We combine the axiverse with a negative cosmological constant $\mathrm{\Lambda }$, both originating from the string landscape, and apply an observation-time-weighted anthropic argument. Adopting a uniform prior on $\mathrm{\Lambda }$ and a typical string-motivated axion decay constant comparable to the reduced Planck scale, this framework predicts a $\sim 40\%$ probability of observing $0.1<{\mathrm{\Omega }}_m<0.9$, thereby naturally resolving the long-standing fine-tuning and coincidence problems of dark energy. Unlike many scalar-field dark energy models, the anthropic Lambda-axion universe (ALAverse) statistically disfavors slow-roll dynamics, as slow-roll requires fine-tuning of the initial field displacement. Moreover, the negative cosmological constant renders fast-roll scenarios anthropically unfavorable, since they typically yield only a very brief observational window with positive dark energy density. Having ruled out both extremes, the ALAverse characteristically predicts a moderate-roll dynamics. We derive a two-parameter parametrization in terms of ${\delta }_{\mathrm{\Omega }}$ and $|{ϵ}_s|$ that covers ALAverse solutions as well as a broad class of canonical and phantom field models. Current observational data yield ${\delta }_{\mathrm{\Omega }}=-0.0498\pm 0.0186$, corresponding to a $2.7\sigma$ rejection of $\mathrm{\Lambda }\mathrm{CDM}$ (${\delta }_{\mathrm{\Omega }}=0$) and single-field thawing phantom models (${\delta }_{\mathrm{\Omega }}>0$). The data also show a mild preference for the ALAverse over slow-roll quintessence, a trend that can be conclusively tested with future high-precision measurements of the Hubble diagram.

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• Anthropic considerations
• Dark energy