Probable Values of the Cosmological Constant in a Holographic Theory
High Energy Physics - Theory
2009-07-09 v1 Astrophysics
General Relativity and Quantum Cosmology
Abstract
We point out that for a large class of universes, holography implies that the most probable value of the cosmological constant is zero. In four spacetime dimensions, the probability distribution takes the Baum-Hawking form, .
Keywords
Cite
@article{arxiv.hep-th/0001145,
title = {Probable Values of the Cosmological Constant in a Holographic Theory},
author = {Petr Horava and Djordje Minic},
journal= {arXiv preprint arXiv:hep-th/0001145},
year = {2009}
}
Comments
8 pages, harvmac (b)