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Equivariant Eikonal Neural Networks: Grid-Free, Scalable Travel-Time Prediction on Homogeneous Spaces

This paper introduces Equivariant Neural Eikonal Solvers, a novel framework that combines Equivariant Neural Fields with Physics-Informed Neural Networks to efficiently predict travel times on arbitrary homogeneous spaces by leveraging a shared backbone conditioned on latent point clouds for enhanced geometric grounding, scalability, and solution steerability.

Original authors: Alejandro García-Castellanos, David R. Wessels, Nicky J. van den Berg, Remco Duits, Daniël M. Pelt, Erik J. Bekkers

Published 2026-07-30
📖 7 min read🧠 Deep dive

Original authors: Alejandro García-Castellanos, David R. Wessels, Nicky J. van den Berg, Remco Duits, Daniël M. Pelt, Erik J. Bekkers

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 you are a master cartographer trying to draw the fastest route for a traveler to get from point A to point B. But here's the twist: the ground beneath them isn't flat or uniform. Sometimes it's a smooth highway, other times it's a muddy swamp, and sometimes the traveler is moving on the curved surface of a giant ball or even a saddle-shaped world. In physics and engineering, figuring out these "fastest arrival times" is governed by a tricky math puzzle called the eikonal equation. Think of it as the ultimate traffic calculator that tells you how long a wave of sound, light, or a robot's movement will take to reach its destination through a complex landscape.

For decades, scientists have used rigid, grid-based tools to solve this puzzle, like trying to draw a smooth curve using only square Lego bricks. If the landscape gets too complex, you need millions of tiny bricks, which takes forever to compute and eats up all your computer's memory. Recently, smart computers (neural networks) started trying to solve this without the bricks, learning the shape of the world directly. But these new methods often had to be retrained from scratch every time the landscape changed, making them too slow for real-time use. They were like a chef who could make a perfect pizza, but if you asked for a burger, they had to go back to culinary school and learn everything again.

This is where a team of researchers from the Netherlands steps in with a clever new idea. They built a "shape-shifting" neural network that doesn't just learn one specific map; it learns the rules of how maps change when you rotate or shift the world. By treating the problem like a game of geometric symmetry, they created a system that can instantly adapt to new terrains without needing to relearn everything. It's like teaching a chef the secret ingredient that makes any dish taste right, so they can instantly switch from pizza to burgers just by changing the ingredients, not the recipe.

The Magic of the "Steerable" Map

The paper introduces a framework called Equivariant Neural Eikonal Solvers (E-NES). To understand how it works, imagine you have a magical, stretchy rubber sheet representing a landscape. If you slide a rock across this sheet, the ripples (the travel times) move with it perfectly. If you rotate the sheet, the ripples rotate too. This property is called equivariance.

Most old neural networks are like rigid statues; if you rotate the input, the output gets scrambled and the network has to guess what happened. The E-NES, however, is built with a "geometric brain." It understands that if you rotate the input (the velocity field or the terrain), the solution (the travel time) must rotate in a matching, predictable way. The researchers achieved this by representing the "conditions" of the problem not as a simple list of numbers, but as a point cloud floating in a special mathematical space called a Lie group. Think of this point cloud as a set of floating anchors that tell the network where the "wind" is blowing or where the "mud" is located.

The genius move here is that the network shares its "muscle memory" (weights) across all these transformations. Instead of learning a separate solution for every possible rotation or shift, it learns one master solution that can be "steered" to fit any orientation. If you tell the network, "Rotate the wind 90 degrees," the network doesn't need to retrain; it simply applies that rotation to its internal logic, and the travel-time map updates instantly and correctly.

What They Found and How They Tested It

The team put their new solver to the test in three very different worlds: flat 2D maps, 3D cubes, and the curved surface of a sphere (like the Earth). They compared their method against the current state-of-the-art, which includes "Neural Operators" (like FC-DeepONet) and other grid-free methods.

In the 2D tests, which used a benchmark dataset called OpenFWI with 10 different types of velocity fields (some flat, some curved, some with faults), the E-NES showed it could be incredibly accurate. When they let the network "autodecode" (fine-tune its internal settings) for about 100 rounds, it beat the competition on seven out of ten datasets. For the trickier, more complex maps, the improvement was substantial. Even when they rushed the process to save time (using a "meta-learning" approach that only took a few steps), the E-NES was still competitive, but with a massive speed boost.

Here is where the numbers get exciting: The traditional methods took hundreds of seconds to fit a single new map. The E-NES, using its meta-learning trick, could fit 100 different velocity fields in less than 6 seconds total. That is a two-orders-of-magnitude improvement. While the "full convergence" mode (where it runs for longer to get the absolute best accuracy) took about 222 seconds for 100 fields, it still produced lower errors than the competitors in most cases.

They also tested the system in 3D. As they increased the grid size from a small 2x2x2 block up to a massive 6x6x6 block, the E-NES kept its error rates stable. Unlike the old grid-based methods (like the Fast Marching Method), which get slower and slower as you add more detail, the E-NES stayed fast because it doesn't rely on a grid at all. It treats the world as a continuous flow, so adding more resolution doesn't break it.

Finally, they took the system to a sphere (the 2-sphere, S2S^2). This is a non-Euclidean world, meaning the geometry is curved like a ball, not flat like a table. They tested it with constant speeds and with "Gaussian obstacle" fields (where a slow zone acts like a bump on the sphere). The E-NES handled this beautifully, achieving a relative error of just 0.013 for constant speeds and 0.015 for the obstacle fields. It even successfully planned geodesic paths (the shortest routes on a sphere), bending the trajectory around obstacles just as physics dictates.

Why This Matters

The paper explicitly rules out the idea that you need to retrain a network for every new scenario or that you are stuck with the limitations of a grid. They argue against the "per-instance training" of older methods, showing that it creates a bottleneck for real-time applications. Instead, they demonstrate that by embedding geometric symmetry directly into the network's architecture, you get a system that is not only more accurate but also "steerable."

This steerability is the key. It means that if you change the input (like rotating a velocity field), the output changes in a mathematically guaranteed way. This allows the system to generalize to arbitrary Riemannian manifolds—whether they are flat, spherical, or hyperbolic—without needing special adjustments. The authors suggest that this approach could revolutionize fields like seismic imaging (mapping underground structures), robotics (planning paths for robots in complex environments), and computer vision (understanding 3D shapes).

In short, the researchers didn't just build a faster calculator; they built a calculator that understands the geometry of the world it's calculating for. They showed that by respecting the symmetries of the universe, you can solve complex travel-time puzzles with a fraction of the effort, opening the door to real-time, high-precision modeling in 2D, 3D, and even on the surface of a sphere.

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