@misc{10481/71132,
year = {2022},
month = {1},
url = {http://hdl.handle.net/10481/71132},
abstract = {The atmospheric neutrino flux includes a component from the prompt decay of charmed hadrons that becomes significant only at E >= 10 TeV. At these energies, however, the diffuse flux of cosmic neutrinos discovered by IceCube seems to be larger than the atmospheric one. Here we study the possibility to detect a neutrino interaction in down-going atmospheric events at km3 telescopes. The neutrino signal will always appear together with a muon bundle that reveals its atmospheric origin and, generically, it implies an increase in the detector activity with the slant depth. We propose a simple algorithm that could separate these events from regular muon bundles.},
organization = {Spanish Ministry of Science, Innovation and Universities	PID2019-107844GB-C21/AEI/10.13039/501100011033},
organization = {Junta de Andalucia
European Commission	FQM 101- SOMM17/6104/UGR- P18-FR-1962- P18-FR-5057},
organization = {Junta de Andalucia},
organization = {Program Es-tancias Postdoctorales en el Extranjero 2019-2020 of CONACYT, Mexico},
organization = {Universidad de Granada/CBUA},
organization = {Catedra Marcos Moshinsky (Fundacion Marcos Moshinsky)},
publisher = {Elsevier},
keywords = {Neutrino telescopes},
keywords = {Muons},
keywords = {Cosmic rays},
title = {Neutrino events within muon bundles at neutrino telescopes},
doi = {10.1016/j.astropartphys.2021.102646},
author = {Gutiérrez González, Miguel and Hernández Tomé, G. and Illana Calero, José Ignacio and Masip Mellado, Manuel},
}