宇宙早期的强子时期，光速比c大，实际上可达v＝75c。故光速随时间缓慢减小，从v降低到今天的值（c）。另一方面，根据对128个类星体吸收线的测量，在过去的6～12Ga期间，精细结构常数α平均增大了6×10^－6，科学家们认为可能是光速变化造成的。对上述效应进行研究以了解宇宙的过去是有趣的。还深入讨论了超光速研究中的一些问题———微观粒子速度的定义，引力速度，量子纠缠态作用速度以及超距作用。对这些概念有了更准确的理解。

In the early stage of the universe, during the hadronic era, the light velocity was larger than c,  in fact was v=75c. This implies that light velocity has been decreasing in time slowly, from v down to the present value c. On the other hand, based on the measurements of 128 quasar absorption lines, the average increase in fine-structure constantαwas6×10^-6 over the past 6~12Ga. Scientists think it was aroused by the light-speed variation. It would be interesting to investigate if these facts have influenced the past history of the universe. This paper also discusses some problems of faster-than-light research profoundly, such as the velocity definition of the microscopic particles, the velocity of gravitation, the interaction speed of the quantum-entangle-state(QES), and the over distance action.