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Charmed baryon-to-meson ratios inside jets as a discriminator of hadronization mechanisms: from color reconnection in p+p to coalescence in Pb+Pb

This paper proposes that the sign of the modification in the in-jet charmed baryon-to-meson ratio (Λc+/D0\Lambda_c^+/D^0) serves as a key discriminator between hadronization mechanisms, where color reconnection in p+p collisions enhances the ratio while coalescence in Pb+Pb collisions suppresses it, offering distinct predictions for future jet-tagged measurements.

Original authors: Zi-Xuan Xu, Wei Dai, Ben-Wei Zhang, Enke Wang

Published 2026-10-23
📖 5 min read🧠 Deep dive

Original authors: Zi-Xuan Xu, Wei Dai, Ben-Wei Zhang, Enke Wang

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

When particles smash together at nearly the speed of light, they create a fleeting, super-hot soup of fundamental building blocks called quarks and gluons. As this soup cools and expands, these particles must stick together to form the matter we see in the universe today, such as protons and neutrons. Physicists have long observed a curious pattern in these collisions: at certain speeds, the universe seems to prefer making heavy, three-part particles called baryons over lighter, two-part particles called mesons. This "baryon enhancement" happens in massive collisions between heavy atomic nuclei, where a large, long-lived soup forms, but it also appears in tiny, high-speed crashes between single protons. The mystery lies in whether this preference comes from the same cause in both cases. In the large collisions, the answer is likely a process where particles merge like droplets of water. In the tiny ones, the cause is less clear, with some theories suggesting it arises from the complex ways particles reconnect their internal color charges before they even form.

To solve this puzzle, a team of researchers turned their attention to jets. When a collision occurs, it often sprays out a narrow, focused beam of particles called a jet, which acts like a spotlight on the original, high-energy crash. By looking only at the particles caught inside these jets, scientists can separate the direct products of the crash from the messy background noise of the rest of the event. The researchers focused on a specific type of heavy particle containing a charm quark, comparing how often they form a three-part baryon versus a two-part meson. They simulated these events using powerful computer models to see how different theories of particle formation would behave when forced into a jet. Their goal was to see if the behavior of these particles inside a jet could reveal whether they were formed by merging with the surrounding soup or by reconfiguring their internal connections in a vacuum.

The team ran simulations for two very different scenarios: collisions between single protons and collisions between heavy lead nuclei. In the proton collisions, they modeled a mechanism where particles rearrange their internal color connections, a process known as color reconnection. They found that when they looked inside the jets, the ratio of baryons to mesons actually increased at lower speeds compared to the overall average. This happened because the particles formed by this color reconnection stayed tightly linked to the original jet, surviving the selection process. In contrast, when they simulated the heavy lead collisions, where a hot, dense soup of matter is created, they used a model where particles form by merging with the surrounding thermal particles. Here, the result was the opposite. Inside the jets, the ratio of baryons to mesons dropped at intermediate speeds. This occurred because the particles formed by merging with the soup carried no memory of the jet's direction; they were scattered randomly and were often filtered out when the researchers selected only those particles moving in line with the jet.

This reversal in behavior provides a powerful tool for distinguishing between the two mechanisms. The researchers found that the sign of the change—whether the ratio goes up or down inside a jet—acts as a fingerprint. If the ratio rises, it suggests the particles formed through color reconnection, staying correlated with the jet. If it falls, it points to coalescence, where the particles formed from the surrounding medium and were largely discarded by the jet selection. The study also examined how these particles are distributed around the center of the jet. In both scenarios, the extra baryons were found further away from the central axis than the mesons, but the specific speed ranges where this effect was strongest differed between the two types of collisions. In the proton collisions, the effect was most visible at the lowest speeds, while in the heavy ion collisions, it peaked at intermediate speeds.

The researchers also looked at how much of the jet's total momentum the heavy particles carried. In both cases, the formation of baryons tended to shift the particles toward carrying a smaller fraction of the jet's momentum, a signature of the merging or reconnection processes. However, the study emphasized that this momentum shift alone could not tell the two mechanisms apart, as both produced a similar trend. It was the combination of the momentum shift with the direction of the ratio change inside the jet and the spatial distribution of the particles that allowed the team to separate the theories. The simulations showed that while the overall number of baryons increases in both systems, the way they are organized inside a jet tells a different story.

These findings offer a clear path forward for experimental physicists. By measuring the ratio of these specific heavy particles inside jets in future experiments, scientists can determine which mechanism is at work without needing to rely on complex, indirect inferences. The study provides a baseline prediction for what should be seen in proton collisions at specific energy levels, which can then be compared with data from heavy ion collisions. If future measurements confirm that the ratio drops inside jets for heavy collisions but rises for light ones, it would confirm that the baryon enhancement in small systems comes from color reconnection, while the enhancement in large systems comes from the merging of particles in a hot medium. This distinction would finally settle the question of whether the same physical laws govern the formation of matter in the smallest and largest cosmic collisions.

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