Abstract
We study the probability of stability of a large complex system of size within the framework of a generalized May model, which assumes a linear dynamics of each population size (with respect to its equilibrium value): . The 's are the intrinsic decay rates, is a real symmetric Gaussian random matrix and measures the strength of pairwise interaction between different species. Unlike in May's original homogeneous model, each species has now an intrinsic damping that may differ from one another. As the interaction strength increases, the system undergoes a phase transition from a stable phase to an unstable phase at a critical value . We reinterpret the probability of stability in terms of the hitting time of the level of an associated Dyson Brownian Motion (DBM), starting at the initial position and evolving in `time' . In the large limit, using this DBM picture, we are able to completely characterize for arbitrary density of the 's. For a specific flat configuration , we obtain an explicit parametric solution for the limiting (as ) spectral density for arbitrary and . For finite but large , we also compute the large deviation properties of the probability of stability on the stable side using a Coulomb gas representation.
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