Probable Values of the Cosmological Constant in a Holographic Theory

Details Probable Values of the Cosmological Constant in a Holographic Theory Probable Values of the Cosmological Constant in a Holographic Theory

2000-01-22

arxiv.org/abs/hep-th/0001145v1

Phys.Rev.Lett.85:1610-1613,2000

Physics

High Energy Physics

High Energy Physics - Theory

8 pages, harvmac (b)

Scientific paper

10.1103/PhysRevLett.85.1610

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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