“If thought corrupts language, language can also corrupt thought.”
Impact-Initiated Fusion (IIF) · Melbourne, Australia
A tale of two projectiles and an eccentric Z-Pinch.
Two Rattler accelerators fire small fuel projectiles into each other at the heart of Helios, a pulsed-power Z-pinch. Collision and pinch are designed to focus their energy into a hot spot. The design has been worked out in simulation. Physical testing is underway.
Simulation: Fig. 1 · The hot spot at first stagnation · t = 2.5 ns
3-D view: drag to rotate. With the view focused, arrow keys turn it, plus and minus zoom, R resets and Space pauses rotation.
Hardware, written like software.
We’re set on changing the shape of how fusion is done.
Nobody has yet built a machine that makes more electricity than it draws from the wall. Our route there starts with simulation software that follows the whole collision in 3-D. Machine learning is built into the design loop. A committee of models, trained on our own simulations, proposes what to try next.
A design change becomes a new run before it becomes a new part. This leads to what we call fusion 2.0: machines as fluid as the code that designs them. We are betting on a world where hardware and software are one and the same.
How IIF works
Impact-Initiated Fusion uses the energy of a collision to start fusion. Four things have to come together.
- Very high impact speed
- Focusing of that energy into a small hot spot
- A magnetic field that slows heat loss
- High fuel density at the moment of collision
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Concept art: Rattler electromagnetic accelerator 01 / 03Accelerate
Two Rattler electromagnetic accelerators fire small fuel projectiles at each other at very high speed. Getting both to arrive at the same point at the same instant, shot after shot, is half of the engineering.
Electromagnetic accelerators -

Concept art: Two projectiles closing on the capsule until they lock 02 / 03Collide
The projectiles meet head-on and the impact drives shock waves inward. Their internal structure is designed to focus those shocks, the way a lens focuses light, onto a small central region.
Shock lensing -

Concept art: Helios centre section, quarter cut-away 03 / 03Pinch
The collision happens at the heart of Helios, a pulsed-power Z-pinch. The fuel carries its own magnetic field, and Helios’s pulsed current is designed to pinch the hot spot, holding it together for longer and cutting heat loss. Neutrons from the reaction go to a lithium blanket, which makes heat for power and tritium for fuel.
Magnetic pinch
Most of the ingredients have been shown to work elsewhere.
- 2022
National Ignition Facility
Converging shock waves created the hot spot behind the National Ignition Facility’s 2022 ignition result.
- Sandia
MagLIF
Sandia’s MagLIF program showed that fuel held in a magnetic field keeps its heat better.
- Classic
Magnetic pinch
Magnetic pinches are one of the oldest tools in fusion.
- 2021
First Light
In 2021, First Light used a projectile to initiate fusion.
What’s different
- 01
Fuel on board.
The projectiles carry the fuel. There is no separate target to make, place and hit for each shot.
- 02
Energy in motion.
Most of a laser’s input energy never reaches the fuel. A projectile brings its energy with it, which in principle is far more efficient.
- 03
Three things invented.
A projectile shaped to focus the collision’s shocks into a hot spot, two accelerators timed to meet exactly on every shot, and an eccentric Z-pinch that sparks the plasma.
Technology readiness1
- Simulation software
- TRL 6
- Hardware
- TRL 2
The simulation software, built on Gkeyll, is well past the concept stage: it models the collision in 3-D on GPU and CPU supercomputers and performs as designed. We cross-check its results against a second solver configuration. The hardware is at the concept stage.
Powered by MATLAB® and Simulink®. Ciral Fusion is a member of the MathWorks Accelerator Program.
Shock lenses
Every face a lens.
Between the two projectiles, the fuel sits at the centre of a faceted shell. Each face is shaped as a lens, designed to bend the collision’s shock toward the centre so the fuel is squeezed evenly from every side.
Whether the lenses even out the implosion is still an open question.




Inside Rattler
A closer look at one of the two electromagnetic accelerators.


