Cosmological Evolution of a Dark Energy Model with Non-Linear Interaction.

In this paper it is considered a holographic dark energy model with a non-linear interaction between the component of dark energy and dark matter in a FRW type flat universe. In this context, the cosmological evolution of the universe is analyzed taking into account the behavior of...

詳細記述

書誌詳細

第一著者:	Oliveros García, A.
フォーマット:	Online
言語:	spa
出版事項:	Universidad Pedagógica y Tecnológica de Colombia 2016
主題:	Cosmología energía oscura. (Cosmology Dark Energy.)
オンライン･アクセス:	https://revistas.uptc.edu.co/index.php/ciencia_en_desarrollo/article/view/4232