中微子振荡的现状
天体物理学
2007-05-23 v1 高能物理 - 唯象学
摘要
太阳和大气中微子数据需要超越标准模型的物理。最简单、最通用但尚未唯一确定的数据解释是中微子振荡。我总结了最新三中微子振荡全局拟合结果，特别是受控实验中对theta_{13}角的限制。尽管数据并未暗示，但双最大化中微子混合模式在层次或准退化中微子情景中显得相当吸引人。
引用
@article{arxiv.astro-ph/0104085,
title = {Status of Neutrino Oscillations},
author = {J. W. F. Valle},
journal= {arXiv preprint arXiv:astro-ph/0104085},
year = {2007}
}
备注
19 pages, latex, 16 figures, adapted summary of review talks delivered recently at various meetings over the past eight months. To be published by the Astronomical Society of the Pacific, conference series, Ed. V. J. Martinez, V. Trimble and M. J. Pons-Borderia