Measurement of time-dependent $CP$ violation parameters in B0KS0π0γB^{0} \to K_{S}^{0} \pi^{0} \gamma decays at Belle and Belle II

Using combined datasets from the Belle and Belle II experiments, this study presents the most precise measurements to date of time-dependent $CP$ violation parameters in B0KS0π0γB^{0} \to K_{S}^{0} \pi^{0} \gamma decays, finding results consistent with Standard Model predictions across both K0(892)K^{*0}(892)-dominated and non-resonant regions.

Original authors: Belle, Belle II Collaborations, :, M. Abumusabh, I. Adachi, A. Aggarwal, Y. Ahn, H. Aihara, M. Akdag, N. Akopov, S. Alghamdi, M. Alhakami, N. Althubiti, K. Amos, M. Angelsmark, N. Anh Ky, C. Antoniol
Published 2026-06-04
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Original authors: Belle, Belle II Collaborations, :, M. Abumusabh, I. Adachi, A. Aggarwal, Y. Ahn, H. Aihara, M. Akdag, N. Akopov, S. Alghamdi, M. Alhakami, N. Althubiti, K. Amos, M. Angelsmark, N. Anh Ky, C. Antonioli, K. Arai, H. Atmacan, V. Aushev, R. Ayad, V. Babu, H. Bae, N. K. Baghel, S. Bahinipati, P. Bambade, Sw. Banerjee, S. Bansal, M. Barrett, M. Bartl, J. Baudot, A. Beaubien, F. Becherer, J. Becker, G. F. Benfratello, J. V. Bennett, F. U. Bernlochner, V. Bertacchi, M. Bertemes, E. Bertholet, M. Bessner, S. Bettarini, V. Bhardwaj, B. Bhuyan, F. Bianchi, T. Bilka, D. Biswas, A. Bobrov, D. Bodrov, A. Bondar, G. Bonvicini, J. Borah, A. Boschetti, A. Bozek, M. Bračko, P. Branchini, N. Brenny, R. A. Briere, T. E. Browder, A. Budano, S. Bussino, F. Callet, Q. Campagna, M. Campajola, L. Cao, M. Carminati, G. Casarosa, C. Cecchi, P. Cheema, L. Chen, B. G. Cheon, C. Cheshta, H. Chetri, K. Chilikin, K. Chirapatpimol, H. -E. Cho, K. Cho, S. -J. Cho, S. -K. Choi, S. Choudhury, S. Chutia, J. Cochran, J. A. Colorado-Caicedo, I. Consigny, L. Corona, H. Crotte Ledesma, S. Cuccuini, J. X. Cui, S. Das, E. De La Cruz-Burelo, S. A. De La Motte, G. de Marino, G. De Nardo, G. De Pietro, R. de Sangro, M. Destefanis, S. Dey, R. Dhayal, A. Di Canto, J. Dingfelder, Z. Doležal, X. Dong, M. Dorigo, G. Dujany, P. Ecker, D. Epifanov, J. Eppelt, R. Farkas, P. Feichtinger, T. Ferber, T. Fillinger, C. Finck, G. Finocchiaro, F. Forti, A. Frey, B. G. Fulsom, A. Gabrielli, P. Gagneja, E. Ganiev, R. Garg, G. Gaudino, V. Gaur, V. Gautam, A. Gaz, A. Gellrich, G. Ghevondyan, D. Ghosh, H. Ghumaryan, R. Giordano, A. Giri, P. Gironella Gironell, B. Gobbo, R. Godang, O. Gogota, W. Gradl, E. Graziani, D. Greenwald, Y. Guan, K. Gudkova, I. Haide, Y. Han, K. Hayasaka, H. Hayashii, S. Hazra, C. Hearty, M. T. Hedges, A. Heidelbach, G. Heine, I. Heredia de la Cruz, T. Higuchi, M. Hoek, M. Hohmann, R. Hoppe, P. Horak, X. T. Hou, C. -L. Hsu, T. Humair, T. Iijima, K. Inami, N. Ipsita, A. Ishikawa, R. Itoh, M. Iwasaki, P. Jackson, D. Jacobi, W. W. Jacobs, E. -J. Jang, Q. P. Ji, S. Jia, Y. Jin, A. Johnson, K. K. Joo, K. H. Kang, G. Karyan, T. Kawasaki, F. Keil, C. Kiesling, C. Kim, D. Y. Kim, H. Kim, J. -Y. Kim, K. -H. Kim, K. Kinoshita, P. Kodyš, T. Koga, S. Kohani, A. Korobov, S. Korpar, E. Kovalenko, R. Kowalewski, P. Križan, P. Krokovny, T. Kuhr, Y. Kulii, R. Kumar, K. Kumara, T. Kunigo, S. Kurokawa, A. Kuzmin, Y. -J. Kwon, S. Lacaprara, Y. -T. Lai, T. Lam, J. S. Lange, T. S. Lau, R. Leboucher, H. Lee, M. J. Lee, P. Leo, P. M. Lewis, C. Li, L. K. Li, Q. M. Li, S. X. Li, W. Z. Li, Y. Li, Y. B. Li, Y. P. Liao, J. Libby, J. Lin, S. Lin, Z. Liptak, V. Lisovskyi, C. Liu, G. Liu, M. H. Liu, Q. Y. Liu, Z. Q. Liu, D. Liventsev, S. Longo, A. Lozar, T. Lueck, J. L. Ma, Y. Ma, M. Maggiora, S. P. Maharana, R. Maiti, G. Mancinelli, R. Manfredi, E. Manoni, M. Mantovano, D. Marcantonio, M. Marfoli, C. Marinas, A. Martens, T. Martinov, L. Massaccesi, M. Masuda, T. Matsuda, D. Matvienko, S. K. Maurya, M. Maushart, J. A. McKenna, Z. Mediankin Gruberová, R. Mehta, F. Meier, D. Meleshko, M. Merola, C. Miller, M. Mirra, K. Miyabayashi, H. Miyake, R. Mizuk, G. B. Mohanty, S. Moneta, A. L. Moreira de Carvalho, H. -G. Moser, N. Mudgal, Th. Muller, H. Murakami, R. Mussa, M. Nakao, Y. Nakazawa, Z. Natkaniec, A. Natochii, M. Neu, S. Nishida, R. Nomaru, S. Ogawa, R. Okubo, H. Ono, Y. Onuki, G. Pakhlova, S. Pardi, J. Park, K. Park, S. -H. Park, A. Passeri, S. Patra, T. K. Pedlar, M. Piccolo, L. E. Piilonen, P. L. M. Podesta-Lerma, T. Podobnik, L. Polat, A. Prakash, V. Prasad, C. Praz, S. Prell, E. Prencipe, M. T. Prim, S. Privalov, I. Prudiiev, H. Purwar, P. Rados, S. Raiz, K. Ravindran, J. U. Rehman, M. Reif, S. Reiter, L. Reuter, D. Ricalde Herrmann, I. Ripp-Baudot, G. Rizzo, S. H. Robertson, J. M. Roney, A. Rostomyan, N. Rout, G. Russo, S. Saha, L. Salutari, D. A. Sanders, S. Sandilya, L. Santelj, C. Santos, V. Savinov, B. Scavino, C. Schmitt, J. Schmitz, G. Schnell, K. Schoenning, C. Schwanda, Y. Seino, K. Senyo, J. Serrano, C. Sfienti, W. Shan, C. P. Shen, X. D. Shi, T. Shillington, T. Shimasaki, J. -G. Shiu, D. Shtol, B. Shwartz, A. Sibidanov, F. Simon, J. B. Singh, J. Skorupa, A. Soffer, A. Sokolov, E. Solovieva, S. Spataro, K. Špenko, B. Spruck, M. Starič, P. Stavroulakis, S. Stefkova, R. Stroili, M. Sumihama, M. Takahashi, M. Takizawa, U. Tamponi, K. Tanida, F. Testa, A. Thaller, D. V. Thanh, T. Tien Manh, O. Tittel, R. Tiwary, E. Torassa, K. Trabelsi, F. F. Trantou, I. Tsaklidis, M. Uchida, I. Ueda, T. Uglov, K. Unger, Y. Unno, K. Uno, S. Uno, Y. Ushiroda, R. van Tonder, K. E. Varvell, M. Veronesi, A. Vinokurova, V. S. Vismaya, L. Vitale, V. Vobbilisetti, R. Volpe, M. Wakai, S. Wallner, M. -Z. Wang, A. Warburton, M. Watanabe, S. Watanuki, C. Wessel, X. P. Xu, B. D. Yabsley, S. Yamada, W. Yan, W. P. Yan, J. Yelton, K. Yi, J. H. Yin, K. Yoshihara, C. Z. Yuan, J. Yuan, L. Yuan, Y. Yusa, L. Zani, F. Zeng, M. Zeyrek, B. Zhang, X. Zhao, V. Zhilich, Q. D. Zhou, X. Y. Zhou, L. Zhu, R. Žlebčík

Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

The Big Picture: Catching a Ghost in the Machine

Imagine you are trying to watch a magic trick performed by two identical twins. One twin is the "good" version, and the other is the "evil" version. In the world of particle physics, these twins are B-mesons (specifically B0B^0 and Bˉ0\bar{B}^0). They are unstable particles that decay (fall apart) very quickly.

