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In the context of Type IIB compactified on a large volume Swiss-Cheeseorientifold in the presence of a mobile space-time filling D3-brane and stacksof fluxed D7-branes wrapping the "big" divisor Sigma_B of a Swiss-Cheese CalabiYau in WCP^4 [1,1,1,6,9], we explore various implications of moduli dynamicsand discuss their couplings and decay into MSSM (-like) matter fields early inthe history of universe to reach thermal equilibrium. Like finite temperatureeffects in O'KKLT, we observe that the local minimum of zero-temperatureeffective scalar potential is stable against any finite temperature corrections(up to two-loops) in large volume scenarios as well. Also, we find that moduliare heavy enough to avoid any cosmological moduli problem.

Moduli Thermalization and Finite Temperature Effects in "Big" Divisor Large Volume D3/D7 Swiss-Cheese Compactification