Pre-bangian origin of our entropy and time arrow
High Energy Physics - Theory
2009-10-31 v1
Abstract
I argue that, in the chaotic version of string cosmology proposed recently, classical and quantum effects generate, at the time of exit to radiation, the correct amount of entropy to saturate a Hubble (or holography) entropy bound (HEB) and to identify, within our own Universe, the arrow of time. Demanding that the HEB be fulfilled at all times forces a crucial "branch change" to occur, and the so-called string phase to end at a critical value of the effective Planck mass, in agreement with previous conjectures.
Cite
@article{arxiv.hep-th/9902126,
title = {Pre-bangian origin of our entropy and time arrow},
author = {G. Veneziano},
journal= {arXiv preprint arXiv:hep-th/9902126},
year = {2009}
}
Comments
Latex file, 8 pages, 1 Figure