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arXiv 2401.09307hep-thastro-ph.COgr-qchep-phquant-ph
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暴胀中的 Krylov 复杂度

Inflationary Krylov complexity

Tao Li, Lei-Hua Liu

AI总结:

本研究系统研究了暴胀中修正色散关系的曲率扰动的 Krylov 复杂度,发现极早期宇宙为最大混沌系统,且 Krylov 复杂度在暴胀期间持续增长,背景变化对其演化有显著影响。

摘要:

在这项工作中,我们利用封闭系统和开放系统中的算法,系统地研究了暴胀中修正色散关系的曲率扰动的 Krylov 复杂度。我们的分析可应用于大多数暴胀模型。遵循 Lanczos 算法,我们发现极早期宇宙是一个无限的、多体的、最大混沌系统。我们的数值结果表明,标准色散关系的 Lanczos 系数和 Lyapunov 指数主要由尺度因子决定。对于修正的情况,它几乎由动量决定。在封闭系统的方法中,我们发现 Krylov 复杂度将在视界退出之前表现出不规则的振荡。修正的情况将在视界退出之后呈现更快的增长。由于整个宇宙是一个开放系统,开放系统的方法更为现实和可靠。然后,我们构造了精确的波函数,该波函数非常稳健,仅要求 Lanczos 系数与 $n$(主量子数)成正比。基于此,我们发现 Krylov 复杂度和 Krylov 熵在弱耗散近似下能够在封闭系统的情况下很好地恢复,在弱耗散近似下,我们的分析表明 Krylov 复杂度的演化将与原始情况不同。我们还发现暴胀时期是一个强耗散系统。同时,我们的数值结果清楚地表明 Krylov 复杂度在整个暴胀期间将增长。但对于小尺度,在视界退出之后将出现一个峰值。我们的分析揭示了背景(暴胀)的剧烈变化将显著影响 Krylov 复杂度的演化。因为曲率扰动将从量子层面过渡到经典层面。

英文摘要:

In this work, we have systematically investigated the Krylov complexity of curvature perturbation for the modified dispersion relation in inflation, using the algorithm in closed system and open system. Our analysis could be applied to the most inflationary models. Following the Lanczos algorithm, we find the very early universe is an infinite, many-body, and maximal chaotic system. Our numerics shows that the Lanczos coefficient and Lyapunov index of the standard dispersion relation are mainly determined by the scale factor. As for the modified case, it is nearly determined by the momentum. In a method of the closed system, we discover that the Krylov complexity will show irregular oscillation before the horizon exits. The modified case will present faster growth after the horizon exists. Since the whole universe is an open system, the approach of an open system is more realistic and reliable. Then, we construct the exact wave function which is very robust only requiring the Lanczos coefficient proportional to $n$ (main quantum number). Based on it, we find the Krylov complexity and Krylov entropy could nicely recover in the case of a closed system under the weak dissipative approximation, in which our analysis shows that the evolution of Krylov complexity will not be the same with the original situation. We also find the inflationary period is a strong dissipative system. Meanwhile, our numerics clearly shows the Krylov complexity will grow during the whole inflationary period. But for the small scales, there will be a peak after the horizon exits. Our analysis reveals that the dramatic change in background (inflation) will significantly impact the evolution of Krylov complexity. Since the curvature perturbation will transit from the quantum level to the classical level.

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