Tachyonic quintessential inflation

Cardenas, VH

Abstract

I study the possibility of constructing an observationally viable scenario where both early inflation and the recently detected accelerated expansion of the universe can be explained by using a single scalar field associated with the tachyon. The reheating phase becomes crucial in enabling us to have a consistent cosmology and also to get a second accelerated expansion period. A discussion using an exponential potential is presented. © 2006 The American Physical Society.

Más información

Título según WOS: Tachyonic quintessential inflation
Título según SCOPUS: Tachyonic quintessential inflation
Título de la Revista: PHYSICAL REVIEW D
Volumen: 73
Número: 10
Editorial: American Physical Society
Fecha de publicación: 2006
Idioma: English
URL: http://link.aps.org/doi/10.1103/PhysRevD.73.103512
DOI:

10.1103/PhysRevD.73.103512

Notas: ISI, SCOPUS