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arxiv: 2507.11145 · v1 · submitted 2025-07-15 · ✦ hep-ex

Observation of the electromagnetic radiative decays of the boldmath{Λ(1520)} and boldmath{Λ(1670)} to boldmath{γSigma⁰}

BESIII Collaboration: M. Ablikim , M. N. Achasov , P. Adlarson , X. C. Ai , R. Aliberti , A. Amoroso , Q. An , Y. Bai
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O. Bakina Y. Ban H.-R. Bao V. Batozskaya K. Begzsuren N. Berger M. Berlowski M. Bertani D. Bettoni F. Bianchi E. Bianco A. Bortone I. Boyko R. A. Briere A. Brueggemann H. Cai M. H. Cai X. Cai A. Calcaterra G. F. Cao N. Cao S. A. Cetin X. Y. Chai J. F. Chang G. R. Che Y. Z. Che C. H. Chen Chao Chen G. Chen H. S. Chen H. Y. Chen M. L. Chen S. J. Chen S. L. Chen S. M. Chen T. Chen X. R. Chen X. T. Chen X. Y. Chen Y. B. Chen Y. Q. Chen Z. Chen Z. J. Chen Z. K. Chen S. K. Choi X. Chu G. Cibinetto F. Cossio J. Cottee-Meldrum J. J. Cui H. L. Dai J. P. Dai A. Dbeyssi R. E. de Boer D. Dedovich C. Q. Deng Z. Y. Deng A. Denig I. Denysenko M. Destefanis F. De Mori B. Ding X. X. Ding Y. Ding Y. X. Ding J. Dong L. Y. Dong M. Y. Dong X. Dong M. C. Du S. X. Du Y. Y. Duan P. Egorov G. F. Fan J. J. Fan Y. H. Fan J. Fang S. S. Fang W. X. Fang Y. Q. Fang R. Farinelli L. Fava F. Feldbauer G. Felici C. Q. Feng J. H. Feng L. Feng Q. X. Feng Y. T. Feng M. Fritsch C. D. Fu J. L. Fu Y. W. Fu H. Gao X. B. Gao Y. Gao Y. N. Gao Y. Y. Gao S. Garbolino I. Garzia P. T. Ge Z. W. Ge C. Geng E. M. Gersabeck A. Gilman K. Goetzen J. D. Gong L. Gong W. X. Gong W. Gradl S. Gramigna M. Greco M. H. Gu Y. T. Gu C. Y. Guan A. Q. Guo L. B. Guo M. J. Guo R. P. Guo Y. P. Guo A. Guskov J. Gutierrez K. L. Han T. T. Han F. Hanisch K. D. Hao X. Q. Hao F. A. Harris K. K. He K. L. He F. H. Heinsius C. H. Heinz Y. K. Heng C. Herold P. C. Hong G. Y. Hou X. T. Hou Y. R. Hou Z. L. Hou H. M. Hu J. F. Hu Q. P. Hu S. L. Hu T. Hu Y. Hu Z. M. Hu G. S. Huang K. X. Huang L. Q. Huang P. Huang X. T. Huang Y. P. Huang Y. S. Huang T. Hussain N. H\"usken N. in der Wiesche J. Jackson Q. Ji Q. P. Ji W. Ji X. B. Ji X. L. Ji Y. Y. Ji Z. K. Jia D. Jiang H. B. Jiang P. C. Jiang S. J. Jiang T. J. Jiang X. S. Jiang Y. Jiang J. B. Jiao J. K. Jiao Z. Jiao S. Jin Y. Jin M. Q. Jing X. M. Jing T. Johansson S. Kabana N. Kalantar-Nayestanaki X. L. Kang X. S. Kang M. Kavatsyuk B. C. Ke V. Khachatryan A. Khoukaz R. Kiuchi O. B. Kolcu B. Kopf M. Kuessner X. Kui N. Kumar A. Kupsc W. K\"uhn Q. Lan W. N. Lan T. T. Lei M. Lellmann T. Lenz C. Li C. H. Li C. K. Li D. M. Li F. Li G. Li H. B. Li H. J. Li H. N. Li Hui Li J. R. Li J. S. Li K. Li K. L. Li L. J. Li Lei Li M. H. Li M. R. Li P. L. Li P. R. Li Q. M. Li Q. X. Li R. Li S. X. Li T. Li T. Y. Li W. D. Li W. G. Li X. Li X. H. Li X. L. Li X. Y. Li X. Z. Li Y. Li Y. G. Li Y. P. Li Z. J. Li Z. Y. Li H. Liang Y. F. Liang Y. T. Liang G. R. Liao L. B. Liao M. H. Liao Y. P. Liao J. Libby A. Limphirat C. C. Lin D. X. Lin L. Q. Lin T. Lin B. J. Liu B. X. Liu C. Liu C. X. Liu F. Liu F. H. Liu Feng Liu G. M. Liu H. Liu H. B. Liu H. H. Liu H. M. Liu Huihui Liu J. B. Liu J. J. Liu K. Liu K. Y. Liu Ke Liu L. C. Liu Lu Liu M. H. Liu P. L. Liu Q. Liu S. B. Liu T. Liu W. K. Liu W. M. Liu W. T. Liu X. Liu X. K. Liu X. Y. Liu Y. Liu Y. B. Liu Z. A. Liu Z. D. Liu Z. Q. Liu X. C. Lou F. X. Lu H. J. Lu J. G. Lu X. L. Lu Y. Lu Y. H. Lu Y. P. Lu Z. H. Lu C. L. Luo J. R. Luo J. S. Luo M. X. Luo T. Luo X. L. Luo Z. Y. Lv X. R. Lyu Y. F. Lyu Y. H. Lyu F. C. Ma H. L. Ma J. L. Ma L. L. Ma L. R. Ma Q. M. Ma R. Q. Ma R. Y. Ma T. Ma X. T. Ma X. Y. Ma Y. M. Ma F. E. Maas I. Mackay M. Maggiora S. Malde Q. A. Malik H. X. Mao Y. J. Mao Z. P. Mao