activity
20062011
most citedLXCDM: a cosmon model solution to the cosmological coincidence problem?

126 citations · 456 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2011★ 33 cited

Generalized LTB model with Inhomogeneous Isotropic Dark Energy: Observational Constraints

J. Grande, L. Perivolaropoulos

We consider on-center and off-center observers in an inhomogeneous, spherically symmetric, isocurvature (flat) concentration of dark energy with typical size of a few Gpc. Such a c…

astro-ph.CO2011★ 109 cited

Hubble expansion and structure formation in the "running FLRW model" of the cosmic evolution

Javier Grande, Joan Sola, Spyros Basilakos +1

A new class of FLRW cosmological models with time-evolving fundamental parameters should emerge naturally from a description of the expansion of the universe based on the first pri…

astro-ph.CO2010★ 47 cited

Cosmic perturbations with running G and Lambda

Javier Grande, Joan Sola, Julio C. Fabris +1

Cosmologies with running cosmological term (Lambda) and gravitational Newton's coupling (G) may naturally be expected if the evolution of the universe can ultimately be derived fro…

astro-ph.CO2009★ 6 cited

Dark energy perturbations and a possible solution to the coincidence problem

Javier Grande, Ana Pelinson, Joan Sola

We analyze some generic properties of the dark energy (DE) perturbations, in the case of a self-conserved DE fluid. We also apply a simple test (the "F-test") to compare a model to…

astro-ph2008★ 84 cited

Dark energy perturbations and cosmic coincidence

Javier Grande, Ana Pelinson, Joan Sola

While there is plentiful evidence in all fronts of experimental cosmology for the existence of a non-vanishing dark energy (DE) density ρ_D in the Universe, we are still far away f…

gr-qc2007★ 11 cited

Cosmologies with variable parameters and dynamical cosmon: implications on the cosmic coincidence problem

Javier Grande, Joan Sola, Hrvoje Stefancic

Dynamical dark energy (DE) has been proposed to explain various aspects of the cosmological constant (CC) problem(s). For example, it is very difficult to accept that a strictly co…