# $D$ - meson production at very forward rapidities: estimating the   intrinsic charm contribution

**Authors:** F. Carvalho, A.V. Giannini, V.P. Goncalves, F.S. Navarra

arXiv: 1701.08451 · 2018-03-09

## TL;DR

This paper investigates how intrinsic charm in the proton influences D-meson production at very forward rapidities, revealing significant effects at LHC energies that impact atmospheric neutrino flux measurements.

## Contribution

It introduces a detailed analysis of intrinsic charm effects on D-meson production at forward rapidities, including predictions beyond current detector coverage and implications for neutrino flux.

## Key findings

- Intrinsic charm significantly alters D-rapidity distributions at LHC energies.
- Enhanced Feynman-x distributions by approximately tenfold at high energies.
- Intrinsic charm effects dominate in the kinematic range relevant for atmospheric neutrino flux.

## Abstract

We study $D$ - meson production at forward rapidities taking into account the non - linear effects in the QCD dynamics and the intrinsic charm component of the proton wave function. The total cross section, the rapidity distributions and the Feynman - $x$ distributions are calculated for $p p$ collisions at different center of mass energies. Our results show that, at the LHC, the intrinsic charm component changes the $D$ rapidity distributions in a region which is beyond the coverage of the LHCb detectors. At higher energies the IC component dominates the $y$ and $x_F$ distributions exactly in the range where the produced $D$ mesons decay and contribute the most to the prompt atmospheric neutrino flux measured by the ICECUBE Collaboration. We compute the $x_F$ - distributions and demonstrate that they are enhanced at LHC energies by approximately one order of magnitude in the $0.2 \le x_F \le 0.8$ range.

## Full text

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## Figures

22 figures with captions in the complete paper: https://tomesphere.com/paper/1701.08451/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/1701.08451/full.md

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Source: https://tomesphere.com/paper/1701.08451