Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2009-02-25
Phys.Rev.D80:023502,2009
Physics
High Energy Physics
High Energy Physics - Theory
9 pages, 3 figures; v2: minor error fixed (results essentially unchanged), reference added; v3: published version, includes a
Scientific paper
10.1103/PhysRevD.80.023502
Arguably a major success of the landscape picture is the prediction of a small, non-zero vacuum energy density. The details of this prediction depends in part on how the diverging spacetime volume of the multiverse is regulated, a question that remains unresolved. One proposal, the causal diamond measure, has demonstrated many phenomenological successes, including predicting a distribution of positive vacuum energy densities in good agreement with observation. In the string landscape, however, the vacuum energy density is expected to take positive and negative values. We find the causal diamond measure gives a poor fit to observation in such a landscape -- in particular, 99.6% of observers in galaxies seemingly just like ours measure a vacuum energy density smaller than we do, most of them measuring it to be negative.
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