Cosmology from Newton–Chern–Simons gravity

S. Lepe, G. Rubio, P. Salgado

Research output: Contribution to journalArticlepeer-review


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.

Original languageEnglish
Article number114838
JournalNuclear Physics B
StatePublished - Jan 2020


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