晶体真空宇宙空间模型的熵界
Entropy Bound for the Crystalline Vacuum Cosmic Space Model
摘要：
应用海森堡的不确定原理，对由引力波形成的宏观量子气体，得到了Bekenstein提出的对任何最大半径R和总能量E的系统的熵的普遍界的表达式。利用这个表达式，在晶体真空宇宙模型的理论方案中，解释了大爆炸开始时的低熵值1088k。根据我们的分析，时间箭头被很好地定义，并且理论时间流仅在一个方向上发生，这是由真空空间晶体结构在平衡条件附近的引力稳定的物理过程所要求的。PACS编号：65.50。+ m，97.60，Lf，03.65。w，61.50。f，98.80英尺，04.20英尺。Q
英文摘要：
By applying the Heisenberg's uncertainty principle for a macroscopic quantum gas formed by gravitational waves an expression for the universal bound on the entropy proposed by Bekenstein for any system of maximum radius R and total energy E has been obtained. By using such expression, in the theoretical scheme of the crystalline vacuum cosmic model, the low entropy value at the Big Bang beginning, 1088k, is explained. According to our analysis the time arrow is well defined and the theoretical time flow occurs only in one direction as requested by the physical processes of gravitational stabilization of the vacuum space crystalline structure around equilibrium conditions. PACS numbers: 65.50.+m, 97.60.Lf, 03.65.-w, 61.50.-f, 98.80.Ft, 04.20.-q
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
