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Interacting models of soft coincidence

Astrophysics, abstract
astro-ph/0606520

From: Diego Pavon [view email]

Date: Wed, 21 Jun 2006 13:21:35 GMT (206kb)

Interacting models of soft coincidence

Authors: Sergio del Campo, Ramon Herrera, German Olivares, Diego Pavon

Comments: 18 pages, 9 figures; to be published in the Physical Review, section D

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 interaction between the dark energy component (either phantom or quintessence) and dark matter can alleviate it. In this scenario the baryon component is independently conserved. This generalizes a previous study [S. del Campo, R. Herrera, and D. Pavon, Phys. Rev. D 71, 123529 (2005)] in which neither baryons nor phantom energy were considered.

http://arxiv.org/abs/astro-ph/0606520

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