S. Marcello A. Marshall F. M. Melendi Y. H. Meng Z. X. Meng G. Mezzadri H. Miao T. J. Min R. E. Mitchell X. H. Mo B. Moses N. Yu. Muchnoi J. Muskalla Y. Nefedov F. Nerling L. S. Nie I. B. Nikolaev Z. Ning S. Nisar Q. L. Niu W. D. Niu C. Normand S. L. Olsen Q. Ouyang S. Pacetti X. Pan Y. Pan A. Pathak Y. P. Pei M. Pelizaeus H. P. Peng X. J. Peng Y. Y. Peng K. Peters K. Petridis J. L. Ping R. G. Ping S. Plura V. Prasad F. Z. Qi H. R. Qi M. Qi S. Qian W. B. Qian C. F. Qiao J. H. Qiao J. J. Qin J. L. Qin L. Q. Qin L. Y. Qin P. B. Qin X. P. Qin X. S. Qin Z. H. Qin J. F. Qiu Z. H. Qu J. Rademacker C. F. Redmer A. Rivetti M. Rolo G. Rong S. S. Rong F. Rosini Ch. Rosner M. Q. Ruan N. Salone A. Sarantsev Y. Schelhaas K. Schoenning M. Scodeggio K. Y. Shan W. Shan X. Y. Shan Z. J. Shang J. F. Shangguan L. G. Shao M. Shao C. P. Shen H. F. Shen W. H. Shen X. Y. Shen B. A. Shi H. Shi J. L. Shi J. Y. Shi S. Y. Shi X. Shi H. L. Song J. J. Song T. Z. Song W. M. Song Y. J. Song Y. X. Song S. Sosio S. Spataro F. Stieler S. S Su Y. J. Su G. B. Sun G. X. Sun H. Sun H. K. Sun J. F. Sun K. Sun L. Sun S. S. Sun T. Sun Y. C. Sun Y. H. Sun Y. J. Sun Y. Z. Sun Z. Q. Sun Z. T. Sun C. J. Tang G. Y. Tang J. Tang J. J. Tang L. F. Tang Y. A. Tang L. Y. Tao M. Tat J. X. Teng J. Y. Tian W. H. Tian Y. Tian Z. F. Tian I. Uman B. Wang Bo Wang C. Wang Cong Wang D. Y. Wang H. J. Wang J. J. Wang K. Wang L. L. Wang L. W. Wang M. Wang N. Y. Wang S. Wang T. Wang T. J. Wang W. Wang W. P. Wang X. Wang X. F. Wang X. J. Wang X. L. Wang X. N. Wang Y. Wang Y. D. Wang Y. F. Wang Y. H. Wang Y. J. Wang Y. L. Wang Y. N. Wang Y. Q. Wang Yaqian Wang Yi Wang Yuan Wang Z. Wang Z. L. Wang Z. Q. Wang Z. Y. Wang D. H. Wei H. R. Wei F. Weidner S. P. Wen Y. R. Wen U. Wiedner G. Wilkinson M. Wolke C. Wu J. F. Wu L. H. Wu L. J. Wu Lianjie Wu S. G. Wu S. M. Wu X. Wu X. H. Wu Y. J. Wu Z. Wu L. Xia X. M. Xian B. H. Xiang D. Xiao G. Y. Xiao H. Xiao Y. L. Xiao Z. J. Xiao C. Xie K. J. Xie X. H. Xie Y. Xie Y. G. Xie Y. H. Xie Z. P. Xie T. Y. Xing C. F. Xu C. J. Xu G. F. Xu H. Y. Xu M. Xu Q. J. Xu Q. N. Xu T. D. Xu W. Xu W. L. Xu X. P. Xu Y. Xu Y. C. Xu Z. S. Xu F. Yan H. Y. Yan L. Yan W. B. Yan W. C. Yan W. H. Yan W. P. Yan X. Q. Yan H. J. Yang H. L. Yang H. X. Yang J. H. Yang R. J. Yang T. Yang Y. Yang Y. F. Yang Y. H. Yang Y. Q. Yang Y. X. Yang Y. Z. Yang M. Ye M. H. Ye Z. J. Ye Junhao Yin Z. Y. You B. X. Yu C. X. Yu G. Yu J. S. Yu L. Q. Yu M. C. Yu T. Yu X. D. Yu Y. C. Yu C. Z. Yuan H. Yuan J. Yuan L. Yuan S. C. Yuan X. Q. Yuan Y. Yuan Z. Y. Yuan C. X. Yue Ying Yue A. A. Zafar S. H. Zeng X. Zeng Y. Zeng Y. J. Zeng X. Y. Zhai Y. H. Zhan A. Q. Zhang B. L. Zhang B. X. Zhang D. H. Zhang G. Y. Zhang H. Zhang H. C. Zhang H. H. Zhang H. Q. Zhang H. R. Zhang H. Y. Zhang J. Zhang J. J. Zhang J. L. Zhang J. Q. Zhang J. S. Zhang J. W. Zhang J. X. Zhang J. Y. Zhang J. Z. Zhang Jianyu Zhang L. M. Zhang Lei Zhang N. Zhang P. Zhang Q. Zhang Q. Y. Zhang R. Y. Zhang S. H. Zhang Shulei Zhang X. M. Zhang X. Y Zhang X. Y. Zhang Y. Zhang Y. T. Zhang Y. H. Zhang Y. M. Zhang Y. P. Zhang Z. D. Zhang Z. H. Zhang Z. L. Zhang Z. X. Zhang Z. Y. Zhang Z. Z. Zhang Zh. Zh. Zhang G. Zhao J. Y. Zhao J. Z. Zhao L. Zhao M. G. Zhao N. Zhao R. P. Zhao S. J. Zhao Y. B. Zhao Y. L. Zhao Y. X. Zhao Z. G. Zhao A. Zhemchugov B. Zheng B. M. Zheng J. P. Zheng W. J. Zheng X. R. Zheng Y. H. Zheng B. Zhong C. Zhong H. Zhou J. Q. Zhou J. Y. Zhou S. Zhou X. Zhou X. K. Zhou X. R. Zhou X. Y. Zhou Y. X. Zhou Y. Z. Zhou A. N. Zhu J. Zhu K. Zhu K. J. Zhu K. S. Zhu L. Zhu L. X. Zhu S. H. Zhu T. J. Zhu W. D. Zhu W. J. Zhu W. Z. Zhu Y. C. Zhu Z. A. Zhu X. Y. Zhuang J. H. Zou J. Zu
This is my paper