Inside Helios

Fired in software first.
Everything below is simulation output: computed, not measured. Physical testing is underway.
The whole collision, cell by cell.
Fuel, shock waves, magnetic field and burn, followed in three dimensions before anything is machined.
- 19.4millioncells in the 3-D grid2, 208 × 208 × 448
- 1,024parallel processes share the run2
- 21full 3-D snapshots3, one every 0.5 ns to 10 ns
- 2.5 and 5.5ns nanoseconds.first and second stagnation3
- 20 and 14keV kiloelectronvolts.average hot-spot ion temperature4
- 0.53 and 1.6g/cm³ grams per cubic centimetre.average hot-spot density4
- 0.37 and 0.18ns nanoseconds.Confinement time superscript 2, one for each stagnation5
- Radiation losses included.6
A hot spot you can turn in your hand.
Volumes show the hot spot as a 3-D object: nested surfaces, each enclosing hotter fuel than the one around it, at the two moments the fuel stagnates.
- Fuel boundary
- Hotter
- Hotter still
- Hottest
With the 3-D view focused, arrow keys turn it, plus and minus zoom, R resets and Space pauses rotation.
Temperature on the left. Burn on the right.
Slices show what happens inside. We cut the fuel along the collision axis at first stagnation: one half shows how hot it is; the other shows where fusion reactions run fastest.
- Ion temperature, cooler to hotter
- Burn rate, slower to faster
- Outer surface of the fuel
Frame by frame.
The first 5.5 nanoseconds of the simulated shot, one frame every half-nanosecond. Times count from the start of the shot.
One state, solved two ways.
We took one saved state of the simulation, from shortly before the times shown, and carried it forward with two solver configurations. In the cavity at the heart of the collision, the overall shape agrees; the fine structure at its centre differs. Comparisons like this show which features depend on the solver configuration.
- Flow speed, slower to faster
- Density, lower to higher
- Cavity wall
Next-generation simulation, at supercomputer scale.
Our simulation software is built on Gkeyll, the open-source plasma-physics framework, and extended by Ciral for IIF. Tested on GPU and CPU supercomputers, the software is at TRL 6.1 It guides what we build, and physical testing will check it against reality.
Frontier Machine Learning Surrogates propose. Physics decides.
Machine learning searches the design space. The full solver has the final word. Every round, the surrogates rank thousands of candidate designs; only the best eight are flown in the full solver.
One design search, evaluation by evaluation
Each dot is one candidate design flown in the 3-D physics engine; the line is the best measured so far.
The first 16 are an even survey; after that, the committee chooses.
Every projectile design has many interacting dimensions, and each full simulation is expensive. So we train fast surrogate models on the simulations we have already run, and let them suggest what to try next.
Three different model families vote: a Transformer, a deep LSTM and a gradient-boosted tree ensemble. Where they disagree, the search looks harder. Every promising candidate is re-run on the full physics solver, at higher resolution, before it counts.
A committee, not an oracle.
Three model families, trained separately, vote on every candidate design.
Disagreement is a signal.
Where the models disagree, the next simulations go.
The solver decides.
Nothing is a result until the full simulation confirms it on a finer grid.
Predicted before it was simulated
For every proposal, the committee’s prediction (made using only earlier results) against what the physics engine then measured.
- Search A (temperature + energy delivery)
- Search B (second architecture)
- Search C (adds a radiation-loss term)
- Diagonal: prediction equals result
Seven searches, seven honest verdicts
Archived design searches run with the Digital Twin’s physics engine in the loop.
| Search | Design space | Surrogate | Design parameters | Evaluations | Rounds after survey | Verdict |
|---|---|---|---|---|---|---|
| Search 1 | Lens geometry | Deep ensemble (5 neural networks) | 9 | 20 | 2 | Fixed budget (2 rounds) |
| Search 2 | Lattice micro-structure | Deep ensemble (5 neural networks) | 12 | 72 | 7 | Plateau |
| Search 3 | Architecture variant 1 | Deep ensemble (5 neural networks) | 12 | 40 | 3 | Plateau |
| Search 4 | Architecture variant 2 | Committee (9 models, 3 families) | 13 | 80 | 8 | Budget spent (still improving) |
| Search 5 | Variant 2 + radiation-loss term | Committee (9 models, 3 families) | 13 | 72 | 7 | Plateau |
| Search 6 | Variant 2 + radiation-loss term (paired test) | Deep ensemble (5 neural networks) | 13 | 40 | 3 | Plateau |
| Search 7 | Architecture variant 3 | Committee (9 models, 3 families) | 14 | 80 | 8 | Plateau |
| 7 searches · 404 evaluations | ||||||
Measured, not predicted.
The models are written in-house and gradient-checked. The search reports what the solver measured, not what a surrogate predicted.
The books balance on every run
Energy-conservation residual of every archived physics-engine evaluation used by the design searches.
Three physical tests, cheapest first
Each test has to pass before the next one is funded. The design has been worked out in simulation, and Phase A is underway.
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Phase AUnderway
The implosion test
Our first implosion runs, on existing test facilities. They show whether the model predicts how a real projectile behaves on impact. No fusion fuel is involved yet.
~12 monthsReal impact behaviour compared with the model
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Phase B
The accelerator
A bench-scale electromagnetic accelerator. We measure how much energy it puts into a projectile and how efficiently, then time two arms to meet.
~2 years from fundingProjectile energy and driver efficiency measured
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Phase C
The hot spot
Both arms fire into a collision chamber. We look for fusion neutrons, and for evidence that they come from a hot spot rather than a few stray fast particles.
~3 years from fundingFusion neutrons from a shaped collision
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After C
Gain, then a pilot plant
The next experiment uses deuterium-tritium fuel and aims for scientific gain: more fusion energy out of the fuel than goes into it. A pilot plant that makes electricity comes after that.
Funded by the next raiseScientific gain with deuterium-tritium fuel

The person behind Ciral
Jax El AntakiFounder
Jax invented Ciral’s approach and built the simulation engine behind it, which we call the Digital Twin. His background is in mathematical physics and machine learning, and he uses both to model the plasma and try designs in software long before anything is built.
LinkedInGet in touch
We’re raising now, in stages tied to the tests above. We’d like to hear from investors, research groups, government partners and data-centre operators planning for firm power in the 2030s.
Melbourne, Australia