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First measurement of the ratio of ψ(2S)\psi(2S)-to-J/ψJ/\psi inclusive production in pArp\mathrm{Ar} and $pp$ collisions at sNN=113GeV\sqrt{s_{\mathrm{NN}}} =113\,\mathrm{GeV} with SMOG2

The LHCb experiment reports the first measurement of the ψ(2S)\psi(2S)-to-J/ψJ/\psi production cross-section ratio in pArp\mathrm{Ar} and $pp$ collisions at sNN=113GeV\sqrt{s_{\mathrm{NN}}}=113\,\mathrm{GeV} using SMOG2, observing a ratio of 0.90±0.04±0.020.90 \pm 0.04 \pm 0.02 in pArp\mathrm{Ar} collisions that signals the emergence of nuclear effects and establishes a baseline for future studies with larger collision systems.

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 2026-09-01
📖 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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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

At the heart of matter lies a force so powerful it binds the smallest building blocks of the universe together. This force, known as the strong interaction, is carried by particles called gluons and acts between quarks, the fundamental constituents of protons and neutrons. When a heavy quark meets its antimatter partner, they can bind together to form a short-lived particle called charmonium. Scientists study these fleeting pairs to understand how the strong force behaves under different conditions. In a vacuum, like a collision between two protons, these particles form and decay in a predictable way. However, when the same collision happens inside a larger nucleus, the environment changes. The dense cloud of other particles surrounding the collision point can interfere with the formation or survival of the charmonium, acting like a thick fog that might dissolve the delicate bond before it fully forms. By comparing how often these particles appear in simple collisions versus those happening inside a heavier nucleus, physicists can map out exactly how this nuclear environment alters the rules of particle physics.

A team of researchers using the LHCb experiment at CERN has taken a fresh look at this phenomenon by smashing protons into argon gas. While the Large Hadron Collider is famous for colliding beams of protons head-on at record-breaking speeds, this experiment utilized a unique setup where a beam of protons was fired into a stationary cloud of gas. This fixed-target approach allowed the scientists to study collisions at a specific energy level of 113 GeV per nucleon pair, a regime that had not been explored with this precision before. The team focused on two specific types of charmonium: the J/psi and the psi(2S). These two particles are essentially the same family, but the psi(2S) is a more excited, loosely bound version of the J/psi. Because the psi(2S) is held together more weakly, theory suggests it should be more fragile and more likely to be destroyed by the surrounding nuclear fog than its sturdier cousin.

To investigate this, the researchers analyzed data collected in 2024, when they injected clouds of hydrogen and argon gas into the path of the proton beam. The hydrogen collisions served as a baseline, representing a clean environment with no nuclear fog, while the argon collisions provided the test case, as argon nuclei are much larger and create a denser environment. By counting how many J/psi and psi(2S) particles were produced in each type of collision, the team calculated a ratio that compares the production rates of the two particles. They found that in the proton-proton collisions, the ratio of psi(2S) to J/psi was slightly higher than in the proton-argon collisions. Specifically, the ratio in the argon collisions was about 10 percent lower than in the proton collisions. This difference suggests that the nuclear environment in the argon gas is indeed suppressing the production of the more fragile psi(2S) particle more than it affects the J/psi.

The study did not stop at a single number; the scientists broke down their findings by looking at the speed and direction of the particles produced. They observed that this suppression effect was most noticeable when the particles were moving slowly and heading backward relative to the proton beam. This pattern aligns with the idea that the nuclear fog is most effective at disrupting the formation of these particles when they have more time to interact with the surrounding matter. The results were compared with previous measurements from other experiments and theoretical models that account for particles moving alongside the charmonium, known as comovers, as well as models of nuclear absorption. The data fits well with the prediction that the nuclear medium is actively interfering with the formation of the psi(2S), though the effect is modest.

This work represents the first precise measurement of this ratio in proton-argon collisions at this specific energy, serving as a crucial benchmark for future studies. The researchers emphasize that while the evidence points toward a suppression effect, the data sample is still relatively small, and a larger dataset will be needed to confirm the finding with greater certainty. The success of this measurement also highlights the capability of the LHCb detector to operate in this fixed-target mode, opening the door for even more detailed investigations into how matter behaves in extreme conditions. By continuing to refine these measurements with different gas targets and larger data samples, physicists hope to build a complete picture of how the strong force operates within the dense nuclear environment, shedding light on the fundamental rules that govern the universe at its smallest scales.

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