Pith reviewed 2026-05-19 05:04 UTC · model grok-4.3

classification ✦ hep-ex
keywords radiative decayLambda(1520)Lambda(1670)branching fractionelectromagnetic transitionflavor SU(3) symmetryhyperon resonanceinvariant mass spectrum
0
0 comments X

The pith

The first observation of radiative decays from the Λ(1520) and Λ(1670) to γΣ⁰ measures a branching fraction for the former that conflicts with relativized constituent quark model predictions.

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

This paper establishes the first observation of the electromagnetic radiative decays of the Λ(1520) and Λ(1670) hyperons to a photon and Σ⁰. Using a large sample of J/ψ events, the branching fraction for Λ(1520) → γΣ⁰ is determined to be (2.95 ± 0.28 ± 0.56) × 10^{-3}, corresponding to a partial width of about 47 keV. This value disagrees with expectations from the relativized constituent quark model and the algebraic model. The ratio of the branching fraction for Λ(1520) → γΛ to that for Λ(1520) → γΣ⁰ is measured as 2.88, which aligns with flavor SU(3) symmetry. A resonant structure near 1.67 GeV/c² in the γΣ⁰ spectrum is identified with the Λ(1670), enabling the first measurement of the product branching fraction from J/ψ production, while an upper limit is placed on the corresponding γΛ mode.

Core claim

The paper reports the observation of Λ(1520) → γΣ⁰ with 16.6σ significance and Λ(1670) → γΣ⁰ with 23.5σ significance. It measures B(Λ(1520)→γΣ⁰) = (2.95±0.28±0.56)×10^{-3} and the partial width Γ(Λ(1520)→γΣ⁰) = 47.2 keV, values inconsistent with relativized constituent quark model and algebraic model predictions. The ratio B(Λ(1520)→γΛ)/B(Λ(1520)→γΣ⁰) = 2.88 agrees with SU(3) symmetry. The product branching fraction B(J/ψ → Λ¯Λ(1670)+c.c.) × B(Λ(1670)→γΣ⁰) is measured as (5.39±0.29±0.44)×10^{-6}, with an upper limit of 5.97×10^{-7} at 90% CL for the γΛ channel.

What carries the argument

The γΣ⁰ invariant mass spectrum, with fits extracting resonant contributions, branching fractions, and statistical significances from the data.

If this is right

  • The measured partial width supplies a new benchmark for refining theoretical calculations of radiative transitions in excited hyperons.
  • The agreement with SU(3) symmetry supports applying flavor symmetry relations to predict rates for related baryon decays.
  • The absence of a visible structure in the γΛ channel for the Λ(1670) points to decay-mode preferences that must be explained by models.
  • These branching fractions can be combined with other data to test the internal quark configuration of the Λ(1520) and Λ(1670).

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Persistent disagreement with quark models may indicate that additional effects, such as meson-baryon components, are needed in the description of these states.
  • Repeating the measurement with different production mechanisms could confirm the extracted rates and reduce systematic uncertainties.
  • The upper limit on the γΛ mode for Λ(1670) suggests possible suppression mechanisms that current models do not fully predict.

Load-bearing premise

The resonant structure around 1.67 GeV/c² is assumed to arise solely from the Λ(1670) without significant interference from other resonances or non-resonant backgrounds.

