Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/139762
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Type: Journal article
Title: Global QCD analysis and dark photons
Author: Hunt-Smith, N.T.
Melnitchouk, W.
Sato, N.
Thomas, A.W.
Wang, X.G.
White, M.J.
Citation: The Journal of High Energy Physics, 2023; 2023(9):96-0-96-15
Publisher: Springer-Verlag
Issue Date: 2023
ISSN: 1029-8479
1029-8479
Statement of
Responsibility: 
N. T. Hunt-Smith, a W. Melnitchouk, a, b N. Sato, b A. W. Thomas, a X. G. Wanga and M. J. Whitea on behalf of the Jefferson Lab Angular Momentum (JAM) collaboration
Abstract: We perform a global QCD analysis of high energy scattering data within the JAM Monte Carlo framework, including a coupling to a dark photon that augments the Standard Model (SM) electroweak coupling via kinetic mixing with the hypercharge B boson. We first set limits on the dark photon mass and mixing parameter assuming that the SM is the true theory of Nature, taking into account also the effect on g – 2 of the muon. If instead we entertain the possibility that the dark photon may play a role in deep-inelastic scattering (DIS), we find that the best fit is preferred over the SM at 6.5σ, even after accounting for missing higher order uncertainties. The improvement in χ² with the dark photon is stable against all the tests we have applied, with the improvements in the theoretical predictions spread across a wide range of x and Q². The largest improvement corresponds to the fixed target and HERA DIS data, while the best fit yields a value of g – 2 which significantly reduces the disagreement with the latest experimental determination.
Keywords: Dark Matter at Colliders; Deep Inelastic Scattering or Small-x Physics; Parton Distributions; Specific QCD Phenomenology
Description: Published: September 15, 2023
Rights: Open Access, © The Authors. Article funded by SCOAP3. Open Access. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
DOI: 10.1007/JHEP09(2023)096
Grant ID: http://purl.org/au-research/grants/arc/CE200100008
http://purl.org/au-research/grants/arc/DP180102209
Published version: http://dx.doi.org/10.1007/jhep09(2023)096
Appears in Collections:Physics publications

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