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Observation of several sources of C ⁣PC\!P violation in B+ ⁣K+π+πB^+ \!\to K^+ \pi^+ \pi^- decays

Using 3 fb⁻¹ of LHCb collision data from 2011–2012, this amplitude analysis of B+ ⁣K+π+πB^+ \!\to K^+ \pi^+ \pi^- decays reports the first observation of six distinct C ⁣PC\!P-violating phenomena, including discoveries in quasi-two-body decays, amplitude-level effects, and significant interference between partial waves.

Original authors: LHCb collaboration, R. Aaij, M. Abdelfatah, A. S. W. Abdelmotteleb, C. Abellan Beteta, F. Abudinén, T. Ackernley, A. A. Adefisoye, B. Adeva, M. Adinolfi, P. Adlarson, C. Agapopoulou, C. A. Aidala, Z.
Published 2026-08-14
📖 6 min read🧠 Deep dive

Original authors: LHCb collaboration, R. Aaij, M. Abdelfatah, A. S. W. Abdelmotteleb, C. Abellan Beteta, F. Abudinén, T. Ackernley, A. A. Adefisoye, B. Adeva, M. Adinolfi, P. Adlarson, C. Agapopoulou, C. A. Aidala, Z. Ajaltouni, S. Akar, K. Akiba, P. Albicocco, J. Albrecht, R. Aleksiejunas, F. Alessio, P. Alvarez Cartelle, R. Amalric, S. Amato, J. L. Amey, Y. Amhis, L. An, L. Anderlini, M. Andersson, P. Andreola, M. Andreotti, S. Andres Estrada, A. Anelli, D. Ao, C. Arata, F. Archilli, Z. Areg, M. Argenton, S. Arguedas Cuendis, L. Arnone, M. Artuso, E. Aslanides, R. Ataíde Da Silva, M. Atzeni, B. Audurier, J. A. Authier, D. Bacher, I. Bachiller Perea, S. Bachmann, M. Bachmayer, J. J. Back, Z. B. Bai, P. Baladron Rodriguez, V. Balagura, A. Balboni, W. Baldini, Z. Baldwin, L. Balzani, H. Bao, J. Baptista de Souza Leite, C. Barbero Pretel, M. Barbetti, I. R. Barbosa, R. J. Barlow, M. Barnyakov, S. Barsuk, W. Barter, J. Bartz, S. Bashir, B. Batsukh, P. B. Battista, A. Bavarchee, A. Bay, A. Beck, M. Becker, F. Bedeschi, I. B. Bediaga, N. A. Behling, S. Belin, A. Bellavista, I. Belov, I. Belyaev, G. Benane, G. Bencivenni, E. Ben-Haim, R. Bernet, A. Bertolin, F. Betti, J. Bex, O. Bezshyyko, S. Bhattacharya, M. S. Bieker, N. V. Biesuz, A. Biolchini, M. Birch, F. C. R. Bishop, A. Bitadze, A. Bizzeti, T. Blake, F. Blanc, J. E. Blank, S. Blusk, J. A. Boelhauve, O. Boente Garcia, T. Boettcher, A. Bohare, C. Bolognani, R. Bolzonella, R. B. Bonacci, A. Bordelius, F. Borgato, S. Borghi, M. Borsato, J. T. Borsuk, E. Bottalico, S. A. Bouchiba, M. Bovill, T. J. V. Bowcock, A. Boyer, C. Bozzi, J. D. Brandenburg, A. Brea Rodriguez, N. Breer, C. Breitfeld, J. Brodzicka, J. Brown, D. Brundu, E. Buchanan, M. Burgos Marcos, C. Burr, C. Buti, J. S. Butter, J. Buytaert, W. Byczynski, S. Cadeddu, H. Cai, Y. Cai, A. Caillet, R. Calabrese, L. Calefice, M. Calvi, M. Calvo Gomez, P. Camargo