What would settle it

An independent experiment measuring the branching fraction of Λ(1520) → γΣ⁰ to a value consistent with relativized constituent quark model predictions would contradict the reported inconsistency.

Figures

Figures reproduced from arXiv: 2507.11145 by A. Amoroso, A. A. Zafar, A. Bortone, A. Brueggemann, A. Calcaterra, A. Dbeyssi, A. Denig, A. Gilman, A. Guskov, A. Khoukaz, A. Kupsc, A. Limphirat, A. Marshall, A. N. Zhu, A. Pathak, A. Q. Guo, A. Q. Zhang, A. Rivetti, A. Sarantsev, A. Zhemchugov, B. A. Shi, B. C. Ke, B. Ding, BESIII Collaboration: M. Ablikim, B. H. Xiang, B. J. Liu, B. Kopf, B. L. Zhang, B. Moses, B. M. Zheng, Bo Wang, B. Wang, B. X. Liu, B. X. Yu, B. X. Zhang, B. Zheng, B. Zhong, C. C. Lin, C. D. Fu, C. F. Qiao, C. F. Redmer, C. F. Xu, C. Geng, Chao Chen, C. H. Chen, C. Herold, C. H. Heinz, C. H. Li, Ch. Rosner, C. J. Tang, C. J. Xu, C. K. Li, C. Li, C. Liu, C. L. Luo, C. Normand, Cong Wang, C. P. Shen, C. Q. Deng, C. Q. Feng, C. Wang, C. Wu, C. Xie, C. X. Liu, C. X. Yu, C. X. Yue, C. Y. Guan, C. Zhong, C. Z. Yuan, D. Bettoni, D. Dedovich, D. H. Wei, D. H. Zhang, D. Jiang, D. M. Li, D. Xiao, D. X. Lin, D. Y. Wang, E. Bianco, E. M. Gersabeck, F. A. Harris, F. Bianchi, F. C. Ma, F. Cossio, F. De Mori, F. E. Maas, Feng Liu, F. Feldbauer, F. Hanisch, F. H. Heinsius, F. H. Liu, F. Li, F. Liu, F. M. Melendi, F. Nerling, F. Rosini, F. Stieler, F. Weidner, F. X. Lu, F. Yan, F. Z. Qi, G. B. Sun, G. Chen, G. Cibinetto, G. F. Cao, G. Felici, G. F. Fan, G. F. Xu, G. Li, G. Mezzadri, G. M. Liu, G. R. Che, G. R. Liao, G. Rong, G. S. Huang, G. Wilkinson, G. X. Sun, G. Y. Hou, G. Y. Tang, G. Yu, G. Y. Xiao, G. Y. Zhang, G. Zhao, H. B. Jiang, H. B. Li, H. B. Liu, H. Cai, H. C. Zhang, H. F. Shen, H. Gao, H. H. Liu, H. H. Zhang, H. J. Li, H. J. Lu, H. J. Wang, H. J. Yang, H. K. Sun, H. L. Dai, H. Liang, H. Liu, H. L. Ma, H. L. Song, H. L. Yang, H. M. Hu, H. Miao, H. M. Liu, H. N. Li, H. P. Peng, H. Q. Zhang, H.-R. Bao, H. R. Qi, H. R. Wei, H. R. Zhang, H. S. Chen, H. Shi, H. Sun, Huihui Liu, Hui Li, H. Xiao, H. X. Mao, H. X. Yang, H. Y. Chen, H. Yuan, H. Y. Xu, H. Y. Yan, H. Y. Zhang, H. Zhang, H. Zhou, I. B. Nikolaev, I. Boyko, I. Denysenko, I. Garzia, I. Mackay, I. Uman, J. B. Jiao, J. B. Liu, J. Cottee-Meldrum, J. D. Gong, J. Dong, J. Fang, J. F. Chang, J. F. Hu, J. F. Qiu, J. F. Shangguan, J. F. Sun, J. F. Wu, J. G. Lu, J. Gutierrez, J. H. Feng, J. H. Qiao, J. H. Yang, J. H. Zou, Jianyu Zhang, J. Jackson, J. J. Cui, J. J. Fan, J. J. Liu, J. J. Qin, J. J. Song, J. J. Tang, J. J. Wang, J. J. Zhang, J. K. Jiao, J. L. Fu, J. Libby, J. L. Ma, J. L. Ping, J. L. Qin, J. L. Shi, J. L. Zhang, J. Muskalla, J. P. Dai, J. P. Zheng, J. Q. Zhang, J. Q. Zhou, J. Rademacker, J. R. Li, J. R. Luo, J. S. Li, J. S. Luo, J. S. Yu, J. S. Zhang, J. Tang, Junhao Yin, J. W. Zhang, J. X. Teng, J. X. Zhang, J. Y. Shi, J. Y. Tian, J. Yuan, J. Y. Zhang, J. Y. Zhao, J. Y. Zhou, J. Zhang, J. Zhu, J. Zu, J. Z. Zhang, J. Z. Zhao, K. Begzsuren, K. D. Hao, Ke Liu, K. Goetzen, K. J. Xie, K. J. Zhu, K. K. He, K. L. Han, K. L. He, K. Li, K. Liu, K. L. Li, K. Peters, K. Petridis, K. Schoenning, K. Sun, K. S. Zhu, K. Wang, K. X. Huang, K. Y. Liu, K. Y. Shan, K. Zhu, L. B. Guo, L. B. Liao, L. C. Liu, Lei Li, Lei Zhang, L. Fava, L. Feng, L. F. Tang, L. Gong, L. G. Shao, L. H. Wu, Lianjie Wu, L. J. Li, L. J. Wu, L. L. Ma, L. L. Wang, L. M. Zhang, L. Q. Huang, L. Q. Lin, L. Q. Qin, L. Q. Yu, L. R. Ma, L. S. Nie, L. Sun, Lu Liu, L. W. Wang, L. Xia, L. X. Zhu, L. Yan, L. Y. Dong, L. Y. Qin, L. Y. Tao, L. Yuan, L. Zhao, L. Zhu, M. Berlowski, M. Bertani, M. C. Du, M. C. Yu, M. Destefanis, M. Fritsch, M. Greco, M. G. Zhao, M. H. Cai, M. H. Gu, M. H. Li, M. H. Liao, M. H. Liu, M. H. Ye, M. J. Guo, M. Kavatsyuk, M. Kuessner, M. L. Chen, M. Lellmann, M. Maggiora, M. N. Achasov, M. Pelizaeus, M. Qi, M. Q. Jing, M. Q. Ruan, M. R. Li, M. Rolo, M. Scodeggio, M. Shao, M. Tat, M. Wang, M. Wolke, M. X. Luo, M. Xu, M. Y. Dong, M. Ye, N. Berger, N. Cao, N. H\"usken, N. in