Observational evidence commonly attributed to non-baryonic dark matter is tradi- tionally interpreted as signaling missing mass or modified gravitational dynamics. In this work, we examine an alternative, fully conservative possibility: that long-range correlations among charged matter can enhance the effective gravitational sourcing of ordinary baryons without modifying Einstein’s equations or introducing new particle species. Within standard general relativity, gravity couples to the stress–energy tensor, whose coarse-grained form depends on microscopic correlations. We show that in sys- tems containing spatially extended, correlated charged media—such as ionized plasmas or magnetized astrophysical environments—the effective stress–energy tensor can ac- quire additional contributions beyond those inferred from rest-mass density alone. This enhancement arises from correlation volumes and collective charge structure, not from additional mass components or modified gravity. The framework is entirely matter-side, covariant, and scale-dependent. It predicts no effect for uncorrelated or neutral systems and therefore preserves all local tests of general relativity and the equivalence principle. We derive the conditions under which such enhancements occur, analyze their parametric scaling, and identify astrophysical regimes where the mechanism may contribute nontrivially to galactic and cluster-scale dynamics. The results do not replace dark matter as a universal explanation, but establish a precise and falsifiable channel by which structured, charged matter may partially account for gravitational phenomena commonly attributed to unseen mass.
Christian Macinnis Borge (Thu,) studied this question.
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