| _version_ | 1866901395123208192 |
|---|---|
| author | Colley, Christopher Leon |
| author_facet | Colley, Christopher Leon |
| contents | <p>This work develops a constraint-based framework for black hole interior dynamics under a minimal and explicit set of physical assumptions: local classical spacetime, finite interactions, scale separation between microscopic and curvature scales, and absence of sustained external driving.</p> <p>Within this domain, general constraints on admissible macroscopic behavior are derived without specifying the underlying microscopic composition. Transport, relaxation, and causal structure together restrict the system to a parametric region of state space characterized by small structure scale (L much less than R), suppressed anisotropy, near-equilibrium behavior, and overdamped dynamics.</p> <p>This region is defined as a constraint corridor. The framework shows that interior states evolve toward this corridor on timescales short compared to macroscopic evolution, and that the influence of interior structure on external observables is parametrically suppressed.</p> <p>The results are conditional and apply only within the stated assumptions. Rather than proposing a specific interior model, this work establishes necessary constraints that any admissible model must satisfy within a well-defined physical regime. The framework is falsifiable: observation of persistent macroscopic structure, sustained anisotropy, or long-lived non-equilibrium behavior within this regime would contradict the derived constraints.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_19414169 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Constraint-Layer Structure of Black Hole Interiors Under Minimal Physical Assumptions Colley, Christopher Leon black holes black hole interiors general relativity relativistic hydrodynamics compact objects theoretical physics non-equilibrium physics astrophysics <p>This work develops a constraint-based framework for black hole interior dynamics under a minimal and explicit set of physical assumptions: local classical spacetime, finite interactions, scale separation between microscopic and curvature scales, and absence of sustained external driving.</p> <p>Within this domain, general constraints on admissible macroscopic behavior are derived without specifying the underlying microscopic composition. Transport, relaxation, and causal structure together restrict the system to a parametric region of state space characterized by small structure scale (L much less than R), suppressed anisotropy, near-equilibrium behavior, and overdamped dynamics.</p> <p>This region is defined as a constraint corridor. The framework shows that interior states evolve toward this corridor on timescales short compared to macroscopic evolution, and that the influence of interior structure on external observables is parametrically suppressed.</p> <p>The results are conditional and apply only within the stated assumptions. Rather than proposing a specific interior model, this work establishes necessary constraints that any admissible model must satisfy within a well-defined physical regime. The framework is falsifiable: observation of persistent macroscopic structure, sustained anisotropy, or long-lived non-equilibrium behavior within this regime would contradict the derived constraints.</p> |
| title | Constraint-Layer Structure of Black Hole Interiors Under Minimal Physical Assumptions |
| topic | black holes black hole interiors general relativity relativistic hydrodynamics compact objects theoretical physics non-equilibrium physics astrophysics |
| url | https://doi.org/10.5281/zenodo.19414169 |