Stability analysis of 5D gravitational solutions with N bulk scalar fields

TL;DR

This paper develops a comprehensive stability analysis framework for 5D gravitational models with multiple scalar fields, accounting for their backreaction and perturbations, and applies it to models relevant for QCD and electroweak physics.

Contribution

It derives a set of coupled equations governing background and perturbations for arbitrary scalar potentials, enabling stability analysis and fluctuation property determination.

Findings

No tachyonic modes found in the studied model

Radion mode mass is suppressed by a large logarithm

Framework applicable to models with multiple scalar fields

Abstract

We study the stability of 5D gravitational solutions containing an arbitrary number of scalar fields. A closed set of equations is derived which governs the background and perturbations of N scalar fields and the metric, for arbitrary bulk and boundary scalar potentials. In particular the effect of the energy-momentum tensor of the scalar fields on the geometry is fully taken into account, together with all the perturbations of the system. The equations are explicitly written as an eigenvalue problem, which can be readily solved to determine the stability of the system and obtain the properties of the fluctuations, such as masses and couplings. As an example, we study a dynamical soft-wall model with two bulk scalar fields used to model the hadron spectrum of QCD and the Higgs sector of electroweak physics. It is shown that there are no tachyonic modes, and that there is a (radion) mode whose mass is suppressed by a large logarithm compared to that of the other Kaluza-Klein modes.