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Black Holes as Phase-Locked Torsional Singularities in G-MaTT: A Geometric Derivation and Novel Predictions

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Zenodo2025-12-17 更新2026-05-26 收录
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Abstract In Generalized Mass as Twisted Time (G-MaTT), black holes are not spacetime singularities but macroscopically coherent topological excitations of the primordial torsion field \(\mathcal{M}_\mu\). We derive their properties from phase synchronization dynamics, showing that the horizon is a phase boundary, entropy arises from braid statistics, and Hawking radiation stems from torsional fluctuations. The information paradox is resolved naturally, as information is encoded in preserved phase relationships. No exotic assumptions are required—black holes emerge purely from the geometry of \(\mathcal{M}_\mu\). Novel predictions include torsion-modulated gravitational waves, quantized area jumps, and ringdown echoes. This framework is consistent with general relativity but extends it to pre-geometric scales, offering testable signatures for LIGO/Virgo, LISA, and future observatories.

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Zenodo
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2025-12-17
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