The questions of what represents space-time in GR, the status of gravitational energy, the substantivalist-relationalist issue, and the (non-)exceptional status of gravity are interrelated. If space-time has energy-momentum, then space-time is substantival. Two extant ways to avoid the substantivalist conclusion deny that the energybearing metric is part of space-time or deny that gravitational energy exists. Feynman linked doubts about gravitational energy to GRexceptionalism, as do Curiel and Duerr; particle physics egalitarianism encourages realism about gravitational energy.In that spirit, this essay proposes a third possible view about spacetime, one involving a particle physics-inspired non-perturbative split that characterizes space-time with a constant background matrix (not a metric tensor), a sort of vacuum value, thus avoiding the inference from gravitational energy to substantivalism. On this proposal, spacetime is M, η , where η = diag(−1, 1, 1, 1) is a spatio-temporally constant numerical signature matrix, a matrix already used in GR with spinors. The gravitational potential, to which any gravitational energy can be ascribed, is g µν (x) − η (up to field redefinitions), an affine geometric object with a tensorial Lie derivative and a vanishing covariant derivative. This non-perturbative split permits strong fields, * Forthcoming in Antonio Vassallo (Ed.), The Foundations of Spacetime Physics: Philosophical Perspectives, Routledge