Detecting Neutrinos from AGNs and Topological Defects with Neutrino Telescopes
高能物理 - 唯象学
2007-05-23 v1
摘要
We evaluate neutrino-nucleon cross section for energies up to 10^{21} eV in light of new information on the small-x behavior of parton distributions. We give predictions for large underground neutrino telescope event rates for ultrahigh-energy neutrinos from Active Galactic Nuclei and from the decay of topological defects formed in the early Universe.
引用
@article{arxiv.hep-ph/9609516,
title = {Detecting Neutrinos from AGNs and Topological Defects with Neutrino Telescopes},
author = {Raj Gandhi and Chris Quigg and M. H. Reno and Ina Sarcevic},
journal= {arXiv preprint arXiv:hep-ph/9609516},
year = {2007}
}
备注
Talk presented by I. Sarcevic at Annual Meeting of Division of Particles and Fields of the APS (DPF'96), Minneapolis, MN, August 10-15, 1996, 3 pp