Parton distributions need representative sampling


Por: Courtoy, Aurore, Huston, Joey, Nadolsky, Pavel, Xie, Keping, Yan, Mengshi, Yuan C.-P.

Publicada: 10 feb 2023
Resumen:
In global QCD fits of parton distribution functions (PDFs), a large part of the estimated uncertainty on the PDFs originates from the choices of parametric functional forms and fitting methodology. We argue that these types of uncertainties can be underestimated with common PDF ensembles in high-stake measurements at the Large Hadron Collider and Tevatron. A fruitful approach to quantify these uncertainties is to view them as arising from sampling of allowed PDF solutions in a multidimensional parametric space. This approach applies powerful insights gained in recent statistical studies of large-scale population surveys and quasi-Monte Carlo integration methods. In particular, PDF fits may be affected by the big data paradox, which stipulates that more experimental data do not automatically raise the accuracy of PDFs-close attention to the data quality and sampling of possible PDF solutions is as essential. To test if the sampling of the PDF uncertainty of an experimental observable is truly representative of all acceptable solutions, we introduce a technique (''a hopscotch scan'') based on a combination of parameter scans and stochastic sampling. With this technique, we examine the PDF uncertainty on key LHC cross sections at 13 TeV obtained with the public NNPDF4.0 fitting code, while accounting for the likelihood distribution. We show that the uncertainties on the charm distribution at a large momentum fraction x and gluon PDF at small x are enlarged. In PDF ensembles obtained in the analytic minimization (Hessian) formalism, the tolerance on the PDF uncertainty must be based on sufficiently complete sampling of PDF functional forms and choices of the experiments.

Filiaciones:
Courtoy, Aurore:
 Instituto de Física, Universidad Nacional Autónoma de México, Apartado Postal 20-364, Ciudad de México, 01000, Mexico

 Univ Nacl Autonoma Mexico, Inst Fis, Apartado Postal 20-364, Mexico City 01000, Mexico

Huston, Joey:
 Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, United States

 Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

Nadolsky, Pavel:
 Department of Physics, Southern Methodist University, Dallas, TX 75275-0181, United States

 Southern Methodist Univ, Dept Phys, Dallas, TX 75275 USA

Xie, Keping:
 Pittsburgh Particle Physics Astrophysics, and Cosmology Center, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, United States

 Univ Pittsburgh, Pittsburgh Particle Phys Astrophys & Cosmol Ctr, Dept Phys & Astron, Pittsburgh, PA 15260 USA

Yan, Mengshi:
 School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing, 100871, China

 Peking Univ, Sch Phys, Beijing 100871, Peoples R China

 Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China

Yuan C.-P.:
 Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, United States
ISSN: 24700010





PHYSICAL REVIEW D
Editorial
AMER PHYSICAL SOC, ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA, Estados Unidos America
Tipo de documento: Article
Volumen: 107 Número: 3
Páginas:
WOS Id: 000932007000003
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