Numerical Analysis of the Causal Action Principle in Low Dimensions
Felix Finster, Robert H. Jonsson, Niki Kilbertus
TL;DR
The paper investigates numerical minimization of the causal action principle for weighted counting measures in low-dimensional causal fermion systems, focusing on $n=1,f=2$ and $n=2,f=4$ to understand asymptotics as the number of spacetime points $m$ grows. It develops differentiable-programming-based optimization to handle nonconvex, high-dimensional problems, and demonstrates that discrete Dirac sphere configurations emerge as absolute minimizers for large $m$ in the minimal Hilbert-space cases, with precise asymptotics for the action and boundedness functionals. The analysis also reveals causal cone structures for spin dimension one and introduces projected spacetime plots to visualize minimizers, aiding intuition and guiding further analytic work. Beyond the minimal cases, the authors begin exploring $n=1,f=3$ and other settings, outlining prospects for convex-relaxation approaches and higher $f$ to broaden understanding of the minimizers' geometry and scaling, with significant implications for the structure of spacetime in causal fermion systems.
Abstract
The numerical analysis of causal fermion systems is advanced by employing differentiable programming methods. The causal action principle for weighted counting measures is introduced for general values of the integer parameters $f$ (the particle number), $n$ (the spin dimension) and $m$ (the number of spacetime points). In the case $n=1$, the causal relations are clarified geometrically in terms of causal cones. Discrete Dirac spheres are introduced as candidates for minimizers for large $m$ in the cases $n=1, f=2$ and $n=2, f=4$. We provide a thorough numerical analysis of the causal action principle for weighted counting measures for large $m$ in the cases $n=1,2$ and $f=2,3,4$. Our numerical findings corroborate that all minimizers for large $m$ are good approximations of the discrete Dirac spheres. In the example $n=1, f=3$ it is explained how numerical minimizers can be visualized by projected spacetime plots. Methods and prospects are discussed to numerically investigate settings in which hitherto no analytic candidates for minimizers are known.
