Dynamical instabilities of the Randall-Sundrum model

Timon Boehm, Ruth Durrer, and Carsten van de Bruck
Phys. Rev. D 64, 063504 – Published 16 August 2001
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Abstract

We derive dynamical equations to describe a single 3-brane containing fluid matter and a scalar field coupling to the dilaton and the gravitational field in a five-dimensional bulk. First, we show that a scalar field or an arbitrary fluid on the brane cannot evolve to cancel the cosmological constant in the bulk. Then we show that the Randall-Sundrum model is unstable under small deviations from the fine-tuning between the brane tension and the bulk cosmological constant and even under homogeneous gravitational perturbations. Implications for brane world cosmologies are discussed.

  • Received 21 February 2001

DOI:https://doi.org/10.1103/PhysRevD.64.063504

©2001 American Physical Society

Authors & Affiliations

Timon Boehm and Ruth Durrer

  • Département de Physique Théorique, Université de Genève, 24 quai E. Ansermet, CH-1211 Geneva 4, Switzerland

Carsten van de Bruck

  • Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom

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Issue

Vol. 64, Iss. 6 — 15 September 2001

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