计算表明分布在一个相当大范围的电子可以在真空中被加速到相对论能量。
The calculation shows that electrons distributed on a large scale can be accelerated to relativistic energy in vacuum.
本文从单粒子模型出发，导出了考虑相对论能量因子一级扰动量影响的色散方程。
In this paper, on the basis of a single-particle model, the dispersion equation is obtained after considering the first perturbation term of relativistic energy factor.
粒子物理学理论预言暗能量的强度要比观测到的大约大120个数量级，而广义相对论不能解释这个巨大的差异。
The theories of particle physics predict the strength of dark energy to be about 120 orders of magnitude larger than what is observed, and general relativity cannot explain this enormous discrepancy.
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