Radio-detection of neutrino-induced air showers: the influence of topography - Archive ouverte HAL Access content directly
Journal Articles Nucl.Instrum.Meth.A Year : 2021

Radio-detection of neutrino-induced air showers: the influence of topography

(1) , (1) , (2) , (3) , (1) , , (4) , , (1)
1
2
3
4

Abstract

Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E > 10 16 eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected.
Fichier principal
Vignette du fichier
S0168900220312006.pdf (2.27 Mo) Télécharger le fichier
Origin : Files produced by the author(s)

Dates and versions

hal-02101669 , version 1 (24-10-2022)

Licence

Attribution - NonCommercial - CC BY 4.0

Identifiers

Cite

V. Decoene, N. Renault-Tinacci, O. Martineau-Huynh, Didier Charrier, K. Kotera, et al.. Radio-detection of neutrino-induced air showers: the influence of topography. Nucl.Instrum.Meth.A, 2021, 986, pp.164803. ⟨10.1016/j.nima.2020.164803⟩. ⟨hal-02101669⟩
78 View
0 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More