Direct photon production and PDF fits reloaded

John M. Campbell, Juan Rojo, Emma Slade*, Ciaran Williams

*Corresponding author for this work

Research output: Contribution to JournalArticleAcademicpeer-review

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Abstract

Direct photon production in hadronic collisions provides a handle on the gluon PDF by means of the QCD Compton scattering process. In this work we revisit the impact of direct photon production on a global PDF analysis, motivated by the recent availability of the next-to-next-to-leading (NNLO) calculation for this process. We demonstrate that the inclusion of NNLO QCD and leading-logarithmic electroweak corrections leads to a good quantitative agreement with the ATLAS measurements at 8 and 13 TeV, except for the most forward rapidity region in the former case. By including the ATLAS 8 TeV direct photon production data in the NNPDF3.1 NNLO global analysis, we assess its impact on the medium-x gluon. We also study the constraining power of the direct photon production measurements on PDF fits based on different datasets, in particular on the NNPDF3.1 no-LHC and collider-only fits. We also present updated NNLO theoretical predictions for direct photon production at 13 TeV that include the constraints from the 8 TeV measurements.

Original languageEnglish
Article number470
Pages (from-to)1-21
Number of pages21
JournalEuropean Journal of Physics C
Volume78
Issue number6
Early online date9 Jun 2018
DOIs
Publication statusPublished - Jun 2018

Funding

Acknowledgements We thank Ulla Blumenschein, Ana Cueto Gómez, Jan Kretzschmar, Claudia Glasman, Matthias Schott, and Juan Ter- rón Cuadrado for information and discussions concerning the ATLAS direct photon measurements. JR and ES are grateful to our colleagues of the NNPDF collaboration for their support and useful discussions. ES thanks Rhorry Gauld for providing useful scripts and Alberto Guf-fanti for help with the production of APPLgrids. JR and ES are supported by the ERC Starting Grant “PDF4BSM”. The work of JR is also supported by the Dutch Organization for Scientific Research (NWO). CW is supported by a National Science Foundation CAREER award PHY-1652066. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics. We thank Ulla Blumenschein, Ana Cueto Gómez, Jan Kretzschmar, Claudia Glasman, Matthias Schott, and Juan Terrón Cuadrado for information and discussions concerning the ATLAS direct photon measurements. JR and ES are grateful to our colleagues of the NNPDF collaboration for their support and useful discussions. ES thanks Rhorry Gauld for providing useful scripts and Alberto Guffanti for help with the production of APPLgrids. JR and ES are supported by the ERC Starting Grant “PDF4BSM”. The work of JR is also supported by the Dutch Organization for Scientific Research (NWO). CW is supported by a National Science Foundation CAREER award PHY-1652066. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics.

FundersFunder number
Fermi Research Alliance, LLC
National Science Foundation1652066, PHY-1652066
U.S. Department of Energy
Office of Science
High Energy Physics
FermilabDE-AC02-07CH11359
H2020 European Research CouncilERC-StG-2012-335260
Seventh Framework Programme335260
European Research Council
Nederlandse Organisatie voor Wetenschappelijk Onderzoek

    Keywords

    • hep-ph
    • hep-ex

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