Instability of Flat Space Enclosed in a Cavity

preprint2013arXivOpen access

Abstract

We consider a spherically symmetric self-gravitating massless scalar field enclosed inside a timelike worldtube R×S3R\times S^3 with a perfectly reflecting wall. Numerical evidence is given that arbitrarily small generic initial data evolve into a black hole.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.