Radiative corrections to the $\rm S, T, U$ parameters and their impact on the $W$ boson mass in the 331 model

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Rehman, Muhammad, Iqbal, Muhammad Adeel, Gomez, Mario E., Panella, Orlando
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866915469821214720
author Rehman, Muhammad
Iqbal, Muhammad Adeel
Gomez, Mario E.
Panella, Orlando
author_facet Rehman, Muhammad
Iqbal, Muhammad Adeel
Gomez, Mario E.
Panella, Orlando
contents We investigate radiative corrections to electroweak precision observables, specifically the Peskin--Takeuchi parameters $\mathrm{S}$, $\mathrm{T}$, and $\mathrm{U}$, in the $SU(3)_C \times SU(3)_L \times U(1)_X$ (331) model with $β= -\sqrt{3}$. Using the SARAH and SPheno packages, we compute the mass spectrum and low-energy observables. We show that these parameters place strong constraints on the model, requiring most of the scalar masses to lie in the TeV range or below, and imposing indirect bounds on the newly predicted gauge bosons. Furthermore, we demonstrate that the model can accommodate the $W$ boson mass anomaly reported by the CDF collaboration, should future measurements confirm its persistence.
format Preprint
id arxiv_https___arxiv_org_abs_2507_18527
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Radiative corrections to the $\rm S, T, U$ parameters and their impact on the $W$ boson mass in the 331 model
Rehman, Muhammad
Iqbal, Muhammad Adeel
Gomez, Mario E.
Panella, Orlando
High Energy Physics - Phenomenology
We investigate radiative corrections to electroweak precision observables, specifically the Peskin--Takeuchi parameters $\mathrm{S}$, $\mathrm{T}$, and $\mathrm{U}$, in the $SU(3)_C \times SU(3)_L \times U(1)_X$ (331) model with $β= -\sqrt{3}$. Using the SARAH and SPheno packages, we compute the mass spectrum and low-energy observables. We show that these parameters place strong constraints on the model, requiring most of the scalar masses to lie in the TeV range or below, and imposing indirect bounds on the newly predicted gauge bosons. Furthermore, we demonstrate that the model can accommodate the $W$ boson mass anomaly reported by the CDF collaboration, should future measurements confirm its persistence.
title Radiative corrections to the $\rm S, T, U$ parameters and their impact on the $W$ boson mass in the 331 model
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2507.18527