Note on "Continuous matter creation and the acceleration of the universe: the growth of density fluctuations"

Details Note on "Continuous matter creation and the acceleration of the universe: the growth of density fluctuations" Note on "Continuous matter creation and the acceleration of the universe: the growth of density fluctuations"

2010-12-22

arxiv.org/abs/1012.5069v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

5 pages, 0 figures

Scientific paper

Recently, de Roany & Pacheco (2010) performed a Newtonian analysis on the evolution of perturbations for a class of relativistic cosmological models with Creation of Cold Dark Matter (CCDM) proposed by the present authors. In this note we demonstrate that the basic equations adopted in their work do not recover the specific (unperturbed) CCDM model. Unlike to what happens in the original CCDM cosmology, their basic conclusions refer to a decelerating cosmological model in which there is no transition from a decelerating to an accelerating regime as required by SNe type Ia and complementary observations.

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