Abstract

Linear stability of braneworld models constructed with multi-scalar fields is very different from that of single-scalar field models. It is well known that both the tensor and the scalar perturbations of the latter are stable at linear level. However, in general there is no effective method to deal with the stability problem of the scalar perturbations for braneworld models constructed with non-minimally coupled multi-scalar fields. In this work we present a systematic covariant approach to deal with the scalar perturbations. By introducing the orthonormal bases in field space and making the Kaluza–Klein decomposition, we get a set of coupled Schrödinger-like equations of the scalar perturbation modes. Using the nodal theorem, we show that the result is model-dependent. For superpotential derived brane models, the scalar perturbations are stable, but there exist normalizable scalar zero modes, which will result in unacceptable fifth force on the brane. We also use this method to analyze the f(R) braneworld model with an explicit solution and find that the scalar perturbations are stable and the scalar zero modes cannot be localized on the brane, which ensures that there is no extra long-range force and the Newtonian potential on the brane can be recovered.

Highlights

  • To get the smooth version of the RS-II model, scalar fields as material are introduced [6]

  • We have investigated the stability of the tensor and scalar perturbations for flat braneworld models constructed by non-minimally coupled multi-scalar fields in the Einstein frame

  • We studied the stability of the tensor perturbation and find that its dynamical equation can be written as a supersymmetric Schrödinger equation, so it is stable at linear level

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Summary

Introduction

To get the smooth version of the RS-II model, scalar fields as material are introduced [6]. The domain wall brane models constructed with K-field were proved to be stable under scalar perturbations [30,31,32,33]. This gives us inspiration that the localized zero modes in braneworld model with multiple canonical scalars may be avoided if the scalars are non-canonical. In this paper we choose a general action and mainly study the scalar perturbations of braneworlds generated by nonminimally coupled multi-scalar fields in the Einstein frame, by using some techniques developed in cosmology. We deal with the scalar perturbations of the f (R) braneworld model in Sect. 4 and give a summary in the last section

General setup
N2 q μρ q ν σ
The action and perturbations
Stability and zero modes of the scalar perturbations
The Einstein frame formalism
Conclusions
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