论文标题
原始量子信息的暗物质
Dark matter from primordial quantum information
论文作者
论文摘要
我们建议宇宙微波背景温度功率峰与通货膨胀慢速参数$ε$之间的一般关系。该关系基于解释变量设置峰的位置为通货膨胀结束和重组之间的量子距离。该距离由Arxiv中引入的原始宇宙学渔民信息确定：2002.04294。宇宙微波背景温度数据设定的观察性约束导致对张量与尺度比率的值非常严格的预测：$ r = 0.01 \ pm 0.002 $。宇宙微波背景的未来极化数据应该能够测量此信号并证实或丢弃我们的模型。
We suggest a general relation between the position of the cosmic microwave background temperature power spectrum peaks and the inflationary slow roll parameter $ε$. This relation is based on interpreting the variable setting the position of the peaks as the quantum distance between the end of inflation and recombination. This distance is determined by the primordial cosmological Fisher information introduced in arXiv:2002.04294. The observational constraints set by cosmic microwave background temperature data lead to a very stringent prediction for the value of the tensor-to-scalar ratio: $r=0.01 \pm 0.002$. Future polarization data of the cosmic microwave background should be able to measure this signal and corroborate or discard our model.
