2010
DOI: 10.1590/s0103-97332010000400007
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Observational consequences of a dark interaction model

Abstract: We study a model with decay of dark energy and creation of the dark matter particles. We integrate the field equations and find the transition redshift where the evolution process of the universe change the accelerated expansion, and discuss the luminosity distance, acoustic oscillations and the statefinder parameters.

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Cited by 1 publication
(2 citation statements)
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“…Using these data in Eq. (27) and Eq. (28) it is possible to get a value for η, this value is 3.95 ± 0.24, while in [32] the value was 3.82.…”
Section: The Abell Cluster A586mentioning
confidence: 99%
See 1 more Smart Citation
“…Using these data in Eq. (27) and Eq. (28) it is possible to get a value for η, this value is 3.95 ± 0.24, while in [32] the value was 3.82.…”
Section: The Abell Cluster A586mentioning
confidence: 99%
“…Most of the models developed until the present time, have studied the dark energy and dark matter coupling; some authors have concluded that there is a energy transfer from dark matter to dark energy, while others stand for the opposite. Thus this is an issue involving much controversy [23][24][25][26][27][28].…”
Section: Introductionmentioning
confidence: 99%