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.
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.
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Publication: arXiv:2302.11126
Presenters
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Anthony W Thomas
- University of Adelaide