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High overtone quasinormal modes of analog black holes and the small scale structure of the background fluid

机译:模拟黑洞的高泛音准正态模式和背景流体的小尺度结构

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The goal of this paper is to build a foundation for, and explore the possibility of, using high overtone quasinormal modes (QNMs) of analog black holes to probe the small scale (microscopic) structure of a background fluid in which an analog black hole is formed. This may provide a tool to study the small scale structure of some interesting quantum systems such as Bose-Einstein condensates (BECs). In order to build this foundation, we first look into the hydrodynamic case where we calculate the high overtone QNM frequencies of a 3+1 dimensional canonical non-rotating acoustic black hole. The leading order calculations have been done earlier in the literature. Here, we obtain the first order correction. We then analyze the high overtone QNMs of acoustic black holes in a BEC using the linearized Gross-Pitaevskii equation. We point out that at the high overtone QNM limit, the only term that is important in the linearized Gross-Pitaevskii equation is the quantum potential term, which is a small scale effect.
机译:本文的目的是为使用模拟黑洞的高泛音准正态模式(QNM)探究模拟黑洞所在的背景流体的小规模(微观)结构奠定基础,并探讨其可能性。形成。这可能提供了研究某些有趣的量子系统(例如玻色-爱因斯坦凝聚物(BEC))的小规模结构的工具。为了建立基础,我们首先研究流体动力学情况,在该情况下我们计算3 + 1维规范非旋转声学黑洞的高泛音QNM频率。提前量计算已在文献中进行过。在这里,我们得到一阶校正。然后,我们使用线性化的Gross-Pitaevskii方程分析了BEC中声学黑洞的高泛音QNM。我们指出,在高泛音QNM限制下,线性化Gross-Pitaevskii方程中唯一重要的项是量子势项,这是小规模效应。

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