Search for the low-lying excited baryon Sigma^*(1/2^-) through process Λ^+_c to Λ K⁰ π^+
Pith reviewed 2026-05-22 12:28 UTC · model grok-4.3
The pith
A model of Λ_c^+ → Λ K^0 π^+ decay predicts a cusp at 1.43 GeV from the low-lying Σ*(1/2^-) baryon.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Incorporating the contribution from the dynamically generated Σ*(1/2^-) resonance via S-wave pseudoscalar meson-octet baryon interactions, in addition to the K*(892) and N(1535) intermediates, the model reproduces the experimental π^+ K^0 invariant mass spectrum and generates a distinct cusp structure around 1.43 GeV in the π^+ Λ invariant mass distribution associated with the Σ*(1/2^-).
What carries the argument
The Σ*(1/2^-) resonance dynamically generated in the S-wave pseudoscalar meson-octet baryon channel, which produces the predicted cusp through its contribution to the decay amplitude.
If this is right
- The model reproduces the BESIII π^+ K^0 invariant mass distribution.
- A distinct cusp structure appears around 1.43 GeV in the π^+ Λ invariant mass distribution.
- Future high-precision measurements at BESIII, Belle II, and Super Tau-Charm Facility can test the existence of the Σ*(1/2^-).
Where Pith is reading between the lines
- Confirmation of the cusp would connect charmed baryon decays to tests of dynamical generation for light baryon states.
- The same framework could be applied to related decay modes to map additional features in the baryon spectrum.
- Absence of the cusp in new data would require revisiting the modeling assumptions for this resonance.
Load-bearing premise
The low-lying excited baryon Σ*(1/2^-) exists as a dynamically generated state from S-wave pseudoscalar meson-octet baryon interactions and produces a visible cusp in the invariant mass distribution.
What would settle it
A precise measurement of the π^+ Λ invariant mass distribution in Λ_c^+ → Λ K^0 π^+ that lacks any cusp feature near 1.43 GeV.
Figures
read the original abstract
Motivated by recent BESIII measurements of the singly Cabibbo-suppressed processes $\Lambda^+_c \to \Lambda K^+ \pi^0$ and $\Lambda^+_c \to \Lambda K_S^0 \pi^+$, we investigate the process $\Lambda^+_c \to \Lambda K^0 \pi^+$ by taking into account the contribution from the low-lying excited baryon $\Sigma^*(1/2^-)$, dynamically generated via the $S$-wave pseudoscalar meson-octet baryon interaction, as well as from the intermediate resonances $K^*(892)$ and $N(1535)$. Our model successfully reproduces the BESIII $\pi^+K^0$ invariant mass distribution, and predicts a distinct cusp structure around 1.43~GeV in the $\pi^+\Lambda$ invariant mass distribution, which is associated with the predicted $\Sigma^*(1/2^-)$. Future high-precise measurements of this process at BESIII, Belle~II, and the proposed Super Tau-Charm Facility experiments will be crucial for testing the existence of $\Sigma^*(1/2^-)$ and advancing our understanding of the light baryon spectrum.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript investigates the singly Cabibbo-suppressed decay Λ_c^+ → Λ K^0 π^+ by constructing an amplitude that includes the dynamically generated Σ*(1/2^-) resonance (from S-wave pseudoscalar meson-octet baryon interactions), together with intermediate K*(892) and N(1535) contributions. The central claims are that the model reproduces the BESIII π^+ K^0 invariant-mass distribution and predicts a distinct cusp near 1.43 GeV in the π^+ Λ invariant-mass spectrum as a signature of the Σ*(1/2^-).
Significance. If the predicted cusp is confirmed by future high-statistics data, the work would furnish a testable signature for the low-lying Σ*(1/2^-) in a new decay channel and thereby strengthen the case for its dynamical generation within chiral-unitary frameworks. The reported reproduction of existing BESIII data provides a non-trivial consistency check, but the overall impact remains conditional on experimental verification of the specific structure.
major comments (2)
- [Abstract and §3 (amplitude construction)] Abstract and model section: the claim of successful reproduction of the BESIII π^+ K^0 invariant mass distribution is stated without supplying the numerical values of the free parameters (cutoff or subtraction constants), the explicit fit procedure, χ² values, or error bands. This absence makes it impossible to judge whether the reproduction is robust or merely qualitative.
