中文

Gravitational instability in higher dimensions

高能物理 - 理论 2009-10-07 v2 广义相对论与量子宇宙学

摘要

We explore a classical instability of spacetimes of dimension D>4D>4. Firstly, we consider static solutions: generalised black holes and brane world metrics. The dangerous mode is a tensor mode on an Einstein base manifold of dimension D2D-2. A criterion for instability is found for the generalised Schwarzschild, AdS-Schwarzschild and topological black hole spacetimes in terms of the Lichnerowicz spectrum on the base manifold. Secondly, we consider perturbations in time-dependent solutions: Generalised dS and AdS. Thirdly we show that, subject to the usual limitations of a linear analysis, any Ricci flat spacetime may be stabilised by embedding into a higher dimensional spacetime with cosmological constant. We apply our results to pure AdS black strings. Finally, we study the stability of higher dimensional ``bubbles of nothing''.

关键词

引用

@article{arxiv.hep-th/0206202,
  title  = {Gravitational instability in higher dimensions},
  author = {Gary Gibbons and Sean A. Hartnoll},
  journal= {arXiv preprint arXiv:hep-th/0206202},
  year   = {2009}
}

备注

1+43 pages. LaTeX. Slight rewording, typos fixed and stability of T^11 corrected