Transport of hard probes in the glasma
This thesis investigates the transport of jets and heavy quarks through the pre-equilibrium glasma phase of heavy-ion collisions using classical and quantum methods, revealing that the glasma induces significantly larger and anisotropic transport coefficients and measurable azimuthal decorrelation, thereby highlighting the necessity of accounting for this stage to avoid biases in extracting QGP properties.
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In the most extreme conditions imaginable, where matter is crushed and heated beyond the point of any solid, liquid, or gas, a new state of existence emerges. This is the quark-gluon plasma, a super-hot soup of the fundamental building blocks of the universe. Scientists recreate this state for fleeting moments by smashing heavy atomic nuclei together at nearly the speed of light in massive particle accelerators. When these collisions occur, they do not produce a smooth, uniform fireball immediately. Instead, they create a chaotic, turbulent prelude known as the "glasma." Think of the glasma as a storm of invisible, powerful magnetic and electric tubes stretching between the colliding nuclei, existing for a fraction of a second before the system settles into the hot plasma. Understanding how this stormy beginning affects the particles flying through it is crucial, because it changes how we interpret the data from these high-energy experiments.
For decades, physicists have studied how "hard probes"—specifically heavy quarks and jets, which are sprays of particles—travel through the resulting hot plasma. These probes act like messengers, carrying information about the medium they traverse. However, a significant gap in our understanding has been the very first moments of the collision, the glasma stage. Most previous studies simply ignored this early phase, assuming the probes only began interacting once the hot plasma had formed. This simplification might have been hiding important details about how these particles lose energy and change direction. Dana Avramescu's doctoral research at the University of Jyväskylä tackles this missing piece, investigating exactly how the turbulent glasma fields influence the journey of these hard probes before they even reach the hot plasma.
The research uses powerful computer simulations to model the glasma as a complex, evolving field of color forces. They then sent virtual heavy quarks and jets through this simulated environment to see how they would react. The results were striking. The study found that the glasma is far more aggressive than previously thought. As these particles move through the glasma, they experience a massive and rapid change in their momentum, far greater than what they would encounter later in the hot plasma. This "momentum broadening" is not uniform; it is highly directional. The particles are pushed much harder in the direction of the collision than they are sideways, creating a distinct anisotropy. The strength of this effect is so intense that the transport coefficients, which measure how easily particles move through the medium, are significantly larger in the glasma than in the established hot plasma.
One of the most compelling findings concerns pairs of heavy quarks produced back-to-back in the initial collision. In a calm environment, these pairs would fly apart in opposite directions, maintaining a straight line. However, the simulations showed that the glasma fields act like a violent wind, deflecting these pairs and scrambling their alignment. The angle between them becomes decorrelated very quickly, within a tiny fraction of a second. This suggests that the glasma leaves a unique fingerprint on the final state of these particles. While the hot plasma also scrambles these pairs, the glasma does so with a different signature, offering a potential way for experimentalists to distinguish the early storm from the later fireball. The research indicates that measuring the angular correlation of heavy quark pairs could provide a direct window into this fleeting, pre-equilibrium stage.
The study also addressed a subtle but critical technical challenge: how to define momentum in a system governed by complex quantum rules. The researchers had to carefully distinguish between the physical momentum of a particle and the mathematical "canonical" momentum used in calculations, which can be distorted by the choice of coordinate system. By applying a specific mathematical adjustment known as the Coulomb gauge, they were able to remove these artificial distortions. This allowed them to confirm that their classical simulations, which treat particles as tiny billiard balls, produce results that align perfectly with more complex quantum calculations. This agreement is vital because it validates the use of simpler models to study these incredibly fast and dense environments.
Ultimately, this work does not claim to have solved the entire puzzle of heavy-ion collisions, but it has illuminated a dark corner of the timeline. The simulations show that the glasma is not a passive backdrop but an active participant that significantly alters the trajectory and energy of hard probes. While the effect on the overall energy loss of a single particle is moderate compared to other factors, the impact on the directional correlation of particle pairs is substantial. By proving that the glasma leaves a measurable mark, the research provides a new tool for physicists. It suggests that by looking closely at how heavy quark pairs are scattered, we can finally see the ghost of the glasma, the turbulent first breath of the universe's most extreme matter, before it settles into the hot plasma we have studied for so long.
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