Krylov complexity and spectral density of BMN matrix model

• URL: http://arxiv.org/abs/2607.24632v1
• Date: Mon, 27 Jul 2026 16:28:49 GMT
• Title: Krylov complexity and spectral density of BMN matrix model
• Abstract summary: We use Krylov complexity as a typical diagnostic of quantum many body dynamics in the context of BMN matrix model at large mass gap.<n>We calculate several physical entities, for example, the moments and return amplitudes at large mass deformation.<n>The linear early time growth of the Krylov entropy confirms the onset of quantum chaos in the matrix model at large mass gap.
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• License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
• Abstract: We use Krylov complexity as a typical diagnostic of quantum many body dynamics in the context of BMN matrix model at large mass gap. We calculate several physical entities, for example, the moments and return amplitudes at large mass deformation. We calculate them for both spread complexity of states as well as Krylov growth of operators in the matrix model. We propose a general expression for the moments at any given order $n$. We also discuss orthogonal polynomials for spread as well as operator Krylov complexity. In the context of the Krylov operator growth we further compute the spectral function and the density of states. A careful analysis of the spectral function near the resonance reveals various IR divergences in addition to the physical collective modes. These collective modes appear to be exceptionally stable due to large mass gap. On the other hand, the UV of the theory appears to be extremely damped due to higher scattering rates. We carefully diagnose these IR divergences near resonance which reveals that these collective modes are in fact non-propagating and should be thought of as diffusion modes or relaxation modes with infinite relaxation time. We also calculate the Krylov variance and Krylov entropy for the matrix model and in particular at early time. The linear early time growth of the Krylov entropy confirms the onset of quantum chaos in the matrix model at large mass gap.

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