Topological production of charmonia with event-shape engineering in $pp$ collisions at s=13\sqrt{s} = 13 TeV using PYTHIA8

This study utilizes PYTHIA8 simulations to investigate the correlation between prompt and nonprompt J/ψJ/\psi production and transverse spherocity in 13 TeV $pp$ collisions, demonstrating how this event-shape observable can distinguish hard QCD processes from underlying events influenced by multiple parton interactions.

Original authors: Aswathy Menon Kavumpadikkal Radhakrishnan, Suraj Prasad, Neelkamal Mallick, Raghunath Sahoo

Published 2026-03-25
📖 5 min read🧠 Deep dive

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

Imagine you are a detective trying to figure out how a chaotic party was organized. You walk into a room where thousands of people (particles) have just collided, creating a massive, swirling crowd. Your job is to understand how specific, rare guests (heavy particles like charm and beauty quarks) managed to show up and form pairs (like the J/ψ particle) amidst the chaos.

This paper is a simulation of that party, run on a supercomputer using a program called PYTHIA8, which acts like a virtual physics engine. The researchers are studying collisions at the world's most powerful particle accelerator (the LHC), but instead of real data, they are looking at a perfect digital model to understand the rules of the game.

Here is the breakdown of their investigation using simple analogies:

1. The Two Types of "Guests" (Prompt vs. Non-Prompt)

In this particle party, there are two ways the star guest, the J/ψ (a heavy particle made of a charm quark and its anti-quark), can arrive:

  • Prompt J/ψ: These are the "VIPs" who arrive directly from the main collision. They are born instantly when the initial crash happens. Think of them as the people who were right in the center of the explosion.
  • Non-Prompt J/ψ: These are the "late arrivals." They don't come from the main crash directly. Instead, they are the children of a heavier, unstable guest (a beauty hadron). The beauty guest arrives, lives for a tiny fraction of a second, and then decays (dies) to produce the J/ψ. It's like a guest bringing a friend who shows up a moment later.

2. The "Shape" of the Party (Transverse Spherocity)

Usually, physicists sort these parties by counting how many people are in the room (multiplicity). But the authors realized that just counting heads isn't enough; you need to know the shape of the crowd.

They introduced a new tool called Transverse Spherocity (let's call it the "Party Shape Meter").

  • Jetty Events (Low Spherocity): Imagine a party where everyone is rushing in two straight, opposite lines, like a high-speed train crash. This is a "Jetty" event. It's chaotic, directional, and usually caused by a single, hard, violent collision.
  • Isotropic Events (High Spherocity): Imagine a party where everyone is standing in a perfect circle, chatting evenly in all directions. This is an "Isotropic" event. It's softer, more uniform, and usually caused by many smaller, gentle interactions happening at once.

3. The Big Discovery: How the Party Shape Affects the Guests

The researchers used the computer to see how the "Party Shape" changes the behavior of the J/ψ guests. Here is what they found:

  • The "Soft" Crowd Makes Harder Particles: Surprisingly, they found that the Prompt J/ψ (the VIPs) were actually moving faster (had higher momentum) in the Isotropic (round/calm) parties than in the Jetty (straight-line) parties.

    • Why? In the round parties, there are many small interactions happening at once (like a crowded dance floor). The computer model suggests that these crowded conditions help the charm quarks "hug" each other and form a J/ψ with a big boost of energy. It's like a crowded dance floor pushing people together with more force than a straight hallway.
  • The "Heavy" Guests Love the "Hard" Collisions: The Non-Prompt J/ψ (the late arrivals from beauty decay) behaved differently. At high speeds, they were more common in the Jetty events.

    • Why? Creating a heavy beauty quark requires a lot of energy, like a sledgehammer hitting a nail. This usually happens in those straight-line, high-energy "Jetty" collisions. Once the beauty guest is created, it flies off and eventually decays into a J/ψ.

4. The "Selfie" Problem (Autocorrelation Bias)

One of the most important lessons in the paper is about bias.

  • Imagine you are trying to measure how loud a party is by asking the people in the room to shout. If you ask the people in the room to define the room, your measurement is biased because they are part of the noise.
  • In physics, if you measure the "shape" of the event using particles from the same place where you are looking for the J/ψ, you get a distorted picture.
  • The authors found that if you look at the "middle" of the collision (mid-rapidity) and use the middle particles to define the shape, you get a false signal. However, if you look at the "front" of the collision (forward rapidity) and use those particles to define the shape, the signal is much cleaner. It's like measuring the noise of a concert by listening to the back of the hall rather than standing right next to the speakers.

5. Why Does This Matter?

This study is like a "flight simulator" for particle physicists.

  • Testing the Theory: It confirms that our current computer models (PYTHIA8) can explain how heavy particles behave in different types of collisions.
  • Future Experiments: Now that we know how the shape of the event changes the outcome, real experiments at the LHC can use this "Party Shape Meter" to separate different types of physics. It helps them understand the "underlying event"—the invisible background noise that affects how particles are created.
  • The "Underlying Event": The paper shows that even though the J/ψ is created in the initial split-second crash, the "background noise" (the underlying event) plays a huge role in shaping its final speed and direction.

Summary

Think of the universe as a giant, chaotic dance floor. This paper teaches us that how the crowd moves (the shape of the event) dictates how the rare dancers (heavy particles) move.

  • If the crowd is swirling in a circle (Isotropic), the "instant" dancers move faster.
  • If the crowd is rushing in straight lines (Jetty), the "heavy" dancers are more likely to appear.

By understanding these patterns, scientists can better decode the fundamental rules of how matter is built from the smallest building blocks.

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