Abstract

We study the behaviour of weak gravitational fields in models where a 4D brane is embedded inside a 5D brane equipped with induced gravity, which in turn is embedded in a 6D spacetime. We consider a specific regularization of the branes internal structures where the 5D brane can be considered thin with respect to the 4D one. We find exact solutions corresponding to pure tension source configurations on the thick 4D brane, and study perturbations at first order around these background solutions. To perform the perturbative analysis, we adopt a bulk-based approach and we express the equations in terms of gauge invariant and master variables using a 4D scalar-vector-tensor decomposition. We then propose an ansatz on the behaviour of the perturbation fields when the thickness of the 4D brane goes to zero, which corresponds to configurations where gravity remains finite everywhere in the thin limit of the 4D brane. We study the equations of motion using this ansatz, and show that they give rise to a consistent set of differential equations in the thin limit, from which the details of the internal structure of the 4D brane disappear. We conclude that the thin limit of the ``ribbon'' 4D brane inside the (already thin) 5D brane is well defined (at least when considering first order perturbations around pure tension configurations), and that the gravitational field on the 4D brane remains finite in the thin limit. We comment on the crucial role of the induced gravity term on the 5D brane.

Highlights

  • The Cosmological Constant problem (CC) and the late time acceleration of the universe (LTA) are two of the most compelling problems in contemporary theoretical physics

  • We studied the behaviour of weak gravitational fields in models where a 4D brane is embedded inside a 5D brane equipped with induced gravity, which in turn is embedded in a 6D spacetime

  • We considered a specific regularization of the branes internal structures where the 5D brane can be considered thin with respect to the 4D one, and studied perturbations at first order around the solutions corresponding to pure tension source configurations on the thick 4D brane

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Summary

Introduction

The Cosmological Constant problem (CC) and the late time acceleration of the universe (LTA) are two of the most compelling problems in contemporary theoretical physics. Despite it has been noted long ago [1] that there is a difference of 60-120 orders of magnitude (depending on the cut-off of the quantum theory) between the theoretical estimates for the vacuum energy and its observed value, a fully convincing explanation of this mismatch is still missing. If we believe that the CC problem and the LTA problem are independent, braneworld models with induced gravity offer the possibility of explaining the late time acceleration in a geometrical way, since they generically admit cosmological solutions which exhibit the phenomenon of self-acceleration

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