Inhomogeneous cosmologies with Q matter and varying [formula presented]
Starting from the inhomogeneous shear-free Nariai metric we show, by solving the Einstein-Klein-Gordon field equations, how a self-interacting scalar field plus a material fluid, a variable cosmological term, and a heat flux can drive the universe to its currently observed state of homogeneous accel...
Publicado: |
1999
|
---|---|
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v60_n10_p_Chimento http://hdl.handle.net/20.500.12110/paper_15507998_v60_n10_p_Chimento |
Aporte de: |
Ejemplares similares
-
Inhomogeneous cosmologies with Q matter and varying [formula presented]
por: Chimento, L.P., et al. -
Inhomogeneous cosmologies with Q matter and varying Λ
Publicado: (1999) -
Inhomogeneous cosmologies with Q matter and varying Λ
por: Chimento, L.P., et al. -
Inhomogeneous universe models with varying cosmological term
por: Chimento, Luis Pascual
Publicado: (1998) -
Inhomogeneous universe models with varying cosmological term
por: Chimento, L.P., et al.