- [§2 (resonance input) and §4 (results)] Theoretical framework: the Σ*(1/2^-) pole position and its coupling to the πΛ channel are imported directly from earlier dynamical-generation calculations; the cusp at ~1.43 GeV is therefore a built-in feature of the input resonance rather than an independent prediction generated within the present amplitude. This reduces the novelty of the test for the resonance’s existence.
minor comments (2)
- [Title and abstract] The title uses K^0 while the abstract and text refer to both K^0 and K_S^0; a brief clarification of the isospin relation and experimental tagging would improve readability.
- [Figure 2 and Figure 3] Figure captions for the invariant-mass distributions should explicitly state the binning, normalization, and whether the curves include interference terms or only the resonant contributions.
Simulated Author's Rebuttal
We thank the referee for the careful reading of the manuscript and the constructive comments. We address each major comment below and indicate the changes made to the revised version.
read point-by-point responses
-
Referee: [Abstract and §3 (amplitude construction)] Abstract and model section: the claim of successful reproduction of the BESIII π^+ K^0 invariant mass distribution is stated without supplying the numerical values of the free parameters (cutoff or subtraction constants), the explicit fit procedure, χ² values, or error bands. This absence makes it impossible to judge whether the reproduction is robust or merely qualitative.
Authors: We agree that the original manuscript lacked sufficient detail on the numerical inputs and fit quality. In the revised version we now explicitly list the cutoff value and subtraction constants used in the chiral-unitary amplitude, describe the fitting procedure to the BESIII π^+ K^0 distribution, report the obtained χ², and display theoretical error bands on the corresponding figure. revision: yes
-
Referee: [§2 (resonance input) and §4 (results)] Theoretical framework: the Σ*(1/2^-) pole position and its coupling to the πΛ channel are imported directly from earlier dynamical-generation calculations; the cusp at ~1.43 GeV is therefore a built-in feature of the input resonance rather than an independent prediction generated within the present amplitude. This reduces the novelty of the test for the resonance’s existence.
Authors: The pole position is indeed taken from prior chiral-unitary work, as is standard when testing a resonance in a new channel. The novelty of the present study lies in the construction of the full decay amplitude for Λ_c^+ → Λ K^0 π^+ that consistently includes the Σ*(1/2^-), K*(892) and N(1535) contributions, and in the resulting prediction of a visible cusp specifically in the π^+ Λ invariant-mass spectrum. This constitutes a new, experimentally testable signature in a decay mode not previously examined for this resonance. revision: no
Circularity Check
No significant circularity: standard chiral-unitary amplitude applied to new decay channel
full rationale
The derivation constructs a decay amplitude that incorporates the Σ*(1/2^-) pole position and couplings obtained from prior S-wave meson-baryon scattering calculations, together with K*(892) and N(1535) contributions. This amplitude is then used to reproduce the measured π⁺K⁰ invariant-mass spectrum and to compute the π⁺Λ spectrum, where a cusp appears at the resonance location. Because the resonance parameters are fixed by the scattering sector (independent of the present decay data) and the new observable is a distinct final-state distribution, the prediction does not reduce to a re-statement of the input by construction. No self-definitional loop, fitted parameter renamed as prediction, or load-bearing self-citation chain is required for the central claim.
Axiom & Free-Parameter Ledger
free parameters (1)
- model cutoff or subtraction constants
axioms (1)
- domain assumption The Σ*(1/2⁻) is dynamically generated from S-wave pseudoscalar meson-octet baryon interaction.
invented entities (1)
-
Σ*(1/2⁻)
no independent evidence
Lean theorems connected to this paper
-
IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
T Σ*(1/2^-) = V_p h_{K0Λ} G_{π+Λ} t_{π+Λ→π+Λ} ... V_ij = -C_ij/(4f²) (2√s - M_i - M_j) ...
-
IndisputableMonolith/Foundation/RealityFromDistinction.leanreality_from_one_distinction unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
dynamically generated via the S-wave pseudoscalar meson-octet baryon interaction
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Forward citations
Cited by 1 Pith paper
-
Probing the isospin structure and low-lying resonances in $\Lambda_c^+ \to n\bar{K}^0 \pi^+$ decays
The chiral unitary calculation predicts a narrow peak from N(1535) in the pi+ n invariant mass spectrum and a dip from Lambda(1670) in the K0bar n spectrum, supporting the molecular interpretation of these resonances.
