Anisotropic flow measurements in OO and Ne-Ne collisions with ALICE
This paper presents ALICE measurements of anisotropic flow in O and Ne collisions using multi-particle cumulants, including the first reconstruction of the elliptic flow probability distribution and the first measurement of the ratio in light-ion systems, to investigate the influence of well-constrained nuclear geometry on collective dynamics.
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 heart of matter, protons and neutrons are not solid, unchanging spheres. Instead, they are bustling cities of quarks and gluons, constantly shifting and interacting. When scientists smash atomic nuclei together at nearly the speed of light, they create a fleeting, super-hot soup of these fundamental particles known as the quark-gluon plasma. This state of matter is believed to have filled the entire universe just moments after the Big Bang. For decades, researchers have studied this plasma by colliding heavy atoms like lead, which create large, chaotic fireballs. However, a surprising discovery in recent years showed that even when smashing much smaller particles, like protons against lead, this same fluid-like behavior emerges. This raised a profound question: is the fluid behavior driven solely by the sheer energy of the collision, or does the specific shape and internal structure of the colliding nuclei play a crucial role in how the plasma flows?
To answer this, a team of physicists using the ALICE detector at the Large Hadron Collider turned their attention to light ions, specifically oxygen and neon. Unlike the heavy lead nuclei, the nuclear structures of oxygen and neon are well-constrained from decades of low-energy physics experiments. By colliding these specific nuclei at an energy of 5.36 TeV, the researchers created a controlled environment to test how the initial geometry of the nuclei influences the resulting flow of particles. They analyzed billions of oxygen-oxygen collisions and hundreds of millions of neon-neon collisions to see if the specific structural differences between the nuclei left a distinct fingerprint on the plasma they created.
The researchers focused on a phenomenon called anisotropic flow, which describes how particles fly out from the collision point. If the collision zone were perfectly round, particles would spray out equally in all directions. However, because the nuclei are not always perfectly aligned, the collision zone often has an oval or triangular shape. This initial shape acts like a mold, pushing the particles to flow more strongly in certain directions than others. By measuring how particles move in relation to one another, the team could reconstruct the hidden shapes of the collision zones and the probability of different flow patterns occurring. They looked at correlations between groups of particles, ranging from pairs up to groups of eight, to get a detailed picture of the underlying distribution of these flows.
The results confirmed that the nuclear shape is indeed a dominant factor. In the most central collisions, where the two nuclei hit each other head-on and overlap completely, the neon-neon collisions produced a stronger elliptical flow than the oxygen-oxygen collisions. This difference suggests a more elliptical shape of the neon nucleus in comparison to the oxygen nucleus, as expected by current models. The data showed that the probability distribution of this flow was wider and more pronounced in neon, matching the expectation that a more elliptical nucleus creates a more elliptical overlap region than a less elliptical one. Furthermore, the study revealed that as the collisions became less central, the flow patterns evolved in a way that tracked the changing geometry of the overlapping nuclei, providing a clear link between the static structure of the atom and the dynamic behavior of the plasma.
Perhaps the most significant finding was the first-ever reconstruction of the full probability distribution for the elliptic flow in these light-ion systems. This allowed the team to see not just the average flow, but the full range of possible flow outcomes for every single collision. They also examined the triangular flow, which arises from random fluctuations in the positions of particles inside the nucleus. In heavy lead collisions, this triangular flow is usually driven almost entirely by random fluctuations because the lead nuclei are so large and round that their initial shape is nearly circular. However, in the neon collisions, the researchers found that the triangular flow was enhanced beyond what random fluctuations alone would produce. This suggests that the initial, non-circular shape of the neon nucleus is actively driving the flow, rather than just random noise. These measurements provide a new, precise way to disentangle the effects of nuclear structure from the properties of the plasma itself, offering a clearer window into the fundamental dynamics of the early universe.
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