Achronal cosmic future
arXiv:astro-ph/0404045 · doi:10.1103/PhysRevLett.93.071301
Abstract
The spherically symmetric accretion of dark and phantom energy onto Morris-Thorne wormholes is considered. It is obtained that the accretion of phantom energy leads to a gradual increase of the wormhole throat radius which eventually overtakes the super-accelerated expansion of the universe and becomes infinite at a time in the future before the occurrence of the big rip singularity. After that time, as it continues accreting phantom energy, the wormhole becomes an Einstein-Rosen bridge whose corresponding mass decreases rapidly and vanishes at the big rip.
5 pages, 3 figures, RevTex, a comment and one reference added to match the version accepted for publication in Physical Review Letters
References in corpus (7)
- Phantom Energy and Cosmic Doomsday
- Black hole mass decreasing due to phantom energy accretion
- The case for dynamical dark energy revisited
- K-Essential Phantom Energy: Doomsday around the corner?
- Testing dark energy beyond the cosmological constant barrier
- Axion Phantom Energy
- Wormholes and Ringholes in a Dark-Energy Universe
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