Calabi-Yau divisor and curve topologies are crucial for generating suitable scalar potentials in KKLT and LVS, and multi-field fibre moduli can drive sufficient e-folds in LVS inflation without approaching individual Kähler cone boundaries.
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String theory offers classes of inflationary models from type IIB Kaehler moduli and dynamical dark energy models, with a working axion hilltop quintessence construction that stresses initial conditions.
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Towards Systematics of Calabi-Yau Landscape for String Cosmology
Calabi-Yau divisor and curve topologies are crucial for generating suitable scalar potentials in KKLT and LVS, and multi-field fibre moduli can drive sufficient e-folds in LVS inflation without approaching individual Kähler cone boundaries.
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Recent progress on inflation and dark energy from string theory
String theory offers classes of inflationary models from type IIB Kaehler moduli and dynamical dark energy models, with a working axion hilltop quintessence construction that stresses initial conditions.