The dynamical stability of the static real scalar field solutions to the Einstein-Klein-Gordon equations revisited
arXiv:gr-qc/9809014 · doi:10.1016/S0375-9601(98)00646-X
Abstract
We re-examine the dynamical stability of the nakedly singular, static, spherical ly symmetric solutions of the Einstein-Klein Gordon system. We correct an earlier proof of the instability of these solutions, and demonstrate that there are solutions to the massive Klein-Gordon system that are perturbatively stable.
13 pages, uses Elsevier style files. To appear in Phys. Lett. A
References in corpus (1)
Cited by in corpus (8)
- TOPICAL REVIEW: General relativistic boson stars
- Chameleon stars
- Decay of Boson Stars with Application to Glueballs and Other Real Scalars
- Axially symmetric Proca-Higgs boson stars
- Spherically symmetric configurations in the quadratic gravity
- Wyman's solution, self-similarity and critical behaviour
- On the stability of electrovacuum space-times in scalar-tensor gravity
- Excited D-branes and Supergravity Solutions