Calculation of atmospheric neutrino flux using the interaction model calibrated with atmospheric muon data
arXiv:astro-ph/0611418 · doi:10.1103/PhysRevD.75.043006
Abstract
Using the ``modified DPMJET-III'' model explained in the previous paper, we calculate the atmospheric neutrino flux. The calculation scheme is almost the same as HKKM04 \cite{HKKM2004}, but the usage of the ``virtual detector'' is improved to reduce the error due to it. Then we study the uncertainty of the calculated atmospheric neutrino flux summarizing the uncertainties of individual components of the simulation. The uncertainty of -production in the interaction model is estimated by modifying FLUKA'97 and Fritiof 7.02 so that they also reproduce the atmospheric muon flux data correctly, and the calculation of the atmospheric neutrino flux with those modified interaction models. The uncertainties of the flux ratio and zenith angle dependence of the atmospheric neutrino flux are also studied.
References in corpus (2)
Cited by in corpus (16)
- Model-Independent Bound on the Dark Matter Lifetime
- High energy neutrinos from neutralino annihilations in the Sun
- Study of TeV Neutrinos with Upward Showering Muons in Super-Kamiokande
- Dark Matter Through the Neutrino Portal
- Neutrino mass hierarchy extraction using atmospheric neutrinos in ice
- Prospects for Detecting Neutrino Signals from Annihilating/Decaying Dark Matter to Account for the PAMELA and ATIC results
- Study of cosmic ray interaction model based on atmospheric muons for the neutrino flux calculation
- Muon Fluxes From Dark Matter Annihilation
- Kinematic reconstruction of atmospheric neutrino events in a large water Cherenkov detector with proton identification
- Probing Dark Matter Dynamics via Earthborn Neutrinos at IceCube
- Probing new physics with long-lived charged particles produced by atmospheric and astrophysical neutrinos
- Cosmic Ray Positrons from Annihilations into a New, Heavy Lepton
- Sensitivity on Earth Core and Mantle densities using Atmospheric Neutrinos
- Neutrino Astronomy with IceCube
- Neutrino Signals from Solar Neutralino Annihilations in Anomaly Mediated Supersymmetry Breaking Model
- The diffuse GeV-TeV -ray emission of the Cygnus region