Radiative corrections to superallowed beta decays at $\mathcal O(\alpha^2 Z)$

TL;DR

This paper calculates second-order radiative corrections to superallowed beta decays using effective field theory, significantly refining theoretical predictions and reducing uncertainties in fundamental parameter extraction.

Contribution

It provides the first systematic computation of $ ext{O}( ext{α}^2 Z)$ ultrasoft photon corrections to superallowed beta decays with analytical techniques, improving theoretical precision.

Findings

Corrections range from 0.7 to 3.6 per mille for different nuclei.

Inclusion of corrections reduces renormalization scale dependence.

Results impact the precision of $V_{ud}$ extraction.

Abstract

We compute $\mathcal O(\alpha^2 Z)$ radiative corrections to superallowed $\beta$ decays with a heavy-particle effective field theory that systematically describes the interactions of low-energy ultrasoft photons with nuclei. We calculate two-loop virtual and one-loop real-virtual amplitudes by reducing the Feynman integrals to a set of master integrals, which we solve analytically using a variety of techniques. These techniques can be applied to other phenomenologically interesting observables. The ultrasoft corrections can then be combined with contributions arising from the exchange of potential photons to obtain the complete $\mathcal O(\alpha^2 Z)$ correction to the decay rate, with resummation of large logarithms of the electron energy times the nuclear radius. We find that $\mathcal O(\alpha^2 Z)$ ultrasoft loops induce a relative correction to the decay rate that ranges from $0.7 \cdot 10^{-3}$ in the decay of $^{10}$C to $3.6 \cdot 10^{-3}$ in the decay of $^{54}$Co, and will thus impact the extraction of $V_{ud}$ at the permille level. We show that the inclusion of these corrections reduces the residual renormalization scale dependence of the decay rate to a negligible level, making missing ultrasoft perturbative corrections a subdominant source of theoretical error.