Singularities as Solitons? Quantum Vacuum Architecture of Black Holes
Abstract
We propose that black holes are soliton-esque objects, where gravitational collapse is balanced by quantum vacuum dispersion, modeled via \(R+α R2\) gravity. Classical singularities are replaced by oscillating, finite-radius cores, thereby evading static no-go theorems. The event horizon is replaced by the Lamarina, a surface of maximum redshift whose surface geometry yields Hawking-like radiation with corrections. The Raychaudhuri equations impose a Dyson-type ceiling on the maximum radiated power \((P∞ c5/G)\), while effective field theory matching dictates a universal minimum Lamarina radius set by the dispersion scale.
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