
arXiv: gr-qc/0006108
handle: 11336/54425
We use exact general solutions for the spatially flat FRW and the anisotropic Bianchi I cosmologies to show that generically uncoupled scalar fields cooperate to make inflation more probable, while the presence of several interacting fields hinders the occurrence of the phenomenon, in accordance with previous results based on particular power-law solutions. Similar conclusions are reached in the case of Bianchi VI$_0$ spacetimes, for power-law solutions which are proved to be attractors.
2 eps figures. To appear in PRD
Bianchi Type I, Bianchi Type Vi0, Assisted Inflation, https://purl.org/becyt/ford/1.3, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), https://purl.org/becyt/ford/1, General Relativity and Quantum Cosmology
Bianchi Type I, Bianchi Type Vi0, Assisted Inflation, https://purl.org/becyt/ford/1.3, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), https://purl.org/becyt/ford/1, General Relativity and Quantum Cosmology
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 15 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 10% |
