Prompt atmospheric neutrinos in the quark–gluon string model

Abstract We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the D mesons and $${\Lambda }^{+}_{c}$$ Λc+ baryons production in pA and $$\pi A$$ πA collisions are calculated in the phenomenological quark–gluon...

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Bibliographic Details
Main Authors: S. I. Sinegovsky, M. N. Sorokovikov
Format: Article
Language:English
Published: SpringerOpen 2020-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-019-7547-0
Description
Summary:Abstract We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the D mesons and $${\Lambda }^{+}_{c}$$ Λc+ baryons production in pA and $$\pi A$$ πA collisions are calculated in the phenomenological quark–gluon string model (QGSM) which is updated using recent measurements of cross sections of the charmed meson production in the LHC experiments. A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit from the IceCube experiment, and with predictions of other charm production models.
ISSN:1434-6044
1434-6052