Magalhaes, J. I. Cambon Bouzas, P. Campana, A. C. Campos, A. F. Campoverde Quezada, Y. Cao, S. Capelli, M. Caporale, L. Capriotti, R. Caravaca-Mora, A. Carbone, L. Carcedo Salgado, R. Cardinale, A. Cardini, P. Carniti, L. Carus, A. Casais Vidal, R. Caspary, G. Casse, M. Cattaneo, G. Cavallero, V. Cavallini, S. Celani, I. Celestino, S. Cesare, A. J. Chadwick, I. Chahrour, H. Chang, M. Charles, Ph. Charpentier, E. Chatzianagnostou, R. Cheaib, M. Chefdeville, C. Chen, J. Chen, S. Chen, Z. Chen, A. Chen Hu, M. Cherif, A. Chernov, S. Chernyshenko, X. Chiotopoulos, G. Chizhik, V. Chobanova, M. Chrzaszcz, V. Chulikov, P. Ciambrone, X. Cid Vidal, G. Ciezarek, P. Cifra, P. E. L. Clarke, M. Clemencic, H. V. Cliff, J. Closier, C. Cocha Toapaxi, V. Coco, J. Cogan, E. Cogneras, L. Cojocariu, S. Collaviti, P. Collins, T. Colombo, M. Colonna, A. Comerma-Montells, L. Congedo, J. Connaughton, A. Contu, N. Cooke, G. Cordova, C. Coronel, I. Corredoira, A. Correia, G. Corti, G. C. Costantino, J. Cottee Meldrum, B. Couturier, D. C. Craik, N. Crepet, M. Cruz Torres, M. Cubero Campos, E. Curras Rivera, R. Currie, C. L. Da Silva, X. Dai, E. Dall'Occo, J. Dalseno, C. D'Ambrosio, J. Daniel, G. Darze, A. Davidson, J. E. Davies, O. De Aguiar Francisco, C. De Angelis, F. De Benedetti, J. de Boer, K. De Bruyn, S. De Capua, M. De Cian, U. De Freitas Carneiro Da Graca, E. De Lucia, J. M. De Miranda, L. De Paula, M. De Serio, P. De Simone, F. De Vellis, J. A. de Vries, F. Debernardis, D. Decamp, S. Dekkers, L. Del Buono, B. Delaney, J. Deng, V. Denysenko, O. Deschamps, F. Dettori, B. Dey, P. Di Nezza, S. Ding, Y. Ding, L. Dittmann, A. D. Docheva, A. Doheny, C. Dong, F. Dordei, A. C. dos Reis, A. D. Dowling, L. Dreyfus, W. Duan, P. Duda, L. Dufour, V. Duk, P. Durante, M. M. Duras, J. M. Durham, O. D. Durmus, A. Dziurda, S. Easo, E. Eckstein, U. Egede, S. Eisenhardt, E. Ejopu, L. Eklund, M. Elashri, D. Elizondo Blanco, J. Ellbracht, S. Ely, A. Ene, J. Eschle, T. Evans, F. Fabiano, S. Faghih, L. N. Falcao, B. Fang, R. Fantechi, L. Fantini, M. Faria, K. Farmer, F. Fassin, D. Fazzini, L. Felkowski, C. Feng, M. Feng, A. Fernandez Casani, M. Fernandez Gomez, A. D. Fernez, F. Ferrari, F. Ferreira Rodrigues, M. Ferrillo, M. Ferro-Luzzi, R. A. Fini, M. Fiorini, M. Firlej, K. L. Fischer, D. S. Fitzgerald, C. Fitzpatrick, T. Fiutowski, F. Fleuret, A. Fomin, M. Fontana, L. A. Foreman, R. Forty, D. Foulds-Holt, V. Franco Lima, M. Franco Sevilla, M. Frank, E. Franzoso, G. Frau, C. Frei, D. A. Friday, J. Fu, Q. Führing, T. Fulghesu, G. Galati, M. D. Galati, A. Gallas Torreira, D. Galli, S. Gambetta, M. Gandelman, P. Gandini, B. Ganie, H. Gao, R. Gao, T. Q. Gao, Y. Gao, Y. Gao, Y. Gao, L. M. Garcia