PPT Slide
Future Work: Basic Theory
Derive Linearized General Relativistic Perturbation Equations
for Warm Inflation Conditions:
- Effects of homogeneous radiation component
- change in background evolution
- themally induced density fluctuations
- Isocurvature fluctuations
- comprehensive identification of mechanisms
- General evolution of adiabatic and isocurvature fluctuations
- feedback effects of entropic pressure.