Exactly solved models of interacting dark matter and dark energy
We introduce an effective one-uid description of the interacting dark sector in a spatially at Friedmann-Robertson-Walker space-time and investigate the stability of the power-law solutions. We find the "source equation" for the total energy density and determine the energy density of each...
Guardado en:
Autor principal: | Chimento, L.P. |
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Formato: | CONF |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0094243X_v1471_n_p30_Chimento |
Aporte de: |
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