
doi: 10.5281/zenodo.19554056 , 10.5281/zenodo.19588928 , 10.5281/zenodo.20118100 , 10.5281/zenodo.20346131 , 10.5281/zenodo.20352877 , 10.5281/zenodo.19778746 , 10.5281/zenodo.20240618 , 10.5281/zenodo.20108462 , 10.5281/zenodo.19767046 , 10.5281/zenodo.19778754 , 10.5281/zenodo.19782559 , 10.5281/zenodo.19592649 , 10.5281/zenodo.19786261 , 10.5281/zenodo.19595687 , 10.5281/zenodo.19842200 , 10.5281/zenodo.19608487 , 10.5281/zenodo.19637777 , 10.5281/zenodo.19856741 , 10.5281/zenodo.19861191 , 10.5281/zenodo.20045816 , 10.5281/zenodo.20185227 , 10.5281/zenodo.20677523 , 10.5281/zenodo.19555566 , 10.5281/zenodo.19848766 , 10.5281/zenodo.19611260 , 10.5281/zenodo.19639049
doi: 10.5281/zenodo.19554056 , 10.5281/zenodo.19588928 , 10.5281/zenodo.20118100 , 10.5281/zenodo.20346131 , 10.5281/zenodo.20352877 , 10.5281/zenodo.19778746 , 10.5281/zenodo.20240618 , 10.5281/zenodo.20108462 , 10.5281/zenodo.19767046 , 10.5281/zenodo.19778754 , 10.5281/zenodo.19782559 , 10.5281/zenodo.19592649 , 10.5281/zenodo.19786261 , 10.5281/zenodo.19595687 , 10.5281/zenodo.19842200 , 10.5281/zenodo.19608487 , 10.5281/zenodo.19637777 , 10.5281/zenodo.19856741 , 10.5281/zenodo.19861191 , 10.5281/zenodo.20045816 , 10.5281/zenodo.20185227 , 10.5281/zenodo.20677523 , 10.5281/zenodo.19555566 , 10.5281/zenodo.19848766 , 10.5281/zenodo.19611260 , 10.5281/zenodo.19639049
The black hole information paradox persists for half a century because the accounting system is incomplete. Conventional thermodynamics assumes a single ledger-the matter phase-where information must either be preserved or lost. We propose a minimal extension: the universe maintains two distinct yet strictly conserved information accounts, the matter phase (Ξ) and the cognitive phase (Ω), coupled by a dimensionless cognitive correlation C. In this framework, the black hole singularity is not a terminal point but a format conversion interface: highly ordered matter information entering the singularity is transformed, via a quantum channel, into cognitive-phase potential. This conversion is governed by a modified first law of black hole thermodynamics, and we derive three testable predictions: non-thermal fluctuations in Hawking radiation, extra dissipation in extreme mass-ratio inspirals, and topological settlement signature. We also reinterpret the third law of thermodynamics as a protection principle from two-phase conservation.
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