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arXiv · 1608.05189

Random Field Theories in The Mirror Quintic Moduli Space

Kate Eckerle·Brian Greene
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Abstract

We investigate the distribution of field theories that arise from the low energy limit of flux vacua built on type IIB string theory compactified on the mirror quintic. For a large collection of these models, we numerically determine the distribution of Taylor coefficients in a polynomial expansion of each model's scalar potential to fourth order, and show that they differ significantly from potentials generated by random choices of such coefficients over a flat measure.

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Kate Eckerle, Brian Greene. 2016-08-18. Random Field Theories in The Mirror Quintic Moduli Space. https://arxiv.org/abs/1608.05189

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