用修正的全息原理进一步解释离散时空的宇宙学常数问题
Further Explanation of the Cosmological Constant Problem by Discrete Space-time through Modified Holographic Principle
摘要：
作者在2001年的论文中提出，假设作为Higgs凝聚相的时空本身是离散的，可以解决宇宙学常数的问题，其计算值与观测值吻合得很好。在此基础上，提出了一种新的方法，即在修正的全息原理的约束下引入真空熵的概念，计算早期宇宙三个不同相变时刻的宇宙学常数。有趣的是，它得出了与前一种方法相同的结论。因此，它揭示了理论中存在着某种基本的东西。讨论了离散时空中洛伦兹不变性的保持问题。
英文摘要：
The author proposed in his previous papers in 2001 that the problem of the cosmological constant could be resolved and its calculated value agrees excellently with the observations by assuming that the space-time itself, as the phase of Higgs condensate, is discrete in nature. Further to such idea, a different approach involving the concept of vacuum entropy that is constrained by the modified Holographic Principle is being used in the calculation of the cosmological constant value at three different phase transition times in the early universe. It is interesting and quite unexpected that it arrives at the same conclusion as the previous approach. It therefore reveals that something fundamental is present in the theory. The problem on the preservation of Lorentz invariance in discrete space-time is also discussed.
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