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Intrinsic charm in the nucleon and forward production of charm: a new constrain from IceCube Neutrino Observatory

by Rafał Maciuła, Victor P. Goncalves, Antoni Szczurek

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Submission summary

Authors (as registered SciPost users): Rafał Maciuła
Submission information
Preprint Link: https://arxiv.org/abs/2107.13852v1  (pdf)
Date accepted: 2022-03-15
Date submitted: 2021-07-30 08:26
Submitted by: Maciuła, Rafał
Submitted to: SciPost Physics Proceedings
Proceedings issue: 28th Annual Workshop on Deep-Inelastic Scattering (DIS) and Related Subjects (DIS2021)
Ontological classification
Academic field: Physics
Specialties:
  • High-Energy Physics - Phenomenology
Approach: Phenomenological

Abstract

The predictions for the atmospheric neutrino flux at high energies strongly depend on the contribution of prompt neutrinos, which are determined by the production of charmed meson in the atmosphere at very forward rapidities. Here we estimate the related cross sections taking into account the presence of an intrinsic charm (IC) component in the proton wave function. The impact on the predictions for the prompt neutrino flux is investigated assuming different values for the probability to find the IC in the nucleon.

Published as SciPost Phys. Proc. 8, 124 (2022)


Reports on this Submission

Report #1 by Anonymous (Referee 1) on 2022-2-22 (Invited Report)

Report

The results are very nicely summarized in the proceedings. I recommend for publication as it is.

  • validity: -
  • significance: -
  • originality: -
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