Abstract
We study the asymptotic dynamics of dark energy as a mixture of presssureless matter and an interacting vacuum component. We find that the only dynamics compatible with current observational data favours an asymptotically vanishing matter-vacuum energy interaction in a model where dark energy is simulated by a generalised Chaplygin gas cosmology.
| Original language | English |
|---|---|
| Pages (from-to) | 621-625 |
| Number of pages | 5 |
| Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 785 |
| DOIs | |
| Publication status | Published - 10 Oct 2018 |
| Externally published | Yes |
Keywords
- Asymptotic analysis
- Chaplygin gas model
- Dark energy
- Dark matter
- Interacting vacuum
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