Yoske Sumitomo, S. -H. Henry Tye
We study the probability distribution P(\Lambda) of the cosmological constant \Lambda in a specific set of KKLT type models of supersymmetric IIB vacua. P(\Lambda) is divergent at \Lambda =0^- and the likely value of \Lambda drops exponentially as the number of complex structure moduli h^{2,1} increases. Also, owing to the hierarchical and approximate no-scale structure, the probability of having a positive Hessian (mass squared matrix) approaches unity as h^{2,1} increases.
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http://arxiv.org/abs/1211.6858
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