期刊
PHYSICAL REVIEW LETTERS
卷 85, 期 8, 页码 1610-1613出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.85.1610
关键词
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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 similar to exp(cM(p)(2)/Lambda)d Lambda.
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