Abstract (EN):
In this paper, we study the effects of an interaction between dark matter and dark energy through a two-scalar-field model with a potential V(phi, chi) = e(-lambda phi) P(phi, chi), where P(phi, chi) is a polynomial. We show that the cosmic expansion dynamics of the Universe is reproduced for a large range of the bare mass of the dark matter field and that there exist solutions with transient accelerated expansion. A modification in the exponential behavior of the potential is studied, with important physical implications, including the possibility of more realistic transient acceleration solutions.
Idioma:
Inglês
Tipo (Avaliação Docente):
Científica
Contacto:
orfeu.bertolami@fc.up.pt; pedro.carrilho@ist.utl.pt; paramos@ist.edu
Nº de páginas:
8