42]
Meinel, Phys
S. Meinel, Phys. Rev. Lett.118, no.8, 082001 (2017)
2017
-
[43]
Meinel, Phys
S. Meinel, Phys. Rev. D97, no.3, 034511 (2018)
2018
-
[44]
Charleset al.[CKMfitter Group], Eur
J. Charleset al.[CKMfitter Group], Eur. Phys. J. C41, no.1, 1-131 (2005)
2005
-
[45]
Adachiet al.[Belle and Belle-II], JHEP10, 045 (2024)
I. Adachiet al.[Belle and Belle-II], JHEP10, 045 (2024)
2024
-
[46]
Jiaet al.[Belle], JHEP06, 160 (2021)
S. Jiaet al.[Belle], JHEP06, 160 (2021)
2021
-
[47]
Liet al.[Belle], Phys
Y. Liet al.[Belle], Phys. Rev. D105, no.1, L011102 (2022)
2022
-
[48]
Ablikimet al.[BESIII], [arXiv:2512.05178 [hep-ex]]
M. Ablikimet al.[BESIII], [arXiv:2512.05178 [hep-ex]]
-
[49]
Ablikimet al.[BESIII], Phys
M. Ablikimet al.[BESIII], Phys. Rev. Lett.131, no.19, 191901 (2023)
2023
-
[50]
Ablikimet al.[BESIII], Chin
M. Ablikimet al.[BESIII], Chin. Phys. C46, no.11, 113003 (2022)
2022
-
[51]
H. B. Liet al.[BESIII], [arXiv:2204.08943 [hep-ex]]
-
[52]
Achasov, X
M. Achasov, X. C. Ai, R. Aliberti, L. P. An, Q. An, X. Z. Bai, Y. Bai, O. Bakina, A. Barnyakov and V. Bli- nov,et al.Front. Phys. (Beijing)19, no.1, 14701 (2024)
2024
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.