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Krylov complexity of fermion chain in double-scaled SYK and power spectrum perspective

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arxiv 2407.13293 v1 pith:5M6B4FDG submitted 2024-07-18 hep-th cond-mat.str-elquant-ph

classification hep-thcond-mat.str-elquant-ph
keywords complexitykrylovgrowthinitialspectrumboundedexponentialpower
verification ladder T0 review T1 audit T2 compute T3 formal
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We investigate Krylov complexity of the fermion chain operator which consists of multiple Majorana fermions in the double-scaled SYK (DSSYK) model with finite temperature. Using the fact that Krylov complexity is computable from two-point functions, the analysis is performed in the limit where the two-point function becomes simple and we compare the results with those of other previous studies. We confirm the exponential growth of Krylov complexity in the very low temperature regime. In general, Krylov complexity grows at most linearly at very late times in any system with a bounded energy spectrum. Therefore, we have to focus on the initial growth to see differences in the behaviors of systems or operators. Since the DSSYK model is such a bounded system, its chaotic nature can be expected to appear as the initial exponential growth of the Krylov complexity. In particular, the time at which the initial exponential growth of Krylov complexity terminates is independent of the number of degrees of freedom. Based on the above, we systematically and specifically study the Lanczos coefficients and Krylov complexity using a toy power spectrum and deepen our understanding of those initial behaviors. In particular, we confirm that the overall sech-like behavior of the power spectrum shows the initial linear growth of the Lanczos coefficient, even when the energy spectrum is bounded.

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Cited by 2 Pith papers

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  1. Holographic timelike complexity for de Sitter

    hep-th 2026-07 conditional novelty 6.0 of 10

    Timelike subregion volume complexity in de Sitter grows exponentially early and diverges hyperfast at a maximal duration; near the SdS black hole horizon the divergence is replaced by slower, claimed-nonlinear growth.

  2. From black hole interior to quantum complexity through operator rank

    hep-th 2024-12 conditional novelty 6.0 of 10

    The Hartman-Maldacena surface area in a black hole interior bounds the boundary circuit depth from below, rigorously at early times and conjecturally later.

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