Heterotic string theory implies the QCD axion mass is bounded below by 0.5 neV and typically falls in [0.5, 0.8] neV across most compactifications.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
fields
hep-th 3years
2026 3verdicts
UNVERDICTED 3roles
background 2polarities
background 2representative citing papers
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.
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.
citing papers explorer
-
Heterotic String Theory Suggests a QCD Axion Near 0.5 neV
Heterotic string theory implies the QCD axion mass is bounded below by 0.5 neV and typically falls in [0.5, 0.8] neV across most compactifications.
-
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.
-
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.