论文标题

挤压的OTOC和宇宙学

The Squeezed OTOC and Cosmology

论文作者

Haque, S. Shajidul, Underwood, Bret

论文摘要

超级阶外相关器(OTOC)的指数增长是量子混乱的重要潜在特征。对于挤压状态,OTOC非常易于计算,其应用在量子光学和宇宙学中经常发现。我们发现,通用高度挤压量子状态的OTOC呈指数较大,这表明高度挤压的状态被“启动”用于量子混乱。经典符号相位空间矩阵的量子概括可用于提取量子Lyapunov谱,并且与任何单个OTOC相比,所有挤压角度都可以更好地捕获所有压缩角度的挤压状态的指数生长。通过描述挤压状态语言中的宇宙学扰动,我们能够将OTOC的计算应用于具有固定状态方程式的任意扩展和收缩背景。我们发现,只有扩大的保健背景在后期才能呈指数增长的OTOC,其推定的Lyapunov指数与其他计算一致。尽管其他宇宙学背景的OTOC的后期行为似乎取决于状态方程,但我们发现量子Lyapunov频谱显示出某种普遍的行为:OTOC的生长与扰动波长的比例因子成正比,比宇宙学Hubble Horizo​​n大。

Exponential growth in the out-of-time-order correlator (OTOC) is an important potential signature of quantum chaos. The OTOC is quite simple to calculate for squeezed states, whose applications are frequently found in quantum optics and cosmology. We find that the OTOC for a generic highly squeezed quantum state is exponentially large, suggesting that highly squeezed states are "primed" for quantum chaos. A quantum generalization of the classical symplectic phase space matrix can be used to extract the quantum Lyapunov spectrum, and we find this better captures the exponential growth of squeezed states for all squeezing angles compared to any single OTOC. By describing cosmological perturbations in the squeezed state language, we are able to apply our calculations of the OTOC to arbitrary expanding and contracting backgrounds with fixed equation of state. We find that only expanding de Sitter backgrounds support an exponentially growing OTOC at late times, with a putative Lyapunov exponent consistent with other calculations. While the late-time behavior of the OTOC for other cosmological backgrounds appears to change depending on the equation of state, we find that the quantum Lyapunov spectrum shows some universal behavior: the OTOC grows proportional to the scale factor for perturbation wavelengths larger than the cosmological Hubble horizon.

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