2006
DOI: 10.1103/physrevlett.97.160201
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Large Deviations of Extreme Eigenvalues of Random Matrices

Abstract: We calculate analytically the probability of large deviations from its mean of the largest (smallest) eigenvalue of random matrices belonging to the Gaussian orthogonal, unitary and symplectic ensembles. In particular, we show that the probability that all the eigenvalues of an (N × N ) random matrix are positive (negative) decreases for large N as ∼ exp [−βθ(0)N 2 ] where the parameter β characterizes the ensemble and the exponent θ(0) = (ln 3)/4 = 0.274653 . . . is universal. We also calculate exactly the av… Show more

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Cited by 218 publications
(425 citation statements)
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“…largest and smallest) eigenvalues of a random matrix. For a large class of random matrix ensembles, including the W W W ensemble [469], one finds [470][471][472] 158) where the function Ψ(ζ), which depends on the particular ensemble and is computable in simple cases, is N -independent at leading order in large N . In summary, eigenvalue repulsion dictates that the probability that a Hessian matrix in the ensemble defined by (3.149) has only positive eigenvalues is given by…”
Section: Random Supergravitymentioning
confidence: 99%
“…largest and smallest) eigenvalues of a random matrix. For a large class of random matrix ensembles, including the W W W ensemble [469], one finds [470][471][472] 158) where the function Ψ(ζ), which depends on the particular ensemble and is computable in simple cases, is N -independent at leading order in large N . In summary, eigenvalue repulsion dictates that the probability that a Hessian matrix in the ensemble defined by (3.149) has only positive eigenvalues is given by…”
Section: Random Supergravitymentioning
confidence: 99%
“…Note that in the usual Gaussian ensembles the second term of S 2 is absent, thus if the average value of the eigenvalues is shifted from zero (and thus we shall see later the value of α is shifted from 1/2) then the constraint increases the action S 2 by a finite value and thus the probability of finding a Gaussian matrix with α = 1/2 is of order exp(−N 2 θ(α)) making the probability of minima for instance extremely small [13,14,15]. This is not the case for the Hessian of a Gaussian random field at a critical point due to the presence of this zero mode.…”
mentioning
confidence: 99%
“…We now adopt the constrained Coulomb gas approach recently introduced in [13] and using standard methods of functional integration [10] we may write…”
mentioning
confidence: 99%
“…Energy landscapes provide a simple conceptual framework for modeling these systems but in fact their use goes much beyond that. For instance the vacua of string theories are expected to proliferate enormously, and the problem of estimating the number of local minima [2,3] [8,9] and the associated problems in random matrix theory [3,10,11]. Typically these systems consider a particle, a configuration of particles, or even a manifold, subject to a random potential.…”
mentioning
confidence: 99%
“…For instance the vacua of string theories are expected to proliferate enormously, and the problem of estimating the number of local minima [2,3] of string energy landscapes is still an open problem. Other examples include rugged (random) energy landscapes in evolutionary biology [4], quantum cosmology [5], manifolds in random media [6], glassy systems [1,7] random potentials [8,9] and the associated problems in random matrix theory [3,10,11]. Typically these systems consider a particle, a configuration of particles, or even a manifold, subject to a random potential.…”
mentioning
confidence: 99%