Probable values of the cosmological constant in a holographic theory
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.
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CIT-USC Center for Theoretical Physics and California Institute of Technology, Pasadena, California 91125, USA.
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