Authors: Jan Sova
This paper proposes a modification of Einstein’s field equations to include an additional tensor that represents the gravitational influence of matter in the mode of potency (textsc{being in potency}), as defined in a prior ontological framework. Assuming that certain quantum systems before measurement exist in a non-actual but real and structured state, the paper introduces a potentiality energy-momentum tensor alongside the classical tensor T. As a physical consequence, the article presents a revised model of black holes in which matter inside the event horizon transitions into a gravitationally effective potent state, avoiding singularities while preserving external field behavior. This approach offers a new avenue for reconciling general relativity with quantum ontological constraints.
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