Worse than a big rip?
arXiv:gr-qc/0612135 · doi:10.1016/j.physletb.2007.10.079
Abstract
We show that a generalised phantom Chaplygin gas can present a future singularity in a finite future cosmic time. Unlike the big rip singularity, this singularity happens for a finite scale factor, but like the big rip singularity, it would also take place at a finite future cosmic time. In addition, we define a dual of the generalised phantom Chaplygin gas which satisfies the null energy condition. Then, in a Randall-Sundrum 1 brane-world scenario, we show that the same kind of singularity at a finite scale factor arises for a brane filled with a dual of the generalised phantom Chaplygin gas.
6 pages, 4 figures, RevTeX 4. Discussion expanded and references added. Version to appear in PLB
Cited by in corpus (9)
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- The future evolution and finite-time singularities in -gravity unifying the inflation and cosmic acceleration
- Classifying and avoiding singularities in the alternative gravity dark energy models
- On the quantum fate of singularities in a dark-energy dominated universe
- On the generalised Chaplygin gas: worse than a big rip or quieter than a sudden singularity?
- Singular fate of the universe in modified theories of gravity
- Phantom-like behaviour in a brane-world model with curvature effects
- Is the accelerated expansion evidence of a forthcoming change of signature on the brane?
- Scalar field cosmological models with finite scale factor singularities