光子质量与甚长基线干涉测量
Photon Mass and Very Long Baseline Interferometry
摘要：
发现了光子质量、光子频率$ν$和由实验者确定的偏转参数$γ$之间的关系（它表征了空间曲率对引力偏转的贡献）。这个令人惊奇的结果使我们能够得出结论，我们只需要知道参数$ν$和$γ$就可以建立光子质量的引力边界。通过考虑作为输入的最新测量的太阳引力偏转的无线电波通过甚长基线干涉测量获得的光子质量的上限估计。
英文摘要：
A relation between the photon mass, its frequency, $ν$, and the deflection parameter, $γ$, determined by experimentalists (which characterizes the contribution of space curvature to gravitational deflection) is found. This amazing result allows us to conclude that the knowledge of the parameters $ν$ and $γ$ is all we need to set up gravitational bounds on the photon mass. By considering as inputs the most recent measurements of the solar gravitational deflection of radio waves obtained via the Very Long Baseline Interferometry, upper bounds on the photon mass are estimated.
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