在霍金辐射模拟中具有零和能量的表面波包对

A. Guha, E. Heifetz, Akanksha Gupta
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引用次数: 2

摘要

在这里,我们提出了一个最小的模拟重力设置,并建议如何选择两个表面重力波包来模拟来自非旋转黑洞视界的霍金辐射的一些关键方面。与传统研究的散射问题不同,我们提出的设置由平坦测深上的恒定平均流组成,其中两个波包具有相同的波作用量,但能量相等且相反(符号),从而模拟了由近视界真空波动产生的虚拟粒子。注意到与波的内在相速和总相速有关的波作用符号和能量范数的物理机制。我们构造等波作用的窄波包,具有正能量和群速的逆平均流传播并以霍金辐射的形式逃离黑洞,而具有负能量和群速的另一个被平均流漂移而落入黑洞。通过构造,我们的最小模型满足了霍金关于低频模式放大的预测。我们发现,波包的质心波数与表面高程幅值之间存在简单的解析关系。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Pairs of surface wave packets with zero-sum energy in the Hawking radiation analog
Here we propose a minimal analog gravity setup and suggest how to select two surface gravity wave packets in order to mimic some key aspects of Hawking radiation from the horizon of non-rotating black holes. Our proposed setup, unlike the scattering problem conventionally studied, constitutes of a constant mean flow over a flat bathymetry, in which the two wave packets possess the same amount of wave action but equal and opposite (sign) amount of energy, thereby mimicking virtual particles created out of near horizon vacuum fluctuations. Attention is given to the physical mechanism relating to the signs of the wave action and energy norm with the wave's intrinsic and total phase speeds. We construct narrow wave packets of equal wave action, the one with positive energy and group speed propagates against the mean flow and escapes from the black hole as Hawking radiation, while the other with negative energy and group speed is drifted by the mean flow and falls into it. Hawking's prediction of low frequency mode amplification is satisfied in our minimal model by construction. We find that the centroid wavenumbers and surface elevation amplitudes of the wave packets are related by simple analytical expressions.
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