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Heuristic Estimation of the Vacuum Energy Density of the Universe: Part I—Analysis Based on Time Domain Electromagnetic Radiation 宇宙真空能量密度的启发式估计:基于时域电磁辐射的分析
Pub Date : 2023-01-01 DOI: 10.4236/jemaa.2023.156006
Vernon Cooray, Gerald Cooray, Marcos Rubinstein, Farhad Rachidi
In this paper, an inequality satisfied by the vacuum energy density of the universe is derived using an indirect and heuristic procedure. The derivation is based on a proposed thought experiment, according to which an electron is accelerated to a constant and relativistic speed at a distance L from a perfectly conducting plane. The charge of the electron is represented by a spherical charge distribution located within the Compton wavelength of the electron. Subsequently, the electron is incident on the perfect conductor giving rise to transition radiation. The energy associated with the transition radiation depends on the parameter L. It is shown that an inequality satisfied by the vacuum energy density will emerge when the length L is pushed to cosmological dimensions and the product of the radiated energy and the time duration of emission are constrained by Heisenberg’s uncertainty principle. The inequality derived is given by ρΛ ≤ 9.9×10-9J/m3 where ρΛ is the vacuum energy density. This result is consistent with the measured value of the vacuum energy density, which is 0.538 × 10-9J/m. Since there is a direct relationship between the vacuum energy density and the Einstein’s cosmological constant, the inequality can be converted directly to that of the cosmological constant.
本文用一种间接启发式方法推导了宇宙真空能量密度所满足的一个不等式。推导是基于一个被提出的思想实验,根据该实验,电子在距离完美导电平面L的距离上被加速到恒定的相对论速度。电子的电荷由位于电子康普顿波长内的球形电荷分布表示。随后,电子入射到完美导体上,产生跃迁辐射。与跃迁辐射相关的能量取决于参数L。结果表明,当长度L被推到宇宙维度时,会出现真空能量密度满足的不等式,辐射能量的乘积和发射的时间持续时间受海森堡测不准原理的约束。得到的不等式为ρΛ≤9.9×10-9J/m3,其中ρΛ为真空能量密度。该结果与真空能量密度的实测值0.538 × 10-9J/m一致。由于真空能量密度与爱因斯坦宇宙常数之间存在直接关系,因此可以将该不等式直接转换为宇宙常数的不等式。
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Journal of Electromagnetic Analysis and Applications
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