Interacting vacuum at infinity
arXiv:1904.09735 · doi:10.1142/S021988781950052X
Abstract
We apply the central extension technique of Poincare to dynamics involving an interacting mixture of pressureless matter and vacuum near a finite-time singularity. We show that the only attractor solution on the circle of infinity is the one describing a vanishing matter-vacuum model at early times
arXiv comment14 pages
References in corpus (13)
- Phantom Energy and Cosmic Doomsday
- Properties of singularities in (phantom) dark energy universe
- Sudden Future Singularities
- The Revival of the Unified Dark Energy-Dark Matter Model ?
- Dynamical Systems Perspective of Cosmological Finite-time Singularities in Gravity and Interacting Multifluid Cosmology
- Inhomogeneous vacuum energy
- Global Hyperbolicity and Completeness
- The Dominant Balance at Cosmological Singularities
- Flat limits of curved interacting cosmic fluids
- Singularities in cosmologies with interacting fluids
- Is interacting vacuum viable?
- Asymptotic Poincaré compactification and finite-time singularities
- The nature of cosmological singularities in isotropic universes and braneworlds