Reference graph
Works this paper leans on
-
[1]
S. K. Choiet al.[Belle], Phys. Rev. Lett.91, 262001 (2003)
work page 2003
-
[2]
H. X. Chen, W. Chen, X. Liu, Y. R. Liu and S. L. Zhu, Rept. Prog. Phys.80, no.7, 076201 (2017)
work page 2017
-
[3]
H. X. Chen, W. Chen, X. Liu, Y. R. Liu and S. L. Zhu, Rept. Prog. Phys.86, no.2, 026201 (2023)
work page 2023
-
[4]
F. K. Guo, C. Hanhart, U. G. Meißner, Q. Wang, Q. Zhao and B. S. Zou, Rev. Mod. Phys.90, no.1, 015004 (2018) [erratum: Rev. Mod. Phys.94, no.2, 029901 (2022)]
work page 2018
-
[5]
E. Oset, W. H. Liang, M. Bayar, J. J. Xie, L. R. Dai, M. Albaladejo, M. Nielsen, T. Sekihara, F. Navarra and L. Roca,et al.Int. J. Mod. Phys. E25, 1630001 (2016)
work page 2016
-
[6]
M. Z. Liu, Y. W. Pan, Z. W. Liu, T. W. Wu, J. X. Lu and L. S. Geng, Phys. Rept.1108, 1-108 (2025)
work page 2025
-
[7]
Navaset al.[Particle Data Group], Phys
S. Navaset al.[Particle Data Group], Phys. Rev. D110, no.3, 030001 (2024)
work page 2024
- [8]
-
[9]
D. Jido, J. A. Oller, E. Oset, A. Ramos and U. G. Meiss- ner, Nucl. Phys. A725, 181-200 (2003)
work page 2003
- [10]
- [11]
-
[12]
E. Wang, L. S. Geng, J. J. Wu, J. J. Xie and B. S. Zou, Chin. Phys. Lett.41, no.10, 101401 (2024)
work page 2024
-
[13]
B. S. Zou, Eur. Phys. J. A35(2008), 325-328
work page 2008
-
[14]
E. Oset, A. Ramos and C. Bennhold, Phys. Lett. B 527, 99-105 (2002) [erratum: Phys. Lett. B530, 260- 260 (2002)]
work page 2002
-
[15]
J. A. Oller and U. G. Meissner, Phys. Lett. B500, 263- 272 (2001)
work page 2001
-
[16]
K. P. Khemchandani, A. Mart´ ınez Torres and J. A. Oller, Phys. Rev. C100, no.1, 015208 (2019)
work page 2019
- [17]
-
[18]
J. A. Oller, Eur. Phys. J. A28, 63-82 (2006)
work page 2006
-
[19]
C. Garcia-Recio, J. Nieves, E. Ruiz Arriola and M. J. Vi- cente Vacas, Phys. Rev. D67, 076009 (2003)
work page 2003
-
[20]
M. F. M. Lutz and E. E. Kolomeitsev, Nucl. Phys. A 700, 193-308 (2002)
work page 2002
- [21]
- [22]
-
[23]
J. J. Wu, S. Dulat and B. S. Zou, Phys. Rev. C81, 045210 (2010)
work page 2010
-
[24]
J. J. Wu, S. Dulat and B. S. Zou, Phys. Rev. D80, 017503 (2009)
work page 2009
-
[25]
P. Gao, J. J. Wu and B. S. Zou, Phys. Rev. C81, 055203 (2010)
work page 2010
-
[26]
L. R. Dai, R. Pavao, S. Sakai and E. Oset, Phys. Rev. D 97, no.11, 116004 (2018)
work page 2018
-
[27]
J. J. Xie and E. Oset, Phys. Lett. B792, 450-453 (2019)
work page 2019
-
[28]
Y. Y. Li, J. Song, E. Oset, W. H. Liang and R. Molina, Eur. Phys. J. C85, no.9, 1086 (2025)
work page 2025
-
[29]
W. T. Lyu, S. C. Zhang, G. Y. Wang, J. J. Wu, E. Wang, L. S. Geng and J. J. Xie, Phys. Rev. D110, no.5, 054020 (2024)
work page 2024
-
[30]
J. J. Xie and L. S. Geng, Phys. Rev. D95, no.7, 074024 (2017)
work page 2017
-
[31]
Y. Li, W. T. Lyu, G. Y. Wang, L. Li, W. C. Yan and E. Wang, Phys. Rev. D111(2025) no.5, 054011
