Renormalized vacuum field interaction as an explanation for dark energy and its implications

In this paper, we attribute the phenomena of dark energy to the interaction of the renormalized vacuum field with charged particles. We test our theory by deriving the dark energy density due to this interaction while staying within the classical domain. Up to a redshift of z = 2, we obtain a value of 5.37x10-10 J/m3, agreeing with observation. We then briefly discuss the implications concerning Hubble tension and the possible support of a proposed dark matter candidate due to the methods we’ve implemented.