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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 |
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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 | |
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Academic field: | Physics |
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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)