Linear and nonlinear interactions in the dark sector
We investigate models of interacting dark matter and dark energy for the Universe in a spatially flat Friedmann-Robertson-Walker space-time. We find the "source equation" for the total energy density and determine the energy density of each dark component. We introduce an effective one-flu...
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Autor principal: | Chimento, L.P. |
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Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_15507998_v81_n4_p_Chimento |
Aporte de: |
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