Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2010-10-25
JHEP 1101:088,2011
Physics
High Energy Physics
High Energy Physics - Theory
23 pages, 3 tables, LaTeX, references added, to appear in JHEP
Scientific paper
10.1007/JHEP01(2011)088
In the context of Type IIB compactified on a large volume Swiss-Cheese orientifold in the presence of a mobile space-time filling D3-brane and stacks of fluxed D7-branes wrapping the "big" divisor Sigma_B of a Swiss-Cheese Calabi Yau in WCP^4 [1,1,1,6,9], we explore various implications of moduli dynamics and discuss their couplings and decay into MSSM (-like) matter fields early in the history of universe to reach thermal equilibrium. Like finite temperature effects in O'KKLT, we observe that the local minimum of zero-temperature effective scalar potential is stable against any finite temperature corrections (up to two-loops) in large volume scenarios as well. Also, we find that moduli are heavy enough to avoid any cosmological moduli problem.
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