Quantifying uncertainties in the high energy neutrino cross-section
arXiv:1108.1755 · doi:10.1007/s12043-012-0452-9
Abstract
We compare predictions for high energy neutrino and anti-neutrino deep inelastic scattering cross-sections within the conventional DGLAP formalism of next-to-leading order QCD, using the latest parton distribution functions such as CT10, HERAPDF1.5 and MSTW08 and taking account of PDF uncertainties. From this we derive a benchmark cross-section and uncertainty which is consistent with the results obtained earlier using the ZEUS-S PDFs. We advocate the use of this for analysing data from neutrino telescopes, in order to facilitate comparison between their results.
4 pages, 4 figures; to appear in Proceedings of the 32nd International Cosmic Ray Conference, Beijing, China, 11-18 August 2011