A Hint of the Existence of a Dark Photon

ORAL

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. 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 best fit yields a value of g−2 which significantly reduces the disagreement with the latest experimental determination.

*This work was supported by the Australian Research Council through the ARC Centre of Excellence for Dark Matter Particle Physics (CE200100008) and the ARC Discovery Project DP180102209 (MJW), as well as by the DOE contract No. DE-AC05-06OR23177, under which Jefferson Science Associates, LLC operates Jefferson Lab.

Publication: arXiv:2302.11126

Presenters

  • Anthony W Thomas

    • University of Adelaide

Authors

  • Anthony W Thomas

    • University of Adelaide
  • Nicholas Hunt-Smith

    • The University of Adelaide
  • Wally Melnitchouk

    • Jefferson Lab
  • Nobuo Sato

    • Jefferson Lab
  • Martin White

    • The University of Adelaide
  • Xuan-Gong Wang

    • The University of Adelaide