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Exposing the parton-hadron transition within jets with energy-energy correlators in pp collisions at s=5.02\sqrt{\textit s}=5.02 TeV

This paper presents a fully-corrected measurement of the energy-energy correlator (EEC) within jets in pp collisions at s=5.02\sqrt{s}=5.02 TeV, revealing a distinct transition region that marks the onset of hadronization and identifies a common energy scale for this process, while demonstrating good agreement with perturbative QCD calculations in the large-angle regime and providing constraints for Monte Carlo event generators.

Original authors: ALICE Collaboration

Published 2026-09-29
📖 5 min read🧠 Deep dive

Original authors: ALICE Collaboration

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

Inside the heart of a particle accelerator, where protons smash together at nearly the speed of light, nature performs a violent transformation. When these tiny packets of energy collide, they shatter into a spray of even smaller fragments called quarks and gluons. These fragments are the fundamental building blocks of matter, but they cannot exist in isolation for long. Almost instantly, they begin to radiate energy and split apart, creating a cascading shower of new particles. As this shower expands, the energy of the original fragments spreads out until the particles are forced to bind together into stable, composite objects known as hadrons, such as protons and pions. This final step, where free-floating energy locks itself into solid matter, is a process called hadronization. It is a crucial moment in the life of a particle collision, yet it remains one of the most difficult to understand because the forces involved are so complex that standard mathematical tools often fail to describe them.

Scientists have long sought a way to watch this transition happen in real time, to see exactly where the smooth, predictable splitting of particles gives way to the chaotic binding of hadrons. To do this, researchers at the Large Hadron Collider turned their attention to a specific measurement called the energy-energy correlator. Instead of looking at individual particles, this method tracks how the energy of two particles relates to the angle between them. By measuring this relationship across a jet of particles, scientists can map the flow of energy from the initial high-speed split down to the final, slow-moving clump of matter. It is a way of tracing the path of energy as it moves from the realm of high-speed physics into the realm where particles stick together.

In a recent study, the ALICE collaboration at CERN used this method to examine jets produced in proton-proton collisions at an energy of 5.02 trillion electron volts. The team focused on jets containing charged particles with a specific range of momentum, looking closely at how the energy correlation changed as the angle between particle pairs varied. They found that the behavior of these jets changes dramatically depending on the distance between the particles. When the particles are far apart, the energy correlation follows a predictable pattern that matches calculations based on the known laws of particle physics. This region represents the early stage of the jet, where particles are still splitting apart freely. However, as the researchers looked at particles that were very close together, the pattern shifted. In this tight space, the correlation grew in a straight, linear line, a signature that the particles were no longer acting as free fragments but were instead being shaped by the forces that bind them into hadrons.

Between these two distinct behaviors lies a transition zone, a narrow window where the physics of the jet changes from one mode to the other. The researchers identified a clear peak in the data that marks this turning point. Remarkably, when they adjusted for the total energy of the jet, this peak appeared at the exact same location for all the different energy levels they tested. This consistency suggests that there is a universal scale for the moment when the free-flowing energy stops splitting and begins to lock into matter. The peak occurred at an angular distance that corresponds to a specific energy scale of about 2.43 GeV/c divided by the jet's momentum. This finding implies that the process of hadronization happens at a characteristic energy threshold, regardless of how much energy the original jet started with.

To ensure these observations were real and not just an artifact of the detector, the team compared their results with sophisticated computer simulations that model how particles should behave. They tested different versions of these simulations, each using different assumptions about how particles break apart and stick together. While the simulations generally matched the data, they showed subtle differences in exactly where the transition peak appeared. Some models placed the peak at slightly different angles, revealing that the details of the hadronization process are still sensitive to the specific rules used in the computer models. This mismatch provides a powerful new tool for physicists: by measuring exactly where the transition happens in the real world, they can now fine-tune their theories to better describe how nature builds matter from energy.

The study represents a significant step forward because it is the first time this specific measurement has been fully corrected for the limitations of the detector in such a low-energy regime at the Large Hadron Collider. Previous measurements often focused on higher energies or left some detector effects uncorrected, which can blur the fine details of the transition. By carefully accounting for how the detector sees the particles, the ALICE team was able to reveal the clean, underlying shape of the energy flow. The results confirm that the transition from free particles to bound matter is not a gradual blur but a distinct event with a predictable location. This clarity allows scientists to probe the fundamental forces of the universe with greater precision, offering a new window into the moment when the invisible becomes visible.

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