Martin, P. Garcia Moreno, J. García Pardiñas, P. Gardner, L. Garrido, C. Gaspar, A. Gavrikov, L. L. Gerken, E. Gersabeck, M. Gersabeck, T. Gershon, S. Ghizzo, Z. Ghorbanimoghaddam, F. I. Giasemis, V. Gibson, H. K. Giemza, A. L. Gilman, M. Giovannetti, A. Gioventù, L. Girardey, M. A. Giza, F. C. Glaser, V. V. Gligorov, C. Göbel, L. Golinka-Bezshyyko, E. Golobardes, A. 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Jiang, X. Jiang, Y. Jiang, Y. J. Jiang, E. Jimenez Moya, N. Jindal, M. John, A. John Rubesh Rajan, D. Johnson, C. R. Jones, S. Joshi, B. Jost, J. Juan Castella, N. Jurik, I. Juszczak, K. Kalecinska, D. Kaminaris, S. Kandybei, M. Kane, Y. Kang, C. Kar, M. Karacson, A. Kauniskangas, J. W. Kautz, M. K. Kazanecki, F. Keizer, M. Kenzie, T. Ketel, B. Khanji, S. Kholodenko, G. Khreich, F. Kiraz, T. Kirn, V. S. Kirsebom, S. Klaver, N. Kleijne, A. Kleimenova, D. Klekots, K. Klimaszewski, M. R. Kmiec, T. Knospe, R. Kolb, S. Koliiev, L. Kolk, A. Konoplyannikov, P. Kopciewicz, P. Koppenburg, A. Korchin, I. Kostiuk, O. Kot, S. Kotriakhova, E. Kowalczyk, O. Kravcov, M. Kreps, W. Krupa, W. Krzemien, O. Kshyvanskyi, S. Kubis, M. Kucharczyk, A. Kupsc, V. Kushnir, B. Kutsenko, J. Kvapil, I. Kyryllin, D. Lacarrere, P. Laguarta Gonzalez, A. Lai, A. Lampis, D. Lancierini, C. Landesa Gomez, J. J. Lane, G. Lanfranchi, C. Langenbruch, J. Langer, T. Latham, F. Lazzari, C. Lazzeroni, R. Le Gac, H. Lee, R. 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Marconi, E. Mariani, S. Mariani, C. Marin Benito, J. Marks, A. M. Marshall, L. Martel, G. Martelli, G. Martellotti, L. Martinazzoli, M. Martinelli, D. Martinez Gomez, D. Martinez Santos, F. Martinez Vidal, A. Martorell i Granollers, A. Massafferri, R. Matev, A. Mathad, C. Matteuzzi, K. R. Mattioli, A. Mauri, E. Maurice, J. Mauricio, P. Mayencourt, J. Mazorra de Cos, M. Mazurek, D. Mazzanti Tarancon, M. McCann, N. T. McHugh, A. McNab, R. McNulty, B. Meadows, S. E. R. Medaer, D. Melnychuk, D. Mendoza Granada, P. Menendez Valdes Perez, F. M. Meng, M. Merk, A. Merli, L. Meyer Garcia, D. Miao, H. Miao, M. Mikhasenko, D. A. Milanes, A. Minotti, E. Minucci, B. Mitreska, D. S. Mitzel, R. Mocanu, A. Modak, L. Moeser, R. D. Moise, E. F. Molina Cardenas, T. Mombächer, M. Monk, T. Monnard, S. Monteil, A. Morcillo Gomez, G. Morello, M. J. Morello, M. P. Morgenthaler, A. Moro, J. Moron, W. Morren, A. B. Morris, A. G. Morris, R. Mountain, Z. Mu, E. Muhammad, F. Muheim, M. Mulder, K. Müller, F. 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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

