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For a universe presently dominated by static or dynamic vacuum energy,cosmological constant (LCDM) or quintessence (QCDM), we calculate theasymptotic collapsed mass fraction as function of the present ratio of vacuumenergy to clustered mass, \Omega_{Q0}/\Omega_{m0}. Identifying these collapsedfractions as anthropic probabilities, we find the value \Omega_{Q0}/\Omega_{m0}\sim 2 to be reasonably likely in LCDM, and very likely in QCDM.Comment: 4 pages, 2 tables, 1 figur

OBSERVED SMOOTH ENERGY IS ANTHROPICALLY EVEN MORE LIKELY AS QUINTESSENCE THAN AS COSMOLOGICAL CONSTANT