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Central exclusive production of η\eta and η′\eta' mesons in diffractive proton-proton collisions at the LHC

This paper utilizes the tensor-pomeron approach, constrained by WA102 data, to predict the central exclusive production cross sections and differential distributions of η\eta and η′\eta' mesons in proton-proton collisions at s=13\sqrt{s} = 13 TeV, demonstrating the feasibility of using these processes to probe the nature of the pomeron at the LHC.

Original authors: Piotr Lebiedowicz, Otto Nachtmann, Antoni Szczurek

Published 2026-10-01
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Original authors: Piotr Lebiedowicz, Otto Nachtmann, Antoni Szczurek

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

In the subatomic world, particles do not merely bounce off one another like billiard balls; they interact through invisible forces that can be thought of as exchanges of other, fleeting particles. When two protons collide at extremely high speeds, they can sometimes pass each other so closely that they exchange these force carriers without shattering, leaving the protons intact but creating new particles in the empty space between them. This process is known as central exclusive production. The force carrier responsible for this interaction at high energies is called the pomeron. For decades, physicists have debated the true nature of the pomeron: is it a simple, scalar object, or does it possess a more complex, tensor structure? Understanding this distinction is crucial because the pomeron governs how matter behaves at the highest energy levels found in the universe, yet its internal character remains one of the great mysteries of particle physics.

A team of researchers has now taken a significant step toward solving this mystery by simulating the creation of two specific particles, the eta and eta-prime mesons, during proton collisions. Using a theoretical framework that treats the pomeron as a tensor object, they calculated what should happen when protons collide at the energies achieved by the Large Hadron Collider. Their work builds on previous measurements taken at lower energies, where the team successfully matched their calculations to experimental data. By applying this same model to the much higher energies of the Large Hadron Collider, they generated precise predictions for how often these mesons should appear and how they should be distributed in space. The results demonstrate the feasibility of studying the production of these mesons to probe the nature of the pomeron, suggesting that if the pomeron were a simple scalar object, these particles would not be produced in the way the model predicts.

The researchers focused on a scenario where two protons collide and emerge unchanged, while a new meson is created in the center of the collision zone. To ensure their model was reliable, they first tuned its parameters using data from an earlier experiment conducted at a much lower energy. Once the model could accurately reproduce the results of that past experiment, they projected its behavior forward to the current energy levels of the Large Hadron Collider. They found that the production of eta and eta-prime mesons is highly sensitive to the internal structure of the pomeron. Because the eta and eta-prime have specific quantum properties that a simple scalar pomeron cannot generate, the successful observation of these particles would confirm that the pomeron must have a tensor nature. The team calculated that at the Large Hadron Collider, the production of eta mesons should occur with a cross section, a measure of probability, reaching up to 2.5 microbarns in the central region and up to 5.6 microbarns in the forward regions. For the heavier eta-prime meson, the predicted rates are lower, ranging between 0.3 and 0.7 microbarns in the center and 0.9 to 2.1 microbarns in the forward regions.

A critical part of their analysis involved accounting for the fact that protons are not just single points but complex clouds of particles that can interact with each other even before the main collision occurs. These secondary interactions, known as absorption effects, significantly reduce the number of particles that are actually produced. The researchers included these effects in their calculations, finding that they play a major role in lowering the final numbers. They also examined the influence of other, less dominant force carriers that might contribute to the process. At the lower energies of the past experiment, these other carriers were important, but at the high energies of the Large Hadron Collider, their contribution becomes negligible, leaving the pomeron interaction as the clear dominant force. This shift allows for a much cleaner test of the pomeron's properties than was possible before.

The study concludes that the experimental observation of these mesons at the Large Hadron Collider would provide a definitive test of the pomeron's nature. If the particles are found at the rates predicted by the tensor model, it would confirm that the pomeron is indeed a tensor object and not a scalar one. This would also settle a long-standing debate regarding whether the eta meson, which has a complex internal structure involving gluons, can be produced by the pomeron. Some had argued that because the pomeron is a singlet and the eta is part of a different group, the specific reaction producing the eta meson should be forbidden. However, the researchers show that the breaking of symmetry in the subatomic world allows this interaction to happen. The findings offer a clear roadmap for experimentalists: by measuring the production rates and distributions of these specific mesons, they can finally pin down the true character of the pomeron, a fundamental piece of the puzzle in understanding how the universe holds itself together at its most energetic levels.

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