work page 2025
-
[32]
L. J. Liu, E. Wang, J. J. Xie, K. L. Song and J. Y. Zhu, Phys. Rev. D98, no.11, 114017 (2018)
work page 2018
-
[33]
E. Wang, J. J. Xie and E. Oset, Phys. Lett. B753, 526- 532 (2016)
work page 2016
-
[34]
Y. H. Lyu, H. Zhang, N. C. Wei, B. C. Ke, E. Wang and J. J. Xie, Chin. Phys. C47, no.5, 053108 (2023)
work page 2023
-
[35]
S. H. Kim, K. P. Khemchandani, A. Martinez Torres, S. i. Nam and A. Hosaka, Phys. Rev. D103, no.11, 8 114017 (2021)
work page 2021
-
[36]
M. Ablikimet al.[BESIII], Phys. Rev. Lett.134, no.2, 021901 (2025)
work page 2025
-
[37]
M. Y. Duan, W. T. Lyu, C. W. Xiao, E. Wang, J. J. Xie, D. Y. Chen and E. Oset, Phys. Rev. D111(2025) no.1, 016004
work page 2025
- [38]
-
[39]
Z. H. Guo and J. A. Oller, Phys. Rev. C87, no.3, 035202 (2013)
work page 2013
- [40]
- [41]
-
[42]
G. Y. Wang, N. C. Wei, H. M. Yang, E. Wang, L. S. Geng and J. J. Xie, Phys. Rev. D106, no.5, 056001 (2022)
work page 2022
-
[43]
Z. Wang, Y. Y. Wang, E. Wang, D. M. Li and J. J. Xie, Eur. Phys. J. C80, no.9, 842 (2020)
work page 2020
-
[44]
C. H. Zeng, J. X. Lu, E. Wang, J. J. Xie and L. S. Geng, Phys. Rev. D102, no.7, 076009 (2020)
work page 2020
-
[45]
X. C. Feng, L. L. Wei, M. Y. Duan, E. Wang and D. M. Li, Phys. Lett. B846, 138185 (2023)
work page 2023
-
[46]
Y. Li, S. W. Liu, E. Wang, D. M. Li, L. S. Geng and J. J. Xie, Phys. Rev. D110, no.7, 074010 (2024)
work page 2024
-
[47]
S. C. Zhang, M. Y. Duan, W. T. Lyu, G. Y. Wang, J. Y. Zhu and E. Wang, Eur. Phys. J. C84, no.12, 1253 (2024)
work page 2024
-
[48]
M. Y. Li, W. T. Lyu, L. J. Liu and E. Wang, Phys. Rev. D111(2025) no.3, 034046
work page 2025
-
[49]
M. Ablikimet al.[BESIII], Phys. Rev. D109, no.3, 032003 (2024)
work page 2024
-
[50]
M. Ablikimet al.[BESIII], Phys. Rev. D111, no.1, 012014 (2025)
work page 2025
-
[51]
B. C. Liu and B. S. Zou, Phys. Rev. Lett.96(2006) no.4, 042002
work page 2006
-
[52]
W. T. Lyu, Y. H. Lyu, M. Y. Duan, D. M. Li, D. Y. Chen and E. Wang, Phys. Rev. D109, no.1, 014008 (2024)
work page 2024
- [53]
-
[54]
K. Miyahara, T. Hyodo, M. Oka, J. Nieves and E. Oset, Phys. Rev. C95, no.3, 035212 (2017)
work page 2017
-
[55]
R. P. Pavao, W. H. Liang, J. Nieves and E. Oset, Eur. Phys. J. C77, no.4, 265 (2017)
work page 2017
- [56]
- [57]
-
[58]
E. Wang, H. X. Chen, L. S. Geng, D. M. Li and E. Oset, Phys. Rev. D93, no.9, 094001 (2016)
work page 2016
-
[59]
W. T. Lyu, Y. H. Lyu, M. Y. Duan, G. Y. Wang, D. Y. Chen and E. Wang, Eur. Phys. J. C85, no.2, 123 (2025)
work page 2025
- [60]
-
[61]
F. Mandl and G. Shaw, QUANTUM FIELD THEORY, Cambridge University Press, New York, 2014
work page 2014
- [62]
-
[63]
H. Y. Cheng, X. R. Lyu and Z. Z. Xing, Chin. Phys. Lett. 42, no.1, 010201 (2025)
work page 2025
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.