Quantum vacuum fluctuations

Serge Reynaud , Astrid Lambrecht , Cyriaque Genet , Marc-Thierry Jaekel
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引用次数: 14

Abstract

The existence of irreducible field fluctuations in vacuum is an important prediction of quantum theory. These fluctuations have many observable consequences, like the Casimir effect, which is now measured with good accuracy and agreement with theory, provided that the latter accounts for differences between real experiments and the ideal situation considered by Casimir. But the vacuum energy density calculated by adding field mode energies is much larger than the density observed around us through gravitational phenomena. This ‘vacuum catastrophe’ is one of the unsolved problems at the interface between quantum theory on one hand, inertial and gravitational phenomena on the other hand. It is however possible to put properly formulated questions in the vicinity of this paradox. These questions are directly connected to observable effects bearing upon the principle of relativity of motion in quantum vacuum.

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量子真空涨落
真空中不可约场涨落的存在是量子理论的一个重要预言。这些波动有许多可观察到的结果,比如卡西米尔效应,它现在被精确地测量出来,并且与理论一致,前提是后者解释了实际实验与卡西米尔所考虑的理想情况之间的差异。但是,通过添加场模能量计算出的真空能量密度比通过引力现象在我们周围观察到的密度要大得多。这种“真空突变”是量子理论与惯性和引力现象之间的一个尚未解决的问题。然而,在这个悖论的附近提出适当的问题是可能的。这些问题与量子真空中运动相对性原理所产生的可观测效应直接相关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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