2025/11/28 by Oscar Loaiza-Brito, Loaiza-Brito, Oscar, J.L. López-Picón +3
Physics and Astronomy · #Black Holes and Theoretical Physics #Astrophysical Phenomena and Observations #Cosmology and Gravitation Theories
paper · pdf · doi:10.48550/arxiv.2511.23338
We use diffeomorphic mappings to connect black hole metrics with complex solutions allowed by the Kontsevich-Segal criterion. By swapping radial and time-like coordinates and applying complex mappings, we derive dynamic metrics suitable for a Quantum Field Theory. This is shown for static and rotating black holes, mapping their interiors into the Kantowski-Sachs and a specific Gowdy-type cosmological model. We offer interpretations of the period during which the Kontsevich-Segal criterion holds.