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arXiv:2509.14742 · Journal of High Energy Physics

Krylov complexity and Wightman power spectrum with positive chemical potential in Schrödinger field theory

Peng-Zhang He, Lei-Hua Liu, Hai-Qing Zhang, Qing-Quan Jiang

Published Feb 26, 2026• 0 citations
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Abstract

A bstract We study Krylov complexity in Schrödinger field theory in the grand canonical ensemble with chemical potential μ , with an emphasis on the qualitatively new features that arise for μ > 0. In this regime the fermionic Wightman power spectrum is effectively single-sided and sharply truncated at ω = μ , which induces a crossover in the Lanczos coefficients and signals a dynamical transition from a bulk-dominated regime to a spectral-edge-dominated regime: b n displays a two-stage linear growth (from an early-time slope π/β to an asymptotic slope 2 /β ), while a n bends from near-zero values to a linear descent with slope −4 /β . We provide analytic support for the resulting complexity growth from three complementary viewpoints: (i) using an SL(2 , ℝ) algebraic construction matched to the asymptotic Lanczos data, we show that the late-time Krylov complexity must grow quadratically, K ( t ) ∝ t 2 ; (ii) by analyzing engineered Wightman spectra with controlled decay and truncation, we identify single-sided exponential decay as the key spectral feature responsible for the quadratic asymptotics, while an approximately even two-sided exponential spectrum explains the early-time K ( t ) ~ sinh 2 ( πt/β ) behavior at large μ ; (iii) we formulate the problem in terms of orthogonal polynomials and estimate the crossover scale separating the early- and late-stage regimes. Overall, our results help clarify the role of chemical potential and spectral truncation in shaping operator growth and Krylov complexity in this non-relativistic quantum field theory setting.

DOI
10.1007/jhep02(2026)259

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We continue the analysis of the Krylov complexity in the IP matrix model. In a previous paper, for a fundamental operator, it was shown that at zero temperature, the Krylov complexity oscillates and does not grow, but in the infinite temperature limit, the Krylov complexity grows exponentially in time as ∼exp⁡(O(t))\sim \exp\left( {\mathcal{O}\left( {\sqrt{t}}\right)} \right)∼exp(O(t​)). We study how the Krylov complexity changes from a zero-temperature oscillation to an infinite-temperature exponential growth. At low temperatures, the spectral density is approximated as collections of infinite Wigner semicircles. We showed that this infinite collection of branch cuts yields linear growth to the Lanczos coefficients and gives exponential growth of the Krylov complexity. Thus the IP model for any nonzero temperature shows exponential growth for the Krylov complexity even though the Green function decays by a power law in time. We also study the Lanczos coefficients and the Krylov complexity in the IOP matrix model taking into account the 1/N21/N^21/N2 corrections. There, the Lanczos coefficients are constants and the Krylov complexity does not grow exponentially as expected.
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A bstract Krylov complexity characterizes the operator growth in the quantum many-body systems or quantum field theories. The existing literatures have studied the Krylov complexity in the low temperature limit in the quantum field theories. In this paper, we extend and systematically study the Krylov complexity and Krylov entropy in a scalar field theory with general temperatures. To this end, we propose a new method to calculate the Wightman power spectrum which allows us to compute the Lanczos coefficients and subsequently to study the Krylov complexity (entropy) in general temperatures. We find that the Lanczos coefficients and Krylov complexity (entropy) in the high temperature limit will behave somewhat differently from those studies in the low temperature limit. We give an explanation of why the Krylov complexity does not oscillate in the high-temperature region. Moreover, we uncover the transition temperature that separates the oscillating and monotonic increasing behavior of Krylov complexity.