Non-Perturbative Modulus Decay and Multi-Component Dark Matter
hep-ph, astro-ph.CO, hep-th
Submitted: 2026-09-18
Updated: 2026-09-18
Terminology
Sources
- Model Independent Properties and Cosmological Implications of the Dilaton and Moduli Sectors of 4-d Strings
- Cosmological Implications of Dynamical Supersymmetry Breaking
- Cosmological Moduli and the Post-Inflationary Universe: A Critical Review
- Supersymmetry Breaking in the Early Universe
- Relaxing the Cosmological Moduli Problem
- Non-thermal Dark Matter and the Moduli Problem in String Frameworks
- A Non-thermal WIMP Miracle
- The Axiverse induced Dark Radiation Problem
- An M theory Solution to the Hierarchy Problem
- Explaining the Electroweak Scale and Stabilizing Moduli in M Theory
- The $G_2$-MSSM - An $M$ Theory motivated model of Particle Physics
- Wino Cold Dark Matter from Anomaly-Mediated SUSY Breaking
- An M Theory Solution to the Strong CP Problem and Constraints on the Axiverse
- Compactified String Theories -- Generic Predictions for Particle Physics
- Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics
- Towards the Theory of Reheating After Inflation
- Dynamics of Symmetry Breaking and Tachyonic Preheating
- Gauge Field Preheating at the End of Inflation
- Cosmological Moduli and Non-perturbative Production of Axions
- Preheating Axions in String Cosmology
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