Black Hole Evaporation as a Topological Inevitability

This paper develops a topological interpretation of black hole evaporation. Instead of treating Hawking radiation as a purely semiclassical effect, the work proposes that horizon dynamics and Euler defects make outward flux a structural necessity. In this view, information is not lost but redistributed through correlated emissions, resolving the apparent conflict with unitarity. The article is part of a broader informational cosmology program https://zenodo.org/communities/horizon-framework, that seeks to explain physical phenomena by analyzing a deeper, topological layer of reality encoded at horizons.