Spectral Kernel Dynamics for Planetary Surface Graphs: Distinction Dynamics and Topological Conservation

• URL: http://arxiv.org/abs/2604.20887v1
• Date: Fri, 17 Apr 2026 23:38:56 GMT
• Title: Spectral Kernel Dynamics for Planetary Surface Graphs: Distinction Dynamics and Topological Conservation
• Abstract summary: We formalise the distinction dynamics equation dc/dt = G[c, h_t], with MaxCal-optimal realisation G_opt.<n>On fixed-topology 3D surface graphs we derive a conditional topology-preserving compression theorem.<n>A triple necessary spectral diagnostic is derived for planetary drainage networks at O(N) cost.
• Score: 0.0
• License: http://creativecommons.org/licenses/by/4.0/
• Abstract: The spectral kernel field equation R[k] = T[k] lacks a conservation-law analog. We prove (i) the fixed-point flow is strictly volume-expanding (tr DF > 0), precluding automatic conservation, and (ii) the conservation deficit per mode equals the Hessian stability margin exactly: D_m = -Delta'. Closing the deficit requires a scene-side compensating contribution, which we formalise as the distinction dynamics equation dc/dt = G[c, h_t], with MaxCal-optimal realisation G_opt. On fixed-topology 3D surface graphs we derive a conditional topology-preserving compression theorem: retaining k >= beta_0 + beta_1 modes (under a spectral-ordering assumption) preserves all Betti-number charges; we include a worked short-cycle counterexample (figure-eight) calibrating when the assumption fails. A triple necessary spectral diagnostic -- Fiedler-mode concentration, elevated curl energy, anomalous beta_1 -- is derived for planetary drainage networks at O(N) cost. Two internal real-data sequences serve as preliminary consistency checks; full benchmarks and adaptive-topology extensions are deferred.

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