Interacting models of soft coincidence

被引：79

作者：

del Campo, Sergio

Herrera, Ramon

Olivares, German

Pavon, Diego

机构：

[1] Pontificia Univ Catolica Valparaiso, Inst Fis, Valparaiso, Chile

[2] Univ Autonoma Barcelona, Dept Fis, Fac Ciencias, E-08193 Barcelona, Spain

来源：

PHYSICAL REVIEW D | 2006年 / 74卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.74.023501

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：9

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