High-energy fluxes of atmospheric neutrinos
High-energy neutrinos from decays of mesons, produced in collisions of cosmic ray particles with air nuclei, form unavoidable background for detection of astrophysical neutrinos. More precise calculations of the high-energy neutrino spectrum are required since measurements in the IceCube experiment...
Saved in:
Main Authors | , , |
---|---|
Format | Journal Article |
Language | English |
Published |
25.06.2013
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | High-energy neutrinos from decays of mesons, produced in collisions of cosmic
ray particles with air nuclei, form unavoidable background for detection of
astrophysical neutrinos. More precise calculations of the high-energy neutrino
spectrum are required since measurements in the IceCube experiment reach the
intriguing energy region where a contribution of the prompt neutrinos and/or
astrophysical ones should be discovered. Basing on the referent hadronic models
QGSJET II-03, SIBYLL 2.1, we calculate high-energy spectra, both of the muon
and electron atmospheric neutrinos, averaged over zenith-angles. The
computation is made using three parameterizations of cosmic ray spectra which
include the knee region. All calculations are compared with the atmospheric
neutrino measurements by Frejus and IceCube. The prompt neutrino flux
predictions obtained with thequark-gluon string model (QGSM) for the charm
production by Kaidalov & Piskunova do not contradict to the IceCube
measurements and upper limit on the astrophysical muon neutrino flux. Neutrino
flavor ratio, $\phi_{\nu_ mu}/\phi_{\nu_e}$, extracted from IceCube data
decreases in the energy range $0.1 - 5$ TeV energy contrary to that one might
expect from the conventional neutrino flux. Presumable reasons of such behavior
are: i) early arising contribution from decays of charmed particle, differing
from predictions of present models, ii) revealed diffuse flux of astrophysical
electron neutrinos. The likely diffuse flux of astrophysical neutrinos related
to the PeV neutrino events, detected in the IceCube experiment, leads to a
decrease of the flavor ratio at the energy below 10 TeV, that is in qualitative
agreement with a rough approximation for theflavor ratio obtained from the
IceCube data. |
---|---|
DOI: | 10.48550/arxiv.1306.5907 |