activity
20062008
most citedDynamics of Interacting Quintessence Models: Observational Constraints

100 citations · 140 across the 3 of their papers we have counts for

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7 papers · 1 filter

astro-ph200840 cited

The Integrated Sachs-Wolfe Effect in Interacting Dark Energy Models

German Olivares, Fernando Atrio-Brandela, Diego Pavon

Models with dark energy decaying into dark matter have been proposed in Cosmology to solve the coincidence problem. We study the effect of such coupling on the cosmic microwave bac…

astro-ph2007100 cited

Dynamics of Interacting Quintessence Models: Observational Constraints

German Olivares, Fernando Atrio-Barandela, Diego Pavon

Interacting quintessence models have been proposed to explain or, at least, alleviate the coincidence problem of late cosmic acceleration. In this paper we are concerned with two a…

astro-ph2006

The matter power spectrum as a tool to discriminate dark matterr-dark energy interactions

German Olivares, Diego Pavon, Fernando Atrio-Barandela

The coincidence problem of late cosmic acceleration gets significantly alleviated when a suitable interaction between matter and dark energy, either of phantom type or not, enters…

astro-ph2006141 cited

Matter density perturbations in interacting quintessence models

G. Olivares, F. Atrio-Barandela, D. Pavon

Models with dark energy decaying into dark matter have been proposed to solve the coincidence problem in cosmology. We study the effect of such coupling in the matter power spectru…

astro-ph2006111 cited

Interacting models of soft coincidence

Sergio del Campo, Ramon Herrera, German Olivares +1

The coincidence problem of late cosmic acceleration is a serious riddle in connection with our understanding of the evolution of the Universe. In this paper we show that an interac…

astro-ph2005

Constraining dark energy interacting models with WMAP

German Olivares, Fernando Atrio-Barandela, Diego Pavon

We determine the range of parameter space of an interacting quintessence (IQ) model that best fits the luminosity distance of type Ia supernovae data and the recent WMAP measuremen…