Demo · Tropical subtraction

Taming a Feynman integral

Feynman integrals are how we turn quantum field theory into numbers — but they are riddled with infinities. Here is how tropical geometry sorts those infinities into a finite, computable list, and how the SubTropica package does it for you.

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Start with an integral

To turn quantum field theory into a number — a cross-section, a decay rate — we evaluate Feynman integrals. Take a one-loop box — four propagators closing into a square. Its value is not finite: somewhere inside, it diverges.

Trade momenta for parameters

Rather than integrate over the loop momentum, rewrite the integral over Feynman parameters — one per propagator — living on a simplex. The whole integrand is built from two Symanzik polynomials, U and F.

Where the infinities hide

The divergences are not scattered everywhere. They sit on the boundary of the simplex, where Feynman parameters vanish. Work in d = 4 − 2ε dimensions and each one surfaces as a pole in ε.

A polytope appears

Which boundaries diverge, and how badly? The answer is combinatorial. Collect the exponents of the Symanzik polynomials as lattice points, take their convex hull, and you have a Newton polytope.

Subtract a facet

Each facet of the Newton polytope is one way the integral diverges. The scheme subtracts a counterterm for it — geometrically, peel that facet off. What remains is the polytope minus that piece.

Subtract another

A neighbouring facet diverges too, so subtract its counterterm as well. But along the edge where the two facets meet, that overlap has now been removed twice.

Add back the overlap

Inclusion–exclusion fixes it: add back their common edge — the piece counted twice. Carry on down the face lattice and every divergence is removed exactly once. The remainder, Iren, is finite.

Try it yourself

SubTropica is open and documented. Point it at your own integral and watch the ε-expansion come back — no tropical bookkeeping by hand.

subtropica.org →

Why tropical geometry?

Tropical means keeping only the leading exponential behaviour — replacing sums by maxima and products by sums. For a Feynman integral that coarse shadow is exactly the data that controls its divergences. The two papers here turn the observation into a method: The Tropical Geometry of Subtraction Schemes sets up the framework, and SubTropica (with M. Giroux & S. Mizera) makes it run inside Mathematica.

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First draft — the physics narrative and the schematic figures are mine to tune. The page reuses the dependency-free scrollytelling pattern (an IntersectionObserver drives the sticky visual).