der Wiesche, N. Kalantar-Nayestanaki, N. Kumar, N. Salone, N. Yu. Muchnoi, N. Y. Wang, N. Zhang, N. Zhao, O. Bakina, O. B. Kolcu, P. Adlarson, P. B. Qin, P. C. Hong, P. C. Jiang, P. Egorov, P. Huang, P. L. Li, P. L. Liu, P. R. Li, P. T. Ge, P. Zhang, Q. A. Malik, Q. An, Q. Ji, Q. J. Xu, Q. Lan, Q. Liu, Q. L. Niu, Q. M. Li, Q. M. Ma, Q. N. Xu, Q. Ouyang, Q. P. Hu, Q. P. Ji, Q. X. Feng, Q. X. Li, Q. Y. Zhang, Q. Zhang, R. A. Briere, R. Aliberti, R. E. de Boer, R. E. Mitchell, R. Farinelli, R. G. Ping, R. J. Yang, R. Kiuchi, R. Li, R. P. Guo, R. P. Zhao, R. Q. Ma, R. Y. Ma, R. Y. Zhang, S. A. Cetin, S. B. Liu, S. C. Yuan, S. Garbolino, S. Gramigna, S. G. Wu, Shulei Zhang, S. H. Zeng, S. H. Zhang, S. H. Zhu, S. J. Chen, S. Jin, S. J. Jiang, S. J. Zhao, S. Kabana, S. K. Choi, S. L. Chen, S. L. Hu, S. L. Olsen, S. Malde, S. Marcello, S. M. Chen, S. M. Wu, S. Nisar, S. Pacetti, S. Plura, S. P. Wen, S. Qian, S. S. Fang, S. Sosio, S. Spataro, S. S. Rong, S. S Su, S. S. Sun, S. Wang, S. X. Du, S. X. Li, S. Y. Shi, S. Zhou, T. Chen, T. D. Xu, T. Hu, T. Hussain, T. J. Jiang, T. J. Min, T. Johansson, T. J. Wang, T. J. Zhu, T. Lenz, T. Li, T. Lin, T. Liu, T. Luo, T. Ma, T. Sun, T. T. Han, T. T. Lei, T. Wang, T. Yang, T. Y. Li, T. Yu, T. Y. Xing, T. Z. Song, U. Wiedner, V. Batozskaya, V. Khachatryan, V. Prasad, W. B. Qian, W. B. Yan, W. C. Yan, W. D. Li, W. D. Niu, W. D. Zhu, W. G. Li, W. Gradl, W. H. Shen, W. H. Tian, W. H. Yan, W. Ji, W. J. Zheng, W. J. Zhu, W. K. Liu, W. K\"uhn, W. L. Xu, W. M. Liu, W. M. Song, W. N. Lan, W. P. Wang, W. P. Yan, W. Shan, W. T. Liu, W. Wang, W. X. Fang, W. X. Gong, W. Xu, W. Z. Zhu, X. B. Gao, X. B. Ji, X. Cai, X. C. Ai, X. Chu, X. C. Lou, X. Dong, X. D. Yu, X. F. Wang, X. H. Li, X. H. Mo, X. H. Wu, X. H. Xie, X. J. Peng, X. J. Wang, X. K. Liu, X. Kui, X. K. Zhou, X. Li, X. Liu, X. L. Ji, X. L. Kang, X. L. Li, X. L. Lu, X. L. Luo, X. L. Wang, X. M. Jing, X. M. Xian, X. M. Zhang, X. N. Wang, X. Pan, X. P. Qin, X. P. Xu, X. Q. Hao, X. Q. Yan, X. Q. Yuan, X. R. Chen, X. R. Lyu, X. R. Zheng, X. R. Zhou, X. Shi, X. S. Jiang, X. S. Kang, X. S. Qin, X. T. Chen, X. T. Hou, X. T. Huang, X. T. Ma, X. Wang, X. Wu, X. X. Ding, X. Y. Chai, X. Y. Chen, X. Y. Li, X. Y. Liu, X. Y. Ma, X. Y. Shan, X. Y. Shen, X. Y. Zhai, X. Y Zhang, X. Y. Zhang, X. Y. Zhou, X. Y. Zhuang, X. Zeng, X. Zhou, X. Z. Li, Yaqian Wang, Y. A. Tang, Y. Bai, Y. Ban, Y. B. Chen, Y. B. Liu, Y. B. Zhao, Y. C. Sun, Y. C. Xu, Y. C. Yu, Y. C. Zhu, Y. Ding, Y. D. Wang, Y. F. Liang, Y. F. Lyu, Y. F. Wang, Y. F. Yang, Y. Gao, Y. G. Li, Y. G. Xie, Y. H. Fan, Y. H. Lu, Y. H. Lyu, Y. H. Meng, Y. H. Sun, Y. Hu, Y. H. Wang, Y. H. Xie, Y. H. Yang, Y. H. Zhan, Y. H. Zhang, Y. H. Zheng, Ying Yue, Yi Wang, Y. Jiang, Y. Jin, Y. J. Mao, Y. J. Song, Y. J. Su, Y. J. Sun, Y. J. Wang, Y. J. Wu, Y. J. Zeng, Y. K. Heng, Y. Li, Y. Liu, Y. Lu, Y. L. Wang, Y. L. Xiao, Y. L. Zhao, Y. M. Ma, Y. M. Zhang, Y. Nefedov, Y. N. Gao, Y. N. Wang, Y. Pan, Y. P. Guo, Y. P. Huang, Y. P. Li, Y. P. Liao, Y. P. Lu, Y. P. Pei, Y. P. Zhang, Y. Q. Chen, Y. Q. Fang, Y. Q. Wang, Y. Q. Yang, Y. R. Hou, Y. R. Wen, Y. Schelhaas, Y. S. Huang, Y. T. Feng, Y. T. Gu, Y. Tian, Y. T. Liang, Y. T. Zhang, Yuan Wang, Y. Wang, Y. W. Fu, Y. X. Ding, Y. Xie, Y. X. Song, Y. Xu, Y. X. Yang, Y. X. Zhao, Y. X. Zhou, Y. Yang, Y. Y. Duan, Y. Y. Gao, Y. Y. Ji, Y. Y. Peng, Y. Yuan, Y. Z. Che, Y. Zeng, Y. Zhang, Y. Z. Sun, Y. Z. Yang, Y. Z. Zhou, Z. A. Liu, Z. A. Zhu, Z. Chen, Z. D. Liu, Z. D. Zhang, Z. F. Tian, Z. G. Zhao, Z. H. Lu, Z. H. Qin, Z. H. Qu, Z. H. Zhang, Zh. Zh. Zhang, Z. J. Chen, Z. Jiao, Z. J. Li, Z. J. Shang, Z. J. Xiao, Z. J. Ye, Z. K. Chen, Z. K. Jia, Z. L. Hou, Z. L. Wang, Z. L. Zhang, Z. M. Hu, Z. Ning, Z. P. Mao, Z. P. Xie, Z. Q. Liu, Z. Q. Sun, Z. Q. Wang, Z. S. Xu, Z. T. Sun, Z. Wang, Z. W. Ge, Z. Wu, Z. X. Meng, Z. X. Zhang, Z. Y. Deng, Z. Y. Li, Z. Y. Lv, Z. Y. Wang, Z. Y. You, Z. Y. Yuan, Z. Y. Zhang, Z. Z. Zhang.

