Remarks about Dyson's instability in the large-N limit
Y. Meurice (KITP, U. of Iowa)

TL;DR
This paper investigates Dyson's instability in the large-N limit using the three-dimensional linear sigma model, analyzing the convergence of perturbative series and the role of field cutoffs in defining effective theories.
Contribution
It demonstrates how a large field cutoff can justify finite-radius convergence despite Dyson's argument suggesting instability at negative coupling.
Findings
A saddle point persists until a critical negative coupling value.
The perturbative series shows a square-root singularity at the critical point.
Finite radius of convergence is linked to a large field cutoff.
Abstract
There are known examples of perturbative expansions in the 't Hooft coupling lt with a finite radius of convergence. This seems to contradict Dyson's argument suggesting that the instability at negative coupling implies a zero radius of convergence. Using the example of the linear sigma model in three dimensions, we discuss to which extent the two points of view are compatible. We show that a saddle point persists for negative values of lt until a critical value -|lt_c| is reached. A numerical study of the perturbative series for the renormalized mass confirms an expected singularity of the form (lt +|lt_c|)^1/2. However, for -|lt_c|< lt <0, the effective potential does not exist if phi^2 >phi^2_{max}(lt) and not at all if lt<-|lt_c|. We show that phi^2_{max}(lt) propto 1/|lt | for small negative lt. The finite radius of convergence can be justified if the effective theory is defined…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Chromodynamics and Particle Interactions · High-Energy Particle Collisions Research
