原始磁场的 CMB 信号
天体物理学
2009-10-31 v1
摘要
原始随机磁场将诱导出宇宙微波背景中的温度和偏振涨落。我们概述了计算这些涨落功率谱的方法，并给出数值结果。
引用
@article{arxiv.astro-ph/0011095,
title = {CMB Signatures of a Primordial Magnetic Field},
author = {Tina Kahniashvili and Arthur Kosowsky and Andrew Mack and Ruth Durrer},
journal= {arXiv preprint arXiv:astro-ph/0011095},
year = {2009}
}
备注
To appear in "Cosmology and Particle Physics" eds J. Garcia-Bellido, R. Durrer, and M. Shaposhnikov, 6 pages, 1 figure, LaTeX uses aipproc.sty (included)