The little sibling of the big rip singularity
Abstract
We present a new cosmological event, which we named the little sibling of the big rip. This event is much smoother than the big rip singularity. When the little sibling of the big rip is reached, the Hubble rate and the scale factor blow up but the cosmic derivative of the Hubble rate does not. This abrupt event takes place at an infinite cosmic time where the scalar curvature explodes. We show that a doomsday \'a la little sibling of the big rip is compatible with an accelerating universe, indeed at present it would mimic perfectly a LCDM scenario. It turns out that eventhough the event seems to be harmless as it takes place in the infinite future, the bound structures in the universe would be unavoidably destroyed on a finite cosmic time from now. The model can be motivated by considering that the weak energy condition should not be abusibely violated in our Universe, and it could give us some hints about the status of recently formulated nonlinear energy conditions.
Keywords
Cite
@article{arxiv.1407.2446,
title = {The little sibling of the big rip singularity},
author = {Mariam Bouhmadi-Lopez and Ahmed Errahmani and Prado Martin-Moruno and Taoufik Ouali and Yaser Tavakoli},
journal= {arXiv preprint arXiv:1407.2446},
year = {2015}
}
Comments
20 pages, 4 figures, clarifications included