We study sectors of an effective gravity aimed at the black hole problem and at the relationship between exterior response, internal states, and evolution. The starting point is the effective action [1], with its additional coefficients, sources, and clock. In the spherical exterior we obtain corrections and an exact two-derivative branch whose minimum areal radius does not, by itself, establish a horizon. The interior structure retains scale selection, hybridization, population preparation, stiffness, poles, and residues. A two-mode realization exhibits a fold and a subsequent response; its coupling to an outgoing channel determines the propagator, self-energy, memory, and emission. Release from a finite reservoir admits causal continuation and an energy calculation by quadratures with controlled error in the fixed-background model.Introducing a free interface yields a second, stronger result within a specified domain: for compatible small data and common coefficients, we construct the same nonlinear radial solution up to any finite time fixed before choosing the amplitude. We prove initial contraction, a first stop, and subsequent positive velocity. A second approximant and a cubic remainder certify outward motion over a post-pulse interval in a nonempty material sector. The conserved Hamiltonian charge, material work, clock, and geometric flux arise from the same system.The populated extension brings together memory, sources, stresses, propagation, and readouts; it contains composite blocks with positive output and a symmetrization of the coupled bulk. Its finite-band verification reveals bulk and flux corrections and a width condition that is not automatically preserved. Matching preparation, emitter, and a finite-energy continuum remains open. We also retain a candidate spectral route to mass and testable relations for the exterior, transition, and clock–energy connection. The formulas retain the assumptions of each sector; a global black hole solution still requires complete matching and causal analysis.
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Tomás Mariano Romero (2026) studied this question.