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 of the cosmological constant is zero. In four spacetime dimensions, the probability distribution takes the Baum-Hawking form, $dP\sim \exp (c{M}_p^2/\Lambda )d\Lambda$.

8 pages, harvmac (b)

References in corpus (1)

• The Cosmic Triangle: Revealing the State of the Universe

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