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Radiative corrections to the subprocess of annihilation of quark-antiquark pair of prompt photon production in proton-proton collisions at NICA energies s\sqrt{\mathbf{s}}= 10 GeV

This paper presents a comprehensive theoretical and numerical study of QCD and QED radiative corrections to prompt photon production via quark-antiquark annihilation in proton-proton collisions at NICA energies (s=10\sqrt{s}=10 GeV), utilizing FeynCalc and PYTHIA 8.316 to analyze differential cross-sections and spin asymmetries, revealing that these corrections are significant at low energies and small transverse momenta with excellent agreement between analytical calculations and simulations.

Original authors: Mohsun R. Alizada, Azar I. Ahmadov

Published 2026-10-02
📖 5 min read🧠 Deep dive

Original authors: Mohsun R. Alizada, Azar I. Ahmadov

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

High-energy physics often feels like trying to understand a storm by studying a single raindrop. In the world of particle accelerators, scientists smash protons together at incredible speeds to break them apart and see what lies inside. Among the debris, photons—particles of light that carry no electric charge and no color charge—play a unique role. Because they do not interact with the strong nuclear force that binds protons together, they can escape the chaotic collision zone without being deflected or absorbed. They act as perfect messengers, flying straight out of the interaction point to tell researchers exactly what happened at the moment of impact. This makes them invaluable for mapping the internal structure of protons, specifically how the smaller particles inside, known as quarks and gluons, are distributed and how they move.

While much of this research happens at the world's most powerful machines, like the Large Hadron Collider, there is a different kind of physics happening at lower energies. At the Nuclotron-based Ion Collider Facility (NICA) in Russia, protons collide at a center-of-mass energy of 10 GeV. This is a much gentler collision compared to the trillions of electron volts seen at the Large Hadron Collider, but it offers a unique window into how matter transitions between different states, such as the formation of a quark-gluon plasma. In this lower-energy regime, the rules of the game change. The dominant processes that create light at the highest energies are not the same ones that matter here. To understand the data coming out of NICA, scientists must calculate exactly how these collisions produce photons, including the subtle, secondary effects that occur when particles emit extra radiation during the crash.

A team of researchers from Baku State University has undertaken a detailed study of one specific way photons are created at NICA: the annihilation of a quark and an antiquark. In this process, a particle of matter meets its antimatter counterpart, and they vanish, converting their mass into energy that manifests as a photon. However, the universe is rarely simple. When these particles collide, they often emit additional particles, such as extra gluons or photons, before or after the main event. These are called radiative corrections. The researchers wanted to know how much these extra emissions change the final result. They focused on three specific variations of this annihilation process: one where the quark and antiquark produce a photon and two gluons, another where they produce a photon and a quark-antiquark pair, and a third where they produce a photon and two photons.

To get a complete picture, the team performed two types of calculations. First, they used rigorous mathematical methods to derive exact formulas for the probability of these events happening. They calculated how the total amount of light produced changes depending on the energy of the collision, the angle at which the photon flies out, and how fast it moves sideways relative to the beam. They also looked at what happens when the protons are polarized, meaning their internal spins are aligned in a specific direction, rather than being randomly oriented. This allowed them to see how the spin of the protons influences the creation of these photons. Second, to ensure their math matched reality, they used a sophisticated computer simulation called PYTHIA. This program mimics the complex chain of events that happens in a real detector, including the cascading showers of particles that occur after the initial collision.

The results revealed a clear hierarchy in how these processes behave. The most common way for these extra particles to appear is through the emission of gluons, which are the carriers of the strong nuclear force. This channel dominates the total production, accounting for the vast majority of the events. The process involving two photons is extremely rare, suppressed by the nature of electromagnetic interactions. A key finding was that these extra emissions are most significant when the collision energy is low and the photons have a small amount of sideways momentum. As the energy increases, the relative importance of these corrections drops, and the behavior of the different processes begins to level off. The researchers also found that the polarization of the protons has a profound effect. When the protons are aligned, the probability of certain outcomes changes dramatically, particularly for the process involving a quark and an antiquark in the final state, which becomes the dominant channel at high sideways momenta.

The study confirmed that the mathematical formulas and the computer simulations agree very well in the central regions where most collisions occur. However, at the very edges of what is physically possible—when the photon carries away almost all the available energy—the two methods diverge. The strict mathematical formulas predict a sharp spike in probability that does not exist in the real world, a phenomenon known as a divergence. The computer simulation, which accounts for the natural "smearing" of energy and the emission of soft particles, smooths out these spikes, providing a more realistic picture. This difference highlights the necessity of using advanced simulation techniques to interpret data at the boundaries of the phase space.

Ultimately, this work provides a precise map of how quark-antiquark annihilation produces light at NICA energies. It shows that while the basic process is well understood, the inclusion of radiative corrections is essential for accurate predictions, especially at lower energies. The research demonstrates that at these specific energy levels, the annihilation channel is a competitive and vital source of photons, unlike at much higher energies where other processes take over. By clarifying the behavior of these corrections and the role of proton polarization, the study offers a solid foundation for future experiments at NICA, helping physicists distinguish between the signals of new physics and the expected background of known particle interactions.

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