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Perturbative QCD below charm threshold: theory and tensions with e+ee^+e^- data

This paper resolves tensions between perturbative QCD predictions and e+ee^+e^- data below the charm threshold by incorporating sizable duality violation contributions up to 2.5 GeV, which significantly improve global agreement despite persistent 3σ\sigma discrepancies with specific BES-III measurements.

Original authors: Diogo Boito, Marcelle Caram

Published 2026-08-26
📖 6 min read🧠 Deep dive

Original authors: Diogo Boito, Marcelle Caram

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 called quarks are the fundamental building blocks of protons and neutrons, the matter that makes up our visible universe. However, quarks are never found alone; they are always bound together in groups by a powerful force known as the strong interaction. Physicists study this force using a theory called Quantum Chromodynamics, or QCD. To test if their theory is correct, scientists smash electrons and positrons together at high speeds. When these particles collide, they can transform into a shower of new particles made of quarks. By measuring how often this happens at different energy levels, researchers can calculate a specific ratio that acts as a fingerprint for the strong force. This fingerprint is crucial for understanding a mysterious property of the muon, a particle similar to an electron but much heavier. The muon's magnetic behavior is one of the most sensitive tests of the Standard Model, the current rulebook of particle physics. If the theory describing the strong force is slightly off, it could throw off the entire calculation of the muon's magnetic moment, potentially hiding signs of new, undiscovered physics.

For decades, physicists have been able to predict this fingerprint with high precision at very high energies, where the strong force behaves in a predictable, mathematical way. However, a puzzle emerged in 2021 when a team at the BES-III laboratory in China released new, highly precise measurements of this ratio in a specific energy range, just below the threshold where charm quarks begin to appear. These new measurements were consistently higher than what the standard theory predicted. This created a tension: either the theory was missing something important, or the new data contained a hidden error. The discrepancy was significant enough to worry researchers, as it sits in an energy zone that contributes to the calculation of the muon's magnetic moment. If the theory is wrong here, the entire Standard Model calculation for the muon could be flawed.

A team of researchers from the University of São Paulo in Brazil has now taken a deep dive into this problem to see if the theory itself could explain the gap. They carefully re-examined the mathematical description of the strong force in this energy region, looking for subtle effects that might have been overlooked. One of the main things they investigated was the behavior of the mathematical series used to calculate the force. In quantum physics, these calculations often involve adding up an infinite number of terms, but in practice, scientists must stop after a certain number. The researchers checked if stopping early was causing the error. They used advanced mathematical techniques to estimate what the missing terms would look like and found that the standard theory is actually very stable and reliable in this region. The uncertainty in the theory is tiny, far smaller than the difference seen in the new data.

The team then turned their attention to a phenomenon called duality violation. In simple terms, the theory assumes that at high enough energies, the chaotic behavior of individual quarks averages out to look smooth and predictable. However, in the real world, the energy levels are not perfectly smooth; they are influenced by the presence of short-lived particle resonances, which are like temporary, heavy versions of the particles being studied. These resonances cause small, wiggly oscillations in the data that the smooth theory does not capture. The researchers modeled these wiggles to see if they could account for the difference between the theory and the BES-III data. They found that these oscillations are indeed real and can be significant at lower energies, specifically below 2.5 GeV. When they added this effect to their theoretical prediction, the agreement with some of the older experimental data improved dramatically, and the theory began to match the wiggles seen in those measurements.

However, the story changes as the energy increases. The researchers found that these oscillating effects become negligible above 2.8 GeV. In the higher energy part of the range, where the BES-III data shows the largest disagreement with the theory, the "wiggles" are essentially gone. This means that the standard theory should be working perfectly well in that region, and there is no hidden mathematical effect left to explain the gap. When the team compared the theory, now including the small oscillation effects, against the combined data from all available experiments, a clear picture emerged. The older data sets, such as those from the KEDR collaboration, fit the theory very well, even without the oscillation corrections. The combined data from all experiments is also reasonably close to the theory, staying within a margin of about two and a half standard deviations, which is acceptable in this field.

The situation with the new BES-III data, however, remains unresolved. Even after accounting for the oscillations and all other known corrections, the BES-III measurements in the higher energy range, specifically above 3.4 GeV, still sit more than three standard deviations away from the theoretical prediction. This is a large gap that suggests a serious problem. The researchers checked if the different experimental data sets were compatible with each other and found that, while there are some local tensions, the data generally agree with one another. The issue is not that the experiments contradict each other, but that the new, precise BES-III results are systematically higher than what the theory predicts. The authors conclude that there is no known mechanism within the current understanding of the strong force that can explain why the BES-III data is so high in this specific energy range. The discrepancy is not a result of a missing piece of the theory, but rather a genuine conflict between the new measurements and the established laws of physics.

This finding leaves the scientific community with a difficult choice. The theory is robust, and the mathematical tools used to describe it are under control. The new data is precise and appears reliable. The fact that they do not agree suggests that either the BES-III measurements have an unaccounted-for systematic error, or there is something fundamental about the strong force in this energy region that is not yet understood. The researchers hope their work will encourage further experimental investigations to re-measure this energy range with different methods. Until then, the tension between the theory and the BES-III data remains one of the most intriguing puzzles in the study of the strong force, standing as a potential signpost for new physics or a call for a closer look at the experimental setup.

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