Imagine the universe as a giant, cosmic dance floor where every particle has a partner. In the perfect world of physics, if you swapped a dancer for their mirror-image twin (an antiparticle), the dance steps should look exactly the same, just in reverse. This is the rule of symmetry. But nature loves a plot twist. Sometimes, the dance changes when you swap the partners. This is called CP violation. It's the reason why, after the Big Bang, the universe didn't just annihilate itself into pure energy, leaving nothing behind. Instead, a tiny bit of "matter" survived the "antimatter" crowd to build the stars, planets, and you.

The Standard Model, our best textbook for how particles behave, explains this asymmetry with a specific mathematical "phase shift" in the way quarks (the building blocks of protons and neutrons) transform into one another. However, the amount of asymmetry this textbook predicts isn't quite enough to explain why we exist at all. Scientists are hunting for extra sources of this asymmetry, looking for hidden moves in the dance that the textbook missed. They do this by watching heavy particles called B-mesons decay (break apart) into lighter particles. If the B-meson and its antimatter twin break apart in slightly different ways, it's a sign of new physics. The LHCb experiment at CERN is like a high-speed camera capturing these fleeting dance moves, trying to spot the tiniest differences in the choreography.


The Paper: A Detective Story in the Decay of a B-Meson

In this paper, the LHCb collaboration acts as a team of forensic detectives, zooming in on a specific crime scene: the decay of a positively charged B-meson (B+B^+) into three lighter particles: a kaon (K+K^+), a positive pion (π+\pi^+), and a negative pion (π\pi^-).

When a B-meson decays, it doesn't just fall apart randomly. It often passes through a "middleman" stage, forming short-lived resonances (like a ρ\rho or a KK^*) before turning into the final three particles. Think of it like a relay race where the baton is passed through a few different runners before crossing the finish line. The scientists wanted to know: Does the race look different if the runner is a B-meson versus an anti-B-meson?

The Challenge: The Foggy S-Wave
The biggest headache for the team was the "S-wave." In particle physics, waves describe how particles spin and move. The S-wave is the simplest, "straightest" path, but in this specific decay, it's a messy, foggy region where many different forces overlap and blur together. It's like trying to hear a single violin in a room where everyone is shouting at once. To solve this, the team didn't just use one method; they used three different "flashlights" to cut through the fog:

  1. The Isobar Model: A standard approach that treats the middlemen as distinct, well-defined particles.
  2. The K-matrix Formalism: A more complex mathematical tool that ensures the laws of probability (unitarity) are strictly followed, using data from other scattering experiments.
  3. The Quasi-Model-Independent (QMI) Approach: A flexible method that lets the data speak for itself in small chunks, without forcing it into a pre-made box.

The Findings: New Moves in the Dance
After analyzing 3 fb1^{-1} of data (a massive amount of collision records from 2011–2012), the team found that the dance does change depending on who is dancing. They didn't just find one difference; they found several distinct sources of asymmetry:

  • The ρ(770)0\rho(770)^0 Resonance: This is a very common middleman particle. The team found a massive difference in how often B-mesons and anti-B-mesons use this path. The asymmetry is huge: a CP-violation parameter (ACPA_{CP}) of +0.280 (with a significance of 7.6 to 10.2 sigma depending on the model). In science, "5 sigma" is the gold standard for a discovery; this is nearly double that. It is the first observation of this specific type of CP violation in the B+ρ(770)0K+B^+ \to \rho(770)^0 K^+ process.
  • The f2(1270)f_2(1270) Resonance: Another middleman, this time with a different spin. The team found strong evidence of CP violation here, with a significance of 8.7 to 9.1 sigma across their models when assessed at the amplitude level. However, the paper explicitly notes that this result does not reach the significance threshold for observation of quasi-two-body CP violation in all S-wave approaches. Despite this technical distinction, it represents a major breakthrough in understanding this decay.
  • The ρ3(1690)0\rho_3(1690)^0 Resonance: This is a spin-3 particle, which is rare and tricky. The team found evidence of CP violation here with a significance of 3.3 to 4.0 sigma. This is the first evidence of CP violation in any decay involving a spin-3 resonance.
  • Interference Effects: Sometimes, the "waves" of different decay paths crash into each other. The team found that the interference between the S-wave and the P-wave (the ρ\rho) creates a significant asymmetry (5.4 sigma). They also found the first evidence for CP violation in the interference between S- and D-waves, with a significance of 4.4 sigma.

What They Ruled Out
The team also looked at a specific theoretical idea: that the difference might be caused by a mixing effect between the ρ\rho and the ω\omega particles (two different types of middlemen that can swap identities). They found no evidence for CP violation associated with this mixing. This is a crucial negative result because it clears up a previous confusion. Earlier measurements of the overall asymmetry in this region seemed to disagree with the new, precise numbers. The team realized that the ρ\rho-ω\omega mixing is "diluting" the signal—like adding water to strong coffee. Once they accounted for this, the numbers finally made sense.

The Bottom Line
The paper concludes that the three different mathematical approaches (Isobar, K-matrix, and QMI) all agree with each other. They have successfully mapped out where the CP violation happens in this complex decay. While these results don't yet prove a "new law of physics" beyond the Standard Model, they provide the most precise "reference points" ever created. They give theorists a clean, solid target to aim at. If the Standard Model can't explain these specific numbers, the cracks in the theory will be much easier to spot. For now, the universe has revealed a few more of its secret dance steps, and the LHCb team has captured them in high definition.

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