One-loop corrections for WW to HH in HEFT with the electroweak chiral Lagrangian

TL;DR

This paper calculates one-loop electroweak radiative corrections to the WW to HH scattering process within the Higgs Effective Field Theory, providing detailed renormalization and numerical analysis of the corrections' impact.

Contribution

It introduces a comprehensive one-loop correction computation for WW to HH in HEFT, including renormalization of 1PI functions and numerical results, extending previous work on related processes.

Findings

One-loop corrections significantly affect the WW to HH cross section.

Renormalized coefficients of EChL are derived for this process.

Comparison with Standard Model results highlights the impact of BSM interactions.

Abstract

In this work we present the computation of the one-loop electroweak radiative corrections to the scattering process $WW\to HH$ within the context of the Higgs Effective Field Theory (HEFT). We assume that the fermionic interactions are like in the Standard Model, whereas the Beyond Standard Model interactions in the bosonic sector are given by the Electroweak Chiral Lagrangian. The computation of the one-loop amplitude and the renormalization program is performed in terms of the involved one-particle-irreducible functions (1PI) and using $R_\xi$ covariant gauges. The renormalization of 1PI functions at arbitrary external momenta is a more ambitious program than just renormalizing the amplitude with on-shell external legs and it has the advantage that they can be used in several scattering amplitudes. In fact, we use here some of the 1PI functions already computed in our previous work (devoted to $WZ \to WZ$). We will complement them here with the computation of the new 1PI functions required for $WW \to HH$. From this renormalization procedure we will also derive the full set of renormalized coefficients of the EChL that are relevant for this scattering process. In the last part, we will present the numerical results for the EChL predictions of the one-loop level cross section, $\sigma(WW \to HH)|_{\rm 1-loop}$, as a function of the center of mass energy, showing the relative size of the one-loop radiative corrections respect to the tree level prediction in terms of the EChL coefficients. The results of the one-loop corrections to $WW \to HH$ for the SM case will be also presented, for comparison with the EChL case, following the same computational method, i.e., by means of the renormalization of 1PI functions.