High Energy Astroparticle Physics
天体物理学
2009-11-11 v1 高能物理 - 唯象学
摘要
We give a brief (and highly incomplete) overview of the current experimental and theoretical status of high energy cosmic rays and their secondary gamma-rays and neutrinos. We focus on the role of large scale magnetic fields and on multi-messenger aspects linking these three channels. We also recall that the flavor composition of neutrino fluxes from astrophysical sources contains information on both the source conditions and neutrino physics.
引用
@article{arxiv.astro-ph/0612240,
title = {High Energy Astroparticle Physics},
author = {Guenter Sigl},
journal= {arXiv preprint arXiv:astro-ph/0612240},
year = {2009}
}
备注
6 papes, 2 figures, proceedings of plenary talk at the Neutrino Oscillation Workshop (NOW 2006), Conca Specchiulla, Italy, September 9-16, 2006