Holographic entropy bounds in the inflationary universe
High Energy Physics - Theory
2016-09-06 v2
Abstract
We introduce the relation between the holographic entropy bounds and the inflationary universe. First the holographic entropy bounds for radiation-dominated universe, radiation-dominated universe with a positive cosmological constant are introduced. For an exact de Sitter phase, we use the maximal entropy bound. We classify the inflation based on the quasi-de Sitter spacetime into three steps: slow-roll period of inflation, epoch of reheating, and radiation-dominated era. Then we study how to apply three entropy bounds to the three steps of the inflation. Finally we discuss our results.
Keywords
Cite
@article{arxiv.hep-th/0301073,
title = {Holographic entropy bounds in the inflationary universe},
author = {Y. S. Myung},
journal= {arXiv preprint arXiv:hep-th/0301073},
year = {2016}
}
Comments
16 pages, two eps figures