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We investigate the distribution of field theories that arise from the lowenergy limit of flux vacua built on type IIB string theory compactified on themirror quintic. For a large collection of these models, we numericallydetermine the distribution of Taylor coefficients in a polynomial expansion ofeach model's scalar potential to fourth order, and show that they differsignificantly from potentials generated by random choices of such coefficientsover a flat measure.

Random Field Theories in The Mirror Quintic Moduli Space