来自先前宇宙的热输入能解释残余引力子的产生吗？
Can thermal input from a prior universe account for relic graviton production?
摘要：
在宇宙暴胀的前10的负43次方秒内，引力子的产生强度如何。此外，几个似乎具有正交结论的宇宙学模型，即LQG及其量子反弹和似乎排除量子反弹行为的膜世界模型，被证明部分地相互融合，作为如何调和S的直接解决方案。卡罗尔的预测低温，低熵作为宇宙膨胀的起点，在古斯式混沌膨胀开始时看到10到12次方度开尔文行为。
英文摘要：
Primer for how intense graviton production can be obtained in the first 10 to the minus 43 seconds of cosmological inflation. In addition several cosmological models which appear to have conclusions which are orthogonal, i.e. LQG and its quantum bounce and Brane world models which appear to rule out quantum bounce behavior, are shown to in part blend into each other as a direct solution to how to reconcile S. Carroll's prediction of low temperature, low entropy as a starting point of cosmological inflation with the ten to the 12 power degree kelvin behavior seen at the onset of Guth style chaotic inflation.
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。
