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Topological deformations of local gauge theories: a presymplectic BV-AKSZ approach

This paper demonstrates that local gauge theories with identical degrees of freedom but distinct gauge structures are related by "topological deformations"—the systematic gauging of symmetries within a presymplectic BV-AKSZ framework—which couples the system to a BF-type sector to either identify global symmetry-related solutions or generate new global degrees of freedom like the cosmological constant.

Original authors: Ivan Dneprov, Alexey Donchenko, Maxim Grigoriev

Published 2026-10-20
📖 5 min read🧠 Deep dive

Original authors: Ivan Dneprov, Alexey Donchenko, Maxim Grigoriev

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

In the vast landscape of theoretical physics, researchers often encounter a peculiar phenomenon where two completely different-looking theories describe the exact same physical reality. Imagine two maps of the same territory: one drawn with a grid of streets, the other with winding rivers. To a traveler, the routes look distinct, and the rules for navigating them seem different, yet both lead to the same destination. In the world of quantum fields and gravity, this happens frequently. A system might be described by a simple scalar field, or by a more complex "two-form" field that behaves like a twisted sheet of energy. While these descriptions look different on paper, they share the same local behavior—the way they wiggle and interact in a small patch of space. However, they often differ in their global structure, meaning how they behave when you look at the entire universe at once, or in how they respond to the shape of spacetime itself.

For decades, physicists have known about these pairs of theories, such as the relationship between a massless scalar field and a two-form gauge field in four-dimensional space, or the connection between standard gravity and a version called unimodular gravity where the cosmological constant acts as a global variable. The mystery has been how to systematically transform one into the other without losing or gaining any physical substance. A team of researchers, Ivan Dneprov, Alexey Donchenko, and Maxim Grigoriev, has now provided a clear, step-by-step method for performing this transformation. They call their approach "topological deformations," a technique that allows one to take a known physical system and gently stretch its mathematical structure to reveal a hidden twin, all while keeping the core local physics exactly the same.

The researchers worked within a sophisticated mathematical framework known as the presymplectic BV-AKSZ approach. While the name sounds intimidating, the core idea is relatively straightforward: they treated physical theories as geometric objects with specific rules for symmetry. In physics, a symmetry is a change you can make to a system without altering its outcome, like rotating a perfect sphere. Usually, these symmetries are global, meaning you apply the same change everywhere at once. The team's innovation was to take these global symmetries and "gauge" them, which means promoting them to local symmetries that can vary from point to point in space. However, they did this in a very specific way that prevents the introduction of new, independent physical particles or waves. Instead, the process couples the original system to a "topological sector," a kind of mathematical background that has no local dynamics but carries global information.

When the researchers applied this gauging procedure to symmetries of a certain type, they found it produced a new kind of physical theory where the coupling constants—numbers that usually determine the strength of an interaction, like the mass of a particle or the value of the cosmological constant—became dynamic fields. In the case of unimodular gravity, for instance, the cosmological constant, which is typically a fixed number in Einstein's equations, emerges naturally as a field that is constant throughout space but can take different values in different solutions. This explains why the theory looks like standard gravity locally but possesses a different global structure where the cosmological constant is a conserved quantity. The process effectively turns a fixed parameter into a dynamical variable that is constrained by the equations of motion to be constant, thereby creating a new global degree of freedom.

Conversely, when the team applied their method to different types of symmetries, they generated what are known as dualities. In these cases, the gauging procedure reduces the number of independent solutions, effectively identifying configurations that were previously distinct. This is how they systematically derived the famous duality between a massless scalar field and a two-form gauge field. By gauging the shift symmetry of the scalar field, they introduced a new field that acts as its dual partner. The resulting theory describes the same local physics but in terms of a completely different set of fields. This confirms that these dualities are not just accidental mathematical coincidences but are the natural result of a systematic procedure that reorganizes the symmetries of the theory.

The power of this work lies in its generality and its ability to handle complex systems like Yang-Mills theory, which describes the strong nuclear force. The researchers showed that by gauging a specific algebra of symmetries, one can promote the structure constants of the theory—which define how the forces interact—to dynamical fields. The equations of motion then force these fields to satisfy specific algebraic conditions, such as the Jacobi identity, which ensures the consistency of the theory. This means the theory naturally selects the correct interaction rules as part of its solution space, rather than having them imposed by hand. The result is a single, unified framework that contains the original theory and all its consistent deformations, with the specific version realized in nature determined by the global values of these new fields.

Ultimately, this research provides a unified language for understanding how different physical theories can be related. It demonstrates that the distinction between a theory with a fixed parameter and one with a dynamical global variable, or between a theory and its dual, is often just a matter of how the symmetries are organized. By treating these transformations as a systematic gauging process, the authors have mapped out a clear path between these different descriptions. Their findings suggest that the global properties of the universe, such as the value of the cosmological constant or the existence of dual formulations, are deeply rooted in the way symmetries are woven into the fabric of the theory. This does not just solve a mathematical puzzle; it offers a new perspective on how physical laws might emerge from a deeper, more flexible geometric structure, where the constants of nature are not fixed from the start but are determined by the global topology of the solution space.

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