activity
20062019
most citedInteracting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models

29 citations · 84 across the 8 of their papers we have counts for

collaborators

8 papers

gr-qc2019★ 17 cited

On sign-changeable interaction in FLRW cosmology

Fabiola Arevalo, Antonella Cid, Luis P. Chimento +1

We investigate an interacting two-fluid model in a spatially flat Friedmann-Lemaître-Robertson-Walker (FLRW) Universe, when the energy transfer between these two dark components is…

gr-qc2016★ 4 cited

Some cosmological solutions in Einstein-Chern-Simons gravity

Luis Avilés, Patricio Mella, Cristian Quinzacara +1

In this paper we find new solutions for the so called Einstein-Chern-Simons Friedmann-Robertson-Walker field equations studied in refs. (Phys. Rev. D 84 (2011) 063506, Eur. Phys. J…

gr-qc2015★ 1 cited

Cosmic anisotropic doomsday in Bianchi type I universes

Mauricio Cataldo, Antonella Cid, Pedro Labraña +1

In order to investigate if the anisotropy of the spacetime may induce future singularities at a finite value of the cosmic time on the evolution of cosmological models, we study va…

hep-th2015★ 2 cited

Randall-Sundrum brane universe as a ground state for Chern-Simons gravity

Fabrizio Cordonier-Tello, Fernando Izaurieta, Patricio Mella +1

In stark contrast with the three-dimensional case, higher-dimensional Chern-Simons theories can have non-topological, propagating degrees of freedom. Finding those vacua that allow…

gr-qc2013★ 15 cited

Canonical and phantom scalar fields as an interaction of two perfect fluids

Mauricio Cataldo, Fabiola Arevalo, Patricio Mella

In this article we investigate and develop specific aspects of Friedmann-Robertson-Walker (FRW) scalar field cosmologies related to the interpretation that canonical and phantom sc…

gr-qc2011★ 6 cited

Interacting Kasner-type cosmologies

Mauricio Cataldo, Fabiola Arevalo, Patricio Mella

It is well known that Kasner-type cosmologies provide a useful framework for analyzing the three-dimensional anisotropic expansion because of the simplification of the anisotropic…