Cargese Lectures on Brane Induced Gravity

TL;DR

This paper introduces brane induced gravity, discusses 5D models with infinite extra dimensions, and explores stable and self-accelerated solutions, highlighting their stability issues and implications for cosmic acceleration.

Contribution

It provides a detailed analysis of 5D brane induced gravity models, including stability properties and the potential for explaining cosmic acceleration through modified gravity.

Findings

Conventional branch offers a perturbatively stable metastable graviton.

Self-accelerated branch suggests a mechanism for universe acceleration.

Non-perturbative solutions indicate potential instability of the self-accelerated branch.

Abstract

A brief introduction is given to the subject of brane induced gravity. The 5D example is discussed in detail. The 4D laws of gravity are obtained on a brane embedded in an infinite volume extra space, where the problem of stabilization of the volume modulus is absent. The theory has two classically disjoint branches of solutions -- the conventional and self-accelerated one. The conventional branch gives a perturbatively stable model of a metastable graviton, with potentially testable predictions within the Solar system. The self-accelerated branch, on the other hand, provides an existence proof for an idea that the accelerated expansion of the Universe could be due to modified gravity. The issue of perturbative stability of the self-accelerated branch is obscured by a breakdown of the conventional perturbative expansion. However, a certain exact non-perturbative solution found in hep-th/0612016 exhibits a net negative gravitational mass, while this mass is positive on the conventional branch. This suggest that the self-accelerated solution must be non-perturbatively unstable. A proposal to overcome this problem in an extension of the original model, that also allows for the quantum gravity scale to be unrestricted, is briefly discussed.