title: Probable values of the cosmological constant in a holographic theory
abstract: We point out that for a large class of universes, holography implies that the most probable value for the cosmological constant is zero. In four space-time dimensions, the probability distribution takes the Baum-Hawking form, dP approximately exp(cM(2)(p)/Lambda)dLambda.
authors.affiliation: CIT-USC Center for Theoretical Physics and California Institute of Technology, Pasadena, California 91125, USA.
authors.initials: P
authors.lastname: Horava
authors.initials: D
authors.lastname: Minic