Measurements of charged-particle pseudorapidity and transverse momentum distributions in O+O and Ne+Ne collisions at sNN=5.36\sqrt{s_{_\text{NN}}} = 5.36 TeV with the ATLAS detector

The ATLAS experiment presents measurements of charged-particle pseudorapidity and transverse momentum distributions in O+O and Ne+Ne collisions at sNN=5.36\sqrt{s_{_\text{NN}}} = 5.36 TeV, characterizing these observables across various centrality intervals and comparing the results with hydrodynamic calculations.

Original authors: ATLAS Collaboration

Published 2026-06-19
📖 5 min read🧠 Deep dive

Original authors: ATLAS Collaboration

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

The Big Picture: Smashing Tiny "Bowling Pins"

Imagine the Large Hadron Collider (LHC) as a massive, high-speed racetrack where scientists smash particles together to see what happens. Usually, they smash giant lead atoms (like bowling balls) together to create a tiny, super-hot drop of "primordial soup" called the Quark-Gluon Plasma (QGP). This soup is the state of matter that existed just after the Big Bang, where particles are so hot they melt into a fluid.

For a long time, scientists wondered: Does this fluid only form when you smash huge atoms together? Or can it form even when you smash tiny atoms?

To answer this, the ATLAS experiment at CERN decided to smash two types of small atoms: Oxygen (O) and Neon (Ne).

  • Oxygen (16O) is like a perfect, round cluster of marbles.
  • Neon (20Ne) is similar in size but shaped differently. Because of how its internal parts (alpha clusters) are arranged, it looks a bit like a bowling pin or a teardrop.

The scientists wanted to see if the shape of the "bowling pin" (Neon) versus the "round ball" (Oxygen) changed how the "primordial soup" flowed and expanded.

The Experiment: A High-Speed Photo Shoot

The team collected data from millions of these collisions. They used the ATLAS detector, which is like a giant, 3D camera surrounding the crash site.

  1. The Crash: They smashed Oxygen and Neon atoms together at nearly the speed of light (5.36 TeV).
  2. The "Centrality" (How Hard the Crash Was): Just like in a car crash, a head-on collision is different from a glancing blow.
    • Central collisions (0–5%): The atoms hit dead center. This creates the biggest, hottest, and most "fluid-like" soup.
    • Peripheral collisions (70–80%): The atoms just grazed each other. This creates a smaller, cooler splash.
  3. The Measurement: They counted how many charged particles (like tiny shrapnel) flew out and measured how fast they were moving. They looked at this from two angles:
    • Pseudorapidity (η\eta): A measure of the angle relative to the beam, which is easy to measure but slightly distorts the view of slow-moving particles.
    • Rapidity (yπy_\pi): A more "true" measure of the particle's motion, calculated by assuming the particles are pions (a common type of particle). This gives a clearer picture of the physics.

The Key Findings

1. The "Bowling Pin" Effect
The scientists found that Neon collisions (the bowling pin shape) produced slightly more particles than Oxygen collisions (the round shape), especially in the most violent, head-on crashes. This suggests that the initial shape of the nucleus matters. The "pin" shape creates a slightly different starting point for the fluid, leading to a different flow pattern.

2. The Flow of the Soup (Radial Flow)
When the atoms smash, the resulting soup expands outward like an exploding balloon. This is called radial flow.

  • The data showed that in the most central (head-on) collisions, the soup expands faster and pushes particles harder.
  • This "hardening" of the particle speeds happened in both Oxygen and Neon, proving that even these tiny collisions create a fluid-like state that behaves like a hydrodynamic system (like water flowing).

3. Comparing the Shapes
When they compared the ratio of Neon to Oxygen results, they found:

  • Particle Count: Neon produced about 5% to 20% more particles than Oxygen, depending on how central the collision was.
  • Particle Speed: The average speed of the particles was almost identical for both. This is a crucial clue: it suggests that while the shape changes the initial explosion, the flow of the fluid is remarkably similar once it gets going.

4. Checking the Math
The scientists compared their real-world data with computer simulations (theoretical models).

  • Some models (like EPOS) did a great job predicting the results.
  • Other models based on fluid dynamics (like IPGlasma and Trento) were close but had some trouble getting the details right, especially in the "grazing" (peripheral) collisions.
  • The fact that the real data didn't perfectly match the models tells scientists they need to refine their understanding of how these tiny nuclei are structured inside.

The Conclusion

This paper is a landmark because it is the first detailed look at how Oxygen and Neon collisions behave at the LHC.

The main takeaway is that size isn't everything. Even with atoms as small as Oxygen and Neon, you can create a state of matter that flows like a fluid. Furthermore, the specific shape of the atom (round vs. bowling pin) leaves a fingerprint on the collision, changing how many particles are produced. This helps scientists understand the very earliest moments of the universe and the fundamental rules that govern how matter behaves under extreme heat and pressure.

In short: They smashed tiny bowling pins and round balls together, watched the splash, and confirmed that even the smallest crashes can create a fluid that flows just like the giant ones.

Drowning in papers in your field?

Get daily digests of the most novel papers matching your research keywords — with technical summaries, in your language.

Try Digest →