极低熵下量子玻色-爱因斯坦凝聚的修正白洞焓耦合

Amos S. Kubeka, Alireza Amani, Mantile Lekala
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引用次数: 0

摘要

我们把宇宙建模为一个白洞,在这个过程中,我们对修改后的白洞的焓方程进行了详细的分析,我们得到了一个更详细的图像,关于何时以及如何;宇宙发生了量子引力(宇宙学)阶段、暴胀阶段和加速阶段。我们确定了修正白洞的场方程,并对尺度因子进行了演化,并将其演化与宇宙的热力学性质进行了比较。我们还说明了强能量条件被违反,但零能量条件和强宇宙审查都没有被违反。最后,我们在量子引力(宇宙学)体制下将焓与极低熵的玻色-爱因斯坦凝聚相耦合。此后,我们确定了玻色-爱因斯坦量子方程的不稳定条件,我们将其解释为大爆炸发生的时刻。
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Modified White Hole Enthalpy Coupled to Quantum Bose-Einstein Condensate at Extremely Low Entropy
We model the universe as a white hole, and in the process we perform detailed analysis of the enthalpy equation of the modified white hole, and we get a much detailed picture of when and how did; quantum gravity (cosmology) phase, inflationary phase, and the acceleration phase of the universe happened. We determine the field equations of the modified white hole and evolve the scale factor and compare the evolution to the thermodynamic properties of the universe. We also illustrate that the strong energy condition is violated, but both the null energy condition and the strong cosmic censorship are not violated. Lastly, we couple the enthalpy to the Bose-Einstein condensate at extremely low entropy at the quantum gravity (cosmology) regime. Thereafter, we determine the unstable condition of the Bose-Einstein quantum equation which we interpret as the moment when the big bang occurred.
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