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High Scale Inflation and Low Scale Supersymmetry

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I discuss the tensions present between combining models of high scale inflation and low scale supersymmetry, which arises from the ability of the large inflationary vacuum energy to cause overshoot and decompactification of otherwise stabilised moduli. I propose a method to combine these hierarchically different scales in a natural fashion, and discuss its advantages and its drawbacks.

This talk is part of the Cosmology Lunch series.

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