Probable Values of the Cosmological Constant in a Holographic Theory
Petr Horava, Djordje Minic
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, dP(cMp2/Λ)dΛ.
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