A Brane World Solution to the Cosmological Constant Problem
高能物理 - 理论
2009-10-31 v1 天体物理学
广义相对论与量子宇宙学
高能物理 - 唯象学
摘要
We consider a model with two parallel (positive tension) 3-branes separated by a distance in 5-dimensional spacetime. If the interbrane space is anti-deSitter, or is not precisely anti-deSitter but contains no event horizons, the effective 4-dimensional cosmological constant seen by observers on one of the branes (chosen to be the visible brane) becomes exponentially small as grows large.
引用
@article{arxiv.hep-th/0006068,
title = {A Brane World Solution to the Cosmological Constant Problem},
author = {S. -H. Henry Tye and Ira Wasserman},
journal= {arXiv preprint arXiv:hep-th/0006068},
year = {2009}
}
备注
10 pages