Inferring the breakdown scales of the chiral expansions for $g_A$ and $m_N$
Andreas Ekström, Daniel R. Phillips, Lucas Platter, Matthias R. Schindler
TL;DR
The paper addresses how the breakdown scale of single-nucleon chiral perturbation theory depends on the observable by inferring $\Lambda_B$ from order-by-order expansions of $g_A$ and $m_N$ using a pointwise Bayesian approach. It expresses the expansions with a natural-coefficient prior and a likelihood based on $Q = M/\Lambda_B$, then infers $\Lambda_B$ from data at two pion masses across different low-energy-constant (LEC) sets. The main findings are that $\Lambda_B$ for $g_A$ is about $251^{+20}_{-50}$ MeV (Set 1) or $211^{+20}_{-30}$ MeV (Set 2), while for $m_N$ it is about $491^{+60}_{-90}$ MeV, indicating substantially slower convergence for $g_A$ than for $m_N$. This demonstrates observable-dependent convergence in baryon $\chi$PT and emphasizes the influence of resonances like the $\Delta(1232)$, with implications for lattice extrapolations and the interpretation of EFT truncation errors.
Abstract
We apply Bayesian inference to the order-by-order chiral perturbation theory ($χ$PT) expansions for the axial-vector coupling constant $g_A$ and the nucleon mass m_N, and thereby infer the scales at which $χ$PT breaks down for these two observables. Using a pointwise Bayesian analysis, we find that the inferred breakdown scales are notably different for the two observables. For the chiral expansion of $g_A$, we obtain $251^{+20}_{-50}$ MeV and $211^{+20}_{-30}$ MeV using two distinct sets of low-energy constants, while for the chiral expansion of $m_N$ we infer a significantly larger breakdown scale of $491^{+60}_{-90}$ MeV.