The scientists at the Belle and Belle II experiments (located in Japan) built massive, ultra-sensitive cameras to watch these twins decay. Their goal was to catch a specific, rare magic trick: a decay where a B-meson turns into a neutral Kaon (KS0K^0_S), a neutral pion (π0\pi^0), and a flash of light (a photon, γ\gamma).

Why do they care? Because in our current understanding of the universe (the Standard Model), this specific trick should happen in a very predictable way. If the twins behave differently than expected, it means there is a "ghost" in the machine—some new, unknown force or particle messing with the rules.

The Setup: A High-Speed Dance

To study this, the researchers smash electrons and positrons (matter and antimatter) together at nearly the speed of light. This collision creates a heavy particle called the Υ(4S)\Upsilon(4S), which immediately splits into a pair of B-mesons.

Think of this like a synchronized dance:

  1. The Twins: One B-meson is the "Signal" (BsigB_{sig}) that performs the magic trick we want to watch. The other is the "Tag" (BtagB_{tag}) that acts as a witness.
  2. The Tag: The Tag twin decays into something easy to identify. This tells the scientists, "Hey, at this exact moment, the Signal twin was the 'good' version (or the 'evil' version)."
  3. The Time Difference: Because the twins are moving, they don't decay at the exact same time. The scientists measure the tiny time gap (Δt\Delta t) between the Tag's death and the Signal's death.

The Mystery: Left-Handed vs. Right-Handed

In the Standard Model, the photon (the flash of light) emitted during this decay is almost always left-handed (like a left-handed screw). It's very rare for it to be right-handed.

If the photon is strictly left-handed, the "good" and "evil" twins should decay at almost the same rate. The difference between them (called CP violation) should be tiny.

  • The Goal: The scientists are looking for a "right-handed" photon. If they find one, it would mean the "good" and "evil" twins are behaving very differently, suggesting new physics (like Supersymmetry) is at play.

They measure two numbers to describe this difference:

  • SS (The Mixing): How much the twins swap identities before decaying.
  • CC (The Direct Difference): How much they prefer to decay as one type over the other immediately.

The Investigation: Two Different Neighborhoods

The researchers looked at the debris from the decay in two different "neighborhoods" based on the mass of the particles involved:

  1. The KK^* Neighborhood (0.8 to 1.0 GeV): This is a busy, well-known area where a specific particle resonance (K(892)K^*(892)) dominates. It's like a crowded city square.
  2. The Non-KK^* Neighborhood (1.0 to 1.8 GeV): This is a quieter, more chaotic area with no single dominant particle. It's like a scattered suburb.

They needed to check both because the rules might be different in the quiet suburb compared to the city square.

The Tools: Better Cameras and Smarter Algorithms

The paper highlights two major upgrades that made this study possible:

  1. More Data: They combined data from the old Belle experiment (running 1999–2010) and the new Belle II experiment. This is like combining 772 million and 521 million photos to get a clearer picture.
  2. Smarter AI: They used a new type of Artificial Intelligence called a Graph Neural Network (GNN). Imagine trying to figure out who is in a crowd photo. Old methods just looked at faces. This new AI looks at how everyone is connected, their movements, and their relationships to figure out exactly who is who. This helped them identify the "Tag" twin much more accurately.

The Results: The Twins Behave Themselves

After crunching the numbers, the scientists found:

  • In the City Square (KK^* region): The difference between the twins was tiny. The numbers were S=0.09S = 0.09 and C=0.09C = -0.09.
  • In the Suburb (Non-KK^* region): The difference was also small, though with slightly larger margins of error. The numbers were S=0.32S = -0.32 and C=0.07C = -0.07.

The Conclusion:
The "ghost" they were looking for wasn't there. The twins behaved exactly as the Standard Model predicted. The "right-handed" photon is still hiding, or at least, it's not showing up in this experiment.

However, this is a good result for science. It's like checking a bridge for cracks. Finding no cracks doesn't mean the bridge is boring; it means the bridge is safe and built exactly to the blueprints. These results are the most precise measurements ever made for this specific decay, improving upon previous attempts by about 24% to 31%.

Summary in One Sentence

Using a massive amount of data and a new AI system, the Belle and Belle II collaborations watched billions of particle "twins" decay and confirmed that they are behaving exactly as our current laws of physics predict, with no sign of mysterious new forces disrupting the process.

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