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PhysRevD.109.014040.pdf
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Affiliation
Department of Physics, University of ArizonaDepartment of Astronomy and Steward Observatory, University of Arizona
Issue Date
2024-01-31
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American Physical SocietyCitation
Bhattacharya, A., Kling, F., Sarcevic, I., & Stasto, A. M. (2024). Forward neutrinos from charm at the Large Hadron Collider. Physical Review D, 109(1), 014040.Journal
Physical Review DRights
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Funded by SCOAP 3.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The currently operating FASER experiment and the planned Forward Physics Facility (FPF) will detect a large number of neutrinos produced in proton-proton collisions at the LHC. In this work, we estimate neutrino fluxes at these detectors from charm meson decays, which will be particularly important for the νe and ντ channels. We make prediction using both the next-to-leading order collinear factorization and the kT-factorization approaches to model the production of charm quarks as well as different schemes to model their hadronization into charm hadrons. In particular, we emphasize that a sophisticated modeling of hadronization involving beam remnants is needed for predictions at FASER and FPF due to the sensitivity to the charm hadron production at low transverse momenta and very forward rapidity. As example, we use the string fragmentation approach implemented in pythia 8. While both standard fragmentation functions and pythia 8 are able to describe LHCb data, we find that pythia 8 predicts significantly higher rate of high energy neutrinos, highlighting the importance of using the correct hadronization model when making predictions. © 2024 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.Note
Open access articleISSN
2470-0010Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1103/PhysRevD.109.014040
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Except where otherwise noted, this item's license is described as Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Funded by SCOAP 3.