Tachyonic quintessential inflation
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 |