Non-linear coupling in the dark sector as a running vacuum model

In this work we study a phenomenological non-gravitational interaction between dark matter and dark energy. The scenario studied in this work extends the usual interaction model proportional to the derivative of the dark component density adding to the coupling a non-linear term of the form Q= ρ′/ 3...

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Detalles Bibliográficos
Publicado: 2018
Materias:
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v50_n8_p_DeSantiago
http://hdl.handle.net/20.500.12110/paper_00017701_v50_n8_p_DeSantiago
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