早期宇宙中的阻尼电磁涨落？
高能物理 - 理论
2014-08-07 v2
摘要
这篇短文探讨了量子理论对暴胀期间及之后磁场线性演化的影响。分析似乎表明，由于欧姆耗散和真空极化的共同作用，磁场在高温辐射时代呈指数衰减。
引用
@article{arxiv.1408.0367,
title = {Damped Electromagnetic fluctuations in the early universe?},
author = {Ian G. Moss},
journal= {arXiv preprint arXiv:1408.0367},
year = {2014}
}
备注
This paper has been withdrawn by the author. The paper only considers the omega>k regime, but the undamped modes have omega<k