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Cosmology from Newton-Chern-Simons gravity

We study a five-dimensional non-relativistic gravity theory whose action is composed of a gravitational sector and a sector of matter where the gravitational sector is given by the so called Newton--Chern--Simons gravity and where the matter sector is described by a perfect fluid. At time to do cosmology, the obtained field equations shows a close analogy with the projectable version of the Hořava--Lifshitz theory in (3+1)-dimensions. Solutions and their asymptotic limits are found. In particular a phantom solution with a future singularity reminiscent of a Litlle Big Rip future singularity is obtained.

preprint2019arXivOpen access
S. LepeG. RubioP. Salgado
hep-th
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Open access3 authors1 topic
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S. LepeG. RubioP. Salgado

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