Holographic dark energy interacting with dark matter in a closed Universe

Norman Cruz, Samuel Lepe, Francisco Peña, Joel Saavedra

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

8 Citas (Scopus)

Resumen

A cosmological model of an holographic dark energy interacting with dark matter throughout a decaying term of the form Q = 3 (λ1 ρDE + λ2 ρm) H is investigated. General constraint on the parameters of the model are found when accelerated expansion is imposed and we found a phantom scenario, without any reference to a specific equation of state for the dark energy. The behavior of equation of state for dark energy is also discussed.

Idioma originalInglés
Páginas (desde-hasta)271-274
Número de páginas4
PublicaciónPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volumen669
N.º5
DOI
EstadoPublicada - 27 nov. 2008
Publicado de forma externa

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