Probing Glueball content of X(2370) through heavy quarkonium radiative decays and electron-positron annihilation
This paper investigates the glueball content of the resonance by analyzing light-cone distribution amplitudes and a tetra-mixing scheme to predict branching ratios for heavy quarkonium radiative decays and electroproduction cross sections, offering testable theoretical predictions for current BESIII and Belle-II experiments.
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
Deep within the subatomic world, where particles interact through the strong nuclear force, physicists have long searched for a ghostly kind of matter made entirely of force itself. In the standard model of particle physics, forces are carried by particles called gluons, which usually bind together to form protons and neutrons. However, theory suggests that gluons can also bind to each other, creating a particle made purely of glue, known as a glueball. Finding one would be a monumental achievement, offering a direct window into how the strong force holds the universe together and why quarks can never be found alone. For decades, these particles remained theoretical, hiding among a crowd of ordinary particles that look and act very similarly.
Recently, a particle named X(2370) has emerged as a prime suspect for being the lightest of these glueballs. Discovered in the debris of particle collisions, it has the right mass and the right quantum properties to be this elusive object. Yet, a simple explanation is not enough; because the strong force is so complex, a glueball might not exist in isolation. It could be a mixture, blending with ordinary particles made of quarks and antiquarks. The big question for physicists is not just whether the glueball exists, but how much of it is actually inside the X(2370). Is it a pure glueball, or is it a hybrid, and if so, how much of each ingredient is present?
A team of researchers has now taken a fresh look at this puzzle by analyzing how heavy particles called quarkonia decay. These heavy particles, such as the J/psi and the psi(2S), are essentially bound states of a charm quark and its antimatter partner. When they decay, they often emit a flash of light, a photon, and leave behind a lighter particle. The researchers focused on the specific process where these heavy particles shed a photon and transform into a pseudoscalar meson, a type of particle that includes the X(2370). By studying the rates at which these decays happen, the team could work backward to determine the internal composition of the resulting particles.
The core of their work involved a sophisticated mixing scheme, a mathematical framework that describes how different types of particles blend together. They treated the X(2370) as a product of four distinct components mixing together: a glueball, a particle made of charm quarks, and two types of particles made of lighter quarks. Using the latest experimental data on how often the J/psi particle decays into various known mesons, the team calculated the specific angles that define this mixture. They found that the data fits a model where the glueball component is significant, but not the only ingredient. The calculations revealed that the mixing between the glueball and the charm-quark particle is very small, but it is crucial for explaining the observed behavior.
One of the most striking findings concerns how the X(2370) behaves when produced by different parent particles. The researchers discovered that the probability of the J/psi decaying into an X(2370) and a photon is extremely sensitive to the exact details of the mixing. In fact, the calculations show that if the mixing angle were slightly different, the production rate would drop to nearly zero due to a cancellation effect, where the different components of the particle interfere with each other destructively. This sensitivity acts like a precise tuning fork; the fact that the X(2370) is observed at all, and with the specific rate measured by experiments, tells us exactly how the ingredients are mixed. The team also predicted that the psi(2S) particle, a heavier cousin of the J/psi, should produce the X(2370) at a different rate, with a similar sensitivity to the mixing angle but occurring at a different value.
Beyond the decay of heavy particles, the study also looked at how these particles are created when electrons and positrons smash into each other. The researchers calculated the likelihood of producing the X(2370) in these collisions, specifically when it is accompanied by a lighter particle called a rho meson. Their theoretical predictions for this process align well with existing measurements for other similar particles, giving confidence in their method. They provided specific predictions for the production rates of the X(2370) at various energy levels, which are now waiting to be tested by current experiments at facilities like BESIII and Belle-II.
The ultimate goal of this work is to move beyond speculation and pin down the true nature of the X(2370). The researchers conclude that the particle is indeed dominated by a glueball component, but it is a complex mixture rather than a pure state. Their analysis suggests that the glueball content is large enough to explain the particle's existence, yet small enough to allow for the mixing effects that make it observable. The findings offer a clear path forward: by measuring the decay rates of the psi(2S) and the production rates in electron-positron collisions, scientists can verify the mixing angles they have calculated. If the new data matches their predictions, it will provide definitive proof that the X(2370) is the long-sought lightest glueball, finally revealing the pure force of the strong interaction in a tangible form.
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