Black holes in effective gravity with quantum response

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.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-30
DOI
https://doi.org/10.5281/zenodo.23070148
Primary Topic
Black Holes and Theoretical Physics
Type
preprint
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preprint

Black holes in effective gravity with quantum response

Tomás Mariano Romero
Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
preprint

Black holes in effective gravity with quantum response

Tomás Mariano Romero
preprint en

Abstract

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.

Zenodo (CERN European Organization for Nuclear Research)
Black Holes and Theoretical Physics
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Black holes in effective gravity with quantum response — Tomás Mariano Romero · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS