# Radiative Corrections to Neutron and Nuclear Beta Decays Revisited

## TL;DR

This paper revisits radiative corrections to neutron and nuclear beta decays using multiple computational methods, reducing previous discrepancies and refining implications for CKM unitarity and neutron lifetime measurements.

## Contribution

It introduces an updated calculation of radiative corrections employing advanced QCD techniques and resonance models, decreasing the discrepancy with dispersion relation results.

## Key findings

- Radiative correction estimate: 2.426(32)%
- Discrepancy with dispersion relation reduced to 1.1σ
- Stronger bounds on exotic neutron decays: <0.16%

## Abstract

The universal radiative corrections common to neutron and super-allowed nuclear beta decays (also known as ``inner'' corrections) are revisited in light of a recent dispersion relation study that found $+2.467(22)\%$, i.e.~about $2.4\sigma$ larger than the previous evaluation. For comparison, we consider several alternative computational methods. All employ an updated perturbative QCD four-loop Bjorken sum rule (BjSR) defined QCD coupling supplemented with a nucleon form factor based Born amplitude to estimate axial-vector induced hadronic contributions. In addition, we now include hadronic contributions from low $Q^2$ loop effects based on duality considerations and vector meson resonance interpolators. Our primary result, $2.426(32)\%$ corresponds to an average of a Light Front Holomorphic QCD approach and a three resonance interpolator fit. It reduces the dispersion relation discrepancy to approximately $1.1\sigma$ and thereby provides a consistency check. Consequences of our new radiative correction estimate, along with that of the dispersion relation result, for CKM unitarity are discussed. The neutron lifetime-$g_A$ connection is updated and shown to suggest a shorter neutron lifetime $< 879$ s. We also find an improved bound on exotic, non-Standard Model, neutron decays or oscillations of the type conjectured as solutions to the neutron lifetime problem, $\text{BR}(n\to \text{exotics}) < 0.16 \%$.