Passing to an effective 4D phantom cosmology from 5D vacuum theory of gravity

Abstract

Starting from a five-dimensional (5D) vacuum theory of gravity where the extra coordinate is considered as noncompact, we investigate the possibility of inducing four-dimensional (4D) phantom scenarios by applying form-invariance symmetry transformations. In particular we obtain phantom scenarios for two cosmological frameworks. In the first framework we deal with an induced 4D de-Sitter expansion and in the second one a 4D induced model where the expansion of the universe is dominated by a decreasing cosmological parameter $\Lambda (t)$ is discussed.

version accepted in Physics Letters B

References in corpus (1)

• Gravitational waves during inflation in presence of a decaying cosmological parameter from a 5D vacuum theory of gravity

Cited by in corpus (1)

• The nature of cosmological singularities in isotropic universes and braneworlds