Instability of Flat Space Enclosed in a Cavity
classification
🌀 gr-qc
hep-th
keywords
enclosedarbitrarilyblackcavityconsiderdataevidenceevolve
read the original abstract
We consider a spherically symmetric self-gravitating massless scalar field enclosed inside a timelike worldtube $R\times S^3$ with a perfectly reflecting wall. Numerical evidence is given that arbitrarily small generic initial data evolve into a black hole.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.