| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8200016 | Physics Letters B | 2006 | 5 Pages |
Abstract
This work deals with cosmological models driven by real scalar field, described by standard dynamics in generic spherical, flat, and hyperbolic geometries. We introduce a first-order formalism, which shows how to relate the potential that specifies the scalar field model to Hubble's parameter in a simple and direct manner. Extensions to tachyonic dynamics, and to two or more real scalar fields are also presented.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
D. Bazeia, C.B. Gomes, L. Losano, R. Menezes,