A model for time-dependent cosmological constant and its consistency with the present Friedmann universe
arXiv:hep-th/0202169 · doi:10.1088/0264-9381/19/11/323
Abstract
We use a model where the cosmological term can be related to the chiral gauge anomaly of a possible quantum scenario of the initial evolution of the universe. We show that this term is compatible with the Friedmann behavior of the present universe.
5 pages, Revtex 4, twocolumn (minor corrections and improved reference list. To appear in Classical and Quantum Gravity)