NestyNet. III. Symbolic Regression from Analytic Neural Surrogates
NestyNet-SR is a novel symbolic regression framework that leverages analytic neural surrogates to recursively decompose complex data into separable components, which are then distilled into exact closed-form expressions, achieving state-of-the-art performance on benchmarks and successfully rediscovering fundamental physical laws from real astronomical data.
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Nature often hides its simplest rules behind a veil of complexity. A physical law might look like a tangled knot of variables when written in raw data, yet it could be a single, elegant sentence if only we knew how to look at it. For centuries, scientists have relied on human intuition to find that right way of looking, to untangle the knot and reveal the clean structure underneath. But as the universe presents us with more data and more intricate systems, our unaided minds can struggle to see the pattern. The question has become whether machines can help us survey a much wider range of possibilities, uncovering relationships that fit the data perfectly and might even predict how things behave in new situations we have never seen before. This is the goal of a field called symbolic regression: the search for the actual mathematical sentences that describe the world, rather than just fitting a curve to a graph.
The challenge is that the number of possible sentences is so vast that searching through them one by one is impossible. It is like trying to find a specific book in a library where every shelf contains every possible combination of words. To solve this, researchers Rodrigo Ibata and his team have developed a new method called NestyNet-SR. Instead of guessing random sentences, their system first builds a highly accurate, flexible model of the data using a type of artificial neural network. This model acts as a surrogate, a stand-in that knows the data intimately. The crucial innovation is that this surrogate is designed to be mathematically transparent; it allows the researchers to calculate exactly how the output changes when they tweak the inputs, down to the finest details. By studying these changes, the system can detect if the data can be broken down into simpler, independent parts. It asks questions like: does this part of the system depend only on temperature, while that part depends only on pressure? Or is there a hidden combination of variables, like a specific ratio or a sum, that makes the whole thing behave simply?
Once the system identifies these simpler building blocks, it moves to the second stage: translating them back into human-readable language. This is where the method shines. It does not just look for a single perfect formula; it separates the search for the structure from the search for the numbers. Imagine trying to find the shape of a key without knowing the exact size of its teeth. The system first finds the shape—the skeleton of the equation—and then fits the precise numbers to it. This approach allows it to handle complex layers of nesting that usually stump other methods. It can discover that a relationship involves a sine wave, or a square root, or a power law, and it can do so even when the data is noisy or comes from multiple different experiments at once. The system is also strict about physical reality; it checks that the units of measurement make sense, ensuring that a formula does not accidentally add meters to seconds.
The team tested their method on a famous set of 120 physics equations, known as the AI Feynman benchmark, which are designed to be difficult for computers to solve. In a world without noise, the system successfully recovered every single one of the 120 equations exactly, a first for this type of benchmark. It did this by finding the hidden internal coordinates that made the complex equations look simple. When they added realistic noise to the data, simulating the imperfections of real-world measurements, the system still managed to find the correct structure for nearly half of the problems, and it could tell the researchers which parts of the structure were still reliable. This ability to distinguish between a true law and a lucky guess is a significant step forward.
To prove the method works on real astronomical data, the researchers applied it to a collection of spiral galaxies from the SPARC survey. They gave the computer only the separate contributions of gas and stars to the galaxy's rotation, without telling it how to combine them. The system was asked to find the rule that governs how these galaxies spin. Without any prior instructions, the algorithm discovered that the rotation speed depends on a single, combined measure of acceleration from both the gas and the stars. It found the correct way to weigh the stars against the gas, matching the known mass-to-light ratio of stellar populations. Furthermore, it confirmed that the relationship between the observed motion and this combined acceleration follows a specific, non-unique form that has been debated in astronomy for years. The system also provided a statistical measure of how confident it was in the slope of this relationship, showing that the deep, slow-moving parts of the galaxy follow a different rule than the fast-moving outer edges.
This work demonstrates that by combining accurate mathematical surrogates with a smart, tiered search strategy, we can move from raw data to interpretable laws of nature. The system does not just predict numbers; it reveals the structure of the universe, showing us that even in the complex dance of galaxies, there are simple, discoverable rules waiting to be found if we know how to look. The researchers have made their code and data available, allowing others to test these methods on their own problems, from the motion of planets to the behavior of fluids. The path from a neural network to a closed-form equation is no longer a mystery; it is a practical route to understanding the fundamental laws that govern our world.
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