Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8200145 | Physics Letters B | 2006 | 6 Pages |
Abstract
The curvaton reheating in a tachyonic inflationary universe model with an exponential potential is studied. We have found that the energy density in the kinetic epoch, has a complicated dependencies of the scale factor. For different scenarios, the temperature of reheating is computed. These temperature result to be analogous to those obtained in the standard case of the curvaton scenario.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Cuauhtemoc Campuzano, Sergio del Campo, Ramón Herrera,