早期宇宙的熵增长和初始大爆炸条件的确认（为什么夸克-胶子模型不是最好的类比）
Entropy growth in the early universe and confirmation of initial big bang conditions (Why the quark-gluon model is not the best analogy)
摘要：
本文展示了如何从一个初始低的大爆炸水平增加熵值可以通过计数残余引力子实验测量。此外，通过与早期宇宙相变的类比，解释了这种熵增加的物理机制。如此提到的熵的快速增加而没有接近突然增加到10的88次方可能足以允许以类似于从真空状态提取零点能量的方式成功地模拟熵的残余引力子产生
英文摘要：
This paper shows how increased entropy values from an initially low big bang level can be measured experimentally by counting relic gravitons. Furthermore the physical mechanism of this entropy increase is explained via analogies with early-universe phase transitions. The rapid increase in entropy so alluded to without near sudden increases up to 10 to the 88 power may be enough to allow successful modeling of relic graviton production for entropy in a manner similar to zero point energy extraction from a vacuum state
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。
