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Probable Values of the Cosmological Constant in a Holographic Theory
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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, $dP\sim\exp(cM_p^2/\Lambda)d\Lambda$.
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Cited by 2 Pith papers
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