Asymptotics of Relativistic Spin Networks
John W Barrett, Christopher M Steele
TL;DR
The paper develops a stationary-phase framework to derive the large-spin asymptotics of relativistic spin networks, focusing on SO(4) 6j (tetrahedron) and 10j (4-simplex) symbols and extending to SO(3,1) Lorentzian cases. It shows that the tetrahedral case reproduces the square of the Ponzano–Regge formula, while the 4-simplex is generically dominated by degenerate (one-dimensional) configurations with a distinctive alpha-dependent decay, and non-degenerate 4D configurations contribute with a faster, oscillatory scaling. The analysis introduces a detailed taxonomy of stationary points (non-degenerate, 1D, 2D, 3D, partly parallel, fully parallel) and clarifies how admissibility conditions and limits of admissibility modify the asymptotics, aligning with prior numerical findings. Overall, the work provides a comprehensive asymptotic picture for both Euclidean and Lorentzian relativistic spin networks, informing the semiclassical behavior of spin-foam models and their connection to discrete gravity.
Abstract
The stationary phase technique is used to calculate asymptotic formulae for SO(4) Relativistic Spin Networks. For the tetrahedral spin network this gives the square of the Ponzano-Regge asymptotic formula for the SU(2) 6j symbol. For the 4-simplex (10j-symbol) the asymptotic formula is compared with numerical calculations of the Spin Network evaluation. Finally we discuss the asymptotics of the SO(3,1) 10j-symbol.
