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Improved capabilities of the TurboGAP code for radiation induced cascade simulations: an illustration with silicon

This paper presents enhanced capabilities of the TurboGAP code for radiation-induced cascade simulations in silicon, featuring a two-temperature model, adaptive timesteps, and realistic electronic stopping power to accurately predict defect clustering and ion-beam mixing in systems up to one million atoms.

Original authors: Uttiyoarnab Saha, Ali Hamedani, Miguel A. Caro, Andrea E. Sand

Published 2026-07-08
📖 5 min read🧠 Deep dive

Original authors: Uttiyoarnab Saha, Ali Hamedani, Miguel A. Caro, Andrea E. Sand

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

Imagine a computer simulation as a giant, high-speed movie camera filming what happens when a single, super-fast bullet (an ion) smashes into a block of silicon. This "bullet" is actually a particle of radiation, and when it hits the silicon, it creates a chaotic chain reaction, knocking atoms around like billiard balls. This is called a "radiation cascade."

For a long time, scientists have struggled to film this movie accurately. They had a choice:

  1. The Super-Detailed Camera: Extremely accurate but so slow it could only film a tiny, tiny speck of silicon for a split second.
  2. The Fast Camera: Could film a huge chunk of silicon for a long time, but the physics were often too simple, missing important details about how the atoms interact.

This paper introduces an upgrade to a software tool called TurboGAP. Think of TurboGAP as a high-performance engine that allows scientists to use the "Super-Detailed" physics (called Machine Learning Interatomic Potentials) but run it at "Fast Camera" speeds. The authors have added three new features to this engine to make it even better at simulating radiation damage.

Here are the three new features, explained with simple analogies:

1. The "Electronic Brake" (Electronic Stopping)

When a fast particle moves through a material, it doesn't just bump into other atoms; it also drags electrons along with it, losing energy like a car driving through thick mud.

  • The Old Way (Friction Model): Imagine trying to stop a sliding puck on ice by applying a brake only if the puck is moving faster than a specific speed. If the puck slows down below that speed, the brake magically turns off. The problem is, scientists had to guess what that "magic speed" was. If they guessed wrong, the simulation gave the wrong results.
  • The New Way (EPH Model): The authors added a smarter system. Instead of a simple on/off brake, they created a "smart thermostat" that connects the moving atoms to a giant, invisible heat bath of electrons. This system automatically adjusts the braking force based on how crowded the electrons are in that specific spot. It doesn't need a "magic speed" cutoff; it just works naturally, slowing the atoms down more realistically.

2. The "Smart Timer" (Adaptive Timestep)

In a simulation, the computer takes tiny "steps" in time to calculate where atoms move next.

  • The Problem: When atoms are flying calmly, the computer can take big steps. But when two atoms crash into each other at high speed, the forces change instantly. If the computer keeps taking big steps, it misses the crash or calculates it wrong.
  • The Solution: The new TurboGAP has a "smart timer." It watches the atoms. If they are moving slowly, it takes big steps to save time. The moment atoms get close to crashing, the timer instantly shrinks the steps to be microscopic, ensuring the crash is captured perfectly. Once the chaos settles, it speeds the steps back up again.

3. The "Cooling Border" (Grouping of Atoms)

When a radiation cascade happens, it creates a massive amount of heat in the center of the simulation. If this heat stays trapped, the whole block of silicon would melt in the computer, which isn't realistic for most experiments.

  • The Solution: The authors added a way to group atoms at the very edge of the simulation box. They act like a cooling jacket, constantly absorbing the excess heat from the center and keeping the edges at a steady temperature. This allows the "heat wave" from the crash to flow out naturally, just like heat flowing out of a hot pan into the air.

What Did They Find?

Using these new tools, the authors simulated a silicon block with one million atoms (a huge number for this type of physics) and shot a particle with up to 10,000 electron-volts of energy into it.

  • The "Magic Speed" Issue: They found that the old "Friction Model" (the one with the guessable speed limit) gave different results depending on what speed limit you picked. The new "Smart Thermostat" (EPH model) gave consistent results without needing any guesses.
  • Defect Clusters: When the atoms settle down after the crash, they form "defects" (holes or extra atoms). The new model showed that these defects tend to clump together into larger, more realistic groups compared to the old model.
  • Mixing: They measured how much the atoms got "mixed up" by the crash. The results from their new, realistic model matched real-world laboratory experiments much better than previous simulations did.

The Bottom Line

The authors didn't just make the software faster; they made it smarter. By adding a realistic way to handle energy loss to electrons, a smart timer for collisions, and a better cooling system, they can now simulate massive radiation events in silicon with high accuracy. This helps scientists understand how materials degrade under radiation without having to guess the rules of the game.

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