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The Little Rip · Around

2011

The Little Rip

Frampton, Paul H., Ludwick, Kevin J., Scherrer, Robert J.

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We examine models in which the dark energy density increases with time (so that the equation-of-state parameter w satisfies w < -1), but w approaches -1 asymptotically, such that there is no future singularity.

We refine previous calculations to determine the conditions necessary to produce this evolution.
Such models can display arbitrarily rapid expansion in the near future, leading to the destruction of all bound structures (a "little rip").
We determine observational constraints on these models and calculate the point at which the disintegration of bound structures occurs.

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