The persistent nonperturbative charm enigma

The question of the existence and possible magnitude of nonperturbative (often called “intrinsic”) charm in the proton has long confounded attempts to cleanly isolate such a contribution in global analyses of high-energy experiments. In this letter, we show that the available (non)perturbative QCD t...

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Main Authors: Marco Guzzi, T.J. Hobbs, Keping Xie, Joey Huston, Pavel Nadolsky, C.-P. Yuan
Format: Article
Language:English
Published: Elsevier 2023-08-01
Series:Physics Letters B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S037026932300309X
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author Marco Guzzi
T.J. Hobbs
Keping Xie
Joey Huston
Pavel Nadolsky
C.-P. Yuan
author_facet Marco Guzzi
T.J. Hobbs
Keping Xie
Joey Huston
Pavel Nadolsky
C.-P. Yuan
author_sort Marco Guzzi
collection DOAJ
description The question of the existence and possible magnitude of nonperturbative (often called “intrinsic”) charm in the proton has long confounded attempts to cleanly isolate such a contribution in global analyses of high-energy experiments. In this letter, we show that the available (non)perturbative QCD theory and hadronic data have still not developed to a sufficient level to clearly resolve this problem. We highlight a number of challenging aspects that must be confronted in extracting nonperturbative charm in PDF fits, and in so doing, present an updated next-to-next-to-leading order CT analysis of fitted charm, CT18 FC, which we also compare to recent studies. We outline the theory developments and future data needed to make progress on this subject.
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spelling doaj.art-8fd7ce4010794a5598ed6c4a76cf252d2023-07-21T04:58:08ZengElsevierPhysics Letters B0370-26932023-08-01843137975The persistent nonperturbative charm enigmaMarco Guzzi0T.J. Hobbs1Keping Xie2Joey Huston3Pavel Nadolsky4C.-P. Yuan5Department of Physics, Kennesaw State University, Kennesaw, GA 30144, USAHigh Energy Physics Division, Argonne National Laboratory, Argonne, IL 60439, USA; Corresponding author.Pittsburgh Particle Physics, Astrophysics, and Cosmology Center, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USADepartment of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USADepartment of Physics, Southern Methodist University, Dallas, TX 75275-0181, USA; Fermi National Accelerator Laboratory, Batavia, IL 60510, USADepartment of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USAThe question of the existence and possible magnitude of nonperturbative (often called “intrinsic”) charm in the proton has long confounded attempts to cleanly isolate such a contribution in global analyses of high-energy experiments. In this letter, we show that the available (non)perturbative QCD theory and hadronic data have still not developed to a sufficient level to clearly resolve this problem. We highlight a number of challenging aspects that must be confronted in extracting nonperturbative charm in PDF fits, and in so doing, present an updated next-to-next-to-leading order CT analysis of fitted charm, CT18 FC, which we also compare to recent studies. We outline the theory developments and future data needed to make progress on this subject.http://www.sciencedirect.com/science/article/pii/S037026932300309XQuantum chromodynamicsParton distribution functionsCollider phenomenology
spellingShingle Marco Guzzi
T.J. Hobbs
Keping Xie
Joey Huston
Pavel Nadolsky
C.-P. Yuan
The persistent nonperturbative charm enigma
Physics Letters B
Quantum chromodynamics
Parton distribution functions
Collider phenomenology
title The persistent nonperturbative charm enigma
title_full The persistent nonperturbative charm enigma
title_fullStr The persistent nonperturbative charm enigma
title_full_unstemmed The persistent nonperturbative charm enigma
title_short The persistent nonperturbative charm enigma
title_sort persistent nonperturbative charm enigma
topic Quantum chromodynamics
Parton distribution functions
Collider phenomenology
url http://www.sciencedirect.com/science/article/pii/S037026932300309X
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