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