Abstract
The development of voids in a flat McVittie background is calculated, in the thin-shell approximation. This work follows closely that of Lake & Pim (1985); the basic modification is the introduction of the McVittie spacetime, which describes a spherical mass embedded in an asymptotically Robertson-Walker spacetime.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 579-584 |
| Number of pages | 6 |
| Journal | Astrophysical Journal |
| Volume | 418 |
| Issue number | 2 |
| DOIs | |
| State | Published - Dec 1 1993 |
Keywords
- Cosmology: theory
- Relativity
Fingerprint
Dive into the research topics of 'Thin shells in flat McVittie spacetimes'. Together they form a unique fingerprint.Cite this
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS