This research proposes a comprehensive program to explore non-zero axion effects in 3D orientifold flux vacua from Type II string compactifications, focusing on moduli stabilization, vacuum structure, and cosmological implications.
Key findings
The inclusion of non-zero axion expectation values opens new avenues for understanding moduli stabilization and vacuum structure.
A general formalism for axion potential generation through flux compactifications is developed.
Conditions for perturbative stability and the interplay between axion dynamics and scale separation are analyzed.
The methodology includes classification of axion-compatible flux configurations and stability analysis of resulting vacua.
Limitations & open questions
The research is in its initial phase with the proposed methodology awaiting full implementation and validation.
The study's predictions require further testing through holographic duality and cosmological observations.