Phys. Rev. Lett. 85, 1610–1613 (2000)Probable Values of the Cosmological Constant in a Holographic TheoryReceived 25 January 2000; published in the issue dated 21 August 2000 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∼exp(cMp2/Λ)dΛ. © 2000 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.85.1610
DOI:
10.1103/PhysRevLett.85.1610
PACS:
98.80.Cq, 04.70.Dy, 11.10.Kk
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