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arXiv 1902.07586hep-th
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全息超导体的复杂度

Complexity of Holographic Superconductors

Run-Qiu Yang, Hyun-Sik Jeong, Chao Niu, Keun-Young Kim

AI总结:

本文利用CV猜想研究全息超导体复杂度,发现超导相复杂度低于正常相,低温下复杂度按温度幂律标度,并发展了数值方法计算时间演化复杂度,验证其增长率不违反Lloyd界限。

摘要:

我们通过“复杂度=体积”(CV)猜想研究全息超导体(d+1维中的Einstein-Maxwell-复标量作用量)的复杂度。首先,似乎存在一个普适性质:在临界温度以下,超导相的复杂度总是小于不稳定的正常相,这与自由能类似。我们研究了复杂度对温度的依赖关系。在低温极限下,(形成)复杂度按T^α标度,其中α是复标量质量m^2、U(1)电荷q和维数d的函数。特别地,对于m^2=0,我们发现α=d-1,与q无关,这可以通过低温全息超导体的近视界几何来解释。接着,我们发展了一种通用的数值方法来计算CV猜想下的时间依赖复杂度。通过这种方法,我们计算了全息超导体的时间依赖复杂度。在正常相和超导相中,复杂度都随时间增加,并且增长率饱和到一个依赖于温度的常数。温度越高,增长率越大。然而,在所有情况下增长率都没有违反Lloyd界限,并且在高温极限下的晚期饱和了Lloyd界限。

英文摘要:

We study the complexity of holographic superconductors (Einstein-Maxwell-complex scalar actions in $d+1$ dimension) by the `complexity = volume' (CV) conjecture. First, it seems that there is a universal property: the superconducting phase always has a smaller complexity than the unstable normal phase below the critical temperature, which is similar to a free energy. We investigate the temperature dependence of the complexity. In the low temperature limit, the complexity (of formation) scales as $T^α$, where $α$ is a function of the complex scalar mass $m^2$, the $U(1)$ charge $q$, and dimension $d$. In particular, for $m^2=0$, we find $α=d-1$, independent of $q$, which can be explained by the near horizon geometry of the low temperature holographic superconductor. Next, we develop a general numerical method to compute the time-dependent complexity by the CV conjecture. By this method, we compute the time-dependent complexity of holographic superconductors. In both normal and superconducting phase, the complexity increases as time goes on and the growth rate saturates to a temperature dependent constant. The higher the temperature is, the bigger the growth rate is. However, the growth rates do not violate the Lloyd's bound in all cases and saturate the Lloyd's bound in the high temperature limit at a late time.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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