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Modification of Υ\Upsilon production in ppO and OO collisions at LHCb

The LHCb collaboration measured Υ\Upsilon meson production in ppO and OO collisions, finding that while ppO collisions show only slight suppression, OO collisions exhibit significant suppression of excited states consistent with quark-gluon plasma formation and color screening effects.

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, S.
Published 2026-08-04
📖 4 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, S. Akar, K. Akiba, H. Al Saleh, P. Albicocco, J. Albrecht, R. Aleksiejunas, F. Alessio, P. Alvarez Cartelle, S. Amato, J. L. Amey, Y. Amhis, Z. Amos, L. An, L. Anderlini, 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, M. Bai, Z. B. Bai, 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, W. Barker, R. J. Barlow, M. Barnyakov, S. Baron, S. Barsuk, W. Barter, J. Bartz, S. Bashir, B. Batsukh, P. B. Battista, A. Bavarchee, A. Bay, A. Beck, M. 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Curras Rivera, R. Currie, C. L. Da Silva, X. Dai, J. Dalseno, C. D'Ambrosio, G. Darze, A. Davidson, 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, F. De Gregorio, E. De Lucia, J. M. De Miranda, L. De Paula, A. De Robertis, E. De Santis, M. De Serio, P. De Simone, F. De Vellis, J. A. de Vries, F. Debernardis, D. Decamp, S. Dekkers, L. Del Buono, B. Delaney, B. Demaire-Lepape, J. Deng, O. Deschamps, F. Dettori, B. Dey, P. Di Nezza, S. Ding, Y. Ding, L. Dittmann, J. F. Diverchy, A. D. Docheva, A. Doheny, C. Dong, F. Dordei, J. Dorta Moreno, A. C. dos Reis, J. Dos Santos Oliveira, A. D. Dowling, L. Dreyfus, W. Duan, P. Duda, L. Dufour, V. Duk, P. Durante, M. M. Duras, J. M. Durham, O. D. Durmus, K. Duwe, 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, T. Evans, F. Fabiano, S. Faghih, L. N. Falcao, B. 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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 kitchen where the most extreme cooking experiments take place. In this kitchen, scientists smash tiny particles together at speeds close to the speed of light. The goal? To recreate the conditions that existed just a fraction of a second after the Big Bang, when the universe was so hot and dense that normal matter couldn't exist. Under these scorching conditions, protons and neutrons—the building blocks of atoms—melt down into a soupy, chaotic mixture of their smaller parts: quarks and gluons. This super-hot, super-dense soup is called a "quark-gluon plasma" (QGP). Think of it like a crowd of people at a concert so packed that you can't tell who is holding hands with whom; everyone is free to move around wildly.

To study this soup, physicists use special "thermometers" made of heavy particles called bottomonium. These are like tiny, heavy couples (a bottom quark and its partner) that usually hold hands very tightly. However, if you throw them into the hot QGP soup, the heat gets so intense that it breaks their grip, separating the couple. By watching how many of these couples survive the crash, scientists can tell how hot and dense the soup is. For a long time, we knew this happened in massive collisions, like smashing two heavy lead atoms together. But a big question remained: could this "soup" form in much smaller collisions, like smashing a single proton into a nucleus, or even two light oxygen atoms? If the soup forms in these tiny systems, it would change our understanding of how the universe behaves at its smallest scales.

This paper, written by the LHCb collaboration at CERN, dives into exactly that question. They took data from three different types of particle crashes: proton-proton (the baseline, like two billiard balls hitting), proton-oxygen (a small nucleus hit by a proton), and oxygen-oxygen (two light nuclei smashing together). They looked specifically at the "bottomonium" couples in three different states of excitement: the calm ground state (Υ(1S)), a slightly excited state (Υ(2S)), and a highly excited, wobbly state (Υ(3S)). The excited states are like couples holding hands loosely; they are much easier to break apart than the calm ones.

The team measured how often these excited couples survived compared to the calm ones in each type of crash. In the proton-proton collisions, the ratio of excited to calm couples was steady and matched what they had seen before at other energies. This served as their control group, showing how these particles behave when there is no "soup" to disrupt them.

When they looked at the proton-oxygen collisions, they found a tiny hint of trouble. The excited couples were slightly harder to find than expected, suggesting that the oxygen nucleus might be causing some minor "cold" disruptions (like a crowded hallway bumping into them) even without a hot soup forming. However, the data wasn't strong enough to say for sure if this was a real effect or just a statistical fluke.

The real story, however, came from the oxygen-oxygen collisions. Here, the results were dramatic. The excited Υ(2S) couples were suppressed by a factor of about two—meaning only half as many survived compared to the calm ones. The highly excited Υ(3S) couples showed evidence of being suppressed as well. This is a massive difference compared to the proton-oxygen results. The authors explain that this strong suppression is too big to be caused just by the "cold" effects of the nucleus; it points to the formation of a hot, deconfined quark-gluon plasma, even in this relatively small collision system.

To make sure this wasn't a fluke, the researchers compared their findings to two advanced computer models. One model, the KSU-Munich, and another, the TAMU-NP, both included the physics of a quark-gluon plasma. Both models successfully predicted the strong suppression seen in the oxygen-oxygen data. The paper concludes that while the small proton-oxygen system showed only a whisper of change, the oxygen-oxygen system shouted a clear signal: a quark-gluon plasma is likely forming in these smaller collisions, breaking apart the excited heavy quark couples just as it does in the massive lead collisions. This suggests that the "soup" of the early universe might be easier to create in smaller, lighter collisions than previously thought.

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