Curvaton reheating in tachyonic inflationary models
C. Campuzano, S. del Campo, R. Herrera

TL;DR
This paper investigates how the curvaton mechanism reheats a tachyonic inflationary universe with an exponential potential, analyzing energy density behavior and reheating temperatures, which are similar to standard models.
Contribution
It provides a detailed analysis of curvaton reheating in tachyonic inflation, highlighting the energy density dynamics and reheating temperatures in this specific scenario.
Findings
Energy density in the kinetic epoch has complex scale factor dependence
Reheating temperatures are comparable to standard curvaton models
Reheating mechanisms in tachyonic inflation are viable and consistent
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.
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