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Abstract: We provide a detailed discussion of the main theoretical and phenomenological challenges of quintessence model building in any parametric or numerically controlled regime of the moduli space of string theory. We argue that a working quintessence model requires a leading order non-supersymmetric (near) Minkowski vacuum with an axionic flat direction away from the boundary of moduli space. This axion, when lifted by subdominant non-perturbative effects, could drive hilltop quintessence only for very tuned initial conditions and a very low inflationary scale.
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