Figure 1
Figure 1. Figure 1: FIG. 1. Fit result of [PITH_FULL_IMAGE:figures/full_fig_p005_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Fit result of [PITH_FULL_IMAGE:figures/full_fig_p006_2.png] view at source ↗
read the original abstract

Using $(10087\pm 44)\times10^6$ $J/\psi$ events collected with the BESIII detector, we report the first observation of the electromagnetic radiative decays of the $\Lambda(1520)$ and $\Lambda(1670)$ to $\gamma\Sigma^0$, with a statistical significance of $16.6\sigma$ and $23.5\sigma$, respectively. The ratio of the branching fractions $\frac{\mathcal{B}(\Lambda(1520)\to\gamma\Lambda)}{\mathcal{B}(\Lambda(1520)\to\gamma\Sigma^0)}$ is determined to be $2.88\pm0.27(\text{stat.})\pm0.21(\text{syst.})$, which is in good agreement with flavor SU(3) symmetry. The branching fraction of $\Lambda(1520)\to\gamma\Sigma^0$ is measured to be $\mathcal{B}(\Lambda(1520)\to\gamma\Sigma^0)=(2.95\pm0.28(\text{stat.})\pm0.56(\text{syst.}))\times 10^{-3}$, corresponding to a partial width of $\Gamma(\Lambda(1520)\to\gamma\Sigma^0)=(47.2\pm4.5(\text{stat.})\pm9.0(\text{syst.}))$ keV, which is inconsistent with predictions from the relativized constituent quark model and the Algebraic model. Additionally, we observe a clear resonant structure in the $\gamma\Sigma^0$ mass spectrum around 1.67 GeV/$c^2$, attributed to the $\Lambda(1670)$. The product branching fraction $\mathcal{B}(J/\psi\to\bar\Lambda\Lambda(1670)+c.c.)\times\mathcal{B}(\Lambda(1670)\to\gamma\Sigma^0)$ is measured for the first time as $(5.39\pm0.29(\text{stat.})\pm 0.44(\text{syst.}))\times 10^{-6}$. However, no corresponding structure is seen in the $\gamma\Lambda$ mass spectrum, so an upper limit on the product branching fraction $\mathcal{B}(J/\psi\to\bar\Lambda\Lambda(1670)+c.c.)\times\mathcal{B}(\Lambda(1670)\to\gamma\Lambda)$ is determined to be $5.97\times10^{-7}$ at the 90\% confidence level.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 1 minor

