$K^\pm\to\pi^\pm a$ at Next-to-Leading Order in Chiral Perturbation Theory and Updated Bounds on ALP Couplings

TL;DR

This paper performs a detailed next-to-leading order analysis of $K^ o\u03c0^ a$ decays within chiral perturbation theory, refining bounds on axion-like particle couplings and exploring their implications for particle physics and astrophysics.

Contribution

It extends chiral perturbation theory calculations to NLO for $K^ o\u03c0^ a$ decays, including isospin-breaking effects and operator basis extensions, providing more precise bounds on ALP couplings.

Findings

NLO corrections modify leading-order results by a few percent.

Bounds on ALP couplings are strongest for $m_a \u2264 300$ MeV.

Implications for ALP-nucleon couplings are discussed.

Abstract

The weak decays $K^\pm\to\pi^\pm a$ offer a powerful probe of axion-like particles (ALPs). In this work, we provide a comprehensive analysis of these processes within chiral perturbation theory, extending existing calculations by including complete next-to-leading order (NLO) contributions and isospin-breaking corrections at first order in $(m_d-m_u)$. We show that the consistent incorporation of ALPs in the QCD and weak chiral Lagrangians requires a non-trivial extension of the corresponding operator bases, which we describe in detail. Furthermore, we show that in the presence of an ALP the so-called ``weak mass term'', which is unobservable in the Standard Model, is non-redundant already at leading order. We find that NLO corrections associated with flavor-violating ALP couplings modify the leading-order result by a few percent, with negligible uncertainties. NLO corrections proportional to flavor-conserving ALP couplings lead to potentially larger corrections, which, however, are accompanied by sizable uncertainties mainly due to the currently limited knowledge of various low-energy constants. We study how these corrections impact bounds on the ALP couplings, first model independently, and then specializing to the case of an ALP with flavor-universal couplings in the UV. Our findings confirm that the decays $K^\pm\to\pi^\pm a$ provide the strongest particle-physics constraints for $m_a\lesssim 300$\,MeV. In addition, we point out that these bounds have interesting implications for the ALP couplings to nucleons, which were so far only constrained by astrophysical measurements and non-accelerator experiments.