Summary. The paper reports the first observation of the electromagnetic radiative decays Λ(1520) → γΣ⁰ and Λ(1670) → γΣ⁰ in a sample of (10087 ± 44) × 10^6 J/ψ events collected with BESIII. It measures B(Λ(1520) → γΣ⁰) = (2.95 ± 0.28 ± 0.56) × 10^{-3} (16.6σ), the ratio B(Λ(1520)→γΛ)/B(Λ(1520)→γΣ⁰) = 2.88 ± 0.27 ± 0.21 consistent with SU(3), the product branching fraction B(J/ψ → Λ-bar Λ(1670) + c.c.) × B(Λ(1670) → γΣ⁰) = (5.39 ± 0.29 ± 0.44) × 10^{-6} (23.5σ), and an upper limit B(J/ψ → Λ-bar Λ(1670) + c.c.) × B(Λ(1670) → γΛ) < 5.97 × 10^{-7} (90% CL).

Significance. If the central results hold, the work supplies the first experimental constraints on these radiative transitions, enabling direct tests of quark-model predictions and SU(3) relations for hyperon electromagnetic decays. The large data set and high statistical significances constitute a clear experimental advance; the measured ratio agreeing with flavor symmetry and the partial width for Λ(1520) → γΣ⁰ being inconsistent with the relativized constituent quark model and Algebraic model are both useful for theory.

major comments (1)
  1. [γΣ⁰ mass-spectrum fit] In the fit to the γΣ⁰ invariant-mass spectrum (results section), the resonant structure near 1.67 GeV/c² is attributed entirely to the Λ(1670) lineshape. The extraction of the product branching fraction (5.39 ± 0.29 ± 0.44) × 10^{-6} and the quoted 23.5σ significance rest on the assumption that interference with nearby resonances, non-resonant contributions, or feed-down are negligible. No explicit test of alternative models (e.g., inclusion of interference phases or additional resonant components) is described; this assumption is load-bearing for the Λ(1670) claim.
minor comments (1)
  1. [Abstract] The abstract states that no corresponding structure is seen in the γΛ spectrum; a brief quantitative statement on the background level or fit quality in that channel would help readers assess the upper-limit procedure.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for the positive assessment of the scientific impact and for the constructive comment on the γΣ⁰ mass-spectrum fit. We address the concern point by point below and have revised the manuscript accordingly.

read point-by-point responses
  1. Referee: [γΣ⁰ mass-spectrum fit] In the fit to the γΣ⁰ invariant-mass spectrum (results section), the resonant structure near 1.67 GeV/c² is attributed entirely to the Λ(1670) lineshape. The extraction of the product branching fraction (5.39 ± 0.29 ± 0.44) × 10^{-6} and the quoted 23.5σ significance rest on the assumption that interference with nearby resonances, non-resonant contributions, or feed-down are negligible. No explicit test of alternative models (e.g., inclusion of interference phases or additional resonant components) is described; this assumption is load-bearing for the Λ(1670) claim.

    Authors: We agree that explicit validation of the fit assumptions strengthens the result. In the revised manuscript we have added a dedicated subsection (now Section 4.3) that describes alternative fits performed on the γΣ⁰ mass spectrum. These include: (i) allowing a coherent interference phase between the Λ(1670) amplitude and a non-resonant background component, (ii) adding a second resonant term with free mass and width in the 1.65–1.70 GeV/c² region to test for possible contributions from Λ(1690) or Σ(1660), and (iii) replacing the nominal background polynomial with a higher-order function or an ARGUS-shaped background. In all cases the extracted product branching fraction varies by at most 8 %, which is already encompassed by the quoted systematic uncertainty. The statistical significance remains above 20σ under these variations. We have also verified that feed-down from known higher-mass hyperons is negligible given the kinematic selection and sideband subtraction. These tests are now documented with figures and tables in the supplementary material. revision: yes

Circularity Check

0 steps flagged

Direct experimental measurement from data fits; no circular derivation chain

full rationale

This is a standard experimental particle physics paper reporting first observations and branching fraction measurements extracted from BESIII J/psi data via invariant-mass spectrum fits and event yields. The central results (16.6σ and 23.5σ significances, product branching fractions) are obtained by fitting resonant structures in γΣ⁰ and γΛ spectra and normalizing to known decays; these steps are data-driven and externally falsifiable. No theoretical derivation, ansatz, or prediction reduces to its own inputs by construction. Self-citations are limited to standard detector or analysis references and are not load-bearing for the claims. The fit assumptions (e.g., attributing the 1.67 GeV peak solely to Λ(1670)) represent modeling choices subject to systematic uncertainty, not circular logic. The paper is self-contained against external benchmarks.

Axiom & Free-Parameter Ledger

1 free parameters · 2 axioms · 0 invented entities

As an experimental observation paper based on abstract only, the claims rest on standard particle physics analysis assumptions for signal extraction rather than new theoretical axioms or free parameters beyond fit yields.

free parameters (1)
  • signal yields in mass spectrum fits
    Event yields for the resonances are determined from fits to data; these are the primary measured quantities rather than inputs.
axioms (2)
  • domain assumption The observed peaks in the γΣ⁰ invariant mass spectrum correspond to the known Λ(1520) and Λ(1670) resonances with PDG parameters.
    Invoked when fitting the mass spectra to extract branching fractions and significances.
  • domain assumption Background contributions and detector efficiencies are accurately estimated using standard simulation and sideband methods.
    Required for converting observed yields to branching fractions.

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Works this paper leans on

28 extracted references · 28 canonical work pages

  1. [1]

    Bertini, Nucl

    R. Bertini, Nucl. Phys. B279, 49 (1987)

  2. [2]

    Isgur and G

    N. Isgur and G. Karl, Phys. Rev. D18, 4187 (1978)

  3. [3]

    Isgur and G

    N. Isgur and G. Karl, Phys. Rev. D20, 1191 (1979)

  4. [4]

    L. Yu, X. L. Chen, W. Z. Deng, and S. L. Zhu, Phys. Rev. D73, 114001 (2006)

  5. [5]

    Ablikimet al.(BESIII Collaboration), Phys

    M. Ablikimet al.(BESIII Collaboration), Phys. Rev. Lett.130, 211901 (2023)

  6. [6]

    Ablikimet al.(BESIII Collaboration), Phys

    M. Ablikimet al.(BESIII Collaboration), Phys. Rev. Lett.129, 212002 (2022)

  7. [7]

    Tayloret al.(CLAS Collaboration), Phys

    S. Tayloret al.(CLAS Collaboration), Phys. Rev. C71, 054609 (2005)

  8. [8]

    L. G. Landsberg, Phys. Atom. Nucl.59, 2080 (1996)

  9. [9]

    Ablikimet al.(BESIII Collaboration), Chin

    M. Ablikimet al.(BESIII Collaboration), Chin. Phys. C 46, 074001 (2022)

  10. [10]

    Kaxiras, E

    E. Kaxiras, E. J. Moniz, and M. Soyeur, Phys. Rev. D 32, 695 (1985)

  11. [11]

    J. W. Darewych, M. Horbatsch, and R. Koniuk, Phys. Rev. D28, 1125 (1983)

  12. [12]

    Warns, W

    M. Warns, W. Pfeil, and H. Rollnik, Phys. Lett. B258, 431 (1991)

  13. [13]

    Umino and F

    Y. Umino and F. Myhrer, Nucl. Phys. A529, 713 (1991)

  14. [14]

    Bijker, F

    R. Bijker, F. Iachello, and A. Leviatan, Annals Phys. 284, 89 (2000)

  15. [15]

    Ablikimet al.(BESIII Collaboration), Nucl

    M. Ablikimet al.(BESIII Collaboration), Nucl. Instrum. Meth. A614, 345 (2010)

  16. [16]

    Ablikimet al

    M. Ablikimet al. (BESIII Collaboration), Chin. Phys. C 44, 040001 (2020)

  17. [17]

    Agostinelliet al.(GEANT4 Collaboration), Nucl

    S. Agostinelliet al.(GEANT4 Collaboration), Nucl. In- strum. Meth. A506, 250 (2003)

  18. [18]

    D. J. Lange, Nucl. Instrum. Meth. A462, 152 (2001)

  19. [19]

    R. G. Ping, Chin. Phys. C32, 599 (2008)

  20. [20]

    Xuet al., Chin

    M. Xuet al., Chin. Phys. C33, 428 (2009)

  21. [21]

    Navaset al.(Particle Data Group), Phys

    S. Navaset al.(Particle Data Group), Phys. Rev. D110, 030001 (2024)

  22. [22]

    J. C. Chen, G. S. Huang, X. R. Qi, D. H. Zhang, and Y. S. Zhu, Phys. Rev. D62, 034003 (2000)

  23. [23]

    R. L. Yang, R. G. Ping, and H. Chen, Chin. Phys. Lett. 31, 061301 (2014)

  24. [24]

    Y. S. Zhu, Chin. Phys. C32, 363 (2008)

  25. [25]

    Ablikimet al.(BESIII Collaboration), Phys

    M. Ablikimet al.(BESIII Collaboration), Phys. Rev. D 83, 112005 (2011)

  26. [26]

    Ablikimet al.(BESIII Collaboration), Phys

    M. Ablikimet al.(BESIII Collaboration), Phys. Rev. D 87, 012002 (2013)

  27. [27]

    J. G. Korner, Z. Phys. C33, 529 (1987)

  28. [28]

    Carimalo, Int

    C. Carimalo, Int. J. Mod. Phys. A2, 249 (1987)